The United States Nuclear Regulatory Commission and Duke University Present: Regulatory and Radiation Protection Issues in Radionuclide Therapy

Size: px
Start display at page:

Download "The United States Nuclear Regulatory Commission and Duke University Present: Regulatory and Radiation Protection Issues in Radionuclide Therapy"

Transcription

1 Th Unitd Stats Nuclar Rgulatory Commission and Duk Univrsity Prsnt: Rgulatory and Radiation Protction Issus in Radionuclid Thrapy Copyright 008 Duk Radiation Safty and Duk Univrsity. All Rights Rsrvd.

2 Wlcom! This is th svnth of a sris of training moduls in Radiation Physics. Ths moduls provid a basic introduction to radiation physics and th intraction of radiation with mattr. Sponsord by th Unitd Stats Nuclar Rgulatory Commission and Duk Univrsity Author: Dr. Rathnayaka Gunasingha, PhD

3 Your Instructor Dr. RathnayakaGunasinghais an Acclrator Physicist with background in High Enrgy physics. Dr. Gunasinghais a physicist in th Radiation Safty division and mmbr of th Faculty of th Duk Mdical Physics Graduat Program. Contact: rathnayaka.gunasingha@duk.du

4 Goals of th Cours Upon complting ths instructional moduls, you should b abl to: undrstand th Basic Intraction of Radiation with Mattr apply th knowldg in various calculations usd in Mdical and Halth Physics undrstand th basic principls bhind various instrumntation usd in Mdical and Halth Physics

5 This Modul Will Covr Soft Collision s or Inlastic Collisions Hard Collisions Inlastic Collisions with nuclus Elastic Collisions with nuclus Bth-Bloch Formula Stopping powr, Rang, Stopping Tim

6 Intraction of Chargd Particls with Mattr Whn a chargd particl ntrs into a mdium, it intracts with lctrons and nucli in th mdium Ths intractions ar calld "collisions" btwn chargd particls and th atomic lctrons and nucli. Th collisions ar lad to th (a) Ionizations - productions of ion-lctron pairs, and (b) Excitations - raising th nrgy of th oribital lctrons into highr stats in th atom

7 Intraction of Chargd Particls with Mattr A chargd particl is calld havy, if its mass is gratr than th rst mass of th lctron xampls: alpha, muon, proton and som fission products A havy chargd particl losss a ngligibl amount of nrgy in a collision with nuclus In this lsson, w nglct th nuclar forcs, and considr only lctromagntic forc ( Coulomb forc) btwn th chrgd particl and th lctrons

8 Intraction of Chargd Particls with Mattr Dpnding on th rlativ siz of th impact paramtr b (i.. shortst distanc btwn th cntr of th atom and th path of th chargd particl), and th radius of th atom a, w can considr four typs of intractions. Q chargd particl b impact paramtr a

9 Intraction of Chargd Particls with Mattr Four typs of intractions: (a). Inlastic or soft collisions ( b >>> a) (b). Hard collsions ( b a) (c). Inlastic collsions with a nuclus ( b << a) (d). Elastic collisions with a nuclus ( b << a)

10 Inlastic or soft collisions ( b>>>a) In this typ, th Coulomb forc du to moving particl affcts th atom as a whol, lading to xcitation of th atomic lctrons or ionization of th atom Largr valus of b ar mor probabl than th nar hits for a chargd particl and thrfor many soft collisions occur This is th main procss of intractions with mattr nrgy transfr for chargd particl

11 Inlastic or soft collisions ( b>>>a) In th procss of soft collisions, whn th vlocity of v p c n and ( βc), xcds th spd of chargd particl light in th mdium with rfractiv indx n,, a small amount of absorbd nrgy is rlasd as photons. this radiation is calld"crnkov ~ Radiation".

12 Crnkov Radiation At tim t 0, particl is at O at t t, particl is at O distanc travlld by th wav front, distanc travlld by th particl, ct OM n OO βct Crnkov ~ photons form a particl. cosθ ct n βct wav front of βn half angl ( 90-θ), bhind th

13 Hard Collisions( b ~ a) Whn b a, chargd particl can xrt an impuls which is nough to jct an lctron from th atom. This jctd lctron is calld a " δ - ray"and it carris kintic nrgy lost by th chargd particl. In th collision, atomic lctron is tratd as "fr" δ - ray has nough nrgy to undrgo its its nrgy along a sprat track own intractions, and losss

14 Inlastic collisions with a nuclus (b<<a) In this typ, Coulomb forc intraction is th nuclus mainly with If th particl is an lctron, Brmstrahlung can occur If b < nuclar radius and chargd particl has nough nrgy, inlastic intraction with th nuclus can lav th nuclus in th xcitd stat. xcitd nuclus thn dcays by mission of nuclons or γ rays.

15 Elastic collisions with a nuclus This typ of intractions ar known as Ruthrford scattring. Thr is no xcitation or radiation. Particl losss nrgy through rcoil of th nuclus

16 Enrgy transfr in a singl collision Considr a havy particl of with an lctron ( mass m ) mass M, vlocity V, collids Assumptions : a. havy particl movs rapidly compard to lctrons orbiting spd ( lctron is considrd fr) b. Enrgy transfr is largr than th binding nrgy of th lctron ( collsion is lastic)

17 Enrgy transfr in a singl collision M, V m M, V m, v BEFORE Collision AFTER Collision Consrvation of MV MV MV MV m v Elastic Collision, consrvation of + Solving (.) and (.) linar momntum + V m v (.) nrgy (.) ( M m ) ( M + m ) V

18 Enrgy transfr in a singl collision Max. Enrgy transfr to th lctron max Q max MV MV whr E 4mM Q. ( M + m ) ( M + m ) ( M + m ) MV kintic nrgy of MV m 4m M ME V havy particl

19 Enrgy transfr in a singl collision If incidnt particl, Q Q max m 500 4m E V If incidnt particl, proton max lctron 3 m V M M E m 836 m

20 Enrgy transfr in a singl collision Rlativistic cas Q m max Q m γ V Q max m M << M m γ V m γ + + M γ β γ β β m c whr, max V c

21 Intractions of Chargd Particls with Mattr Considr a particl of mass M, charg straight lin with vlocity v. z moving along a M Q z x O v b impact paramtr Elctron is at O r y θ b q Q z q x O

22 Intractions of Chargd Particls with Mattr kqq Coulomb forc F r Whn a particl passs O', F and no nt motion of kqq nt forc on lctron, F cosθ r momntum impartd to th lctron dp F dt p cosθ b r ; F dt dx dt x x υ ; kz r tanθ x lctron along x - dirction cosθ dt x b componnt of ; sc θ dθ forc rvrs dx b vdt b ; dt bsc θ dθ υ

23 Intractions of Chargd Particls with Mattr ( ) Th nrgy transfrd to th lctron, cos sc. cos sc b m V k z E m b V k z m p E Vb zk p d b kz d b b kz p π π π π θ θ υ θ υ θ θ θ

24 Intractions of Chargd Particls with Mattr x m c b k z m p E c b zk p p E dy c V 4 Enrgy transfr to th lctron, Kintic unchangd is incrasd by factor dcrasd by a Rlativistic Cas β β γ γ β

25 Intractions of Chargd Particls with Mattr This nrgy is dtrmind by b db b p dx Probability that nrgy lost btwn E, E + de is givn by probability that b b, b + db b E b + db E + de thn P( E) de p '( b) db ( b incras rsults dcras in E)

26 Intractions of Chargd Particls with Mattr ZN A p ( E) de πbdb ρdx, A ZN A whr ρdx is th numbr of lctrons pr unit ara A b p( E) de 4 z k β m c E p( b) db Man nrgy loss dt πzn Aρdxk z β m c A dt 4 bdb E E max min E [ ln E ] max 4 z k β m c 4 πzn Aρdx z k A β m c E P( E) de E min de E de E

27 Intractions of Chargd Particls with Mattr Dfin constant C πn dt m c C β Whn E to priod of lctron in atomic orbit τ < f rot kzz bv min from ρ ( b F Zz A max max y kzz b A k m c Emax ( ρdx)[ ln E] C ( ρdx)[ lnb] ) collision is soft and collision tim shortr compard but τ τ γ τ τ b γβc 4 b γβc 4 E min m c β Zz A b b max min

28 Intractions of Chargd Particls with Mattr b γβc b γβc b max < < f h I rot γβch I hf rot I h plank constant man ionization potntial

29 Intractions of Chargd Particls with Mattr b min : to M At th rst fram, lctron movs with βc with rspct Minimum valu of b, (uncrtainity principl dos not allow b Brogli's chargd particl) is quivalnt wav lngth in th rlativ coordinat systm of b min h p h ( m C) cγβ to th d Brogli wav lngth to b mor prcis than d and

30 Intractions of Chargd Particls with Mattr Substituting, mc dt C β According to this quation : (a.) (b.) dt dt kintic nrgy of b dt mc C β Zz A Zz A ( ρdx) ( ρdx) γ ln havy particl γβch mγβc ln. I h β m C I c

31 Stopping Powr Considr any chargd particl of typ Y and kintic nrgy T, in a mdium of atomic numbr Z Th xpctation valu of th rat of nrgy loss pr unit lngth is calld th stopping powr dt is th nrgy loss in stopping powr dx, thn dt dx Y, T, Z Units: MV. cm or J. m

32 Mass Stopping Powr Dividing th stopping powr, by th dnsity of th mdium is calld Mass Stopping Powr mass stopping powr dt ρdx units: Mv. cm g

33 Stopping Powr Dpnding on th nrgy lost by chargd particls, stopping powr is subdividd into two:. Collision stopping powr: rat of nrgy loss from th sum of soft and hard collisions ( collision intractions). Radiativ stopping powr: rat of nrgy loss from radiativ intractions. i.. mainly from brmstrahlung productions

34 Bth Formula for dt/dx Using rlativistic quantum mchanics (assuming havy particl vlocity [ v βc]is much gratr than th Bohr - orbit vlocity of atomic lctron) Bth drivd th following hard collisions) whr dt ρdx K m C K ln I Cm c β z formula (combining soft and ( β ) β β C N π A A k 4 ( z) ( ) m c

35 Bth Formula for dt/dx Substituting valus for N, π, K, m c K Zz Aβ a MV cm g Th trms in th brackts ar unitlss; I and m c sould b in V dt Zz β ln ( m c ) + ln ln ( I ) ρ dx Aβ β β dt Zz β ln ln + ( I ) β ρ dx Aβ β z atomic numbr of th particl Z atomic numbr of th mdium A mass numbr of mdium

36 Important faturs of this formula Man ionization potntial I ( ) V (xitation nrgy) dfind as th gomtric man valu of all ionizations and xitation potntials of an atom in th absorbing mdium I is calculatd using th quation for dt. Also it can b ρ dx dt masurd if all othr quantitis in ar known ρ dx

37 Important faturs of this formula Logarithm of I is ntrd in abov formula. Thrfor following approximat mpirical valus can b usd to stimat I in V. I 9.0 ( V ) Z Z (V) Z Z ( V ) Z > 3

38 Important faturs of this formula I for a compound or mixtur considr th individual contribution from with lmnt thn, nln N ( I ) Z N ln( I ) i n atoms cm N i Z i i i -3 i for i th lmnt with and and ach total numbr of lctrons in th mixtur Z i Z i I i For a pur compund n, n i z i rplacd by lctron numbrs

39 Important faturs of this formula Exampl : ( ) Calculat I for watr H O. I H 9 V I V n 0 N N n ln I N Z ln I i i 0ln I ln ln V H ( ( )) ( )

40 Important faturs of this formula Exampl: Solution : dt Zz β ln dx A β ρ β β For proton z watr Z 0 A 8 ρ at ρ dt dx dt dx Calculat th mass collision stopping powr of for MV MV protons. 0 8β β β ln β β MV cm g ln I ln watr ( I ) V

41 Dpndnc on th mdium dt Zz β + ρ dx Aβ β ln β ln ( I ) Z Whn Z (mdium) is incrasd, numbr of lctrons pr unit mass A dcrasd ( I ) Whn Z incrasd ln incrasd ; dt Thrfor dcrasd. ρdx

42 Dpndnc on particl vlocity Whn v incrass, β incrass. Bcaus of β brackt dt ρdx dcrass outsid of th Whn particl charg z incrass dt ρdx incrass

43 Dpndnc on particl mass Particl mass dos not appar in dt ρdx formula. So, dt ρdx dos not dpnd on particl mass.

44 Rlation btwn kintic nrgy T and β (Rlativistic scaling) ( ) -. is connctd to th paramtr mass rst particl of a of how th kintic nrgy Following shows c M T c M T c M T c M T c M c M T M T β β β β β γ β

45 Rlativistic Scaling Particl Rst mass for som havy particls Mc ( MV) Z muon pion proton nutron dutron α

46 Rlation btwn kintic nrgy T and β (Rlativistic scaling) For any two particls A and nrgis, T T A B M M ( γ ) ( γ ) which givs th rlation, A B c c B, for a givn valu β, T T A B M M A B kintic i.. If two particls travl at th sam spd, thir ratio of kintic nrgis ar proportional to th ratios of thir rst masss.

47 Minimum ionizing particls Variation figur. of dt ρdx with T, for som particls is shown in

48 Minimum ionizing particls dt Th valu of for many diffrnt particls approachs a constant ρdx broad minimum valu at highr nrgis. dt ρdx For light matrials thus valu corrsponds to MV. cm g. Bcaus of thir similar nrgy loss bhavior, ths rlativ particls ar calld "Minimum Ionizing Particls"

49 Shll Corrction trm In Born approximation, vlocity of passing gratr than that of atomic lctrons. particl is much K - shll lctron of atom has th highst vlocity. th highst nrgy and hnc Whn passing particl vlocity falls blow, K - shll vlocity, thn K - shll lctrons do not contribut to dt ρdx.

50 Shll Corrction trm Corrctd for combind ffct of all i shlls into a singl trm C Z β + ρdx Aβ β Z dt Zz C ln ln β ( I ) Anothr corrction is th δ ( β ), which is a function of β and dilctric constant of mdium, is known as "dnsity ffct" or "polarization ffct" and important for dns mdia such as solid. It is ngligibl for havy chargd particls.

51 Rang Considr a charg particl ntring into a mdium with kintic nrgy T0. Thn th avrag valu of th distancs ( l) coming to rst, is calld th "Rang". that a particl travls bfor A B T 0 l t f

52 Projctd Rang Avrag valu of th farthst dpth of pntration of th particl in its initial dirction is calld th "Projctd Rang". units g.cm t f Th rciprocal of th mass stopping powr is usd to calculat th rang. Thn, T 0 0 dt Rang R( T ) dt, T0 strating nrgy of th particl ρdx units: g.cm

53 Projctd Rang This quantity is somtims mntiond as Continuous Slowing Down Approximation (CSDA) rang. dt Using th valu for in th dfinition of ρdx a rlation for R in th following way, rang R, w can driv dt ρdx Zz Aβ β ln β β ln I 0 R T dt 0 dt ρdx z dt ' G( β )

54 Projctd Rang ( ) ( ) th havy particl. th rang of givs and, function of a is ) ( ) ( ) ( Thn,. of ar functions ) and g( ) ( whr ) ( Sinc, 0 R f f z M d G g z M R G d Mg dt Mc Mc T β β β β β β β β β β β β γ β

55 Projctd Rang ( ) For two havy paricls A M, z and B( M, z ) with th A A B B sam vlocity, th ratio of thir rangs R and R is givn by, A B R A M A z B RB M B za If w know th rang of particl A, thn w can find th rang partilc B using this formula.

56 Projctd Rang 3 + Exampl: Find rang for 40 MV H ions in watr H Z M 3 T 40 MV 3 + p Z M T? T T A B M M A B MV H corrsponds to 3.3 MV proton which has a rang R p ( β ) 0.93 g.cm 3 40 T 3 RA M A Z B RH 3 RB M B Z A Rp 4 R H T T H 0.45 g.cm p R H p 0.93 ( 3 ) 4

57 Projctd Rang What w hav larnd All particls with sam vlocity ( β ) hav kintic nrgis in proportion to thir rst mass T T A B M M A B All singlly chargd havy particls with sam β, hav sam stopping powr Rang of singlly chargd particls of sam β, ar proportional to thir rst masss RA M A z B RB M B za

58 Stopping Tim Stopping tim ( Slowing down tim): Tim takn by a havy chargd particl to stop in th mattr Slowing down for a chargd particl in a mdium, can b calculatd using th rat of nrgy loss. By using th chain rul of diffrntiation, an xprssion for rat of nrgy loss can b drivd as follows, dt dt ρdx dt dt ( ρv) ρv dt ρdx dt ρ dx ρdx

59 Stopping Tim Thn, assuming th rat of nrgy loss is constant, slowing down tim is givn by, T T t dt dt ρv dt ρdx If kintic nrgy T is givn, valu for v can b found using th rlation btwn T and β.

60 Stopping Tim Exampl: Calculat th slowing down tim for 0 MV protons in watr. dt dt ρ gcm ; T 0 MV ; 45.9 MVcm g vρ dt ρdx -3 at 0 MV, β v c dt c MV s dt stimat stopping tim t is 0 MV 0 0 t 5 0 dt dt.99 0 ρv ρdx dt - s

61 Bragg Curv A plot of rat of nrgy loss along a track of a chargd particl is known as "Bragg Curv". Figur shows a bragg curv for a particl. /ρ(dt/dt) or (de/dx) Distanc of pntration

62 Bragg Curv Bragg curv is a consqunc of β dpndnc of stopping powr. A pak occurs at th nd of th track, bcaus th intraction cross sction incrass as th th particl vlocity dcrass. At th nd of and th curv falls off th track, charg is rducd through lctron pickup, Maximum nrgy loss occurs at th nd of th track

63 Enrgy Straggling Enrgy loss by a havy chargd particl collision in a statistical or stochastic procss. mdium is a Whn mononrgtic bam of particls passs through a mdium, a sprad of nrgis rsults around th avrags as it passs a givn dpth. This unqual nrgy losss for th bam of calld "Enrgy Straggling". similar condition is

64 Enrgy Straggling Figur shows th nrgy distribution of mononrgtic chargd particls at various points along its path. First portion, nrgy distribution bcoms widr with distanc. At th nd of th track distribution narrows, sinc th particl has lss nrgy.

65 Rang Straggling Fluctuation of path lngth of individual particls of th sam nrgy is calld "Rang Straggling". Following stup, a dtctor and an absorbr of changabl thicknss can b usd to dtrmin th "Rang Straggling". Sourc I/I 0 Dt 0.5 t R m R t

66 Rang Straggling In figur, w dfin two rangs: Man Rang and th Extrapolat Rang. Man Rang ( ): Th valu of th absorbr thicknss at which rlativ count I rat 0.5 is dfind as man rang. I 0 R m R Extrapolat Rang( ) : Th valu of thicknss obtaind by xtrapolating th linar portion of th nd of th curv, is calld th xtrapolat rang.

67 Scaling Laws ( Bragg-Klman s Rul) dt Som tims Rang (R) or stopping powr ar not availabl ρdx for mixturs. Assuming stopping powr pr atom of compound is additiv, w can dfin th stopping powr for a compound, by dt dti Wi N dx i N dx c c i i dt stopping powr N atomic dnsity Wi wight fraction dx

68 Scaling Laws ( Bragg-Klman s Rul) Rang for a compound or a mixtur is givn by : M c Rc A i ni R i R Rang of lmnts, n numbr of atoms of lmnt i in A i Atomic wight M c th molcul molcular wight

69 Scaling Laws ( Bragg-Klman s Rul) Whn Rang data is not availabl for on lmnt, w can us th valu of a known rang. if R is known and R is unknown, R R ρ ρ A A ρ dnsity, i A i atomic wight of absorbing matrial

70 Crdits and Rfrncs Attix, F.H: Introduction to th Radiological Physics and Radiation Dosimtry, Wily-VCH

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

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

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

(most) due to long range e m forces i.e. via atomic collisions or due to short range nuclear collisions or through decay ( = weak interactions)

(most) due to long range e m forces i.e. via atomic collisions or due to short range nuclear collisions or through decay ( = weak interactions) Spring 01, P67, YK Monday January 30, 01 8 Obsrvabl particl dtction ffcts ar : (most) du to long rang m forcs i.. via atomic collisions or du to short rang nuclar collisions or through dcay ( = wak intractions)

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

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

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

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

Precise Masses of particles

Precise Masses of particles /1/15 Physics 1 April 1, 15 Ovrviw of topic Th constitunts and structur of nucli Radioactivity Half-lif and Radioactiv dating Nuclar Binding Enrgy Nuclar Fission Nuclar Fusion Practical Applications of

More information

ECE507 - Plasma Physics and Applications

ECE507 - Plasma Physics and Applications ECE507 - Plasma Physics and Applications Lctur 7 Prof. Jorg Rocca and Dr. Frnando Tomasl Dpartmnt of Elctrical and Computr Enginring Collisional and radiativ procsss All particls in a plasma intract with

More information

26-Sep-16. Nuclear energy production. Nuclear energy production. Nuclear energy production. Nuclear energy production

26-Sep-16. Nuclear energy production. Nuclear energy production. Nuclear energy production. Nuclear energy production Aim: valuat nrgy-gnration rat pr unit mass. Sun: (chck L /M, human ) nrgy-gnration rat producd from fusion of two nucli a + A: nrgy rlasd pr raction raction rat pr unit volum (includs cross sction and

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

Lecture 2. Interaction of Radiation with Matter

Lecture 2. Interaction of Radiation with Matter Lctur Intraction of Radiation with Mattr Dats 14.10. Vorlsung 1 T.Stockmanns 1.10. Vorlsung J.Ritman 8.10. Vorlsung 3 J.Ritman 04.11. Vorlsung 4 J.Ritman 11.11. Vorlsung 5 J.Ritman 18.11. Vorlsung 6 J.

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

1.2 Faraday s law A changing magnetic field induces an electric field. Their relation is given by:

1.2 Faraday s law A changing magnetic field induces an electric field. Their relation is given by: Elctromagntic Induction. Lorntz forc on moving charg Point charg moving at vlocity v, F qv B () For a sction of lctric currnt I in a thin wir dl is Idl, th forc is df Idl B () Elctromotiv forc f s any

More information

Contemporary, atomic, nuclear, and particle physics

Contemporary, atomic, nuclear, and particle physics Contmporary, atomic, nuclar, and particl physics 1 Blackbody radiation as a thrmal quilibrium condition (in vacuum this is th only hat loss) Exampl-1 black plan surfac at a constant high tmpratur T h is

More information

E hf. hf c. 2 2 h 2 2 m v f ' f 2f ' f cos c

E hf. hf c. 2 2 h 2 2 m v f ' f 2f ' f cos c EXPERIMENT 9: COMPTON EFFECT Rlatd Topics Intractions of photons with lctrons, consrvation of momntum and nrgy, inlastic and lastic scattring, intraction cross sction, Compton wavlngth. Principl Whn photons

More information

Lecture 28 Title: Diatomic Molecule : Vibrational and Rotational spectra

Lecture 28 Title: Diatomic Molecule : Vibrational and Rotational spectra Lctur 8 Titl: Diatomic Molcul : Vibrational and otational spctra Pag- In this lctur w will undrstand th molcular vibrational and rotational spctra of diatomic molcul W will start with th Hamiltonian for

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

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

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

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

Structure of the Atom. Thomson s Atomic Model. Knowledge of atoms in Experiments of Geiger and Marsden 2. Experiments of Geiger and Marsden

Structure of the Atom. Thomson s Atomic Model. Knowledge of atoms in Experiments of Geiger and Marsden 2. Experiments of Geiger and Marsden CHAPTER 4 Structur of th Atom 4.1 Th Atomic Modls of Thomson and Ruthrford 4. Ruthrford Scattring 4.3 Th Classic Atomic Modl 4.4 Th Bohr Modl of th Hydrogn Atom 4.5 Succsss & Failurs of th Bohr Modl 4.6

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

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

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

Lecture Outline. Skin Depth Power Flow 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3e

Lecture Outline. Skin Depth Power Flow 8/7/2018. EE 4347 Applied Electromagnetics. Topic 3e 8/7/018 Cours Instructor Dr. Raymond C. Rumpf Offic: A 337 Phon: (915) 747 6958 E Mail: rcrumpf@utp.du EE 4347 Applid Elctromagntics Topic 3 Skin Dpth & Powr Flow Skin Dpth Ths & Powr nots Flow may contain

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

2. Laser physics - basics

2. Laser physics - basics . Lasr physics - basics Spontanous and stimulatd procsss Einstin A and B cofficints Rat quation analysis Gain saturation What is a lasr? LASER: Light Amplification by Stimulatd Emission of Radiation "light"

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

Electromagnetism Physics 15b

Electromagnetism Physics 15b lctromagntism Physics 15b Lctur #8 lctric Currnts Purcll 4.1 4.3 Today s Goals Dfin lctric currnt I Rat of lctric charg flow Also dfin lctric currnt dnsity J Charg consrvation in a formula Ohm s Law vryon

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

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

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

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

1973 AP Calculus AB: Section I

1973 AP Calculus AB: Section I 97 AP Calculus AB: Sction I 9 Minuts No Calculator Not: In this amination, ln dnots th natural logarithm of (that is, logarithm to th bas ).. ( ) d= + C 6 + C + C + C + C. If f ( ) = + + + and ( ), g=

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

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

0 +1e Radionuclides - can spontaneously emit particles and radiation which can be expressed by a nuclear equation.

0 +1e Radionuclides - can spontaneously emit particles and radiation which can be expressed by a nuclear equation. Radioactivity Radionuclids - can spontanously mit particls and radiation which can b xprssd by a nuclar quation. Spontanous Emission: Mass and charg ar consrvd. 4 2α -β Alpha mission Bta mission 238 92U

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

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

Chapter. 3 Wave & Particles I

Chapter. 3 Wave & Particles I Announcmnt Cours wbpag http://highnrgy.phys.ttu.du/~sl/2402/ Txtbook PHYS-2402 Lctur 8 Quiz 1 Class avrag: 14.2 (out of 20) ~ 70% Fb. 10, 2015 HW2 (du 2/19) 13, 17, 23, 25, 28, 31, 37, 38, 41, 44 Chaptr.

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

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

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

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

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

Introduction to Condensed Matter Physics

Introduction to Condensed Matter Physics Introduction to Condnsd Mattr Physics pcific hat M.P. Vaughan Ovrviw Ovrviw of spcific hat Hat capacity Dulong-Ptit Law Einstin modl Dby modl h Hat Capacity Hat capacity h hat capacity of a systm hld at

More information

Interaction of particles with matter

Interaction of particles with matter Introduction to Elmntary Particl Physics. Not 1 Pag 1 of 15 Intraction of particls with mattr 1. Particls and intractions. Wak intractions (nutrinos) 3. Elctromagntic intractions (chargd particls) 3.1.

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

Alpha and beta decay equation practice

Alpha and beta decay equation practice Alpha and bta dcay quation practic Introduction Alpha and bta particls may b rprsntd in quations in svral diffrnt ways. Diffrnt xam boards hav thir own prfrnc. For xampl: Alpha Bta α β alpha bta Dspit

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

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

Phys 402: Nonlinear Spectroscopy: SHG and Raman Scattering

Phys 402: Nonlinear Spectroscopy: SHG and Raman Scattering Rquirmnts: Polariation of Elctromagntic Wavs Phys : Nonlinar Spctroscopy: SHG and Scattring Gnral considration of polariation How Polarirs work Rprsntation of Polariation: Jons Formalism Polariation of

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

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

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

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

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

University of Illinois at Chicago Department of Physics. Thermodynamics & Statistical Mechanics Qualifying Examination

University of Illinois at Chicago Department of Physics. Thermodynamics & Statistical Mechanics Qualifying Examination Univrsity of Illinois at Chicago Dpartmnt of hysics hrmodynamics & tatistical Mchanics Qualifying Eamination January 9, 009 9.00 am 1:00 pm Full crdit can b achivd from compltly corrct answrs to 4 qustions.

More information

A=P=E M-A=N Alpha particle Beta Particle. Periodic table

A=P=E M-A=N Alpha particle Beta Particle. Periodic table Nam Pr. Atomic Structur/Nuclar Chmistry (Ch. 3 & 21) OTHS Acadmic Chmistry Objctivs: Undrstand th xprimntal dsign and conclusions usd in th dvlopmnt of modrn atomic thory, including Dalton's Postulats,

More information

Chapter 6: Polarization and Crystal Optics

Chapter 6: Polarization and Crystal Optics Chaptr 6: Polarization and Crystal Optics * P6-1. Cascadd Wav Rtardrs. Show that two cascadd quartr-wav rtardrs with paralll fast axs ar quivalnt to a half-wav rtardr. What is th rsult if th fast axs ar

More information

y = 2xe x + x 2 e x at (0, 3). solution: Since y is implicitly related to x we have to use implicit differentiation: 3 6y = 0 y = 1 2 x ln(b) ln(b)

y = 2xe x + x 2 e x at (0, 3). solution: Since y is implicitly related to x we have to use implicit differentiation: 3 6y = 0 y = 1 2 x ln(b) ln(b) 4. y = y = + 5. Find th quation of th tangnt lin for th function y = ( + ) 3 whn = 0. solution: First not that whn = 0, y = (1 + 1) 3 = 8, so th lin gos through (0, 8) and thrfor its y-intrcpt is 8. y

More information

6. The Interaction of Light and Matter

6. The Interaction of Light and Matter 6. Th Intraction of Light and Mattr - Th intraction of light and mattr is what maks lif intrsting. - Light causs mattr to vibrat. Mattr in turn mits light, which intrfrs with th original light. - Excitd

More information

Chapter 7b Electron Spin and Spin- Orbit Coupling

Chapter 7b Electron Spin and Spin- Orbit Coupling Wintr 3 Chm 356: Introductory Quantum Mchanics Chaptr 7b Elctron Spin and Spin- Orbit Coupling... 96 H- atom in a Magntic Fild: Elctron Spin... 96 Total Angular Momntum... 3 Chaptr 7b Elctron Spin and

More information

surface of a dielectric-metal interface. It is commonly used today for discovering the ways in

surface of a dielectric-metal interface. It is commonly used today for discovering the ways in Surfac plasmon rsonanc is snsitiv mchanism for obsrving slight changs nar th surfac of a dilctric-mtal intrfac. It is commonl usd toda for discovring th was in which protins intract with thir nvironmnt,

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

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

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

Physics 2D Lecture Slides Lecture 14: Feb 1 st 2005

Physics 2D Lecture Slides Lecture 14: Feb 1 st 2005 Physics D Lctur Slids Lctur 14: Fb 1 st 005 Vivk Sharma UCSD Physics Compton Effct: what should Happn Classically? Plan wav [f,λ] incidnt on a surfac with loosly bound lctrons intraction of E fild of EM

More information

Definition1: The ratio of the radiation intensity in a given direction from the antenna to the radiation intensity averaged over all directions.

Definition1: The ratio of the radiation intensity in a given direction from the antenna to the radiation intensity averaged over all directions. Dirctivity or Dirctiv Gain. 1 Dfinition1: Dirctivity Th ratio of th radiation intnsity in a givn dirction from th antnna to th radiation intnsity avragd ovr all dirctions. Dfinition2: Th avg U is obtaind

More information

CHAPTER 1. Introductory Concepts Elements of Vector Analysis Newton s Laws Units The basis of Newtonian Mechanics D Alembert s Principle

CHAPTER 1. Introductory Concepts Elements of Vector Analysis Newton s Laws Units The basis of Newtonian Mechanics D Alembert s Principle CHPTER 1 Introductory Concpts Elmnts of Vctor nalysis Nwton s Laws Units Th basis of Nwtonian Mchanics D lmbrt s Principl 1 Scinc of Mchanics: It is concrnd with th motion of matrial bodis. odis hav diffrnt

More information

Physics 2D Lecture Slides Lecture 12: Jan 28 th 2004

Physics 2D Lecture Slides Lecture 12: Jan 28 th 2004 Brian Wcht, th TA, is away this wk. I will substitut for his offic hours (in my offic 3314 Mayr Hall, discussion and PS sssion. Pl. giv all rgrad rqusts to m this wk (only) Quiz 3 Will Covr Sctions.1-.5

More information

Physics. X m (cm)

Physics. X m (cm) Entranc xa 006-007 Physics Duration: hours I- [ pts] An oscillator A chanical oscillator (C) is ford of a solid (S), of ass, attachd to th xtrity A of a horizontal spring of stiffnss (constant) = 80 N/

More information

APP-IV Introduction to Astro-Particle Physics. Maarten de Jong

APP-IV Introduction to Astro-Particle Physics. Maarten de Jong APP-IV Introduction to Astro-Particl Physics Maartn d Jong 1 cosmology in a nut shll Hubbl s law cosmic microwav background radiation abundancs of light lmnts (H, H, ) Hubbl s law (199) 1000 vlocity [km/s]

More information

Neutrinos are chargeless, nearly massless particles Most abundant particle in the Universe Interact with matter via weak nuclear force

Neutrinos are chargeless, nearly massless particles Most abundant particle in the Universe Interact with matter via weak nuclear force By Wndi Wamlr Nutrinos ar charglss, narly masslss articls Most abundant articl in th Univrs Intract with mattr via wak nuclar forc Narly transarnt to mattr Only known ty of articl that can sca from th

More information

Molecular Orbitals in Inorganic Chemistry

Molecular Orbitals in Inorganic Chemistry Outlin olcular Orbitals in Inorganic Chmistry Dr. P. Hunt p.hunt@imprial.ac.uk Rm 167 (Chmistry) http://www.ch.ic.ac.uk/hunt/ octahdral complxs forming th O diagram for Oh colour, slction ruls Δoct, spctrochmical

More information

PHYS-333: Problem set #2 Solutions

PHYS-333: Problem set #2 Solutions PHYS-333: Problm st #2 Solutions Vrsion of March 5, 2016. 1. Visual binary 15 points): Ovr a priod of 10 yars, two stars sparatd by an angl of 1 arcsc ar obsrvd to mov through a full circl about a point

More information

4.2 Design of Sections for Flexure

4.2 Design of Sections for Flexure 4. Dsign of Sctions for Flxur This sction covrs th following topics Prliminary Dsign Final Dsign for Typ 1 Mmbrs Spcial Cas Calculation of Momnt Dmand For simply supportd prstrssd bams, th maximum momnt

More information

5. Equation of state for high densities

5. Equation of state for high densities 5 1 5. Equation of stat for high dnsitis Equation of stat for high dnsitis 5 Vlocity distribution of lctrons Classical thrmodynamics: 6 dimnsional phas spac: (x,y,z,px,py,pz) momntum: p = p x+p y +p z

More information

Math 34A. Final Review

Math 34A. Final Review Math A Final Rviw 1) Us th graph of y10 to find approimat valus: a) 50 0. b) y (0.65) solution for part a) first writ an quation: 50 0. now tak th logarithm of both sids: log() log(50 0. ) pand th right

More information

PARTICLE MOTION IN UNIFORM GRAVITATIONAL and ELECTRIC FIELDS

PARTICLE MOTION IN UNIFORM GRAVITATIONAL and ELECTRIC FIELDS VISUAL PHYSICS ONLINE MODULE 6 ELECTROMAGNETISM PARTICLE MOTION IN UNIFORM GRAVITATIONAL and ELECTRIC FIELDS A fram of rfrnc Obsrvr Origin O(,, ) Cartsian coordinat as (X, Y, Z) Unit vctors iˆˆj k ˆ Scif

More information

Chemical Engineering 412

Chemical Engineering 412 Chical Enginring 4 Introductory Nuclar Enginring Lctur 6 Nuclar Radiation Typs Ky oints Typs of cay Na roprtis athatical scriptions Cavats cay Charts (KNOW HOW TO USE!) Nuclar Equation for cay -Valus for

More information

PH300 Modern Physics SP11 Final Essay. Up Next: Periodic Table Molecular Bonding

PH300 Modern Physics SP11 Final Essay. Up Next: Periodic Table Molecular Bonding PH Modrn Physics SP11 Final Essay Thr will b an ssay portion on th xam, but you don t nd to answr thos qustions if you submit a final ssay by th day of th final: Sat. 5/7 It dosnʼt mattr how smart you

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

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

7.4 Potential Difference and Electric Potential

7.4 Potential Difference and Electric Potential 7.4 Potntial Diffrnc and Elctric Potntial In th prvious sction, you larnd how two paralll chargd surfacs produc a uniform lctric fild. From th dfinition of an lctric fild as a forc acting on a charg, it

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

2. Background Material

2. Background Material S. Blair Sptmbr 3, 003 4. Background Matrial Th rst of this cours dals with th gnration, modulation, propagation, and ction of optical radiation. As such, bic background in lctromagntics and optics nds

More information

u 3 = u 3 (x 1, x 2, x 3 )

u 3 = u 3 (x 1, x 2, x 3 ) Lctur 23: Curvilinar Coordinats (RHB 8.0 It is oftn convnint to work with variabls othr than th Cartsian coordinats x i ( = x, y, z. For xampl in Lctur 5 w mt sphrical polar and cylindrical polar coordinats.

More information

AerE 344: Undergraduate Aerodynamics and Propulsion Laboratory. Lab Instructions

AerE 344: Undergraduate Aerodynamics and Propulsion Laboratory. Lab Instructions ArE 344: Undrgraduat Arodynamics and ropulsion Laboratory Lab Instructions Lab #08: Visualization of th Shock Wavs in a Suprsonic Jt by using Schlirn tchniqu Instructor: Dr. Hui Hu Dpartmnt of Arospac

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

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

Lecture 19: Free Energies in Modern Computational Statistical Thermodynamics: WHAM and Related Methods

Lecture 19: Free Energies in Modern Computational Statistical Thermodynamics: WHAM and Related Methods Statistical Thrmodynamics Lctur 19: Fr Enrgis in Modrn Computational Statistical Thrmodynamics: WHAM and Rlatd Mthods Dr. Ronald M. Lvy ronlvy@tmpl.du Dfinitions Canonical nsmbl: A N, V,T = k B T ln Q

More information

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics

fiziks Institute for NET/JRF, GATE, IIT JAM, M.Sc. Entrance, JEST, TIFR and GRE in Physics Atoic and olcular Physics JEST Q. Th binding nrgy of th hydrogn ato (lctron bound to proton) is.6 V. Th binding nrgy of positroniu (lctron bound to positron) is (a).6 / V (b).6 / 8 V (c).6 8 V (d).6 V.6

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

Chapter 1. Chapter 10. Chapter 2. Chapter 11. Chapter 3. Chapter 12. Chapter 4. Chapter 13. Chapter 5. Chapter 14. Chapter 6. Chapter 7.

Chapter 1. Chapter 10. Chapter 2. Chapter 11. Chapter 3. Chapter 12. Chapter 4. Chapter 13. Chapter 5. Chapter 14. Chapter 6. Chapter 7. Chaptr Binomial Epansion Chaptr 0 Furthr Probability Chaptr Limits and Drivativs Chaptr Discrt Random Variabls Chaptr Diffrntiation Chaptr Discrt Probability Distributions Chaptr Applications of Diffrntiation

More information

Estimation of the two-photon QED background in Belle II

Estimation of the two-photon QED background in Belle II Estimation of th two-photon QED background in Bll II Elna Ndlkovska, Christian Kisling Max-Planck Institut for physics, Munich Upgrad to th Bll II dtctor Expctd background at Bll II QED xprimnts prformd

More information

PRINCIPLES OF PLASMA PROCESSING Course Notes: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA

PRINCIPLES OF PLASMA PROCESSING Course Notes: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA Atomic Collisions and Spctra 125 PRINCIPLES OF PLASMA PROCESSING Cours Nots: Prof. J. P. Chang Part B3: ATOMIC COLLISIONS AND SPECTRA I. ATOMIC ENERGY LEVELS Atoms and molculs mit lctromagntic radiation

More information