Hadronic Structure Functions 1

Size: px
Start display at page:

Download "Hadronic Structure Functions 1"

Transcription

1 Hadronic Structur Functions 1 arxiv:hp-x/ v1 5 Sp 2000 Martin Erdmann Institut für Exprimntll Krnphysik, Univrsität Karlsruh, Engssrstr. 7, D Karlsruh, Martin.Erdmann@dsy.d Abstract Exprimntal rsults on hadronic structurs ar discussd in viw of our physics undrstanding. Achivmnts and challngs ar notd. 1 Invitd opning plnary talk at th 8th Intrnational Workshop on Dp Inlastic Scattring and QCD, Livrpool, UK (2000)

2 1 Motivation Today s motivation of masuring lpton hadron scattring procsss is at last four-fold. Fig.1 shows basic diagrams at lctron positron, hadron hadron, and lpton hadron collidrs: Only in lpton hadron collisions is th fusion diagram forbiddn within th Standard Modl, which strongly motivats sarchs for nw physics,.g. lptoquarks. Th xchang of bosons allows diffrnt hadronic structurs to b probd: Th prototyp for xisting hadronic structurs is th proton which currntly is th most prcisly studid hadronic objct. Gnsis of hadronic structurs is analysd using th structur dvloping in quantum fluctuations of th photon. Colour singlt xchang constituts a procss byond singl boson xchang. It s succssful dscription provids a prim challng for QCD. It is th purpos of this contribution to undrlin ths diffrnt aspcts of lpton-hadron scattring physics and thir prspctivs using as much as possibl th masurmnts thmslvs. LEP/TESLA TEV/LHC HERA LEP/TESLA q, g q, g? q, g q, g q q Figur 1: Basic diagrams at lctron positron, hadron hadron, and lpton hadron collidrs. Only th last diagram is forbiddn within th Standard Modl. 2 Lpton Quark Scattring at Attomtr Distanc Th larg cntr of mass nrgy at HERA of s p = 318 GV allows lpton quark scattring to b analysd at distancs down to almost 1 Attomtr = m. Both nutral and chargd currnt intractions (Fig.2) ar usd to tst th Standard Modl prdictions. Th doubl diffrntial cross sctions in trms of th rsolution scal Q 2, which dnots th ngativ squard 1

3 Nutral and chargd currnt intractions obsrvd with th ZEUS and H1 xpri- Figur 2: mnts. four-momntum transfr carrid by th boson, and th quark fractional momntum x rlativ to th proton ar givn by: d 2 σ NC dq 2 dx d 2 σ CC dq 2 dx α Q 4 x Φ NC(x, Q 2 ) (1) ( ) M G W 1 F MW 2 + Q2 x Φ CC (x, Q 2 ). (2) Hr α and G F dnot th coupling strngth of th lctromagntic and wak intraction procsss. M W is th W -boson mass. Th Φ trms dnot th spin charactristics of th scattring togthr with th probabilitis xf(x, Q 2 ) of finding th diffrnt quark flavours in th proton. In addition Φ NC contains trms for Z xchang and γ-z intrfrnc. At high Q 2 it is ( ( )) ( Φ p θ NC 1 + cos (xu + xū) + 1 ) 9 (xd + x d ) ± add. trms with γ, Z (3) ( ) Φ p θ CC xu + cos 4 x 2 d (4) ( ) Φ + p θ CC xū + cos 4 xd. (5) 2 θ dnots th scattring angl in th lpton-quark cntr of mass systm and can b calculatd from cos 4 (θ /2) = (1 Q 2 /s p /x) 2. Th two componnts in th angular distribution rsult from two spin configurations of th colliding lpton and quark: if th spins add up to zro, any scattring angl is allowd. If th spins add up to 1, backward scattring is forbiddn for masslss quarks and th angular distribution is wightd by cos 4 (θ /2). In chargd currnt intractions also th quark typ can b analysd:.g., positrons coupl only to ngativly chargd quarks. In addition, right-handd positrons coupl only to right-handd antiquarks, or lft-handd quarks. This offrs a uniqu handl to diffrntiat btwn quark flavours in th proton. 2

4 Elctron Proton Collisions dσ dq 2 p γ,z p W Q 2 [GV 2 ] Figur 3: Diffrntial cross sction for nutral and chargd currnt intractions as a function of th rsolution scal Q 2 from H1 and ZEUS data. Intgrating th doubl diffrntial cross sctions ovr x givs th singl diffrntial cross sction which is shown in Fig.3 as a function of Q 2 from H1 [1] and ZEUS [2] data. Around Q GV 2 th cross sctions ar found to b of qual magnitud. Sinc in both nutral currnt and chargd currnt lctron-proton scattring at high Q 2 primarily th u-valnc quarks ar probd, qs. (3, 4), ths data stablish dirct obsrvation of th unification of th nutral currnt and chargd currnt intractions at a rsolution scal corrsponding to about 10 Attomtr. In Fig.4, th spin charactristics of chargd currnt positron-proton scattring is tstd in th masurmnt of th wightd cross sctions Φ, q. (2), as a function of cos 4 (θ /2) [3]. Within th prcision of th masurmnt, th data ar in ach x-bin compatibl with a linar ris as xpctd from q. (5). Th xtrapolation of th linar bhavior to th backward scattring rgion (cos 4 (θ /2) = 0) rvals a non-vanishing contribution of th ngativly chargd antiquarks, mainly ū. Thir rlativ contribution dcrass as x incrass. Th rising componnt rflcts th contribution of th d-valnc quarks. Th d-quark dnsity can b rad off th forward scattring cross sction (cos 4 (θ /2) = 1). Also in nutral currnt intractions, th data ar ovr a wid rang compatibl with a linar ris: thy rflct two qually larg componnts, xplaind by th two spin configurations of th lctromagntic procsss, q. (3). Th forward scattring rgion (cos 4 (θ /2) = 1) shows 3

5 φ CC 0.5 Chargd Currnt x=0.08 H1 + p Standard Modl (NLO QCD Fit) 0 xd xū φ NC Nutral Currnt x=0.08 H1 + p Standard Modl (NLO QCD Fit) γ-exchang Fit 4 9 xu 4 9 xu x=0.13 x= x= x= (1-y) 2 cos 4 θ (1-y) 2 cos 4 θ 2 Figur 4: H1 masurmnts of th doubl diffrntial chargd and nutral currnt positronproton cross sctions as a function of cos 4 (θ /2) in diffrnt bins of th parton fractional momntum x. θ dnots th scattring angl in th lpton-quark cntr of mass systm. approximatly th u-quark dnsity in th proton: 2 4/9 xu xu. In th rgion of backward scattring procsss (cos 4 (θ /2) = 0), th cross sction masurmnts dviat from th linar ris and dmonstrat th onst of a nw intraction: th lowr cross sction rsults from th ngativ intrfrnc btwn th photon and th Z-boson. Th comparison of th positron-proton nutral currnt and chargd currnt data in th forward scattring rgion of Fig.4 dmonstrats dirctly from th data that th u-quark dnsity is twic that of th d-quark. Thrfor th proton consists of th uud quark configuration also at th small distanc scals probd at HERA. Th HERA luminosity upgrad program, starting to tak data in 2001, is agrly awaitd: much mor prcis data will challng th Standard Modl prdictions for p procsss in th Attomtr rgim. 4

6 3 Existing Hadronic Structur: Proton As discussd in th prvious sction, th uud valnc structur of th proton has bn rconfirmd in th high Q 2 nutral and chargd currnt masurmnts at HERA. In th following our physics undrstanding of th proton structur function F 2 is discussd. F 2 is dtrmind from masurmnts of th doubl diffrntial nutral currnt cross sction (compar with qs. (1, 3)) d 2 σ dq 2 dx 1 α2 Q 4 (1 + cos 4 ( θ 2 )) 1 x F 2(x, Q 2 ) (6) and contains th individual quark distributions, wightd by th quark squard chargs: F 2 (x, Q 2 ) 4 9 (xu + xū ) (xd + x d ) + 1 (xs + x s ) +... (7) 9 Th QCD volution quations prdict that masurmnts of hadronic structurs dpnd on th logarithm of th rsolution scal Q 2 at which th structur is probd. On this basis, th following ansatz to analys th x-dpndnc of structur function data is xplord [4]: F 2 (x, Q 2 ) = a(x) [ ln ( )] Q 2 κ(x). (8) Hr Λ is a scal paramtr, a rflcts th charg squard wightd quark distributions xtrapolatd to ln(q 2 /Λ 2 ) = 1, and κ dtrmins th positiv and ngativ scaling violations of F 2. In Fig.5, publishd ZEUS [5] low-x data of th proton structur function F 2 for Q 2 > 2 GV 2 ar shown. In ach x-bin, th rsult of a two-paramtr fit according to q. (8) is shown, using a fixd valu of Λ = 0.35 GV which rprsnts a typical valu of th strong intraction scal. Only th total xprimntal rrors hav bn usd, ignoring corrlations btwn individual data points. Th sam fitting procdur has bn applid to BCDMS data [6] which ar takn hr as a rfrnc sampl for th high-x rgion. Th rsulting paramtrs a and κ ar summarizd in Fig.6 as a function of x togthr with fits to th publishd H1 low-x data [7]. Also shown ar fits to th prliminary H1 data [8] which ar much mor prcis than th prvious masurmnts. For a, th data fits xhibit two distinct rgions: around x 0.3 thy rflct th valnc quark distributions, implying that ach valnc quark carris 1/3 of th proton momntum. At low x, a(x) is compatibl with convrging to a constant valu. A comparison of th lowst point, drivd from th H1 prliminary masurmnt, with th nw ZEUS prliminary data prsntd at this confrnc will b of intrst. Th rsulting scaling violation trm κ appars to ris as x dcrass, xhibiting th ngativ and positiv scaling violations of F 2 for x abov and blow 0.1 rspctivly. Th rrors in Fig.6 rprsnt th statistical rrors of th fits. Both paramtrs a and κ ar anti-corrlatd as can b sn from nighbouring points. No significant Q 2 -dpndnc of a and κ has bn found in th publishd data whn th fits wr rpatd for two intrvals in Q 2 (abov and blow 20 GV 2 ). Λ 2 5

7 Figur 5: ZEUS and BCDMS masurmnts of th proton structur function F 2 ar shown as a function of Q 2 in th rang 10 4 < x < 1. Thy ar compard to th 2-paramtr fits according to q. (8) in ach x-bin. With a bing approximatly constant blow x 10 2, changs of F 2 at low x rsult from th scaling violation trm κ alon, indicativ of th intraction dynamics that drivs F 2 and in support of th prdictions [9, 10]. Th paramtr a has alrady bn idntifid as th charg squard wightd quark distributions xtrapolatd to ln (Q 2 /Λ 2 ) = 1 which corrsponds hr to Q 2 = 0.3 GV 2. An undrstanding of th paramtrs Λ and κ can b achivd by comparison with th QCD volution quation which is writtn hr in th lading ordr DGLAP approximation: df i (x, Q 2 ) = α s(q 2 ) d lnq 2 2π j 1 x dy y P ij ( ) x f j (y, Q 2 ). (9) y 6

8 sa quarks valnc quarks Figur 6: Th quark distribution a(x) of th proton xtrapolatd to Q 2 = 0.3 GV 2 and th scaling violations κ(x) from th fits to th publishd H1, ZEUS, BCDMS, and to th H1 prliminary data according to q. (8). Th dottd lins srv to guid th y. Hr f i, f j dnot th parton dnsitis, P ij ar th splitting functions, and is th strong coupling constant. α s = b ln (Q 2 /Λ 2 QCD ) (10) Th drivativ of th ansatz chosn hr, q. (8), with rspct to ln Q 2 givs df 2 (x, Q 2 ) d lnq 2 = 1 ln (Q 2 /Λ 2 ) κ(x) F 2(x, Q 2 ), (11) whr rlating 1/ ln(q 2 /Λ 2 ) with α s in q. (9) implis association of th scal paramtr Λ in q. (8) with th QCD paramtr Λ QCD. Th trm κ rlats to th sum ovr th diffrnt parton radiation trms in q. (9) dividd by F 2. κ incrass towards small x, consistnt with largr phas spac availabl for parton radiation. 7

9 Figur 7: Masurmnts of th photon structur function ar shown as a function of Q 2. Thy ar compard to th 2-paramtr fits according to q. (8) in ach x-bin. To match th dscription chosn hr, q. (8), with th doubl asymptotic approximation xpctd from QCD for th gluon-dominatd rgion at small x, F 2 xp ln x ln (ln (Q 2 /Λ 2 )) [9, 11], th scaling violation trm κ is rquird to hav a dpndnc lik ln x κ ln (ln (Q 2 /Λ 2 )). (12) Th Q 2 -dpndnc of κ is thrfor xpctd to b vry small which is in agrmnt with th xprimntal obsrvation statd abov. Mor prcis data and data raching smallr valus of x will dtrmin whthr or not th scaling violations furthr incras towards low-x and thrfor giv valuabl information on th parton dnsitis in th proton as x approachs 0. 4 Gnsis of Hadronic Structur: Photon Th photon structur rsults from fluctuations of a photon into a colour nutral and flavour nutral hadronic stat. For comparison with th proton data, th sam fits according to q. (8) hav bn applid to rcnt masurmnts of th photon structur function F γ 2 which hav bn prformd at + collidrs [12] (Fig.7). Th valus of th paramtrs a and κ ar shown in Fig.8 as th opn circls. Both paramtrs ar distinct from thos of a hadronic bound stat lik th proton: in a(x) th photon data xhibit no valnc quark structur. Instad, in th low-x rgion around x 0.1 th photon data prfr similar valus of a to th proton data for x Th scaling violations κ ar positiv at all valus of x and κ is approximatly 1. This is as xpctd from QCD calculations which prdict F γ 2 for 0.1 < x < 1 [13]. 8

10 Figur 8: Th hadronic structurs a(x), xtrapolatd to Q 2 = 0.3 GV 2, and th scaling violations κ(x) from fits to structur function data according to q. (8) ar compard btwn th proton, photon, and colour singlt xchang. Th diagrams of splitting functions indicat rgions thy contribut to th QCD volution. Th lins srv to guid th y. Judgmnt on a univrsal low-x bhaviour of hadronic structurs will rsult from mor prcis masurmnts and lowr-x data of th photon structur function. If th photon data show a constant quark dnsity at small x similar to th low-x proton data, scaling violations of F γ 2, which dviat from thos rsulting from th photon splitting into quark-antiquark pairs and approach thos obsrvd for th proton, could bcom visibl blow or slightly abov x = 10 2 whr also for th proton data it is κ 1. Intrsting information on th qustion of univrsality coms alrady from masurmnts of th gluon in th photon probd in strong intraction procsss in photon-proton collisions. Th production of two-jt vnts is snsitiv to th gluons dvloping in photon fluctuations. In Fig.9, a rcnt masurmnt of xg(x) is shown [14]. Th gluons appar as th low-x companions of th nwly built hadronic structur: at larg x th gluon dnsity is small; it riss towards small valus of x. 9

11 p p Figur 9: Comparison of th H1 photon and proton gluon distributions as a function of x. In th sam figur, this gluon distribution is compard to th gluon distribution of th proton, dtrmind from masurmnts of th proton structur function [8]. Although th rror bars of th photon masurmnt ar larg and Q 2 and p 2 t may not rprsnt th vry sam rsolution scal, th similarity of th nwly built and th alrady xisting gluon distribution is striking. This obsrvation may b a first xprimntal indication of a univrsal gluon distribution dvloping in hadronic structurs. 5 Colour Singlt Exchang Furthr information on gluons in hadronic structurs rsults from structur function masurmnts of colour singlt xchang. In Fig.10, H1 F D(3) 2 data [15] ar compard to th sam two-paramtr fits as usd abov, q. (8). Hr x (frquntly calld β) dnots th fractional momntum of th scattrd parton rlativ to th colour nutral objct, which itslf carris a fractional momntum ξ = rlativ to th proton and thrfor blongs to th low-x companions of th proton. Also ths data xhibit scaling violations κ that ar diffrnt from th proton masurmnts at th sam valus of x (Fig.8). Instad, for x < 0.5 thy hav th tndncy of bing largr than th photon data and ar similar to th low-x proton data. Th larg rat of vnts with colour singlt xchang togthr with th larg scaling violations of F D(3) 2 is suggstiv of a gluon dominatd xchang. 10

12 p Figur 10: H1 masurmnts of th structur function of colour singlt xchang ar shown as a function of Q 2. Thy ar compard to th 2-paramtr fits according to q. (8) in ach x-bin. Th valus of th normalization a ris towards x = 1 to about a = 10 (in Fig. 8, th paramtr a has bn scald by 1/25). Ths valus hav larg uncrtaintis of th ordr of 100%. If mor prcis data support such a singular parton dnsity for x 1 at low Q 2, thn ths colour nutral fluctuations consist of on gluon carrying ssntially all th colour singlt momntum and (at last) on furthr gluon with vry low momntum nutralizing th colour. 6 Prdictiv Powr for Proton Intraction Procsss Th proton structur rvals amazing simplicity: at low rsolution scal Q 2, th thr valnc quarks uud ach carry fractional momntum x = 1/3 (s sctions 2, 3). Th sa quark contribution is at low valus of x indpndnt of x (s sction 3). Gluons accompany th proton at low x with a possibly univrsal momntum distribution (s sction 4). Gluons initiat colour nutral configurations togthr with othr vry low momntum gluons (s sction 5). Howvr, to prdict intractions with protons, full information on all individual parton distributions of th proton ar rquird. Whil such parton distribution functions xf i hav bn availabl from global fits for many yars, rcnt pionring work has succdd in dtrmining th prcision of ths distribution functions taking into account th prcision of th masurmnts and corrlations btwn th diffrnt functions xf i [16] (Fig.11). This analysis shows a good knowldg of th functions xf i ovr a wid rang in x. Howvr, th knowldg for x 1 is not satisfactory: larg valus of x corrspond to high rsolution powr at hadron collidrs (.g. LHC) and point at th potntial discovry rgion for nw physics. An improvd dtrmination of th proton parton distribution as x approachs 1 by dp inlastic scattring xprimnts is thrfor mandatory and currntly is undr discussion [17]. 11

13 xq i d u x Figur 11: Parton distribution functions and d/u ratio as a function of x at Q 2 = 10 GV 2 from a global fit which taks into account xprimntal rrors and corrlations btwn th individual parton distribution functions. x Furthr qustions on th prdictiv powr of QCD calculations for proton-proton intractions rsult from th masurmnts of forward jt and forward π cross sctions in p collisions,.g. [18]. Ths masurmnts xplicitly tst QCD volution ovr som rapidity distanc and may signal limitations of th currnt approximations of QCD volution to simpl procss configurations at small distancs. Hr thortical work is ndd and ongoing. 7 Achivmnts and Challngs W currntly clbrat th 30 yars knowldg of valnc quarks in th proton. Th nw contribution of th HERA collidr xprimnts to th undrstanding of th proton is th low-x structur which appars as a consqunc of QCD dynamics. Opn qustions ar: is th parton dnsity of th proton finit as x 0? What is th parton dnsity at x 1? Is th QCD volution approximatd corrctly? Masurmnts on th gnsis procss of hadronic structurs us quantum fluctuations of th photon: sinc ovr 20 yars w know th momntum distributions of quarks rsulting from th photon splitting into quark-antiquark pairs. For th first tim, th HERA and LEP xprimnts hav masurd th gluon distribution of nwly built hadronic configurations, which is found to b vry similar to th gluon distribution masurd in protons. Th opn qustion to th photon data is: is hadronic structur at low x univrsal, i.., do th low-x partons know about th partons in th high-x rgion? Masurmnts of th partonic structur of colour singlt xchang at HERA and th TEVA- TRON [19] for th first tim show that such objcts dominantly consist of gluons. Will ths 12

14 masurmnts srv as a rfrnc procss for a gluon drivn rgim and offr nw insight into QCD dynamics? Major contributions of lpton-hadron scattring in th past 10 yars dpn our undrstanding of hadronic structurs. Burning opn qustions nsur that this fild of rsarch will rmain vry activ also in th coming dcad. Acknowldgmnts I wish to thank vry much th Livrpool tam for a wondrful confrnc! For carful rading and commnts to th manuscript I am gratful to E. Elsn and B. Fostr. I wish to thank Th. Müllr and th IEKP group of th Univrsity Karlsruh for thir hospitality, and th Dutsch Forschungsgminschaft for th Hisnbrg Fllowship. Rfrncs [1] H1 Collab., Masurmnt of th Chargd and Nutral Currnt Cross Sctions at HERA, contrib. papr 157b, Intrnational Europhysics Confrnc on High Enrgy Physics (HEP99), Tampr, Finland, 1999 [2] ZEUS Collab., Masurmnt of High Q 2 Nutral, Chargd Currnt Dp Inlastic Scattring Cross Sctions in p scattring at HERA, contrib. paprs 549, 558, Intrnational Europhysics Confrnc on High Enrgy Physics (HEP99), Tampr, Finland, 1999 [3] H1 Collab., C. Adloff t al., Eur. J. Phys. C 13, 609 (2000) [4] M. Erdmann, hp-x/ , Phys. Ltt. B 488, 131 (2000) [5] ZEUS Collab., M. Drrick t al., Z. Phys. C 72, 399 (1996) [6] BCDMS Collab., A.C. Bnvnuti t al., Phys. Ltt. B 223, 485 (1989) [7] H1 Collab., S. Aid t al., Nucl. Phys. B 470, 3 (1996) [8] M. Klin for th H1 Collab., hp-x/ , Proc. XIX Int. Symp. on Lpton and Photon Intractions at High Enrgis, Stanford, USA (1999) [9] A. D Rujula t al., Phys. Rv. D 10, 1649 (1974) [10] M. Glück, E. Rya, and A. Vogt, Z. Phys. C 53, 127 (1992) [11] R.D. Ball and S. Fort, Phys. Ltt. B 335, 77 (1994) [12] Photon structur function data from rviw by R. Nisius, hp-x/ , Phys. Rpt. 332, 165 (2000) [13] E. Wittn, Nucl. Phys. B 120, 189 (1977) 13

15 [14] H1 Collab., C. Adloff t al., Phys. Ltt. B 483, 36 (2000) [15] H1 Collab., C. Adloff t al., Z. Phys. C 76, 613 (1997) [16] M. Botj, hp-ph/ , Eur. J. Phys. C 14, 285 (2000) [17] Workshop on th Nuclon Structur in High x-bjorkn Rgion, HiX2000, Tmpl Univrsity, Jffrson Lab, Philadlphia, USA (2000) [18] H1 Collab., C. Adloff t al., Phys. Ltt. B 462, 440 (1999) [19] CDF Collab., T. Affoldr t al., Phys. Rv. Ltt. 84, 232 (2000) 14

Electroweak studies and search for new phenomena at HERA

Electroweak studies and search for new phenomena at HERA Elctrowak studis and sarch for nw phnomna at HERA A.F.Żarncki Warsaw Univrsity for ZEUS A.F.Żarncki Elctrowak studis and sarch for nw phnomna at HERA p./25 Outlin Introduction HERA and xprimnts A.F.Żarncki

More information

Searches for Contact Interactions at HERA

Searches for Contact Interactions at HERA Sarchs for Contact Intractions at HERA A.F.Żarncki Univrsity of Warsaw for ZEUS XVI Intrnational Workshop on Dp-Inlastic Scattring and Rlatd Subjcts 7- April 2008, Univrsity Collg London A.F.Żarncki Sarchs

More information

HERA - Structure of Matter and QCD

HERA - Structure of Matter and QCD HERA - Structur of Mattr and QCD p Contnts 5 yar running of HERA and H/ZEUS Elctrowak rsults Structur of th proton Katsuo Tokushuku (KEK, ZEUS) DESY/HERA HERA 99-7 H ZEUS HERA: (7.5GV lctron 9GVproton)

More information

Standard Model - Electroweak Interactions. Standard Model. Outline. Weak Neutral Interactions. Electroweak Theory. Experimental Tests.

Standard Model - Electroweak Interactions. Standard Model. Outline. Weak Neutral Interactions. Electroweak Theory. Experimental Tests. Standard Modl - Elctrowak Intractions Outlin ak Nutral Intractions Nutral Currnts (NC) Elctrowak Thory ± and Z and γ Discovry of ± Exprimntal Tsts LEP Z Boson Mass and idth Numbr of Nutrinos ± Boson ±

More information

Diffractive Dijet Production with Leading Proton in ep Collisions at HERA

Diffractive Dijet Production with Leading Proton in ep Collisions at HERA Diffractiv Dijt Production with Lading Proton in p Collisions at HERA JHEP [arxiv:150.01683] Radk Žlbčík Charls Univrsity Eric 015 Diffraction Th scattrd proton stays intact Exchang with vacuum quantum

More information

arxiv: v1 [hep-ex] 21 May 2013

arxiv: v1 [hep-ex] 21 May 2013 ELECTROWEAK RESULTS FROM HERA arxiv:5.98v [hp-x] May A.F. ŻARNECKI (on bhalf of th H and ZEUS collaborations) Faculty of Physics, Univrsity of Warsaw, Hoża 69, -68 Warszawa, Poland Nutral and chargd currnt

More information

DIS-Parity. Search for New Physics Through Parity Violation In Deep Inelastic Electron Scattering. The Physics Case

DIS-Parity. Search for New Physics Through Parity Violation In Deep Inelastic Electron Scattering. The Physics Case DIS-Parity Sarch for Nw Physics Through Parity Violation In Dp Inlastic Elctron Scattring Th Physics Cas R. Arnold for th DIS-Parity Collaboration Exprimnt Plan by Stv Rock will follow 12 Jun 2003 DIS-Parity

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

Forces. Quantum ElectroDynamics. α = = We have now:

Forces. Quantum ElectroDynamics. α = = We have now: W hav now: Forcs Considrd th gnral proprtis of forcs mdiatd by xchang (Yukawa potntial); Examind consrvation laws which ar obyd by (som) forcs. W will nxt look at thr forcs in mor dtail: Elctromagntic

More information

Neutrino Mass and Forbidden Beta Decays

Neutrino Mass and Forbidden Beta Decays NUCLEAR THEORY Vol. 35 016) ds. M. Gaidarov N. Minkov Hron Prss Sofia Nutrino Mass and Forbiddn Bta Dcays R. Dvornický 1 D. Štfánik F. Šimkovic 3 1 Dzhlpov Laboratory of Nuclar Problms JINR 141980 Dubna

More information

arxiv:hep-ph/ v1 21 May 1998

arxiv:hep-ph/ v1 21 May 1998 hp-ph/980540 VUTH 98-6 NIKHEF 98-0 FNT/T-98/04 SPIN PHYSICS WITH SPIN-0 HADONS arxiv:hp-ph/980540v May 998. JAKOB Univrsità di Pavia and INFN, Szion di Pavia, Via Bassi 6, I-700 Pavia, Italy, -mail:jakob@pv.infn.it

More information

Γ W. (GeV) 3. τ e universality in W decays

Γ W. (GeV) 3. τ e universality in W decays UCR/DØ/99-22 FERMILAB-CONF-99/39-E W and Z Proprtis at th Tvatron arxiv:hp-x/99137v1 18 Oct 1999 1 Introduction John Ellison (for th CDF and DØ Collaborations) Dpartmnt of Physics, Univrsity of California,

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

Extraction of Doping Density Distributions from C-V Curves

Extraction of Doping Density Distributions from C-V Curves Extraction of Doping Dnsity Distributions from C-V Curvs Hartmut F.-W. Sadrozinski SCIPP, Univ. California Santa Cruz, Santa Cruz, CA 9564 USA 1. Connction btwn C, N, V Start with Poisson quation d V =

More information

HERA. Marc DAVID. On behalf of. H1 and ZEUS COLLABORATIONS. luminosity that increases steadily from year to year. The positron beam energy E e is 27.

HERA. Marc DAVID. On behalf of. H1 and ZEUS COLLABORATIONS. luminosity that increases steadily from year to year. The positron beam energy E e is 27. OBSERVATION OF EVENTS AT HIGH Q 2 IN REACTIONS + p! + X AT HERA Marc DAVID CEA-Saclay,DSM/DAPNIA/SPP,99 Gif-sur-Yvtt,FRANCE On bhalf of and ZEUS COLLABORATIONS Both HERA colliding xprimnts, and ZEUS hav

More information

Outline. Thanks to Ian Blockland and Randy Sobie for these slides Lifetimes of Decaying Particles Scattering Cross Sections Fermi s Golden Rule

Outline. Thanks to Ian Blockland and Randy Sobie for these slides Lifetimes of Decaying Particles Scattering Cross Sections Fermi s Golden Rule Outlin Thanks to Ian Blockland and andy obi for ths slids Liftims of Dcaying Particls cattring Cross ctions Frmi s Goldn ul Physics 424 Lctur 12 Pag 1 Obsrvabls want to rlat xprimntal masurmnts to thortical

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

Why is a E&M nature of light not sufficient to explain experiments?

Why is a E&M nature of light not sufficient to explain experiments? 1 Th wird world of photons Why is a E&M natur of light not sufficint to xplain xprimnts? Do photons xist? Som quantum proprtis of photons 2 Black body radiation Stfan s law: Enrgy/ ara/ tim = Win s displacmnt

More information

Neutrino Physics. Caren Hagner, Universität Hamburg

Neutrino Physics. Caren Hagner, Universität Hamburg Nutrino Physics Carn Hagnr, Univrsität Hamburg What ar nutrinos? Nutrino mass and mixing Nutrino oscillations Nutrino bams: OPERA Oscillation of acclrator nutrinos Solar Nutrinos: BOREXINO (KamLAND ractor

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

Classical Magnetic Dipole

Classical Magnetic Dipole Lctur 18 1 Classical Magntic Dipol In gnral, a particl of mass m and charg q (not ncssarily a point charg), w hav q g L m whr g is calld th gyromagntic ratio, which accounts for th ffcts of non-point charg

More information

Hydrogen Atom and One Electron Ions

Hydrogen Atom and One Electron Ions Hydrogn Atom and On Elctron Ions Th Schrödingr quation for this two-body problm starts out th sam as th gnral two-body Schrödingr quation. First w sparat out th motion of th cntr of mass. Th intrnal potntial

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

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

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics NUCLEAR AND PARTICLE PHYSICS NET/JRF (JUNE-2011)

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics NUCLEAR AND PARTICLE PHYSICS NET/JRF (JUNE-2011) NUCLEAR AND PARTICLE PHYSICS NET/JRF (JUNE-) 64 Q. Th radius of a 9Cu nuclus is masurd to b 4.8 - cm. (A). Th radius of a 7 Mg nuclus can b stimatd to b.86 - cm (b) 5. - cm (c).6 - cm (d) 8.6 - cm (c)

More information

Title: Vibrational structure of electronic transition

Title: Vibrational structure of electronic transition Titl: Vibrational structur of lctronic transition Pag- Th band spctrum sn in th Ultra-Violt (UV) and visibl (VIS) rgions of th lctromagntic spctrum can not intrprtd as vibrational and rotational spctrum

More information

EXST Regression Techniques Page 1

EXST Regression Techniques Page 1 EXST704 - Rgrssion Tchniqus Pag 1 Masurmnt rrors in X W hav assumd that all variation is in Y. Masurmnt rror in this variabl will not ffct th rsults, as long as thy ar uncorrlatd and unbiasd, sinc thy

More information

The pn junction: 2 Current vs Voltage (IV) characteristics

The pn junction: 2 Current vs Voltage (IV) characteristics Th pn junction: Currnt vs Voltag (V) charactristics Considr a pn junction in quilibrium with no applid xtrnal voltag: o th V E F E F V p-typ Dpltion rgion n-typ Elctron movmnt across th junction: 1. n

More information

IV. e + e annihilation experiments 1. Experimental methods Discovery of the Tau-Lepton 5. hadrons 6. Hadronic resonances

IV. e + e annihilation experiments 1. Experimental methods Discovery of the Tau-Lepton 5. hadrons 6. Hadronic resonances IV. annihilation xprimnts 1. Exprimntal mthods. 3. 4. Discovry of th Tau-Lpton 5. (γ ) µ µ (γ ) hadrons 6. Hadronic rsonancs Lit.: H.U Martyn, Tst of QED in Quantum Elctrodynamics, T.Kinoshita (d.) 1.

More information

PHYSICS 489/1489 LECTURE 7: QUANTUM ELECTRODYNAMICS

PHYSICS 489/1489 LECTURE 7: QUANTUM ELECTRODYNAMICS PHYSICS 489/489 LECTURE 7: QUANTUM ELECTRODYNAMICS REMINDER Problm st du today 700 in Box F TODAY: W invstigatd th Dirac quation it dscribs a rlativistic spin /2 particl implis th xistnc of antiparticl

More information

High Energy Physics. Lecture 5 The Passage of Particles through Matter

High Energy Physics. Lecture 5 The Passage of Particles through Matter High Enrgy Physics Lctur 5 Th Passag of Particls through Mattr 1 Introduction In prvious lcturs w hav sn xampls of tracks lft by chargd particls in passing through mattr. Such tracks provid som of th most

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

Search for the Dark Photon at Belle for 0.27 < m A < 3 GeV/c 2

Search for the Dark Photon at Belle for 0.27 < m A < 3 GeV/c 2 Sarch for th Dark Photon at Bll for.7 < m A < 3 GV/c Igal Jagl Univrsity of Hawai i at Mānoa for th Bll Collaboration QCD, Montpllir, 6 Juillt BELLE Igal Jagl (UH) Sarch for th Dark photon at Bll QCD /

More information

Addition of angular momentum

Addition of angular momentum Addition of angular momntum April, 07 Oftn w nd to combin diffrnt sourcs of angular momntum to charactriz th total angular momntum of a systm, or to divid th total angular momntum into parts to valuat

More information

Davisson Germer experiment

Davisson Germer experiment Announcmnts: Davisson Grmr xprimnt Homwork st 5 is today. Homwork st 6 will b postd latr today. Mad a good guss about th Nobl Priz for 2013 Clinton Davisson and Lstr Grmr. Davisson won Nobl Priz in 1937.

More information

Davisson Germer experiment Announcements:

Davisson Germer experiment Announcements: Davisson Grmr xprimnt Announcmnts: Homwork st 7 is du Wdnsday. Problm solving sssions M3-5, T3-5. Th 2 nd midtrm will b April 7 in MUEN E0046 at 7:30pm. BFFs: Davisson and Grmr. Today w will go ovr th

More information

LEP Higgs Search Results. Chris Tully Weak Interactions and Neutrinos Workshop January 21-26, 2002

LEP Higgs Search Results. Chris Tully Weak Interactions and Neutrinos Workshop January 21-26, 2002 LEP Higgs Sarch Rsults Chris Tully Wak Intractions and Nutrinos Workshop January 1-6, 00 Viw of LEP Exprimnts Spontanous Symmtry Braking Higgs Fild 1-complx doublt Hyprcharg(Y) U(1) Y Symmtry Lft-Handd

More information

hep-lat/ Dec 93

hep-lat/ Dec 93 GLUON VERSUS MESON EXCHANGE IN HADRON-HADRON SYSTEMS ON THE LATTICE 1 H. MARKUM, K. RABITSCH, W. SAKULER Institut fur Krnphysik, Tchnisch Univrsitat Win A-100 Vinna, Austria hp-lat/931059 15 Dc 93 Th intraction

More information

Addition of angular momentum

Addition of angular momentum Addition of angular momntum April, 0 Oftn w nd to combin diffrnt sourcs of angular momntum to charactriz th total angular momntum of a systm, or to divid th total angular momntum into parts to valuat th

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

Studies of Turbulence and Transport in Alcator C-Mod Ohmic Plasmas with Phase Contrast Imaging and Comparisons with GYRO*

Studies of Turbulence and Transport in Alcator C-Mod Ohmic Plasmas with Phase Contrast Imaging and Comparisons with GYRO* Studis of Turbulnc and Transport in Ohmic Plasmas with Phas Contrast Imaging and Comparisons with GYRO* L. Lin 1, M. Porkolab 1, E.M. Edlund 1, J.C. Rost 1, M. Grnwald 1, D.R. Mikklsn 2, N. Tsujii 1 1

More information

Self-interaction mass formula that relates all leptons and quarks to the electron

Self-interaction mass formula that relates all leptons and quarks to the electron Slf-intraction mass formula that rlats all lptons and quarks to th lctron GERALD ROSEN (a) Dpartmnt of Physics, Drxl Univrsity Philadlphia, PA 19104, USA PACS. 12.15. Ff Quark and lpton modls spcific thoris

More information

Precision Standard Model Tests (at JLab)

Precision Standard Model Tests (at JLab) Prcision Standard Modl Tsts (at JLab) Xiaochao Zhng Jun 21st, 2018 Th Standard Modl of Particl Physics How should w sarch for nw physics? Prcision SM tsts at Jffrson Lab Qwak, PVDIS Mollr, 12 GV PVDIS

More information

Background: We have discussed the PIB, HO, and the energy of the RR model. In this chapter, the H-atom, and atomic orbitals.

Background: We have discussed the PIB, HO, and the energy of the RR model. In this chapter, the H-atom, and atomic orbitals. Chaptr 7 Th Hydrogn Atom Background: W hav discussd th PIB HO and th nrgy of th RR modl. In this chaptr th H-atom and atomic orbitals. * A singl particl moving undr a cntral forc adoptd from Scott Kirby

More information

On the Hamiltonian of a Multi-Electron Atom

On the Hamiltonian of a Multi-Electron Atom On th Hamiltonian of a Multi-Elctron Atom Austn Gronr Drxl Univrsity Philadlphia, PA Octobr 29, 2010 1 Introduction In this papr, w will xhibit th procss of achiving th Hamiltonian for an lctron gas. Making

More information

Higher order derivatives

Higher order derivatives Robrto s Nots on Diffrntial Calculus Chaptr 4: Basic diffrntiation ruls Sction 7 Highr ordr drivativs What you nd to know alrady: Basic diffrntiation ruls. What you can larn hr: How to rpat th procss of

More information

SCALING OF SYNCHROTRON RADIATION WITH MULTIPOLE ORDER. J. C. Sprott

SCALING OF SYNCHROTRON RADIATION WITH MULTIPOLE ORDER. J. C. Sprott SCALING OF SYNCHROTRON RADIATION WITH MULTIPOLE ORDER J. C. Sprott PLP 821 Novmbr 1979 Plasma Studis Univrsity of Wisconsin Ths PLP Rports ar informal and prliminary and as such may contain rrors not yt

More information

Principles of Humidity Dalton s law

Principles of Humidity Dalton s law Principls of Humidity Dalton s law Air is a mixtur of diffrnt gass. Th main gas componnts ar: Gas componnt volum [%] wight [%] Nitrogn N 2 78,03 75,47 Oxygn O 2 20,99 23,20 Argon Ar 0,93 1,28 Carbon dioxid

More information

Pair (and Triplet) Production Effect:

Pair (and Triplet) Production Effect: Pair (and riplt Production Effct: In both Pair and riplt production, a positron (anti-lctron and an lctron (or ngatron ar producd spontanously as a photon intracts with a strong lctric fild from ithr a

More information

2008 AP Calculus BC Multiple Choice Exam

2008 AP Calculus BC Multiple Choice Exam 008 AP Multipl Choic Eam Nam 008 AP Calculus BC Multipl Choic Eam Sction No Calculator Activ AP Calculus 008 BC Multipl Choic. At tim t 0, a particl moving in th -plan is th acclration vctor of th particl

More information

BETA DECAY VISUAL PHYSICS ONLINE

BETA DECAY VISUAL PHYSICS ONLINE VISUAL PHYSICS ONLINE BETA DECAY Suppos now that a nuclus xists which has ithr too many or too fw nutrons rlativ to th numbr of protons prsnt for stability. Stability can b achivd by th convrsion insid

More information

Cramér-Rao Inequality: Let f(x; θ) be a probability density function with continuous parameter

Cramér-Rao Inequality: Let f(x; θ) be a probability density function with continuous parameter WHEN THE CRAMÉR-RAO INEQUALITY PROVIDES NO INFORMATION STEVEN J. MILLER Abstract. W invstigat a on-paramtr family of probability dnsitis (rlatd to th Parto distribution, which dscribs many natural phnomna)

More information

Today. Wave-Matter Duality. Quantum Non-Locality. What is waving for matter waves?

Today. Wave-Matter Duality. Quantum Non-Locality. What is waving for matter waves? Today Wav-Mattr Duality HW 7 and Exam 2 du Thurs. 8pm 0 min rcap from last lctur on QM Finish QM odds and nds from ch.4 Th Standard Modl 4 forcs of Natur Fundamntal particls of Natur Fynman diagrams EM

More information

Properties of Quarks ( ) Isospin. π = 1, 1

Properties of Quarks ( ) Isospin. π = 1, 1 Proprtis of Quarks Isospin So far, w hav discussd thr familis of lptons but principally concntratd on on doublt of quarks, th u and d. W will now introduc othr typs of quarks, along with th nw quantum

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

Nuclear reactions The chain reaction

Nuclear reactions The chain reaction Nuclar ractions Th chain raction Nuclar ractions Th chain raction For powr applications want a slf-sustaind chain raction. Natural U: 0.7% of 235 U and 99.3% of 238 U Natural U: 0.7% of 235 U and 99.3%

More information

GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES. Eduard N. Klenov* Rostov-on-Don, Russia

GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES. Eduard N. Klenov* Rostov-on-Don, Russia GEOMETRICAL PHENOMENA IN THE PHYSICS OF SUBATOMIC PARTICLES Eduard N. Klnov* Rostov-on-Don, Russia Th articl considrs phnomnal gomtry figurs bing th carrirs of valu spctra for th pairs of th rmaining additiv

More information

Elements of Statistical Thermodynamics

Elements of Statistical Thermodynamics 24 Elmnts of Statistical Thrmodynamics Statistical thrmodynamics is a branch of knowldg that has its own postulats and tchniqus. W do not attmpt to giv hr vn an introduction to th fild. In this chaptr,

More information

de/dx Effectively all charged particles except electrons

de/dx Effectively all charged particles except electrons de/dx Lt s nxt turn our attntion to how chargd particls los nrgy in mattr To start with w ll considr only havy chargd particls lik muons, pions, protons, alphas, havy ions, Effctivly all chargd particls

More information

4. Money cannot be neutral in the short-run the neutrality of money is exclusively a medium run phenomenon.

4. Money cannot be neutral in the short-run the neutrality of money is exclusively a medium run phenomenon. PART I TRUE/FALSE/UNCERTAIN (5 points ach) 1. Lik xpansionary montary policy, xpansionary fiscal policy rturns output in th mdium run to its natural lvl, and incrass prics. Thrfor, fiscal policy is also

More information

The Relativistic Stern-Gerlach Force C. Tschalär 1. Introduction

The Relativistic Stern-Gerlach Force C. Tschalär 1. Introduction Th Rlativistic Strn-Grlach Forc C. Tschalär. Introduction For ovr a dcad, various formulations of th Strn-Grlach (SG) forc acting on a particl with spin moving at a rlativistic vlocity in an lctromagntic

More information

Radiation Physics Laboratory - Complementary Exercise Set MeBiom 2016/2017

Radiation Physics Laboratory - Complementary Exercise Set MeBiom 2016/2017 Th following qustions ar to b answrd individually. Usful information such as tabls with dtctor charactristics and graphs with th proprtis of matrials ar availabl in th cours wb sit: http://www.lip.pt/~patricia/fisicadaradiacao.

More information

Learning Spherical Convolution for Fast Features from 360 Imagery

Learning Spherical Convolution for Fast Features from 360 Imagery Larning Sphrical Convolution for Fast Faturs from 36 Imagry Anonymous Author(s) 3 4 5 6 7 8 9 3 4 5 6 7 8 9 3 4 5 6 7 8 9 3 3 3 33 34 35 In this fil w provid additional dtails to supplmnt th main papr

More information

Einstein Rosen inflationary Universe in general relativity

Einstein Rosen inflationary Universe in general relativity PRAMANA c Indian Acadmy of Scincs Vol. 74, No. 4 journal of April 2010 physics pp. 669 673 Einstin Rosn inflationary Univrs in gnral rlativity S D KATORE 1, R S RANE 2, K S WANKHADE 2, and N K SARKATE

More information

The DELPHI experiment at the LEP accelerator at the CERN laboratory

The DELPHI experiment at the LEP accelerator at the CERN laboratory Th DELPHI xprimnt at th LEP acclrator at th CERN laboratory Part 1. Th LEP acclrator Part 2. Th DELPHI xprimnt Part 3. Particl physics rsarch at LEP Th LEP acclrator Th study of collisions btwn lctrons

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

Introduction to the quantum theory of matter and Schrödinger s equation

Introduction to the quantum theory of matter and Schrödinger s equation Introduction to th quantum thory of mattr and Schrödingr s quation Th quantum thory of mattr assums that mattr has two naturs: a particl natur and a wa natur. Th particl natur is dscribd by classical physics

More information

Schrodinger Equation in 3-d

Schrodinger Equation in 3-d Schrodingr Equation in 3-d ψ( xyz,, ) ψ( xyz,, ) ψ( xyz,, ) + + + Vxyz (,, ) ψ( xyz,, ) = Eψ( xyz,, ) m x y z p p p x y + + z m m m + V = E p m + V = E E + k V = E Infinit Wll in 3-d V = x > L, y > L,

More information

DVCS and extraction of cross sections in Hall A

DVCS and extraction of cross sections in Hall A DVCS and xtraction of cross sctions in Hall A Eric FUCHEY Ph.D Studnt Laboratoir d Physiqu Corpusculair UMR 6533 CNRS/INP3 Unirsité Blais Pascal Clrmont Frrand Outlin Gnralizd Parton Distributions / DVCS

More information

Atomic energy levels. Announcements:

Atomic energy levels. Announcements: Atomic nrgy lvls Announcmnts: Exam solutions ar postd. Problm solving sssions ar M3-5 and Tusday 1-3 in G-140. Will nd arly and hand back your Midtrm Exam at nd of class. http://www.colorado.du/physics/phys2170/

More information

Brief Notes on the Fermi-Dirac and Bose-Einstein Distributions, Bose-Einstein Condensates and Degenerate Fermi Gases Last Update: 28 th December 2008

Brief Notes on the Fermi-Dirac and Bose-Einstein Distributions, Bose-Einstein Condensates and Degenerate Fermi Gases Last Update: 28 th December 2008 Brif ots on th Frmi-Dirac and Bos-Einstin Distributions, Bos-Einstin Condnsats and Dgnrat Frmi Gass Last Updat: 8 th Dcmbr 8 (A)Basics of Statistical Thrmodynamics Th Gibbs Factor A systm is assumd to

More information

Data Assimilation 1. Alan O Neill National Centre for Earth Observation UK

Data Assimilation 1. Alan O Neill National Centre for Earth Observation UK Data Assimilation 1 Alan O Nill National Cntr for Earth Obsrvation UK Plan Motivation & basic idas Univariat (scalar) data assimilation Multivariat (vctor) data assimilation 3d-Variational Mthod (& optimal

More information

5.80 Small-Molecule Spectroscopy and Dynamics

5.80 Small-Molecule Spectroscopy and Dynamics MIT OpnCoursWar http://ocw.mit.du 5.80 Small-Molcul Spctroscopy and Dynamics Fall 008 For information about citing ths matrials or our Trms of Us, visit: http://ocw.mit.du/trms. Lctur # 3 Supplmnt Contnts

More information

That is, we start with a general matrix: And end with a simpler matrix:

That is, we start with a general matrix: And end with a simpler matrix: DIAGON ALIZATION OF THE STR ESS TEN SOR INTRO DUCTIO N By th us of Cauchy s thorm w ar abl to rduc th numbr of strss componnts in th strss tnsor to only nin valus. An additional simplification of th strss

More information

There is an arbitrary overall complex phase that could be added to A, but since this makes no difference we set it to zero and choose A real.

There is an arbitrary overall complex phase that could be added to A, but since this makes no difference we set it to zero and choose A real. Midtrm #, Physics 37A, Spring 07. Writ your rsponss blow or on xtra pags. Show your work, and tak car to xplain what you ar doing; partial crdit will b givn for incomplt answrs that dmonstrat som concptual

More information

Chemical Physics II. More Stat. Thermo Kinetics Protein Folding...

Chemical Physics II. More Stat. Thermo Kinetics Protein Folding... Chmical Physics II Mor Stat. Thrmo Kintics Protin Folding... http://www.nmc.ctc.com/imags/projct/proj15thumb.jpg http://nuclarwaponarchiv.org/usa/tsts/ukgrabl2.jpg http://www.photolib.noaa.gov/corps/imags/big/corp1417.jpg

More information

The Matrix Exponential

The Matrix Exponential Th Matrix Exponntial (with xrciss) by D. Klain Vrsion 207.0.05 Corrctions and commnts ar wlcom. Th Matrix Exponntial For ach n n complx matrix A, dfin th xponntial of A to b th matrix A A k I + A + k!

More information

Event shapes and subjet distributions at HERA

Event shapes and subjet distributions at HERA Evnt shaps and subjt distributions at HERA arxiv:hp-x/5v Dc 5 C. Glasman (on bhalf of th Collaboration) Univrsidad Autónoma d Madrid, Spain Abstract Rcnt rsults on subjt distributions from ar prsntd. h

More information

Determination of Vibrational and Electronic Parameters From an Electronic Spectrum of I 2 and a Birge-Sponer Plot

Determination of Vibrational and Electronic Parameters From an Electronic Spectrum of I 2 and a Birge-Sponer Plot 5 J. Phys. Chm G Dtrmination of Vibrational and Elctronic Paramtrs From an Elctronic Spctrum of I 2 and a Birg-Sponr Plot 1 15 2 25 3 35 4 45 Dpartmnt of Chmistry, Gustavus Adolphus Collg. 8 Wst Collg

More information

General Notes About 2007 AP Physics Scoring Guidelines

General Notes About 2007 AP Physics Scoring Guidelines AP PHYSICS C: ELECTRICITY AND MAGNETISM 2007 SCORING GUIDELINES Gnral Nots About 2007 AP Physics Scoring Guidlins 1. Th solutions contain th most common mthod of solving th fr-rspons qustions and th allocation

More information

A Prey-Predator Model with an Alternative Food for the Predator, Harvesting of Both the Species and with A Gestation Period for Interaction

A Prey-Predator Model with an Alternative Food for the Predator, Harvesting of Both the Species and with A Gestation Period for Interaction Int. J. Opn Problms Compt. Math., Vol., o., Jun 008 A Pry-Prdator Modl with an Altrnativ Food for th Prdator, Harvsting of Both th Spcis and with A Gstation Priod for Intraction K. L. arayan and. CH. P.

More information

Coupled Pendulums. Two normal modes.

Coupled Pendulums. Two normal modes. Tim Dpndnt Two Stat Problm Coupld Pndulums Wak spring Two normal mods. No friction. No air rsistanc. Prfct Spring Start Swinging Som tim latr - swings with full amplitud. stationary M +n L M +m Elctron

More information

First derivative analysis

First derivative analysis Robrto s Nots on Dirntial Calculus Chaptr 8: Graphical analysis Sction First drivativ analysis What you nd to know alrady: How to us drivativs to idntiy th critical valus o a unction and its trm points

More information

ELECTRON-NEUTRINOS, v e. G. R. Kalbfleisch Brookhaven National Laboratory ABSTRACT

ELECTRON-NEUTRINOS, v e. G. R. Kalbfleisch Brookhaven National Laboratory ABSTRACT -1- SS -121 2251 ELECTRON-NEUTRINOS, v G. R. Kalbflisch Brookhavn National Laboratory ABSTRACT Elctron (rathr than muon) nutrino intractions ar proprly th ons to us in comparing rsults with -p intractions.

More information

Homotopy perturbation technique

Homotopy perturbation technique Comput. Mthods Appl. Mch. Engrg. 178 (1999) 257±262 www.lsvir.com/locat/cma Homotopy prturbation tchniqu Ji-Huan H 1 Shanghai Univrsity, Shanghai Institut of Applid Mathmatics and Mchanics, Shanghai 272,

More information

The failure of the classical mechanics

The failure of the classical mechanics h failur of th classical mchanics W rviw som xprimntal vidncs showing that svral concpts of classical mchanics cannot b applid. - h blac-body radiation. - Atomic and molcular spctra. - h particl-li charactr

More information

Collisions between electrons and ions

Collisions between electrons and ions DRAFT 1 Collisions btwn lctrons and ions Flix I. Parra Rudolf Pirls Cntr for Thortical Physics, Unirsity of Oxford, Oxford OX1 NP, UK This rsion is of 8 May 217 1. Introduction Th Fokkr-Planck collision

More information

Gamma-ray burst spectral evolution in the internal shock model

Gamma-ray burst spectral evolution in the internal shock model Gamma-ray burst spctral volution in th intrnal shock modl in collaboration with: Žljka Marija Bošnjak Univrsity of Rijka, Croatia Frédéric Daign (Institut d Astrophysiqu d Paris) IAU$Symposium$324$0$Ljubljana,$Sptmbr$2016$

More information

Einstein Equations for Tetrad Fields

Einstein Equations for Tetrad Fields Apiron, Vol 13, No, Octobr 006 6 Einstin Equations for Ttrad Filds Ali Rıza ŞAHİN, R T L Istanbul (Turky) Evry mtric tnsor can b xprssd by th innr product of ttrad filds W prov that Einstin quations for

More information

Answer Homework 5 PHA5127 Fall 1999 Jeff Stark

Answer Homework 5 PHA5127 Fall 1999 Jeff Stark Answr omwork 5 PA527 Fall 999 Jff Stark A patint is bing tratd with Drug X in a clinical stting. Upon admiion, an IV bolus dos of 000mg was givn which yildd an initial concntration of 5.56 µg/ml. A fw

More information

Brief Introduction to Statistical Mechanics

Brief Introduction to Statistical Mechanics Brif Introduction to Statistical Mchanics. Purpos: Ths nots ar intndd to provid a vry quick introduction to Statistical Mchanics. Th fild is of cours far mor vast than could b containd in ths fw pags.

More information

EFFECT OF BALL PROPERTIES ON THE BALL-BAT COEFFICIENT OF RESTITUTION

EFFECT OF BALL PROPERTIES ON THE BALL-BAT COEFFICIENT OF RESTITUTION EFFECT OF BALL PROPERTIES ON THE BALL-BAT COEFFICIENT OF RESTITUTION A. M. NATHAN 1 AND L. V. SMITH 2 1 Univrsity of Illinois, 1110 W. Grn Strt, Urbana, IL 61801, USA, E-mail: a-nathan@illinois.du 2 Washington

More information

Intro to Nuclear and Particle Physics (5110)

Intro to Nuclear and Particle Physics (5110) Intro to Nuclar and Particl Physics (5110) March 09, 009 Frmi s Thory of Bta Dcay (continud) Parity Violation, Nutrino Mass 3/9/009 1 Final Stat Phas Spac (Rviw) Th Final Stat lctron and nutrino wav functions

More information

The Matrix Exponential

The Matrix Exponential Th Matrix Exponntial (with xrciss) by Dan Klain Vrsion 28928 Corrctions and commnts ar wlcom Th Matrix Exponntial For ach n n complx matrix A, dfin th xponntial of A to b th matrix () A A k I + A + k!

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

Pipe flow friction, small vs. big pipes

Pipe flow friction, small vs. big pipes Friction actor (t/0 t o pip) Friction small vs larg pips J. Chaurtt May 016 It is an intrsting act that riction is highr in small pips than largr pips or th sam vlocity o low and th sam lngth. Friction

More information

Cosmology and particle physics

Cosmology and particle physics Cosmology and particl physics Lctur nots Timm Wras Lctur 8 Th thrmal univrs - part IV In this lctur w discuss th Boltzmann quation that allows on to dscrib th volution of procsss in our univrs that ar

More information

Part 7: Capacitance And Capacitors

Part 7: Capacitance And Capacitors Part 7: apacitanc And apacitors 7. Elctric harg And Elctric Filds onsidr a pair of flat, conducting plats, arrangd paralll to ach othr (as in figur 7.) and sparatd by an insulator, which may simply b air.

More information

10. The Discrete-Time Fourier Transform (DTFT)

10. The Discrete-Time Fourier Transform (DTFT) Th Discrt-Tim Fourir Transform (DTFT Dfinition of th discrt-tim Fourir transform Th Fourir rprsntation of signals plays an important rol in both continuous and discrt signal procssing In this sction w

More information

Exam 1. It is important that you clearly show your work and mark the final answer clearly, closed book, closed notes, no calculator.

Exam 1. It is important that you clearly show your work and mark the final answer clearly, closed book, closed notes, no calculator. Exam N a m : _ S O L U T I O N P U I D : I n s t r u c t i o n s : It is important that you clarly show your work and mark th final answr clarly, closd book, closd nots, no calculator. T i m : h o u r

More information