1 of 46. Abbreviated title: [SAP-SVT-Nmsm-g & 137] - Updated on 07 Oct, 09. Shankar V.Narayanan

Size: px
Start display at page:

Download "1 of 46. Abbreviated title: [SAP-SVT-Nmsm-g & 137] - Updated on 07 Oct, 09. Shankar V.Narayanan"

Transcription

1 1 of 46 Subatomic Particls ad thir FOUR Itractios icludig (g &17) (p&) factors with Spac Vortx Thory (A No matrial shll modl) (Part 1 of ) (Th cotts of this txt ar th sam as i ONE EQUATION ad FOUR Subatomic Particls Itractios titl oly chagd i ordr to mak it mor xplicit) Abbrviatd titl: [SAP-SVT-Nmsm-g & 17] Corrspodig Author: V Shakar Narayaa - tolratsam@gmail.com Updatd o 07 Oct, 09 Shakar V.Narayaa Ky Words: 1) Nuclar Particls ) Wak Itractios ) Gravitatio 4) Ds Mattr, 5) Black Hol Physics 6) Elctro lctric dipol momt 7) Smi-classical mthod. 8) Corrctios to a boud lctro ( g factor). 9).Elmtary Particls Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

2 of 46 Abstract This proposd dyamically stabl o-matrial shll modl is a atural outcom from (mass-rgy) to (fild rgy) quivalc for a spiig chargd particl that follows by aalyzig a pair aihilatio procss ad corrlatio with may xprimtal fidigs ad obsrvatios by usig prov laws. I 190, Paul Dirac dvlopd a w vrsio of th Schrödigr Wav Equatio which was rlativistically ivariat, ad prdictd th magtic momt corrctly, ad at th sam tim tratd th lctro as a poit particl. Though Dr: Dirac dalt th lctro as a poit particl oly from a mathmatical tratmt poit of viw, it will b show hr its partial implicatio o uclo forcs ad furthr Ifiit gativ rgy o Gravitatio. Coicidtally th high rgy xprimts idicatig towards a poit particl for lctro is a clar misitrprtatio that is ladig us away from th classical Physics which may usd to udrstad. Hr agai it will b show why a lctro td to idicat smallr radius at highr ad highr rgis ad what is its tru o rlativistic radius is also show with xprimtal backig. This proposd modl is foud to rplac th prst mpirical formula for uclar siz, itroducs w prcis quatio for uclar pottial barrir, siz ad spacig btw uclos for vry idividual bidig rgy of lmts ad furthr it sms to provid a mor appropriat modl i plac of th prst quarks ad itrrlats all four particl itractios. Howvr may othr xprimtal fidigs hav hlpd i dirctig th dvlopmt of th modl spcially i fixig th uclo siz ad magtic momts- (g ad 17) factors, o utros i utro bta dcay if lctros wr to b poit particls ad hc this modl may b xpctd to prdict particl itractios i a largr prspctiv with a smi classical approach. All this is possibl with Spac Vortx cocpt with a slightly diffrt approach ivolvig simpl mathmatics ad a cospicuous approach ladig to highly accurat rsults although focusd maily o scholarly physicists is also slightly dtaild kpig i mid graduat studts ad itrdiscipliary participatio for furthr all roud dvlopmt of th subjct. Th xprimts coductd by Sir: J.J.Thomso i attachd at th d of txt alog with th rsults backd by his ow quatio ad that o Kli-Nishia formula substatiats that th lctro radius is its classical radius. Th dtaild low rgy xprimt is rpatabl at ay rasoably quippd laboratory ay tim ay whr. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

3 of 46 Th sam quatios ad photo-lctro scattrig also disprovs Kitic rgy part of currt Spcial Thory of Rlativity. Also kpig i mid studts som aspcts ar strssd with a clos aalogy ad som spcific commts o currt physics ar brought out bcaus it may ot b asily availabl from ducatioal wbsits or from books.. Classificatio Schm Nos. : PACS Nos (Dr) (1.90+f), (.40-S, Bw) (1.10.g) PACS: 1.0.Jp, 1.0.Js, 1.15xg, 0.0 +p. Itroductio Th ida, that th uivrsality of all mattr could b i [rgy- form] xists right from th first thought giv by th mit scitist Sir:J.J. Thomso ad othr scitists of his tim, ad o th basis of which, thy furthr argud that, thr caot b two kids of masss ad that all mass must b lctrical mass ad such a swpig gralizatio was too prmatur to b accptd at that tim [Though Eisti did ot rfut this thought h had oly isistd that v lctrical rgy mass should td to ifiity as particl vlocity approachs that of light i his Spcial Thory] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

4 4 of 46 Rvivig thir thoughts with th hlp of Spac Vortx Thory ad may cotributios mad by mit scitists ad xprimtr s so far, this basic modl procds from strog forc to magtic momts up to gravitatioal attractio ad furthr to rsolv som puzzls i currt physics with a smi classical approach. Summary of th compariso with Currt Physics Rfrcs quotd i th txt for g:-cmp-ab-9 implis [Cocpt of Modr Physics-By Arthur Bisr-Pag-9] Fidigs i Modr Sl.N Proprty/ As foud i this proposd physics thory / o Natur thory Exprimt Rfrc 1 Subatomic Particls Poit particl Dyamically stabl Sphrical zo of comprssiv forc & vlopd i a positiv CMP AB-78, AP-JBR-70, 1068 NP-NR-AK 54 NP-IK-64/414 outward lctric fild forc outsid th shll itrfac. Subatomic Poit mass/poit Fiit siz/fiit fild CMP-ABparticl siz charg/ifiit fild itsity. itsity/dyamically stabl. Nuclo Pottial barrir No prcis xprssio hc assumd squar Drivd xprssio with w quatios for spacig, bidig rgy pr uclo. CMP-AB-406 NPNR-AK 94 NP-IK 50 wll. 4 Valu of [Ro] 1. fm Empirical [1.165 fm] at itrfac drivd xprssio NPNR-AK-77 CMP-AB-89 5 Rag of uclar forc Approx [1.7 fm] By Mso thory [1.7 fm] for [0.8 MV to 5 MV] with drivd xprssio. Nutro bcoms gativly chargd i th uclus; hc o mso xchag is dd. 6 Spacig Not prcisly Drivd xprssio CMP-AB-410 Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

5 5 of 46 btw kow from thory uclos i a uclus 7. Nuclar Not prcisly Slightly lss tha [0.49fm] NPNR-AK-96 itractio kow from thory from thory NP-IK-56 chag but Idicativ from AP-JBR-19 from xprimts of attractio about [0.5 fm] to rpulsio. 8. Siz of a Not prcisly About [ fm] for uclos kow proto ad (0.484fm) for utro from thory. 9. Rsoac [549 MV], [78 [549 MV], [78 MV] CMP-AB particls MV] from icludd withi th uclo xprimts for particl structur. msos. 10 Nuclo Agrs with Agrs with xprimts as AP-JBR-1191,18 magtic xprimts Quark Shll substructur modl CMP-AB-91 momt modl [itgral charg [but fractioal frmios].th / factor charg frmios] coms aturally 11 Quark (10-15 to )m Ucrtai Ergy Sub- At (1.6 x10-18 )m rgy rag (115 Mv to shlls lvl width (.5 Mv) ad 17,000 Mv) Ergy (-p) distac of (0.49fm) lvl width 1 Wak itractio ad bta dcay attractio, Rag M ma lif 10-5 Scs Rag M s ma lif tim 10-5 Sc. CMP-AB-46,0 497 NP-IK 59 1 Gravitatioal Yt to b likd Du to implosiv cavity POFPGD-PT Nutro Star with othr forcs /ctriptal forc from CMP-AB-, Black hol. isid th cor of th 86.9,499, 504 particl Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

6 6 of Elctro spi agular momtum dfiitio-g-fi structur costat With Smi Classical Approach Exprimts shows g-factor Nutrios Rquird to xplai bta dcay 15 Tul Rquird to xplai ffct Alpha particl ad dcay ad Casimir attractio btw ffct two plats i mpty spac g-factor (Basd o dcimal placs for physical costats) α 1 ( ).Nw agular momtum ratio dfiitio Nutro Bta dcay- Cosrvatio of rgy violatio-if th lctro siz is lss tha its classical radius. (Smi classical approach) Tul ffct was dd sic uclo siz ad th spacig btw thm is ot v kow. CERN (Appdix (1 of ) Appdix ( of ) Postd as 1) Alpha Particl Dcay- Is it rquird to Tul through th pottial barrir? Not cssary. 16 Elctro Siz Not Cocludd but lss tha (10-18 m) Cocludd ad sam as classical radius of lctro 1.0 STUCTURE OF SUBATOMIC PARTICLES A Lik btw (mass rgy) ad (fild rgy) A. From th atur of particls ad atiparticls, it is wll stablishd, that a atiparticl has th sam mass, spi ad liftim [If ustabl], but th charg although qual i Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

7 7 of 46 magitud has th opposit sig. Th aligmt or ati-aligmt btw its spi ad magtic momt ar also opposit to that of a particl. Cosidrig o such pair, th lctro ad a positio for th purpos of aalysis hr, sic thy hav mass togthr with charg, th (fild-rgy) associatd with a particl ca b compard from th kow (mass rgy) xprssio alog with th xprimtally vrifid rst mass-rgy rsult (0.511 MV) for a positro or a lctro. I ordr to valuat th (charg rgy), say for istac, if a positro is ar to a lctro, th two will com togthr udr th ifluc of thir opposit chargs ad i doig so, ad th particls acquir lctric pottial rgy. For th compariso btw th rst mass rgy ad th lctric pottial rgy gai th followig xprssio is cosidrd. q m 0C k d q m 0 C k (1.1) d Whr 1 K ad [d] is th distac btw th ctr s of lctro ad positro. 4πε 0 Though th abov quatios ar th sam mathmatically, th physical itrprtatio is as follows Th gativ sig hr i quatio (1.1) is ot mat as gativ mass sic this is a o -matrial modl ad by dividig by radius vctor) rprsts iward forc (ctriptal forc) i th cavity of a subatomic particls proposd hr.(that is Implosiv cavity ad a xplosiv lctric fild) Ad this modl is abl to tak us through all four particl itractios ad forms th basis for this proposd o-matrial shll modl. That is rgy rmais i th rgy form ad dos ot tak a matrial or a kot form for th Subatomic Particls ad thir proposd Sub shlls i this modl Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

8 8 of 46 B. Exprimtal obsrvatios ad fidigs Furthr, this procss has b obsrvd to tak plac i amorphous substacs ad it turd out to tak plac maily aftr th positro slows dow i th substac ad dos ot radily aihilat i most of th cass, but forms a boud systm with a xtraous lctro of a ati-paralll spi i th form of a parapositroium for a short tim of about scods ad thy d to com closr so as to mt th cosrvatio of rgy rquirmts (v if thy ar to b poit particls) two particls th thrads ito o aothr ad wh thir combid rgy is qual to (1.0 MV), thy aihilat by simultaously mittig two Gamma ray photos, ach with a rgy of (0.511 MV) ad wr dtctd i xprimts. Th two photos flw strictly i opposit dirctios from th targt irradiatd by positros. Th abov procss is i accordac with cosrvatio of rgy ad th rsultig momtum of th stoppd positro ad lctro is zro, as wll it mts charg cosrvatio [NPNR-AK-55] Thrfor, th (mass-rgy) of aihilatio of th two masss is th sum of thir (mass- rgy) of th pairs ad th (charg rgy) is that cotributd by th chargs o th pairs. From quatio (1.1), th total rgy of masss ad that of chargs ca b writt as blow. Whr, subscripts [p] is for positio ad [] for lctro. Sic th mass ad th charg for th two particls ar th sam umrically, quatio () ca b writt as m C kq d (1.) Whr, (m o m p m rst mass) ad [d] is th distac btw th particl ctrs This quatio is a rgy trasformatio quatio from pottial rgy to th kitic rgy form of two photos for both positiv lctromagtic rgy ad for th gativ rgy [gravitatioal fild rgy] is put forward i sctio [5.1] aftr gravitatioal attractio Pair productio rgy discrpacy: By isrtig th valus for th costats i quatio (1.) ad th kow total mass rgy of (1.0 MV), th distac btw th particl ctrs ds to b qual to (d Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

9 9 of x M) i ordr for th particls to gai a total pottial rgy quivalt to th total mass-rgy of (1.0 MV) as show hr Pottial rgy btw th pairs at distac d btw th particls ctrs Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: kq d [ x Jouls 1.04 MV Th abov [ctr to ctr] distac btw th particls is th sam as that of th classical radius of th lctro (Sic w ar dalig with a o matrial modl th classical matrial approach is ot big cosidrd ad th sphrical itrfac at this radius r is th radius at which a stat trasitio from lctromagtic to strog itractio forc is proposd to tak plac for a poit particl approach) ad furthr from Ruthrford s scattrig xprimts with alpha particls o light alumium ucli cofirm th validity of Coulomb s law just about this distac (d)] ad th xprimtal vidc for it is as blow from From xprimts for th cas of a alumium uclus of mass umbr [7], Coulomb s law was foud to brakdow i xprimts at about [6 to 8] fm, with th valu of ( R 0 1,4fm) with alpha particl rgy [NP-IK-64] Now, cosidrig a avrag distac of (7.0fm) from abov, th distac at which th Coulomb s law braks dow is qual to: ( 7 1.4x 7). 8 fm Which is i agrmt with th abov said thrshold distac as arrivd at abov. Th valu of R 0 will dpd o bidig rgy as will b dtaild i latr sctio-. Furthr, with th prst matrial cocpt, wh th positro ad th lctro is at a distac of (r ), th total rgy rquird for a pair productio will b qual to ( x rst rgy of lctro + bidig rgy btw th pairs) ( ) Mv 19 ] th

10 10 of 46 Whras, a pair productio rgy that is foud to b rquird from xprimts is (1.0 Mv) This discrpacy ariss, bcaus th two particls ar big tratd as partly matrial ad partly charg rgy mass. Furthr a photo has all its rgy i lctromagtic form whil i motio ad its rst mass is zro, thrfor it would b appropriat that a liarly movig photo wh mad to slow dow i th strog uclar fild appars to coil up to bcom two chargd /spiig particls formig lctro/positro pairs which also rflct thir rgy i th particl form as lctric ad magtic rgy Thrfor, mass must tirly b fild rgy mass for a spiig chargd particl i ordr to rsolv th abov discrpacy. Th [poit charg] particl cocpt would lad to ifiit lctric fild itsity ad its associatd rgis, whos partial ffcts ar laboratd i sctio [.4] udr th subtitl [A lik btw Coulomb s law ad strog itractio] ad also why possibly th xprimts idicat a smallr d-brogli wav lgths (that is, a poit- lik particl) is also icludd i sctio [.5], [.] Th aforsaid procss of rgy ad agular momtum covrsio with frmios of (+/-half spi) ad photo of (+/- 1 spi) may b rprstd Fig-1 It follows from quatio (1.), that th bidig rgy pr particl at th spcifid distac [r ] would also b qual to th rst rgy of o particl ad th distac btw th particls [d], i ordr to acquir th total aihilatio rgy is qual to [r ] kq That is m C (1.) d Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

11 11 of 46 C. Shll structur ad its dyamic stability: Thus for a pair aihilatio to occur, th distac btw th particls is dd to b qual to th radius of th particls thmslvs (that is [d] r ) ad hc th sphrical surfacs will hav to ovrlap as show i Fig. 1. I ordr satisfy this rquirmt, a spiig dyamically stabl sphrical Hol lik structur i say Athr (idirct vidc for Athr ar icludd i supplmtary to this papr o Rviw of Spcial Thory of Rlativity ) with a flxibl boudary may b cosidrd, bcaus such a lastic sphrical structur holdig a gativ rgy stat i th cor ad vlopd i a lctric fild rprsts both mass ad th charg o a particl ad at th sam tim its flxibility would prmit th cssary thrshold approach distac btw thir ctrs to abl a pair aihilatio. I additio to this, th vlopig lctric fild itsity aroud such a structur ovrcoms th problm of ifiit lctric fild itsity/rgy ad also abls cotiuity of fild lis. [POFPG-PT-7] 1.4. Dyamic stability of th shll structur: For this shll structur, sic th (mass-rgy) is i fact ow th (charg-rgy) ad ar qual i magitud for a particls as i quatio [1.], th dyamic stability at th particl itrfac ca th b aalyzd as blow By dividig quatio [1.4] by th radius of th particl [r] (say for a lctro) m C r kq r m C r 1 4πε That is ( 1.4) o q r Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

12 1 of 46 By dimsioal aalysis, sic 1 ML ε0 T Q th abov quatio (1.5) turs out as ML T ML T Thus th trm o th lft sid of th quatio (1.4) is a ctriptal forc dirctd towards th ctr of th shll structur ad that o th right is a outward forc du to th lctric fild itsity. Th ivolvmt of th vlocity factor C shows th dyamic spi stat of th structur. By substitutig umrical valus i quatio (1.4) th followig ar th obsrvatios. a] for r r, both th iward ad outward forcs ar balacd at th itrfac of th structur which is th stabl stat. b] For [r] > [ r ], m C > r kq r Which rsults is a iward forc ad th structur is rstord to its stabl stat of [rr ] m C < kq c) For [r] < [r], r r Rsultig i a outward forc that acts to rstor th structur to its stabl stat of [r r ] d) Th gativ rgy withi th shll is always qual to fild rgy outsid th shll i th form of lctric filds [E] ad magtic filds [B] Furthr sic th spi of a subatomic particl is proposd to b is always at th spd of a lctromagtic wav[c], th classical xprssio [ECxB] holds good ) Th sphrical shll (rgy-mass) ad its associatd charg at th itrfac is quivalt to a poit mass/ charg at its ctr Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

13 1 of 46 A. Siz of uclos.0 NUCLEON AND NUCLEAR PROPERTIES A Corrlatio btw Rst Ergy with Bidig Ergy pr Nuclo Sic th mass of th protos ad utros ar much havir tha th lctros, thy will b rflctd i thir corrspodig [mass rgis]. Thrfor, th rgy dsity withi a shll structur will rflct as mass-rgy to volum ratio. From th shll structur for a particl as i prvious sctio [1.4], th cor of th particl m C 0 is rprstd by from which it follows that, sic th vlocity C is a costat, r th mass of a particl is ivrsly proportioal to th radius of th structur. With th abov, th rgy dsity xprssio for a uclo ca b corrlatd with that of a lctro whos (mass rgy) togthr with its radius ar kow. Rst rgy of a uclo Rst rgy of a lctro Volum of a lctro Volum of a uclo r That is RE RE...(..1) r Th subscripts (- for a lctro), (-for a uclo) ad (RE for th rst rgy of th corrspodig particl) th xprssio (.1), ca b rarragd to obtai a rlatio for th radius of a uclo. RE r r...(.) RE Whr (r ) - is th radius of a uclo ad (r ) th classical radius of a lctro By drawig quivalc from th pair aihilatio for th itrfac ovrlappig as i Fig (1) ad th ots blow it, ad furthr by xtdig this to (Gaussia surfac) aroud a quivalt poit charg at th ctr of th Sphrical Shll Structur th followig ar th itrprtatio. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

14 14 of 46 Fig. (GS)- Gaussia Surfac, (S.S.I) Sphrical Shll itrfac of uclos I fig- APpBDr GS Whr (r GS ) Is always lss tha (r ) Th quivalt itrprtatio for uclo at th Gaussia radius from quatios (1.1), (.1), (.) ad figurs [1] ad [] would b Tabl of Equivalc-1 a Th radius of a lctro-positro-[r ] Th distac btw thir th ctrs [d] b Th rst rgy of lctro-[re] Bidig rgy pr lctro at [r d] c Th radius of a GS [r GS ] Th distac btw th uclo ctrs [D] Equivalc from [a] d Rst rgy withi th GS(REGS) Equivalc from [b] [BE/] at [D] Ad thrfor for th itrmdiat bidig rgis pr uclo ad th spacig btw th abov (c) ad (d) ca b xtdd by makig th followig chags to quatio (.1) ad (.) by rplacig (RE ) with (BE ) ad (r ) with (D). Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

15 15 of 46 I othr words, this is th xtsio of rgy dsity ratio as i sctio [.1], but btw th rgy dsity withi th Gaussia sphr i compariso with lctro rgy dsity Thrfor Bidig rgy/uclo at distac [D] btw ctrs [ / ] [ r BE D] xre (.) Th distac btw uclo ctrs [D] at th spcifid bidig rgy/uclo RE BE [ D ] r.....(.4 ) Th quatios (.) ad (.4) ar applicabl oly for valus of [D] [0.7 to.8] fm byod which th uclar forcs saturat o ithr sid B. Siz of a Nuclus Th siz of a uclus [R] ca b obtaid by multiplyig quatio [.4] by th cub root of th mass umbr of th rlatd uclus. R r A BE Th siz of th uclus [ ]......(.5) A workd out xampl for [R 0 ] hr will giv a dirct compariso with th mpirical formula [with typical Bidig rgy of 8 Mv/particl] i cotmporary physics [CMP AB- 88, 97] RE Th valu for (R O ) so obtaid is approximatly [1. fm] Now from quatio (.4), substitutig for th kow rst rgy of a lctro alog with th avrag bidig rgy/uclo (8 MV/) R O R 0 [1.165 fm].818fm Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

16 16 of 46 Th valu of is R 0 som what varid, dpdig o th masurmt tchiqu ad th valu ow arrivd at [ R fm] is wll i accord with xprimts ad furthr idividual bidig rgis ca b substitutd for ach lmt Thus, Equatio (.) ad (.4) is wly itroducd i plac of th prst Squar wll. [CMP-AB-406] Equatio (.4) - Is wly itroducd for spacig btw uclos. Equatio (.5) - Rplacs th prst mpirical formula C. Pottial barrir ad Spacig btw uclos: A pottial barrir ca b costructd from quatio [.5] for a [utro- proto] itractio, similar to th o availabl for a Dutrium for a compariso [CMP -AB- 97/98] Tabl 1 BE/ [R O ] Spacig Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

17 17 of 46 Figur Bidig Ergy/Nuclo Spac ig Bt, Nuc los Not: Th plottig of Figur- is oly idicativ ad is (ot to scal) with rspct to th ratio of (X/Y) axs ad th stpss of fall may v b sharpr i actual scal Nots o th Tabl- 1 a] Th distac btw [-p] ctrs for a dutrium is [.18fm] b] Th spa for th spacig btw [-p] for a bidig rgy rag of (0.511 to 5) MV is ( ) fm (.1fm) which agrs wll with that calculatd valu basd o a Squar wll from wav mchaics (.1 fm for 5 MV dpth) c] Bcaus of th cotiuity of quatio (.5) with roudd corrs, th spacig ad rag for a strog itractio ca ow b wll dfid to dmarcat from wak itractios.(not that thr is d to assum roudd corr i currt thoris ad hr w gt this as a atural outcom) [CMP-AB-405/406] d) Bidig rgy will howvr dpd o othr factors such as (umbr of uclos to umbr of proto i a uclus), thir pairig ad quadrupol momt. Howvr sic th ma bod rgy is about 8Mv, th kitic rgy of motio of uclos i th ucli is about 5Mv. (NPNR-AK-95,100) (CMP-AB-406,407) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

18 18 of 46 f] Coulomb s law would b dirctly applicabl for distac btw uclo ctrs qual to or gratr tha (.8 fm] D. Coulomb s law ad Strog itractio [uclar forc] [Which follows from sctio [.1] that th magitud of th mass rgy closd withi a Gaussia sphr is qual to th charg rgy outsid th Gaussia Sphr] It follows dirctly from th proposd shll structur ad alog with th applicatio of Gaussia surfac aroud th charg ctr of th sphrical shll as show i Fig []; th followig would b applicabl outsid th Gaussia Surfac. a] th lctric fild itsity at th Gaussia surfac will b ivrsly proportioal to its surfac ara ad its pottial ivrsly proportioal to th radius of th surfac. Not: It implis that th [charg] o th shll is a ivariat ad has th magitud of a lctro charg. Equatio [.] is copid hr for asy rfrc Bidig rgy pr uclo BE r D RE BE r D r kq D r...(.6) Whr [r >D>0.7] fm r Hr th first trm D is th cotributio to th bidig rgy du to icras i th lctric fild itsity at D. Th scod trm r D is th cotributio du to th icrasd pottial at D. Kq Th third trm r Mv is th limit for th Coulomb s law as mtiod i sctio [1] Th abov factors modify Coulomb s law ad it rflcts as strog itractio btw uclos for (r >D>0.7) fm. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

19 19 of 46 This is o of th rasos why a poit charg cocpt for th particls was dd to th kpt asid i sctio [1.]. E. Costituts isid uclos [Quarks] Ulik lctros, a proto or a utro has costituts [Substructurs] [SS]. Thrfor, thir ovrall siz will dpd upo th umbr of costituts [Substructurs] ad corrspodigly th rgy cotaid withi ach substructur. Howvr th sum of th idividual rgy cott withi th substructurs isid a uclo must b qual to th rst rgy of th uclo Th charg o vry shll will always b qual to lctro charg ad positiv or gativ will b rflctd i thir dirctio of spi rotatio Th radius of a shll substructur was show to b rlatd to its rst rgy through quatio (.) is copid hr for quick rfrc. RE r RE r Whr (r, r ) is th radius of a uclo or a lctro ad (RE,) - Rst rgy of uclo or a lctro I ordr to mak a choic o th umbr of substructur [costituts] ad thir rgy cott, th followig factors ar cosidrd. a) That (o two) costituts (Shlls) hav th sam rgy stat i accordac with xclusio pricipl. b) Sic th radius is ivrsly proportioal to th rgy cott i th substructur, th choic of this rgy has b mad, such that it satisfis th obsrvd xprimtal facts lik rsoac particls tc. c) With th abov cosidratios th sub shll structur cofiguratio for a last rgy stat would b Coctric Substructurs / Sub shll Modl which ar also dyamically stabl from [Sc-1.4] [aalogous to coctric sphrical capacitors] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

20 0 of 46 From th abov formula for (r ) th radius of ach sub shll ca b foud by rplacig RE by th proposd rgy cott withi th sub shll. Furthr ths valus hav b chos so that th rsults obtaid from this would b dd to vrify th rsoac particl rgis [ Eta ad ω - msos] also. F. Radius of Sub shlls (itgral charg) withi, th Nuclos [Quarks- fractioal charg)] Proto A proto cosistig of thr coctric sub shlls (SS) of rgy, [4 MV], [155. MV] ad [549 MV] ad ar chos, so that thir sum is qual to th rst rgy of a proto [98. MV] Th radius of th [SS] cotaiig ru fm [4 Mv] ru fm Similarly for th (SS) with [155. MV] Ad for th [SS] with [549 MV] ru fm rd fm Whr ru 1, ad ru ar similar i trmiology as adoptd for up quark which forms th outrmost ad irmost shlls. rd1 is similarly a dow quark which is th irmost sphrical shll [549 MV]. Th combiatio of [SS] of [549MV] with th [SS] of proto of [4 MV] yilds th valu of [78 MV] th othr rsoac particl [ω mso] Nutro: For a utro, it is proposd with two coctric [SS] of rgy cott [71] MV] ad a [669 MV], th sum of which is qual to th rst rgy of a utro [940 MV]. Th radius of [SS] with [71 MV] rd fm Th radius of [SS] with [669 MV] ru fm ( It may otd that this sub shll would split ito two rgy lvls udr th ifluc of Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

21 1 of 46 magtic fild of a ighborig proto as will b put forward latr) [CMP AB- 0,9] Th [ctr to ctr] distac btw th proto ad th utro, wh th abov itrfacs ar just i cotact with o aothr, is qual to (0.76 fm). Howvr th closst distac at which a abrupt chag from attractiv uclo forc to rpulsiv should b of ordr of a uclo siz as th particls hav flxibl itrfac ad would dform to som dgr as s i fig-1 ad th xprimtal vrificatio idicats about [0.5 fm]. [AK 96, AP 17] Th split cll will hav radial sparatio of (1.18x10-18 ) ad a rgy lvl width of (.5 Mv) for a (-p) distac of 0.49fm. This radial sparatio abls a virtual rgy of about (17,000 Mv) Th othr fiv radial sparatios btw sub shlls rag from (10-15 to ) m givig ffct to othr valus of Quark itractio forcs ad rgy lvl widths G. Nuclo magtic momt From classical physics a spiig charg givs ris to a magtic momt, ad th gyro magtic twic that of orbital which is xprssd as blow [CMP-AB-0] Spi magtic momt of a chargd particl is q ± µ s ± S m Whr [±q] rfrs to a positiv or a gativ charg whos magitud is qual to that of th lctro charg, [m] th mass of th particl ad S is th spi agular momtum vctor [CMP AB-0,91] [AP-JBR- 1191] A shll or a [sub- shll] ar frmios of half-spi ad th charg o thm is always qual i magitud to that of a lctro chargs [q 1.60 x C] ad oly th charg dsity ad pottial that will b diffrt for th idividual shlls dpdig o its radius as show i sctio [.4]. Th momt of Irtia for a sphrical shll, of rgy mass about a axis passig through its ctr is. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

22 of 46 I mr Whr m ad r ar th lctric fild rgy-mass ad radius of th shll ad sic its C quatorial vlocity of spi of th shll is C th agular vlocity. r Quatizd Spi agular momtum alog-z-axis [S Z ] mr c r 1 mcr Substitutig for S i th quatio for th spi magtic momt ±µ SZ ± 1 qcr......(.7) Proto Magtic momt: From prvious sctio a proto was cosidrd to b built up of thr sphrical shll substructurs. Whos workd out radii wr [ru fm], [ru fm] ad [rd fm] [Whr, u or d ar up or dow stats i accordac with quark covtio]. By assumig that th irmost [549 Mv] chargd substratum has a opposit spi with rspct to th othr two associatd sub shlls its magtic momt will b [-v], th ffct of which is tak ito cosidratio i its corrspodig radius as rd 1 [-0.75fm]. Ad th charg [q] is th sam for all th sub shlls, which, for thr [SS] will b [+q]. Thrfor th rsultat magtic 1 Momt for a proto alog Z-axis ( µ P ) qc ( r ) Z u1 + ru + rd µ PZ qc( ) fm 14.1x10 J / T By xprimt th valu obtaid for proto magtic momts is qual to.79 x x 10-7 J/T 14.1 x 10-7 J/T [CMP AB-91] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

23 of 46 Atiproto [Th chag of th stats of th abov substructur to th opposit atur [that is by chagig th sig] of a proto lads to a atiproto cofiguratio]. Nutro Magtic Momt Th followig factors obsrvd i th xprimts ar cosidrd i ordr to arriv at th [spi dirctio] of th two costituts i th utro. From th proprtis of a utro, it follows that a] A fr utro is a ustabl particl which has a ma liftim of [889scs] ad dcays by mittig a proto, lctro ad a atiutrio [CMP-AB- 45/47] b] Wh a utro is i a boud stat with a proto [for istac i a dutrium], th ma lif tim of utro is xtdd idfiitly du to xchag of rgy btw thm [CMP-AB-85,410] c] Also from th boud stat of [proto utro] thy hav a strog magtic couplig bcaus of thir clos distacs i a uclus shll modl [CMP ] d] Although th ovrall utro charg is zro, th costitut shlls ar quivalt to two oppositly spiig chargd sphr, ad its magtic momt is gativ dpdig o th rsultig gativ charg [CMP-AB-91] [AP-JBR-1191] ) I th absc of a magtic fild, a fr uclo ca hav thir spi i ay arbitrary dirctio but its compots i ay chos rfrc i a uiform magtic fild will b quatizd ad maigful [CMP-AB-09] Thus i ordr to mak a masurmt of th magtic momt of a fr utro a xtral fild would b rquird, whras i a boud stat th utro has a rfrc magtic fild from, that gratd by th ighborig proto. From prvious sctio [.6], th radius for th substructurs was calculatd to b For [71 MV] shll has as radius rd [ fm] For [.75 MV] shll has th of radius about rd 1 [-0.5 fm] Ad for th othr [6.5 Mv ] shll has th radius of about ru 1 [+4fm] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

24 4 of 46 Th [669 Mv] shll of th fr utro splits du to th strog magtic fild from th ighborig proto i th uclos Wh a fr utro is ot udr th ifluc of a magtic fild, th ir shll is assumd to b spiig i th opposit dirctio of th gativ outr shll (-q), so that th rsultat of th two proposd sub shlls, th t charg bcoms zro. Howvr, wh a utro is subjctd to a strog magtic fild du to magtic couplig with a ighborig proto, th ir shll splits ito spi up (+q) ad spi dow (-q) ad its magtic dipol gts aligd with rspct to its ighborig proto, thus givig ffct to a t gativ charg/magtic momt, which is rflctd as a gativ sig o th radius as itrprtd for th proto prviously. Hc o mso xchag is dd. [CMP- 9, 48] [P-R&H-9] Nutro magtic momt 1 µ Z qc( ru 1 + ( rd 1 + rd ) fm (Not that r d1 ad r d arly cacl out) Nutro Magtic momt alog Z-axis 1 7 qc ( 0.484) fm ( 9.66x10 ) J / T By xprimtd fidigs [-1.91 x x 10-7 ] [-9.66 x 10-7 J/T] Atiutro Th chag of th stats of th substructurs to th opposit atur [that is, by chagig th dirctio of spis of shlls] of a utro lads to a atiutro cofiguratio..0 WEAK INTERACTIONS AND (WIMPS) A. With all th dtails giv for [Nuclar Elctros] i txt book [CMP-AB-88,45,497] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

25 5 of 46 Th abov phomo of th [wak itractio], ca ow b aalyzd with th hlp of a [Shll structur] for th particl Rfrrig first ow to th Bta dcay, th avrag kitic rgy of a lctro is about [0. MV] ad sic a lctro i a particl form caot prxist withi a uclus, th Bta dcay rgy of [0. MV] may b vrifid from th outr priphry of th uclus Th abov phomo of th wak itractio ca ow b aalyzd with th shll structur of th particls. Th siz of outr shll of a utro shll ad a proto shll wr calculatd ad foud to b qual to [0.484 fm] ad [ fm] rspctivly, ad that of a lctro is (.818 fm). [Sctio-.6] Th [utro lctro] pottial rgy ca b calculatd from thir ctr-to-ctr distac, wh thir itrfacs ar just i cotact. Thrfor [D] [-] [ ] fm.17fm [D] [p ] [ ] fm.4 fm. From arlir sctio, th uclo itractio saturats at a distac of [.818 fm] ad hc th Coulombs law is dirctly applicabl for ay distac gratr tha this, thrfor th pottial rgy accordigly will b Btw asct [proto lctro] 9 9x10 x1.60 x x Mv This diffrc i mass rgy btw a utro ad a proto0.78mv of which th bidig rgy ad magtic couplig btw th proto ad th lctro ar to b ovrcom ad th rst is carrid of as kitic rgy of lctro ad th proposd structur prmits a cotiuous spctrum. Th spi agular momtum cosrvatio is dtaild i Appdix- ( of ) i ordr to aalyz a d for a atiutrio. It may otd that if lctros ar to b poit particls (<10-18 m) accordig to currt thoris th th stimatd bidig rgy btw th lctro ad th proto will hav to b gratr tha (155Mv) ad bta dcay caot occur. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

26 6 of 46 Th diffrc btw ay two substructurs withi th uclos ad that btw th outrmost structur of th utro ad th proto ar mostly i th rag of [10-17 to ] mtrs, i accordac with th charactristic rag of th Wak Itractio" i th figur blow. Th ir sub shll of (669 Mv) of utro with two shlls would split i th clos proximity of Proto B. Wak itractig massiv particls [Wimps] Th charactristics of th itrmdiat vctor bosos hav a Rag M Ad rgy >80 tims th proto rst rgy for [Wimp s] [CMP-497] This ca b dirctly applid to th Shll structur from quatio [.] for th radius of a uclo. r RE.818fm For a W [+/-], 0 Z - th rgy is 80 tims th proto rst rgy or gratr. Thrfor RE [80 x 98 MV] 75,040 M V Substitutig, i th abov quatio for r 17 r w mtrs Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

27 7 of 46 Th phomo is basd o th ivrs proportioality btw th rgy ad th volum as drivd i sctio [] Such a phomo is xpctd for all th othr virtual stats ad thy should also shrik i siz, which is why, wh particl siz dducd from high rgy [lctrolctro] scattrig xprimts quit possibly idicat as if thy ar poit charg Howvr, ths stats big o th dcay mod, th particl siz will bouc back to its stabl siz as i sctio [1.4] 4.0 UNIVERSAL LAW OF GRAVITATION A. Th forc of attractio btw two masss i accordac with Nwto s Law is, F Gm1m D F G C m C D m C D 1 4 (4.1) Th itrprtatio of this is as blow, Th first costat trm is ot a mr scalar costat but has th dimsios of ivrs of forc-g forc Th scod ad th third trms ar th ctriptal forc from th cor of th gativ rgy stat isid th corrspodig subatomic particls. Thrfor th ractio forc btw particls is idpdt of spi dirctio of th cor of th particls ad will always b attractiv, ad furthr this xplais th ivrs squar law of forcs. It may b rcalld that th Spac Tim Curvatur was a suitabl optio as bcaus Sir: Isaac Nwto s law of gravitatio had o immdiat xplaatio for Actio at a distac. [P-R&H-Vol-1-88] [POFPG-PT] Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

28 8 of 46 Sic th lctric ad magtic ffcts ar ullifid at th atomic lvl itslf i most of th objcts, th oly domiat forc that prvails is that of gravitatio. W kow th complxity for this applicatio to mor tha two objcts; though th itractio of th rst of th Uivrs will b rflctd i th local ffcts of th Earth s gravitatio B. Nutro Star ad possibly Black Hols: Fig [4] I th cas of a utro star whos atoms hav b so comprssd that, most of thir protos ad lctros hav fusd ito utro, for which this shll modl appars to b mor appropriat. Th W[±] ad Z virtual particls ivolvd i th wak itractio, shows o sig of saturatio of th lctric fild aroud th shll structur, bcaus th particl boucs back to its origial stabl siz,du to th dyamic stability of th shll structur as s i sctio. Howvr, at a much dpr lvl th lctric fild may radiat away [Hawkig Radiatio] ad a imbalac may st i with th rsult that a iward pull will th domiat accordig th proposd shll structur. [CMP-4, 86,1,9,496,504] Elctro Spi Magtic Momt Aomaly (g, 17) ad a Agular Momtum Dfiitio of Fi Structur Costat, Smi-Classical Approach) Author: V. Shakar Narayaa Shakar V. Narayaa PACS: 1.0.Jp, 1.0.Js, 1.15xg, 0.0 +p. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

29 9 of 46 ABSTRACT: ABSTRACT: This is a attmpt to rsolv th dcad s log lctro magtic momt aomaly from smi classical approach by aalyzig its ffct at th Bohr radius from first pricipls with classical lctro radius. g- Factor ad α 1 ( ) By xprimt ( ) Cocpts of Modr Physics-Fifth Editio-Arthur Bisr-Mc-Graw-Hill,Ic (CMP-) rfrs to pag umbr () of th Book. Ky Words: 1) Elctro lctric dipol momt ) Smi-classical mthod. ) Corrctios to a boud lctro ( g factor). 4). Elmtary Particls INTRODUCTION: A lctro is ot a poit particl but has a radius qual to classical radius of lctro Th total orbital magtic momt coupld with th spi magtic momt at th Bohr orbit ca b xprssd i trms of charg, vlocitis, radii ad th multiplyig factors for thir rspctiv momt of irtia as proposd blow. (CMP-10,,8,9,0) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

30 0 of 46 µ B Bohr Orb Smi. classical ( m VBa0 µ B Bohr Orb Classical (1) 9.74x10 h µ B ( Quatum Orbital) ml ( ) (1A) 9.74x10 m π µ µ S Z S T ( lctro. Spi. Classical Z Axis) ( lctro. Spi. Classical Total) µ By. classical. approach. lt. factor. for µ µ ST Cr ( ) (4) SZ ST h ) π µ SZ ( 1 ( m ( m ) Iω 4 1 ( )( m a V ) x( a J / T ( CMP ) 4 0 J / T ( CMP ) VBa ) Cr 6 ) x mcr () 7.814x10 J / T ) x mcr Cr () 1.54x10 m m 6 J / T 1. so. that. symmtrical. agl. for. Cosθ 45.dg rs. B 0 0 µ V B 6 ( Orbital. Vlocity. at. Bohr. radius).188x10 m / s ( CMP 15) 11 a 0( Bohr. radius) 5.9x10 m ( CMP 11) Spi ( Quatum Spi) m spi ( m h ) ± π h ) 9.74x10 π Not : That gyromagtic ratio. of. spi. is. twic as. that. of. orbital. quatio(1 A) which.. is. a approximatio that. latr. lad. to. aomaly ( CMP 8,46) h X10 J S π 8 lctro spi Vlocity about. its. ow. axis.( C).998x10 m / s m mass of lctro 9.11x x10 19 ( Coulomb) 1 1 ( kg m 4 J / T (A) ( CMP 0) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

31 1 of 46 Spi Orbit. Coupld. µ Th. sam. is.xp rssd. as. blow Comparig. Equatios(1) & (4).. µ B BST µ ST ( µ B + ) µ µ ST g. factor g µ BST B ( µ Cr ) 9.841x10 V a J / T Clos. to.xp rimtd. valu. of ( ) Howvr. at. Cosθ 47.7.dg rs. th. rsult. would. b. xactly. as xp rimtd. valu. up. to. all. dcimals. show. abov. I. accordac. with. currt. thory. Cosθ dg rs Cosθ Th. agl. btw. total. agular. momtum. to. its. compot.. o Z axis B + B 0 4 VBa0 Th valu for ( ) Cr turs out to b α 1 ( ) Coclusio for Appdix (1 of ): Th sigificac of th fi structur costat (Plas brows th t for itrstig dtails o this) is wll kow to may disciplis of scic ad hr w gt a clar w dfiitio with th abov total magtic momt ratio, i othr words, wh rprstd i trms of total agular momtum by rplacig with m. This i additio mphasizs that lctros ar ot poit particls ad idd hav classical radius of lctro. I ordr to apprciat othr fudamtal aspcts plas also fid a figur at th d of this work ad th w fidigs through othr postd works of this author alog with this, with a classical approach. It is also importat to ot hr that v though Quatum thortical calculatios with a arly poit siz lctro approach may agr up to svral dcimal placs with xprimts is otworthy that a classical approach provids clarity ad visibility ad furthr th sam poit particl approach has causd substatial hidracs o othr aspcts too such as itractios lik Nuclar pottial barrir ad its magtic momts, Alpha dcay, utro bta dcay, ad abov all th currt cocpts thmslvs ar dd to challgd. (How a poit lik lctro ca rsult i such accurat agrmt with th xprimt is lft to radrs ow judgmt) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

32 of 46 Th followig has b tak from ducatioal wbsits. It is ot possibl to giv a qualitativ dscriptio of th ffcts which giv ris to th g-factor aomaly of th lctro. Th dtaild thortical calculatio of th quatity is i th domai of quatum lctrodyamics, ad ivolvs th itractio of th zro-poit oscillatio of th lctromagtic fild with th lctro. Compariso of thortical dtrmiatio of a with its xprimtal masurmt costituts th most accurat ad dirct xistig tst of th thory of quatum lctrodyamics. I th sam mar as abov th followig ot shows th cosquc of a poit particl cocpt. Wh th ida of lctro spi was first itroducd i 195, v Wolfgag Pauli had troubl accptig Ralph Kroig's modl. Th problm was ot that a rotatig chargd particl would hav giv ris to a magtic fild, but that th lctro was so small that th quatorial spd of th lctro would hav to b gratr tha th spd of light for th magtic momt to b of th obsrvd strgth. Furthr th postd works of this author o Casimir Effct ad No bta dcay possibl with a poit lctro i fr utro dcay falsifis th cocpt of Zro Poit Oscillatios ad Nutrios. Th aomaly i g-factor of lctro magtic momt as w kow ow was ursolvd bcaus th Plak s agular momtum was hld a costat whil allowig violatio of C is th caus which is far highr i cas of poit particls (a fals otio). This sam aalysis is furthr put forward for utrios i th followig appdix. Som high rgy xprimts it sms appar to idicat that thr is possibly a chag to th Fi Structur Costat du to th chag of lctro charg could v b du to chag i mass ad cosqutly o charg mass ratio. Howvr v so, part ( of ) postd o this sam wbsit dscribs th atur of charg ad ca accommodat such a chag to lctro charg. (It may b otd that thr is o clar itrisic dfiitio for a charg so far ad its possibl atur is icludd with Athr proprtis i Spcial thory of Rlativity as (part-) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

33 of 46 (A figur showig th furthr w fidigs o 17 factor ca b foud at th d). r RE RE...(..1) r RE r r...(.) RE From Cor Ctr 1) First itrfac of Cor of Proto (0.75fm) It appars as though a positro is shildd by a atiproto is a utro of (0.484fm) ) Scod Itrfac of Proto (0.605fm) ) Outrmost Itrfac of Proto (0.4194fm) 4) Elctro Itrfac (.818fm) 5) Plack s (h/pi) -d- Brogli-Compto wavlgth (.86x10-1 m) (h/pixm C) 6) Eisti- Radius (5.9x10-1 m) (Commt-4 - blow) 7) Plack s-bohr Orbit (5.9x10-11 m) Agular momtum/radius ad (17 factors) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

34 4 of 46 1) Th ratio of agular momtum (w) btw (7) ad (4) 17 ) Th ratio radius btw (7) ad (4) 17 ) Plack s d Brogli- Compto wavlgth rlatio (5) x17 (7) 4) Eisti- radius at which spis vlocity is C ad at which agular momtum will b 05.5 (1.5x17) tims lss tha half spi. 5) Itrstigly v th ratio btw th agular momtum of utro to proto quatios (6)/(7) o pag () (1.7/) xm 6) Coditio for stabl atomic orbits (xh/pi) (1.058x 10-4 ) ( ) π. x10x17 7) Multiplyig (6) by (pi) as w kow is Plack s costat h 6.649x10-4 Som of abov may alrady xist ad a thig to otic with this umbr is its coicidc with svral stabl stats that may ivolv a rsoac phomo. Rfrcs: 1) Cocpts of Modr Physics-Fifth Editio-Arthur Bisr-Mc-Graw-Hill,Ic ) Msur d précisio du magétism d l'élctro URL: 000: Th Amrica Physical Socity No Nutro Bta dcay (If lctros ar lss tha its classical radius) (Smi classical approach) Corrspodig Author: V. Shakar Narayaa Abstract: Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

35 5 of 46 This scop of this cocis work is a attmpt to show that bta dcay of a utro is ot possibl if lctros ar to b lss tha its classical radius ad furthr to show that by holdig Plack s spi agular momtum a costat as i currt thoris lads to mor discrpacis o magtic momts of subatomic particls. PACS Numbr: g, St, 14.0Dh,.40Bw Ky Words:1) Elmtary particls ) Wak Itractios ad lptos ) Nutrios 4) Bta Dcay Aalysis: Is basd o 1) Violatio of C is ot accptd as it will challg mass rgy quivalc. Th followig work shows th xtt to which C is violatd by maitaiig (h/pi) a costat ad th dgr of dpartur for magtic momts from a Classical approach. )This is basd o a o matrial shll modl for subatomic particls whos spi momt of irtia is (/)mr ( whr m is lctromagtic rgy mass)ad that th orbital vlocity of lctros ad uclos ar far lss tha C ad thrfor rlativistic ffcts for mass icras ar isigificat. Furthr this particl modl also provs that durig high-rgy scattrig xprimts th sub atomic particls would momtarily shrik posig as though thy ar poit particls (particularly lctro). Aalysis: 1) If lctros ar to b tratd as poit particls i accordac with currt thoris,, th bta dcay is impossibl? O cosrvatio of rgy frot, sic lctros ar clos to poit particls (<10^ -18m) accordig to currt thoris th bidig rgy btw a asct proto ad a lctro durig a fr utro dcay th distac btw thm ar about (0.51) fm ad at this distac th bidig rgy btw thm should b gratr tha (9 Mv). Hc how a fr utro ca dcay at all if lctros wr to b poit lik particls? Howvr at th proposd classical radius for lctros th followig ar th outcom. Rst Ergy (utro) - (proto + lctro) 0.78Mv with which th asct lctro ds to ovrcom th lctric bidig rgy of th Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

36 6 of 46 asct proto of about a distac with classical radius for lctro is ( ) fm with Coulombs law is about (0.445 Mv) ad th rst is carrid off as lctro kitic rgy which is i agrmt with xprimts. ) Aalysis o Agular momtum of utrio: Dfiitio of Plack s agular momtum (h/pi) mvr Whr (V B - Orbital vlocity of th particl ad Vs- quatorial vlocity of spi of a particl a costat) ( C.998x10^8m/s), (radius of th particl udr cosidratio markd with subscript -for lctro,-p-for proto..) Th umrical valu of h x10-4 J-S π 1) At Bohr radius Quatum ad Classical agular momtum ar th sam. By rplacig charg with lctro mass w gt th ratio agular momtum. Sic, th magtic momts ar xprimtally vrifid ad furthr thm big dirctly proportioal to agular momtum th aalysis is proposd to bgi by comparig magtic momts. V B VBa0 4 µ B Bohr Classical (1) 9.74x10 J / T ( CMP ) h 4 µ B ( Quatum Orbital) ml ( ) (1A) 9.74x10 J / T ( CMP ) m π 6 ( Orbital. Vlocity. at. Bohr. radius).188x10 m / s ( CMP 15) a ( Bohr. radius) 5.9x10 m ( CMP ) h 1 1 VB mvba Iω ( m a0 ) x( ) 4π a At classical radius of lctro (r ) 0 0 µ Sz ( Spi. Classical. Total) ( m ) x mcr Cr (1B ) 7.814x10 6 J / T Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

37 7 of 46 ( Agular Momtum). h π Iω m r C x( ) r 1 mcr By rplacig charg with mass of lctro i quatios (1) ad (1B) abov hbar mvba0 Th valu for ( ) h m Cr spi turs out to b α 1 ( ) Thus it r-mphasizs th sigificac of lctro classical radius. ) Elctro (g-factor aomaly) th first idicator of dviatio of Quatum with Classical agular momtum for boud lctros i a atom. From its rlatio for lctro spi h π Iω ( mr V ) x( r spi mv ) V Thrfor quatorial spi vlocity C spi spi r () h 4π. m r C () µ B By comparig quatios (1A) with (1B) ( ) (4) µ Thus by maitaiig (h/pi) a costat th xtt of violatio of C is carrid ovr to th magtic momts which xplais th aomalous-g-factor- Zma ffct. sz If th lctro wr to b a poit particl th violatio of C far xcds byod ay justificatio. ) For uclos Quatum ad Classical agular momtum. Th costacy of spi vlocity C is violatd v for hadros which hav a structur of radius (0.5 fm) as show blow for Baryos, of siz approximatly (1 fm across) Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

38 8 of 46 (V/C) 0.6 (CMP-AB-481) May virtual particls hav diffrt masss ad sizs which agai will hav to rflct o th spi vlocity. Now by maitaiig th costacy of th spi vlocity of light C th variatio of agular momtum is as follows for lctro ad uclos. Plack' s. agular. momtum." h" Th. rsultig. agular. momtum. of.(5,6 & 7) x10 r ( r h ( Spi Classical agular momtum lctro) h ( Spi Classical agular momrtum Pr oto) h ( Spi Classical agular momtum utro).818 fm ( lctro classical radius) p p 0.51fm),( r mcr 1 ( mcr ) 4.44x10 1 ( m 1 ( m J S which.. is. lss. tha. half. spi 0.48 fm) ar clos to 0.5 fm xprimts ( CMP 481) 4 p 7 Cr ) x10 p 4 Cr ) x10 J S (5) J S (6) 4 J S (7) µ. µ pz z m m p x m x m p Cr Cr 14.1x x10 Th rsults of (8 & 9) cofirms th validity of quatios (6 & 7) Half Plack Spi is about 0.5x10 p 7 7 J / T (8) sam as J / T (9) sam as foud i xp rmt 4 J S foud i xp rimt By comparig from abov valus for uclos agular momtum with that of lctro is lss by a factor of (8) folds for proto, (7) for utro ad (119) folds with rspct to half Plack s spi ad thus its ffct durig bta dcay is ot flt ad thrfor th cosrvatio of agular momtum (h bar/) that is big tratd a costat uiformly for all particls i currt thoris bcoms qustioabl. But th qustio is what th valu is for half spi (spior) is? Ad furthr this mchaical uit is ot a masurabl quatity. Subatomic Particls ad Four Itractios (A omatrial shll modl (Part -1 of STR-GTR-Athr-(Part of ) ad) CopyrightDposit.com,umbr: 00047

1 of 42. Abbreviated title: [SAP-SVT-Nmsm-g & 137] - Updated on 31 July, 09. Shankar V.Narayanan

1 of 42. Abbreviated title: [SAP-SVT-Nmsm-g & 137]  - Updated on 31 July, 09. Shankar V.Narayanan 1 of 4 ONE EQUATION ad FOUR Subatomic Particls ad thir FOUR Itractios icludig (g &17) factors with Spac Vortx Thory (A No matrial shll modl) (Part 1 of ) (Th cotts of this txt ar th sam as i Subatomic

More information

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted?

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted? All bodis at a tmpratur T mit ad absorb thrmal lctromagtic radiatio Blackbody radiatio I thrmal quilibrium, th powr mittd quals th powr absorbd How is blackbody radiatio absorbd ad mittd? 1 2 A blackbody

More information

They must have different numbers of electrons orbiting their nuclei. They must have the same number of neutrons in their nuclei.

They must have different numbers of electrons orbiting their nuclei. They must have the same number of neutrons in their nuclei. 37 1 How may utros ar i a uclus of th uclid l? 20 37 54 2 crtai lmt has svral isotops. Which statmt about ths isotops is corrct? Thy must hav diffrt umbrs of lctros orbitig thir ucli. Thy must hav th sam

More information

z 1+ 3 z = Π n =1 z f() z = n e - z = ( 1-z) e z e n z z 1- n = ( 1-z/2) 1+ 2n z e 2n e n -1 ( 1-z )/2 e 2n-1 1-2n -1 1 () z

z 1+ 3 z = Π n =1 z f() z = n e - z = ( 1-z) e z e n z z 1- n = ( 1-z/2) 1+ 2n z e 2n e n -1 ( 1-z )/2 e 2n-1 1-2n -1 1 () z Sris Expasio of Rciprocal of Gamma Fuctio. Fuctios with Itgrs as Roots Fuctio f with gativ itgrs as roots ca b dscribd as follows. f() Howvr, this ifiit product divrgs. That is, such a fuctio caot xist

More information

coulombs or esu charge. It s mass is about 1/1837 times the mass of hydrogen atom. Thus mass of electron is

coulombs or esu charge. It s mass is about 1/1837 times the mass of hydrogen atom. Thus mass of electron is 1 ATOMIC STRUCTURE Fudamtal Particls: Mai Fudamtal Particl : (a) Elctro: It is a fudamtal particl of a atom which carris a uit gativ charg. It was discovrd by J.J. Thomso (1897) from th studis carrid out

More information

Session : Plasmas in Equilibrium

Session : Plasmas in Equilibrium Sssio : Plasmas i Equilibrium Ioizatio ad Coductio i a High-prssur Plasma A ormal gas at T < 3000 K is a good lctrical isulator, bcaus thr ar almost o fr lctros i it. For prssurs > 0.1 atm, collisio amog

More information

5.1 The Nuclear Atom

5.1 The Nuclear Atom Sav My Exams! Th Hom of Rvisio For mor awsom GSE ad lvl rsourcs, visit us at www.savmyxams.co.uk/ 5.1 Th Nuclar tom Qustio Papr Lvl IGSE Subjct Physics (0625) Exam oard Topic Sub Topic ooklt ambridg Itratioal

More information

Physics 2D Lecture Slides Lecture 14: Feb 3 rd 2004

Physics 2D Lecture Slides Lecture 14: Feb 3 rd 2004 Bria Wcht, th TA is back! Pl. giv all rgrad rqusts to him Quiz 4 is This Friday Physics D Lctur Slids Lctur 14: Fb 3 rd 004 Vivk Sharma UCSD Physics Whr ar th lctros isid th atom? Early Thought: Plum puddig

More information

1985 AP Calculus BC: Section I

1985 AP Calculus BC: Section I 985 AP Calculus BC: Sctio I 9 Miuts No Calculator Nots: () I this amiatio, l dots th atural logarithm of (that is, logarithm to th bas ). () Ulss othrwis spcifid, th domai of a fuctio f is assumd to b

More information

8(4 m0) ( θ ) ( ) Solutions for HW 8. Chapter 25. Conceptual Questions

8(4 m0) ( θ ) ( ) Solutions for HW 8. Chapter 25. Conceptual Questions Solutios for HW 8 Captr 5 Cocptual Qustios 5.. θ dcrass. As t crystal is coprssd, t spacig d btw t plas of atos dcrass. For t first ordr diffractio =. T Bragg coditio is = d so as d dcrass, ust icras for

More information

How many neutrino species?

How many neutrino species? ow may utrio scis? Two mthods for dtrmii it lium abudac i uivrs At a collidr umbr of utrio scis Exasio of th uivrs is ovrd by th Fridma quatio R R 8G tot Kc R Whr: :ubblcostat G :Gravitatioal costat 6.

More information

MILLIKAN OIL DROP EXPERIMENT

MILLIKAN OIL DROP EXPERIMENT 11 Oct 18 Millika.1 MILLIKAN OIL DROP EXPERIMENT This xprimt is dsigd to show th quatizatio of lctric charg ad allow dtrmiatio of th lmtary charg,. As i Millika s origial xprimt, oil drops ar sprayd ito

More information

A Simple Proof that e is Irrational

A Simple Proof that e is Irrational Two of th most bautiful ad sigificat umbrs i mathmatics ar π ad. π (approximatly qual to 3.459) rprsts th ratio of th circumfrc of a circl to its diamtr. (approximatly qual to.788) is th bas of th atural

More information

Outline. Ionizing Radiation. Introduction. Ionizing radiation

Outline. Ionizing Radiation. Introduction. Ionizing radiation Outli Ioizig Radiatio Chaptr F.A. Attix, Itroductio to Radiological Physics ad Radiatio Dosimtry Radiological physics ad radiatio dosimtry Typs ad sourcs of ioizig radiatio Dscriptio of ioizig radiatio

More information

LECTURE 13 Filling the bands. Occupancy of Available Energy Levels

LECTURE 13 Filling the bands. Occupancy of Available Energy Levels LUR 3 illig th bads Occupacy o Availabl rgy Lvls W hav dtrmid ad a dsity o stats. W also d a way o dtrmiig i a stat is illd or ot at a giv tmpratur. h distributio o th rgis o a larg umbr o particls ad

More information

Bipolar Junction Transistors

Bipolar Junction Transistors ipolar Juctio Trasistors ipolar juctio trasistors (JT) ar activ 3-trmial dvics with aras of applicatios: amplifirs, switch tc. high-powr circuits high-spd logic circuits for high-spd computrs. JT structur:

More information

Electromagnetic radiation and steady states of hydrogen atom

Electromagnetic radiation and steady states of hydrogen atom Elctromagtic radiatio ad stady stats of hydrog atom Jiaomig Luo Egirig Rsarch Ctr i Biomatrials, Sichua Uivrsity, 9# Wagjiag Road, Chgdu, Chia, 610064 Abstract. Elctromagtic phoma i hydrog atom ar cotrolld

More information

(Reference: sections in Silberberg 5 th ed.)

(Reference: sections in Silberberg 5 th ed.) ALE. Atomic Structur Nam HEM K. Marr Tam No. Sctio What is a atom? What is th structur of a atom? Th Modl th structur of a atom (Rfrc: sctios.4 -. i Silbrbrg 5 th d.) Th subatomic articls that chmists

More information

DTFT Properties. Example - Determine the DTFT Y ( e ) of n. Let. We can therefore write. From Table 3.1, the DTFT of x[n] is given by 1

DTFT Properties. Example - Determine the DTFT Y ( e ) of n. Let. We can therefore write. From Table 3.1, the DTFT of x[n] is given by 1 DTFT Proprtis Exampl - Dtrmi th DTFT Y of y α µ, α < Lt x α µ, α < W ca thrfor writ y x x From Tabl 3., th DTFT of x is giv by ω X ω α ω Copyright, S. K. Mitra Copyright, S. K. Mitra DTFT Proprtis DTFT

More information

Bohr type models of the atom give a totally incorrect picture of the atom and are of only historical significance.

Bohr type models of the atom give a totally incorrect picture of the atom and are of only historical significance. VISUAL PHYSICS ONLIN BOHR MODL OF TH ATOM Bhr typ mdls f th atm giv a ttally icrrct pictur f th atm ad ar f ly histrical sigificac. Fig.. Bhr s platary mdl f th atm. Hwvr, th Bhr mdls wr a imprtat stp

More information

Triple Play: From De Morgan to Stirling To Euler to Maclaurin to Stirling

Triple Play: From De Morgan to Stirling To Euler to Maclaurin to Stirling Tripl Play: From D Morga to Stirlig To Eulr to Maclauri to Stirlig Augustus D Morga (186-1871) was a sigificat Victoria Mathmaticia who mad cotributios to Mathmatics History, Mathmatical Rcratios, Mathmatical

More information

Option 3. b) xe dx = and therefore the series is convergent. 12 a) Divergent b) Convergent Proof 15 For. p = 1 1so the series diverges.

Option 3. b) xe dx = and therefore the series is convergent. 12 a) Divergent b) Convergent Proof 15 For. p = 1 1so the series diverges. Optio Chaptr Ercis. Covrgs to Covrgs to Covrgs to Divrgs Covrgs to Covrgs to Divrgs 8 Divrgs Covrgs to Covrgs to Divrgs Covrgs to Covrgs to Covrgs to Covrgs to 8 Proof Covrgs to π l 8 l a b Divrgt π Divrgt

More information

NET/JRF, GATE, IIT JAM, JEST, TIFR

NET/JRF, GATE, IIT JAM, JEST, TIFR Istitut for NET/JRF, GATE, IIT JAM, JEST, TIFR ad GRE i PHYSICAL SCIENCES Mathmatical Physics JEST-6 Q. Giv th coditio φ, th solutio of th quatio ψ φ φ is giv by k. kφ kφ lφ kφ lφ (a) ψ (b) ψ kφ (c) ψ

More information

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted?

Blackbody Radiation. All bodies at a temperature T emit and absorb thermal electromagnetic radiation. How is blackbody radiation absorbed and emitted? All bodis at a tmpratur T mit ad absorb thrmal lctromagtic radiatio Blackbody radiatio I thrmal quilibrium, th powr mittd quals th powr absorbd How is blackbody radiatio absorbd ad mittd? 1 2 A blackbody

More information

MONTGOMERY COLLEGE Department of Mathematics Rockville Campus. 6x dx a. b. cos 2x dx ( ) 7. arctan x dx e. cos 2x dx. 2 cos3x dx

MONTGOMERY COLLEGE Department of Mathematics Rockville Campus. 6x dx a. b. cos 2x dx ( ) 7. arctan x dx e. cos 2x dx. 2 cos3x dx MONTGOMERY COLLEGE Dpartmt of Mathmatics Rockvill Campus MATH 8 - REVIEW PROBLEMS. Stat whthr ach of th followig ca b itgratd by partial fractios (PF), itgratio by parts (PI), u-substitutio (U), or o of

More information

APPENDIX: STATISTICAL TOOLS

APPENDIX: STATISTICAL TOOLS I. Nots o radom samplig Why do you d to sampl radomly? APPENDI: STATISTICAL TOOLS I ordr to masur som valu o a populatio of orgaisms, you usually caot masur all orgaisms, so you sampl a subst of th populatio.

More information

H2 Mathematics Arithmetic & Geometric Series ( )

H2 Mathematics Arithmetic & Geometric Series ( ) H Mathmatics Arithmtic & Gomtric Sris (08 09) Basic Mastry Qustios Arithmtic Progrssio ad Sris. Th rth trm of a squc is 4r 7. (i) Stat th first four trms ad th 0th trm. (ii) Show that th squc is a arithmtic

More information

Fermi Gas. separation

Fermi Gas. separation ri Gas Distiguishabl Idistiguishabl Classical dgrat dd o dsity. If th wavlgth siilar to th saratio tha dgrat ri gas articl h saratio largr traturs hav sallr wavlgth d tightr ackig for dgracy

More information

PURE MATHEMATICS A-LEVEL PAPER 1

PURE MATHEMATICS A-LEVEL PAPER 1 -AL P MATH PAPER HONG KONG EXAMINATIONS AUTHORITY HONG KONG ADVANCED LEVEL EXAMINATION PURE MATHEMATICS A-LEVEL PAPER 8 am am ( hours) This papr must b aswrd i Eglish This papr cosists of Sctio A ad Sctio

More information

Chapter 2 Infinite Series Page 1 of 11. Chapter 2 : Infinite Series

Chapter 2 Infinite Series Page 1 of 11. Chapter 2 : Infinite Series Chatr Ifiit Sris Pag of Sctio F Itgral Tst Chatr : Ifiit Sris By th d of this sctio you will b abl to valuat imror itgrals tst a sris for covrgc by alyig th itgral tst aly th itgral tst to rov th -sris

More information

Probability & Statistics,

Probability & Statistics, Probability & Statistics, BITS Pilai K K Birla Goa Campus Dr. Jajati Kshari Sahoo Dpartmt of Mathmatics BITS Pilai, K K Birla Goa Campus Poisso Distributio Poisso Distributio: A radom variabl X is said

More information

Solution to 1223 The Evil Warden.

Solution to 1223 The Evil Warden. Solutio to 1 Th Evil Ward. This is o of thos vry rar PoWs (I caot thik of aothr cas) that o o solvd. About 10 of you submittd th basic approach, which givs a probability of 47%. I was shockd wh I foud

More information

Ideal crystal : Regulary ordered point masses connected via harmonic springs

Ideal crystal : Regulary ordered point masses connected via harmonic springs Statistical thrmodyamics of crystals Mooatomic crystal Idal crystal : Rgulary ordrd poit masss coctd via harmoic sprigs Itratomic itractios Rprstd by th lattic forc-costat quivalt atom positios miima o

More information

Statistics 3858 : Likelihood Ratio for Exponential Distribution

Statistics 3858 : Likelihood Ratio for Exponential Distribution Statistics 3858 : Liklihood Ratio for Expotial Distributio I ths two xampl th rjctio rjctio rgio is of th form {x : 2 log (Λ(x)) > c} for a appropriat costat c. For a siz α tst, usig Thorm 9.5A w obtai

More information

2617 Mark Scheme June 2005 Mark Scheme 2617 June 2005

2617 Mark Scheme June 2005 Mark Scheme 2617 June 2005 Mark Schm 67 Ju 5 GENERAL INSTRUCTIONS Marks i th mark schm ar plicitly dsigatd as M, A, B, E or G. M marks ("mthod" ar for a attmpt to us a corrct mthod (ot mrly for statig th mthod. A marks ("accuracy"

More information

INTRODUCTION TO SAMPLING DISTRIBUTIONS

INTRODUCTION TO SAMPLING DISTRIBUTIONS http://wiki.stat.ucla.du/socr/id.php/socr_courss_2008_thomso_econ261 INTRODUCTION TO SAMPLING DISTRIBUTIONS By Grac Thomso INTRODUCTION TO SAMPLING DISTRIBUTIONS Itro to Samplig 2 I this chaptr w will

More information

EE 232 Lightwave Devices Lecture 3: Basic Semiconductor Physics and Optical Processes. Optical Properties of Semiconductors

EE 232 Lightwave Devices Lecture 3: Basic Semiconductor Physics and Optical Processes. Optical Properties of Semiconductors 3 Lightwav Dvics Lctur 3: Basic Smicoductor Physics ad Optical Procsss Istructor: Mig C. Wu Uivrsity of Califoria, Brly lctrical girig ad Computr Scics Dpt. 3 Lctur 3- Optical Proprtis of Smicoductors

More information

On the approximation of the constant of Napier

On the approximation of the constant of Napier Stud. Uiv. Babş-Bolyai Math. 560, No., 609 64 O th approximatio of th costat of Napir Adri Vrscu Abstract. Startig from som oldr idas of [] ad [6], w show w facts cocrig th approximatio of th costat of

More information

How many neutrons does this aluminium atom contain? A 13 B 14 C 27 D 40

How many neutrons does this aluminium atom contain? A 13 B 14 C 27 D 40 alumiium atom has a uclo umbr of 7 ad a roto umbr of 3. How may utros dos this alumiium atom cotai? 3 4 7 40 atom of lmt Q cotais 9 lctros, 9 rotos ad 0 utros. What is Q? calcium otassium strotium yttrium

More information

Discrete Fourier Transform (DFT)

Discrete Fourier Transform (DFT) Discrt Fourir Trasorm DFT Major: All Egirig Majors Authors: Duc guy http://umricalmthods.g.us.du umrical Mthods or STEM udrgraduats 8/3/29 http://umricalmthods.g.us.du Discrt Fourir Trasorm Rcalld th xpotial

More information

10. Joint Moments and Joint Characteristic Functions

10. Joint Moments and Joint Characteristic Functions 0 Joit Momts ad Joit Charactristic Fctios Followig sctio 6 i this sctio w shall itrodc varios paramtrs to compactly rprst th iformatio cotaid i th joit pdf of two rvs Giv two rvs ad ad a fctio g x y dfi

More information

Narayana IIT Academy

Narayana IIT Academy INDIA Sc: LT-IIT-SPARK Dat: 9--8 6_P Max.Mars: 86 KEY SHEET PHYSIS A 5 D 6 7 A,B 8 B,D 9 A,B A,,D A,B, A,B B, A,B 5 A 6 D 7 8 A HEMISTRY 9 A B D B B 5 A,B,,D 6 A,,D 7 B,,D 8 A,B,,D 9 A,B, A,B, A,B,,D A,B,

More information

3.1 Atomic Structure and The Periodic Table

3.1 Atomic Structure and The Periodic Table Sav My Exams! Th Hom of Rvisio For mor awsom GSE ad lvl rsourcs, visit us at www.savmyxams.co.uk/ 3. tomic Structur ad Th Priodic Tabl Qustio Par Lvl IGSE Subjct hmistry (060) Exam oard ambridg Itratioal

More information

Figure 2-18 Thevenin Equivalent Circuit of a Noisy Resistor

Figure 2-18 Thevenin Equivalent Circuit of a Noisy Resistor .8 NOISE.8. Th Nyquist Nois Thorm W ow wat to tur our atttio to ois. W will start with th basic dfiitio of ois as usd i radar thory ad th discuss ois figur. Th typ of ois of itrst i radar thory is trmd

More information

Chapter Taylor Theorem Revisited

Chapter Taylor Theorem Revisited Captr 0.07 Taylor Torm Rvisitd Atr radig tis captr, you sould b abl to. udrstad t basics o Taylor s torm,. writ trascdtal ad trigoomtric uctios as Taylor s polyomial,. us Taylor s torm to id t valus o

More information

Time Dependent Solutions: Propagators and Representations

Time Dependent Solutions: Propagators and Representations Tim Dpdt Solutios: Propagators ad Rprstatios Michal Fowlr, UVa 1/3/6 Itroductio W v spt most of th cours so far coctratig o th igstats of th amiltoia, stats whos tim dpdc is mrly a chagig phas W did mtio

More information

NEW VERSION OF SZEGED INDEX AND ITS COMPUTATION FOR SOME NANOTUBES

NEW VERSION OF SZEGED INDEX AND ITS COMPUTATION FOR SOME NANOTUBES Digst Joural of Naomatrials ad Biostructurs Vol 4, No, March 009, p 67-76 NEW VERSION OF SZEGED INDEX AND ITS COMPUTATION FOR SOME NANOTUBES A IRANMANESH a*, O KHORMALI b, I NAJAFI KHALILSARAEE c, B SOLEIMANI

More information

Electronic Supplementary Information

Electronic Supplementary Information Elctroic Supplmtary Matrial (ESI) for Joural of Matrials Chmistry A. This joural is Th Royal Socity of Chmistry 2016 Elctroic Supplmtary Iformatio Photolctrochmical Watr Oxidatio usig a Bi 2 MoO 6 / MoO

More information

Discrete Fourier Transform. Nuno Vasconcelos UCSD

Discrete Fourier Transform. Nuno Vasconcelos UCSD Discrt Fourir Trasform uo Vascoclos UCSD Liar Shift Ivariat (LSI) systms o of th most importat cocpts i liar systms thory is that of a LSI systm Dfiitio: a systm T that maps [ ito y[ is LSI if ad oly if

More information

Time : 1 hr. Test Paper 08 Date 04/01/15 Batch - R Marks : 120

Time : 1 hr. Test Paper 08 Date 04/01/15 Batch - R Marks : 120 Tim : hr. Tst Papr 8 D 4//5 Bch - R Marks : SINGLE CORRECT CHOICE TYPE [4, ]. If th compl umbr z sisfis th coditio z 3, th th last valu of z is qual to : z (A) 5/3 (B) 8/3 (C) /3 (D) o of ths 5 4. Th itgral,

More information

Washington State University

Washington State University he 3 Ktics ad Ractor Dsig Sprg, 00 Washgto Stat Uivrsity Dpartmt of hmical Egrg Richard L. Zollars Exam # You will hav o hour (60 muts) to complt this xam which cosists of four (4) problms. You may us

More information

Atom as a Dressed Nucleus

Atom as a Dressed Nucleus tom as a Drssd Nuclus Vladimir Kalitviaski Comissariat à l Ergi tomiqu (CE), Grobl 38054, Frac vladimir.kalitviaski@waadoo.fr W show that th lctrostatic pottial of a atomic uclus "s" by a fast chargd projctil

More information

Lecture #2: Wave Nature of the Electron and the Internal Structure of an Atom

Lecture #2: Wave Nature of the Electron and the Internal Structure of an Atom 5.61 Fall 013 Lctur # pag 1 Lctur #: Wav Natur of t Elctro ad t Itral Structur of a Atom Last tim: Surpris Ligt as particl 1. Potolctric ffct, spcially KE vs. ν. Ligt as packts of rgy, calld potos, E =

More information

ELECTRONIC APPENDIX TO: ELASTIC-PLASTIC CONTACT OF A ROUGH SURFACE WITH WEIERSTRASS PROFILE. Yan-Fei Gao and A. F. Bower

ELECTRONIC APPENDIX TO: ELASTIC-PLASTIC CONTACT OF A ROUGH SURFACE WITH WEIERSTRASS PROFILE. Yan-Fei Gao and A. F. Bower ELECTRONIC APPENDIX TO: ELASTIC-PLASTIC CONTACT OF A ROUGH SURFACE WITH WEIERSTRASS PROFILE Ya-Fi Gao ad A. F. Bowr Divisio of Egirig, Brow Uivrsity, Providc, RI 9, USA Appdix A: Approximat xprssios for

More information

ln x = n e = 20 (nearest integer)

ln x = n e = 20 (nearest integer) H JC Prlim Solutios 6 a + b y a + b / / dy a b 3/ d dy a b at, d Giv quatio of ormal at is y dy ad y wh. d a b () (,) is o th curv a+ b () y.9958 Qustio Solvig () ad (), w hav a, b. Qustio d.77 d d d.77

More information

Chapter Five. More Dimensions. is simply the set of all ordered n-tuples of real numbers x = ( x 1

Chapter Five. More Dimensions. is simply the set of all ordered n-tuples of real numbers x = ( x 1 Chatr Fiv Mor Dimsios 51 Th Sac R W ar ow rard to mov o to sacs of dimsio gratr tha thr Ths sacs ar a straightforward gralizatio of our Euclida sac of thr dimsios Lt b a ositiv itgr Th -dimsioal Euclida

More information

Partition Functions and Ideal Gases

Partition Functions and Ideal Gases Partitio Fuctios ad Idal Gass PFIG- You v lard about partitio fuctios ad som uss ow w ll xplor tm i mor dpt usig idal moatomic diatomic ad polyatomic gass! for w start rmmbr: Q( N ( N! N Wat ar N ad? W

More information

to the SCHRODINGER EQUATION The case of an electron propagating in a crystal lattice

to the SCHRODINGER EQUATION The case of an electron propagating in a crystal lattice Lctur Nots PH 411/511 ECE 598 A. La Rosa INTRODUCTION TO QUANTUM MECHANICS CHAPTER-9 From th HAMILTONIAN EQUATIONS to th SCHRODINGER EQUATION Th cas of a lctro propagatig i a crystal lattic 9.1 Hamiltoia

More information

STIRLING'S 1 FORMULA AND ITS APPLICATION

STIRLING'S 1 FORMULA AND ITS APPLICATION MAT-KOL (Baja Luka) XXIV ()(08) 57-64 http://wwwimviblorg/dmbl/dmblhtm DOI: 075/МК80057A ISSN 0354-6969 (o) ISSN 986-588 (o) STIRLING'S FORMULA AND ITS APPLICATION Šfkt Arslaagić Sarajvo B&H Abstract:

More information

Worksheet: Taylor Series, Lagrange Error Bound ilearnmath.net

Worksheet: Taylor Series, Lagrange Error Bound ilearnmath.net Taylor s Thorm & Lagrag Error Bouds Actual Error This is th ral amout o rror, ot th rror boud (worst cas scario). It is th dirc btw th actual () ad th polyomial. Stps:. Plug -valu ito () to gt a valu.

More information

EAcos θ, where θ is the angle between the electric field and

EAcos θ, where θ is the angle between the electric field and 8.4. Modl: Th lctric flux flows out of a closd surfac around a rgion of spac containing a nt positiv charg and into a closd surfac surrounding a nt ngativ charg. Visualiz: Plas rfr to Figur EX8.4. Lt A

More information

September 23, Honors Chem Atomic structure.notebook. Atomic Structure

September 23, Honors Chem Atomic structure.notebook. Atomic Structure Atomic Structur Topics covrd Atomic structur Subatomic particls Atomic numbr Mass numbr Charg Cations Anions Isotops Avrag atomic mass Practic qustions atomic structur Sp 27 8:16 PM 1 Powr Standards/ Larning

More information

Folding of Hyperbolic Manifolds

Folding of Hyperbolic Manifolds It. J. Cotmp. Math. Scics, Vol. 7, 0, o. 6, 79-799 Foldig of Hyprbolic Maifolds H. I. Attiya Basic Scic Dpartmt, Collg of Idustrial Educatio BANE - SUEF Uivrsity, Egypt hala_attiya005@yahoo.com Abstract

More information

Chapter 11.00C Physical Problem for Fast Fourier Transform Civil Engineering

Chapter 11.00C Physical Problem for Fast Fourier Transform Civil Engineering haptr. Physical Problm for Fast Fourir Trasform ivil Egirig Itroductio I this chaptr, applicatios of FFT algorithms [-5] for solvig ral-lif problms such as computig th dyamical (displacmt rspos [6-7] of

More information

A Propagating Wave Packet Group Velocity Dispersion

A Propagating Wave Packet Group Velocity Dispersion Lctur 8 Phys 375 A Propagating Wav Packt Group Vlocity Disprsion Ovrviw and Motivation: In th last lctur w lookd at a localizd solution t) to th 1D fr-particl Schrödingr quation (SE) that corrsponds to

More information

Lectures 9 IIR Systems: First Order System

Lectures 9 IIR Systems: First Order System EE3054 Sigals ad Systms Lcturs 9 IIR Systms: First Ordr Systm Yao Wag Polytchic Uivrsity Som slids icludd ar xtractd from lctur prstatios prpard by McCllla ad Schafr Lics Ifo for SPFirst Slids This work

More information

Chapter (8) Estimation and Confedence Intervals Examples

Chapter (8) Estimation and Confedence Intervals Examples Chaptr (8) Estimatio ad Cofdc Itrvals Exampls Typs of stimatio: i. Poit stimatio: Exampl (1): Cosidr th sampl obsrvatios, 17,3,5,1,18,6,16,10 8 X i i1 17 3 5 118 6 16 10 116 X 14.5 8 8 8 14.5 is a poit

More information

THE WEAK INTERACTION. e - MISN by J. Christman. 1. Overview Assigned Readings... 1

THE WEAK INTERACTION. e - MISN by J. Christman. 1. Overview Assigned Readings... 1 MISN0281 THE WEAK INTERACTION by J. Christma THE WEAK INTERACTION 1. Ovrviw.................................................. 1 2. Assigd Radigs....................................... 1 s d d _ u d s d

More information

Joule-Lenz Energy of Quantum Electron Transitions Compared with the Electromagnetic Emission of Energy

Joule-Lenz Energy of Quantum Electron Transitions Compared with the Electromagnetic Emission of Energy Joural of Modr Physics, 06, 7, 440-448 Publishd Oli August 06 i SciRs http://wwwscirporg/joural/jmp http://dxdoiorg/0436/jmp0673 Joul-Lz Ergy of Quatum Elctro Trasitios Compard with th Elctromagtic Emissio

More information

Physics of the Interstellar and Intergalactic Medium

Physics of the Interstellar and Intergalactic Medium PYA0 Sior Sophistr Physics of th Itrstllar ad Itrgalactic Mdium Lctur 7: II gios Dr Graham M. arpr School of Physics, TCD Follow-up radig for this ad t lctur Chaptr 5: Dyso ad Williams (lss dtaild) Chaptr

More information

CDS 101: Lecture 5.1 Reachability and State Space Feedback

CDS 101: Lecture 5.1 Reachability and State Space Feedback CDS, Lctur 5. CDS : Lctur 5. Rachability ad Stat Spac Fdback Richard M. Murray ad Hido Mabuchi 5 Octobr 4 Goals: Di rachability o a cotrol systm Giv tsts or rachability o liar systms ad apply to ampls

More information

Chapter 4 - The Fourier Series

Chapter 4 - The Fourier Series M. J. Robrts - 8/8/4 Chaptr 4 - Th Fourir Sris Slctd Solutios (I this solutio maual, th symbol,, is usd for priodic covolutio bcaus th prfrrd symbol which appars i th txt is ot i th fot slctio of th word

More information

ECE594I Notes set 6: Thermal Noise

ECE594I Notes set 6: Thermal Noise C594I ots, M. odwll, copyrightd C594I Nots st 6: Thrmal Nois Mark odwll Uivrsity of Califoria, ata Barbara rodwll@c.ucsb.du 805-893-344, 805-893-36 fax frcs ad Citatios: C594I ots, M. odwll, copyrightd

More information

On a problem of J. de Graaf connected with algebras of unbounded operators de Bruijn, N.G.

On a problem of J. de Graaf connected with algebras of unbounded operators de Bruijn, N.G. O a problm of J. d Graaf coctd with algbras of uboudd oprators d Bruij, N.G. Publishd: 01/01/1984 Documt Vrsio Publishr s PDF, also kow as Vrsio of Rcord (icluds fial pag, issu ad volum umbrs) Plas chck

More information

CDS 101: Lecture 5.1 Reachability and State Space Feedback

CDS 101: Lecture 5.1 Reachability and State Space Feedback CDS, Lctur 5. CDS : Lctur 5. Rachability ad Stat Spac Fdback Richard M. Murray 7 Octobr 3 Goals: Di rachability o a cotrol systm Giv tsts or rachability o liar systms ad apply to ampls Dscrib th dsig o

More information

Topological Insulators in 2D and 3D

Topological Insulators in 2D and 3D Topological Isulators i D ad 3D 0. Elctric polarizatio, Chr Numbr, Itgr Quatum Hall Effct I. Graph - Halda modl - Tim rvrsal symmtry ad Kramrs thorm II. D quatum spi Hall isulator - Z topological ivariat

More information

22/ Breakdown of the Born-Oppenheimer approximation. Selection rules for rotational-vibrational transitions. P, R branches.

22/ Breakdown of the Born-Oppenheimer approximation. Selection rules for rotational-vibrational transitions. P, R branches. Subjct Chmistry Papr No and Titl Modul No and Titl Modul Tag 8/ Physical Spctroscopy / Brakdown of th Born-Oppnhimr approximation. Slction ruls for rotational-vibrational transitions. P, R branchs. CHE_P8_M

More information

ELECTRON-MUON SCATTERING

ELECTRON-MUON SCATTERING ELECTRON-MUON SCATTERING ABSTRACT Th lctron charg is considrd to b distributd or xtndd in spac. Th diffrntial of th lctron charg is st qual to a function of lctron charg coordinats multiplid by a four-dimnsional

More information

Restricted Factorial And A Remark On The Reduced Residue Classes

Restricted Factorial And A Remark On The Reduced Residue Classes Applid Mathmatics E-Nots, 162016, 244-250 c ISSN 1607-2510 Availabl fr at mirror sits of http://www.math.thu.du.tw/ am/ Rstrictd Factorial Ad A Rmark O Th Rducd Rsidu Classs Mhdi Hassai Rcivd 26 March

More information

t i Extreme value statistics Problems of extrapolating to values we have no data about unusually large or small ~100 years (data) ~500 years (design)

t i Extreme value statistics Problems of extrapolating to values we have no data about unusually large or small ~100 years (data) ~500 years (design) Extrm valu statistics Problms of xtrapolatig to valus w hav o data about uusually larg or small t i ~00 yars (data h( t i { h( }? max t i wids v( t i ~500 yars (dsig Qustio: Ca this b do at all? How log

More information

Lecture 37 (Schrödinger Equation) Physics Spring 2018 Douglas Fields

Lecture 37 (Schrödinger Equation) Physics Spring 2018 Douglas Fields Lctur 37 (Schrödingr Equation) Physics 6-01 Spring 018 Douglas Filds Rducd Mass OK, so th Bohr modl of th atom givs nrgy lvls: E n 1 k m n 4 But, this has on problm it was dvlopd assuming th acclration

More information

SOLUTIONS TO CHAPTER 2 PROBLEMS

SOLUTIONS TO CHAPTER 2 PROBLEMS SOLUTIONS TO CHAPTER PROBLEMS Problm.1 Th pully of Fig..33 is composd of fiv portios: thr cylidrs (of which two ar idtical) ad two idtical co frustum sgmts. Th mass momt of irtia of a cylidr dfid by a

More information

Electromagnetic Time Dilation and Contraction, and a Geometrodynamic Foundation of Classical and Quantum Electrodynamics

Electromagnetic Time Dilation and Contraction, and a Geometrodynamic Foundation of Classical and Quantum Electrodynamics Jay R. Yablo, Sptbr 6, 16 Elctromagtic Tim Dilatio ad Cotractio, ad a Gomtrodyamic Foudatio of Classical ad Quatum Elctrodyamics Jay R. Yablo 91 Northumbrlad Driv Schctady, Nw York 139-814 yablo@alum.mit.du

More information

Class #24 Monday, April 16, φ φ φ

Class #24 Monday, April 16, φ φ φ lass #4 Moday, April 6, 08 haptr 3: Partial Diffrtial Equatios (PDE s First of all, this sctio is vry, vry difficult. But it s also supr cool. PDE s thr is mor tha o idpdt variabl. Exampl: φ φ φ φ = 0

More information

Review Exercises. 1. Evaluate using the definition of the definite integral as a Riemann Sum. Does the answer represent an area? 2

Review Exercises. 1. Evaluate using the definition of the definite integral as a Riemann Sum. Does the answer represent an area? 2 MATHEMATIS --RE Itgral alculus Marti Huard Witr 9 Rviw Erciss. Evaluat usig th dfiitio of th dfiit itgral as a Rima Sum. Dos th aswr rprst a ara? a ( d b ( d c ( ( d d ( d. Fid f ( usig th Fudamtal Thorm

More information

Circular Array of Tapered Nylon Rod Antennas: A Computational Study

Circular Array of Tapered Nylon Rod Antennas: A Computational Study tratioal Joural of Elctroics ad Commuicatio Egirig. SSN 974-266 Volum 4, Numbr (2), pp.3-38 tratioal Rsarch Publicatio Hous http://www.irphous.com Circular Array of Taprd Nylo Rod Atas: A Computatioal

More information

orbiting electron turns out to be wrong even though it Unfortunately, the classical visualization of the

orbiting electron turns out to be wrong even though it Unfortunately, the classical visualization of the Lctur 22-1 Byond Bohr Modl Unfortunatly, th classical visualization of th orbiting lctron turns out to b wrong vn though it still givs us a simpl way to think of th atom. Quantum Mchanics is ndd to truly

More information

Scattering Parameters. Scattering Parameters

Scattering Parameters. Scattering Parameters Motivatio cattrig Paramtrs Difficult to implmt op ad short circuit coditios i high frqucis masurmts du to parasitic s ad Cs Pottial stability problms for activ dvics wh masurd i oopratig coditios Difficult

More information

Derivation of Electron-Electron Interaction Terms in the Multi-Electron Hamiltonian

Derivation of Electron-Electron Interaction Terms in the Multi-Electron Hamiltonian Drivation of Elctron-Elctron Intraction Trms in th Multi-Elctron Hamiltonian Erica Smith Octobr 1, 010 1 Introduction Th Hamiltonian for a multi-lctron atom with n lctrons is drivd by Itoh (1965) by accounting

More information

Chapter 8: Electron Configurations and Periodicity

Chapter 8: Electron Configurations and Periodicity Elctron Spin & th Pauli Exclusion Principl Chaptr 8: Elctron Configurations and Priodicity 3 quantum numbrs (n, l, ml) dfin th nrgy, siz, shap, and spatial orintation of ach atomic orbital. To xplain how

More information

Reliability of time dependent stress-strength system for various distributions

Reliability of time dependent stress-strength system for various distributions IOS Joural of Mathmatcs (IOS-JM ISSN: 78-578. Volum 3, Issu 6 (Sp-Oct., PP -7 www.osrjourals.org lablty of tm dpdt strss-strgth systm for varous dstrbutos N.Swath, T.S.Uma Mahswar,, Dpartmt of Mathmatcs,

More information

Ch. 24 Molecular Reaction Dynamics 1. Collision Theory

Ch. 24 Molecular Reaction Dynamics 1. Collision Theory Ch. 4 Molcular Raction Dynamics 1. Collision Thory Lctur 16. Diffusion-Controlld Raction 3. Th Matrial Balanc Equation 4. Transition Stat Thory: Th Eyring Equation 5. Transition Stat Thory: Thrmodynamic

More information

Solid State Device Fundamentals

Solid State Device Fundamentals 8 Biasd - Juctio Solid Stat Dvic Fudamtals 8. Biasd - Juctio ENS 345 Lctur Cours by Aladr M. Zaitsv aladr.zaitsv@csi.cuy.du Tl: 718 98 81 4N101b Dartmt of Egirig Scic ad Physics Biasig uiolar smicoductor

More information

Key words Non-uniform; specific energy; critical; gradually-varied steady flow; water surface profiles

Key words Non-uniform; specific energy; critical; gradually-varied steady flow; water surface profiles Chaptr NON-UNIFORM FLOW 4.. Itroductio 4.. Gradually-varid stady 4.3. Typs of watr surfac profils 4.4. Drawig watr surfac profils Summary Likig up with Chaptr, dalig with uiform i op chals, it may b otd

More information

An Introduction to Asymptotic Expansions

An Introduction to Asymptotic Expansions A Itroductio to Asmptotic Expasios R. Shaar Subramaia Asmptotic xpasios ar usd i aalsis to dscrib th bhavior of a fuctio i a limitig situatio. Wh a fuctio ( x, dpds o a small paramtr, ad th solutio of

More information

Part B: Transform Methods. Professor E. Ambikairajah UNSW, Australia

Part B: Transform Methods. Professor E. Ambikairajah UNSW, Australia Part B: Trasform Mthods Chaptr 3: Discrt-Tim Fourir Trasform (DTFT) 3. Discrt Tim Fourir Trasform (DTFT) 3. Proprtis of DTFT 3.3 Discrt Fourir Trasform (DFT) 3.4 Paddig with Zros ad frqucy Rsolutio 3.5

More information

Quasi-Classical States of the Simple Harmonic Oscillator

Quasi-Classical States of the Simple Harmonic Oscillator Quasi-Classical Stats of th Simpl Harmonic Oscillator (Draft Vrsion) Introduction: Why Look for Eignstats of th Annihilation Oprator? Excpt for th ground stat, th corrspondnc btwn th quantum nrgy ignstats

More information

The van der Waals interaction 1 D. E. Soper 2 University of Oregon 20 April 2012

The van der Waals interaction 1 D. E. Soper 2 University of Oregon 20 April 2012 Th van dr Waals intraction D. E. Sopr 2 Univrsity of Orgon 20 pril 202 Th van dr Waals intraction is discussd in Chaptr 5 of J. J. Sakurai, Modrn Quantum Mchanics. Hr I tak a look at it in a littl mor

More information

Available online at Energy Procedia 4 (2011) Energy Procedia 00 (2010) GHGT-10

Available online at   Energy Procedia 4 (2011) Energy Procedia 00 (2010) GHGT-10 Availabl oli at www.scicdirct.com Ergy Procdia 4 (01 170 177 Ergy Procdia 00 (010) 000 000 Ergy Procdia www.lsvir.com/locat/procdia www.lsvir.com/locat/xxx GHGT-10 Exprimtal Studis of CO ad CH 4 Diffusio

More information

Numerov-Cooley Method : 1-D Schr. Eq. Last time: Rydberg, Klein, Rees Method and Long-Range Model G(v), B(v) rotation-vibration constants.

Numerov-Cooley Method : 1-D Schr. Eq. Last time: Rydberg, Klein, Rees Method and Long-Range Model G(v), B(v) rotation-vibration constants. Numrov-Cooly Mthod : 1-D Schr. Eq. Last tim: Rydbrg, Kli, Rs Mthod ad Log-Rag Modl G(v), B(v) rotatio-vibratio costats 9-1 V J (x) pottial rgy curv x = R R Ev,J, v,j, all cocivabl xprimts wp( x, t) = ai

More information