Section VIII. The Weak Interaction
|
|
- Harvey Singleton
- 6 years ago
- Views:
Transcription
1 Sction VIII Th ak Intraction
2 Th ak Intraction Th AK intraction accont for many cay in particl phyic xampl: Charactriz by long liftim an mall cro-ction - - p n π ; ; 69
3 Two typ of AK intraction: CHARGD CURRNT (CC): ± Boon NUTRAL CURRNT (NC): Z Boon Th AK forc i miat by MASSIV VCTOR BOSONS: M ~ 8 GV xampl: M Z ~ 9 GV ak intraction of lctron an ntrino: Z Z 7
4 Boon Slf-Intraction In QCD th glon carry COLOUR charg. In th AK intraction th ± an Z boon carry th AK CHARG ± alo carry M charg BOSON SLF-INTRACTIONS γ Z Z Z Z γ γ γ 7
5 Frmi Thory ak intraction takn to b a 4-frmion contact intraction No propagator Copling trngth givn by th FRMI CONSTANT, G F G F.66 x -5 GV - β Dcay in Frmi Thory p n p - n G F U Frmi Goln Rl to gt th tranition rat Γ π M fi ( ) whr M if i th matrix lmnt an ρ( f ) i th nity of final tat. ρ f ( ) ρ f N f 7
6 Dnity of Final Stat: -boy v. -boy (pag 46) TO BODY FINAL STAT: N π ( ) Ω Rlativitic ( ~ p) i.. nglct ma of final tat particl. Only conir on of th particl inc th othr fix by (,p) conrvation. THR BODY FINAL STAT (.g. β cay): N Ω ( π) ( π) Now ncary to conir two particl th thir i givn by (,p) conrvation. Ω 7
7 In nclar β cay, th nrgy rla in th nclar tranition,, i har btwn th lctron, ntrino an th rcoil kintic nrgy of th ncl: Trcoil Sinc th ncl i mch mor maiv than th lctron /ntrino: an th nclar rcoil nr momntm conrvation. For a GIVN lctron nrgy : N N Ω ( π) ( π) Ω 74
8 Aming iotropic cay itribtion an intgrating ovr Ω Ω giv: N ( ) ( ) 4π ( ) ( ) π Γ Γ π π M fi M fi 4π 4 ( ) ( ) π 4 4π 4π 4 Matrix lmnt In Frmi thory, M G an trat, a fr particl fi M fi F G F ψ n ψ ψ ψ p p ψ v v ip ψ v r ( p p ) v v r ψ n r v ψ 4-point intraction v r v ip v r 75
9 p v r v Typically, an hav nrgi ~ MV, o << iz of ncl an ψ,ψ Corrpon to zro anglar momntm (l ) tat for th an. ALLOD TRANSITIONS - Th matrix lmnt i thn givn by M fi GF ψ p ψn r v G F M nclar whr th nclar matrix lmnt accont for th ovrlap of th nclar wav-fnction. If th n an p wav-fnction ar vry imilar, th nclar matrix lmnt M nclar M nclar M fi larg an β cay i favor: SUPRALLOD TRANSITIONS 76
10 M nclar Hr, am (prallow tranition): Γ Γ Γ G π F GF π GF 6π ( ) 5 ( ) G π F M fi G F SARGNT RUL: 5.g. - an - cay ( latr) By tying liftim for nclar bta cay, w can trmin th trngth of th wak intraction in Frmi thory: β G F -5 (. 6 ±.) GV 77
11 Bta-Dcay Spctrm Γ G F ( ) Γ Plot of vr i linar ( ) π Γ ( ) KURI PLOT Γ H H ( kv ) 78
12 Ma m (nglct ma of final tat particl) n point of lctron pctrm m (allow for ma of final tat particl) p Dnity of tat N Ω N Ω (pag 46) π ( π) p ( ) Γ G π F ( ) m ( ) m m known, m mall only ignificant ffct i whr 79
13 KURI PLOT Γ Γ ( ) m Γ 4 m ( ) 4 xprimntal roltion Mot rcnt rlt (999) Tritim β cay: m < V If ntrino hav ma, m << m hy o mall? 8
14 Ntrino Scattring in Frmi Thory (Invr β Dcay). σ σ π M GF π n p fi N π whr i th nrgy of th in th cntr-of-ma ytm an i th nrgy in th cntr-of-ma ytm. In th laboratory fram: ( pag 6) σ G F ( π) only intract AKLY hav vry mall intraction cro-ction Hr AK impli that yo n approximatly 5 light-yar of watr to top a MV ntrino! Howvr, a th cro-ction can bcom vry larg. Violat maximm allow val by conrvation of probability at (UNITARITY LIMIT). Ω Frmi thory brak own at high nrgi. m n -4 ( in MV) cm ~ Appnix F n G F p 74 GV 8
15 ak Charg Crrnt: ± Boon Frmi thory brak own at high nrgy Tr intraction crib by xchang of CHARGD ± BOSONS Frmi thory i th low nrgy q << m FFCTIV thory of th AK intraction. β Dcay: n Scattring: p ( ) G F n G F g g q M p 8
16 Compar AK an QD intraction: α AK g 4π g g q M QD γ g m gm q g m α 4 π CHARGD CURRNT AK INTRACTION At low nrgi, q << M, propagator q M M i.. appar a POINT-LIK intraction of Frmi thory. Maiv propagator hort rang M 8.4 GV Rang ~. fm M xchang boon carri lctromagntic charg. FLAVOUR CHANGING ONLY AK intraction chang flavor PARITY VIOLATING ONLY AK intraction can violat parity conrvation. 8
17 Compar Frmi thory c.f. maiv propagator - q << M G F For compar matrix lmnt: G F i mall bca m i larg. Th prci rlationhip i: g - Th nmrical factor ar partly of hitorical origin ( Prkin 4 th., pag ). M 8.4 GV an GF g an α 5 GV Th intrinic trngth of th AK intraction i GRATR than that of th lctromagntic intraction. At low nrgi (low q ), it appar wak to th maiv propagator. 84 g 4π g M g 8M G g F G F α ( latr to why β iffrnt to ) 4π 7 G F
18 Ntrino Scattring with a Maiv Boon Rplac contact intraction by maiv boon xchang iagram: q Intgrat to giv: g g σ σ M GF π GF M π σ q π ( q M ) with q inϑ whr θ i th cattring angl. g 4 (imilar to pag 48) << >> M M Appnix G Total cro-ction now wll bhav at high nrgi. 85
19 Parity Violation in Bta Dcay Parity violation wa firt obrv in th β cay of 6 Co ncli (C.S. t. al. Phy. Rv. 5 (957) 4) Align 6 Co ncli with fil an look at irction of miion of lctron Unr parity: B Co Ni B v v v r v r; v v L r p J5 J4 Pˆ v v p v p v L; If PARITY i CONSRVD, xpct qal nmbr of lctron paralll an antiparalll to B v B v - 86
20 Polariz T. K Unpolariz A 6 Co hat p, thrmal xcitation ranomi th pin Mot lctron mitt oppoit to irction of fil PARITY VIOLATION in β DCAY 87
21 Origin of Parity Violation SPIN an HLICITY Conir a fr particl of contant momntm, p v. v v v Total anglar momntm, J L S, i ALAYS conrv. v v v Th orbital anglar momntm, L r p, i prpniclar to p v Th pin anglar momntm,, can b in any irction rlativ to p v Th val of pin S v along p v S v i alway CONSTANT. Dfin th ign of th componnt of pin along th irction of motion a th HLICITY v p v h v p v h v p v h RIGHT-HANDD LFT-HANDD p v 88
22 Th AK intraction itingih btwn LFT an RIGHT-HANDD tat. Th wak intraction copl prfrntially to LFT-HANDD PARTICLS an RIGHT-HANDD ANTIPARTICLS v v p v p v In th ltra-rlativitic (mal) limit, th copling to RIGHT-HANDD particl vanih. i.. vn if RIGHT-HANDD xit thy ar nobrvabl! 6 Co xprimnt: p v B 6 Co 6 Ni J5 J4 p v 89
23 Parity Violation Th AK intraction trat LH an RH tat iffrntly an thrfor can violat PARITY (i.. th intraction Hamiltonian o not commt with Pˆ ). xampl J P P PARITY i ALAYS conrv in th STRONG/M intraction η η π π P π π PARITY CONSRVD π π π ( ) ( ) ( L L P π P π )( ) ( ) P ; L L! PARITY VIOLATD Branching fraction % Branching fraction <.% η J P P η π π P π π π ( ) ( P π )( ) L P ; L 9
24 PARITY i USUALLY violat in th AK intraction bt NOT ALAYS! xampl J P K P K P ; L PARITY VIOLATD π π π π P π P π ( ) ( )( ) L ( ) ( ) ( )( ) L ( ) L Branching fraction ~ % Branching fraction ~ 6% J P P π K π π K π π π - P π P π P π P ; L L PARITY CONSRVD! 9
25 Th ak CC Lpton Vrtx All wak charg crrnt lpton intraction can b crib by th boon propagator an th wak vrtx:,,,, α g 4π g STANDARD MODL AK CC LPTON VRTX antiparticl Boon only copl to th lpton an ntrino within th SAM gnration.g. no copling Univral copling contant g 9
26 xampl: - -,, -, -, -,, n p - - n Bc J ψ p Bc b c c c J ψ 9
27 Dcay Mon ar fnamntal lpton (m ~ 6 m ). lctromagntic cay i NOT obrv; th M intraction o not chang flavor. Only th AK CC intraction chang flavor. Mon cay wakly: γ g - g - G F m << M A can FRMI thory to calclat cay with (analogo to β cay). 94
28 FRMI thory giv cay with proportional to (Sargnt rl). 5 m Howvr, mor complicat pha pac intgration (prvioly nglct kintic nrgy of rcoiling ncl) giv Γ G F 5 m 9π Mon ma an liftim known with high prciion. 6 (.97±.4) U mon cay to fix trngth of AK intraction G F G F (.66.) 5 ± GV G F i on of th bt trmin fnamntal qantiti in particl phyic. 95
29 Univrality of ak Copling Can compar G F mar from cay with that from β cay. g - From mon cay mar: From β cay mar: Ratio G F β G F G G β F F g Concl that th trngth of th wak intraction i ALMOST th am for lpton a for qark. will com back to th origin of thi iffrnc ( coϑ C ) n (.66.) 5 ± GV -5 (. 6 ±.) GV.974 ±. p 96
30 Th ma i rlativly larg an a m m > Dcay (.777 ±.) GV { m, m, m,k} thr ar a nmbr of poibl cay mo. π ρ xampl Ta branching fraction: haron (7.8 ±.%) (7. ±.%) (64.7 ±.%) 97
31 Lpton Univrality Tt whthr all lpton hav th am AK copling from marmnt of th cay rat an branching fraction. Compar g - Γ g GF 9π If nivral trngth of AK intraction, xpct m 5 5 m MV m, m, ar all mar prcily m ( 777. ±.) MV.97±.4 Prict (.9± Mar (.9±.) m 5.78 m B( ) g Γ g GF.78 9π B( ) m 5 ( 7.8 ±.% ) 6 ( ) SAM AK CC COUPLING FOR AND 98
32 Alo compar g g g g IF am copling xpct: B B ( - ) ( - ).976 (th mall iffrnc i to th light rction in pha pac to th non-ngligibl mon ma). ( ) - B Th obrv ratio ( ).974 ±.5 i conitnt with - th priction. B SAM AK CC COUPLING FOR, AND LPTON UNIVRSALITY 99
33 ak Intraction of Qark In th Stanar Mol, th lptonic wak copling tak plac within a particlar gnration: - Natral to xpct am pattrn for QUARKS, i.. b Unfortnatly, not that impl!! xampl: Th cay K ggt a copling c t K
34 For-Flavor Qark Mixing Cabibbo Mixing Angl Th tat which tak part in th AK intraction ar ORTHOGONAL combination of th tat of finit flavor (, ) For 4 flavor, {,, an c}, th mixing can b crib by a ingl paramtr o CABIBBO ANGL (from xprimnt) ak igntat Copling bcom: co ϑ co ϑ C C in ϑ in ϑ C C co ϑ in ϑ c g C g C ϑc in ϑ co ϑ co ϑ C co ϑ C C C c Flavor igntat g g in ϑc in ϑc c
35 xampl: Nclar β cay Rcall β G F G F n -5 (. 6 ±.) GV (.66.) 5 ± GV p trngth of copling β M co ϑ ( ) C G F Hnc, xpct It work, g co G β F GF coϑ C.6.66 ϑ C o co ϑc o Cabibbo Favor M co ϑc Cabibbo Sppr g g co ϑ C in ϑ C M in ϑc g g co ϑ C in ϑ C c c
36 xampl: K copling Cabibbo ppr M in ϑc K g in ϑ C g xampl: D xpct c D g Γ Γ K coϑ C g π, D K K π coϑ C π 4 K π in ϑ 4 K π co ϑ.8 ( D ) ( D ) C C D c - g in ϑ C g in ϑ C π K Mar.8 ±.8 D K π i DOUBLY Cabibbo ppr
37 CKM Matrix Cabibbo-Kobayahi-Makawa Matrix xtn to gnration b V ak igntat CKM Giving copling V V V c t g V V V V c t V V V b cb tb V b coϑc in ϑ. C CKM g V b in ϑ coϑ C c C.5 Flavor igntat..5 λ λ λ g V b λ λ λ t λ λ λ in ϑ C b 4
38 Th ak CC Qark Vrtx All wak charg crrnt qark intraction can b crib by th boon propagator an th wak vrtx: q {,c,t} α g V qq g 4π q {,,b} STANDARD MODL AK CC QUARK VRTX antiparticl boon CHANG qark flavor lik to copl to qark in th SAM gnration, bt qark tat mixing man that CROSS-GNRATION copling can occr. -Lpton copling contant -Qark copling contant g g V CKM 5
39 B xampl: b M g V cb g Ma (Log cal) 4 B g D 4 in ϑc t c - ϕ π K D c D Charg / Charg -/ K c M g V c g g 4 V b 4 co ϑc ϕ π g w V, V c, V tb O() g w V c, V O(λ) g w V cb, V t O(λ ) t, b O(λ ) vry mall ϕ - M g V g 4 λ in ϑ C K g V 4 in ϑc 6 K
40 Smmary AK INTRACTION (CHARGD CURRNT) ak forc miat by maiv boon ak forc intrinically trongr than M intraction α cf αm 7 Univral copling to qark an lpton Qark tak part in th intraction a mixtr of th flavor igntat Parity can b VIOLATD to th HLICITY trctr of th intraction Strngth of th wak intraction givn by G F M ( 8.4 ±.8) GV (.66.) 5 ± GV from mon cay. 7
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 informationForces. 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 informationMixing in Weak Decays
Mixing in ak Dcay Chargd ak Currnt xchang of cau on mmbr of a wak doublt to chang into th othr Tau and muon thrfor dcay into th lightt mmbr of th doublt thir nutrino lctron ar tabl a th,nu doublt i th
More informationSelf-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 informationPair (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 informationa 1and x is any real number.
Calcls Nots Eponnts an Logarithms Eponntial Fnction: Has th form y a, whr a 0, a an is any ral nmbr. Graph y, Graph y ln y y Th Natral Bas (Elr s nmbr): An irrational nmbr, symboliz by th lttr, appars
More informationPrecision 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 informationProperties 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 informationAntonio Pich. IFIC, CSIC Univ. Valencia.
Antonio Pich IFIC, CSIC Univ. Valncia Antonio.Pich@crn.ch Th Standard Modl A. Pich - CERN Summr Lcturs 2005 1. Constitunts & Intractions 2. Quarks 3. Gaug Invarianc 4. Quantum Chromodynamics 5. Elctrowak
More informationNeutrino 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 informationPHYSICS 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 informationThe 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 informationBETA 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 informationIntro 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 informationOutline. 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 informationDerivation 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 informationNeutrinos 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 informationNuclear 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(1) Then we could wave our hands over this and it would become:
MAT* K285 Spring 28 Anthony Bnoit 4/17/28 Wk 12: Laplac Tranform Rading: Kohlr & Johnon, Chaptr 5 to p. 35 HW: 5.1: 3, 7, 1*, 19 5.2: 1, 5*, 13*, 19, 45* 5.3: 1, 11*, 19 * Pla writ-up th problm natly and
More informationNeutrino 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 informationDIS-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 informationNuclear and Particle Physics - Lecture 16 Neutral kaon decays and oscillations
1 Introction Nclear an Particle Phyic - Lectre 16 Netral kaon ecay an ocillation e have alreay een that the netral kaon will have em-leptonic an haronic ecay. However, they alo exhibit the phenomenon of
More information1.2 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 informationSearches 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 informationHigh 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 informationFirst order differential equation Linear equation; Method of integrating factors
First orr iffrntial quation Linar quation; Mtho of intgrating factors Exampl 1: Rwrit th lft han si as th rivativ of th prouct of y an som function by prouct rul irctly. Solving th first orr iffrntial
More informationELECTRON-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 informationOn 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 informationToday. 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 informationfiziks 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 informationLecture 9: Fundamental particle discoveries 2 nd generation Strange quark:
PYP High Enrgy Phyic Hanot #5 Lctr 9-8 th Janary 8 Pag Ra & Chaptr.5 in connction with icovry of W ± an Z boon. Lctr 9: Fnantal particl icovri n gnration trang ark: Prvioly icovr in trang on an baryon:
More informationThe Standard Model Lagrangian
Th Standard Modl aranian Elmntary Particl Physics Stron Intraction Fnomnoloy Dio Bttoni Acadmic ar - D. Bttoni Fnomnoloia Intrazioni Forti Dirac Formalism m i j Consrvd Currnt i i i 5 i m Gau Invarianc
More informationCh. 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 informationde/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 informationAPP-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 informationCoupled 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 informationCosmology 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 informationMultiple Short Term Infusion Homework # 5 PHA 5127
Multipl Short rm Infusion Homwork # 5 PHA 527 A rug is aministr as a short trm infusion. h avrag pharmacokintic paramtrs for this rug ar: k 0.40 hr - V 28 L his rug follows a on-compartmnt boy mol. A 300
More informationPion condensation with neutrinos
Pion condnsation with nutrinos Or how dos QCD bhav undr high dnsitis of lctron/muon nutrinos Harmn Warringa, Goth Univrsität, Frankfurt Basd on work don with Hiroaki Abuki and Tomas Braunr arxiv:0901.2477
More informationHydrogen 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 informationAddition 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 informationPHYS ,Fall 05, Term Exam #1, Oct., 12, 2005
PHYS1444-,Fall 5, Trm Exam #1, Oct., 1, 5 Nam: Kys 1. circular ring of charg of raius an a total charg Q lis in th x-y plan with its cntr at th origin. small positiv tst charg q is plac at th origin. What
More informationAddition 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 informationThe 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 informationContemporary, 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 informationChapter 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 informationParticle Physics. Dr M.A. Thomson. ν e. e + W + Z 0 e + e - W - Part II, Lent Term 2004 HANDOUT VI. Dr M.A. Thomson Lent 2004
Particle Physics Dr M.A. Thomson e + W + Z 0 e + q q Part II, Lent Term 2004 HANDOUT VI 2 The Weak Interaction The WEAK interaction acconts for many ecays in particle physics e.g. μ! e νeνμ, fi! e νeνfi,
More informationIV. Weak interaction 1. Phenomenology of weak decays 2. Parity violation and neutrino helicity 3. V-A theory 4. Neutral currents
IV. Wak intraction. hnonology of wak dcays. arity violation and ntrino hlicity 3. V-A thory 4. Ntral crrnts Th wak intraction was and is a toic with a lot of srriss: ast: Flavor violation, and C violation.
More informationNeutrino Probes of Dark Energy and Dark Matter
SNOWPAC@Snowbird March 25, 2010 Nutrino Probs of Dark Enrgy and Dark Mattr Shin ichiro Ando California Institut of Tchnology Dark Enrgy and Dark Mattr 2.0 1.5 1.0 No Big Bang SN Most of th nrgy in th Univrs
More informationClassical 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 informationTitle: 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 informationPrinciples 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 informationElectroweak 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 informationLecture 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(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 informationChemical 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 informationConstruction of asymmetric orthogonal arrays of strength three via a replacement method
isid/ms/26/2 Fbruary, 26 http://www.isid.ac.in/ statmath/indx.php?modul=prprint Construction of asymmtric orthogonal arrays of strngth thr via a rplacmnt mthod Tian-fang Zhang, Qiaoling Dng and Alok Dy
More informationCalculation of electromotive force induced by the slot harmonics and parameters of the linear generator
Calculation of lctromotiv forc inducd by th lot harmonic and paramtr of th linar gnrator (*)Hui-juan IU (**)Yi-huang ZHANG (*)School of Elctrical Enginring, Bijing Jiaotong Univrity, Bijing,China 8++58483,
More information1 Isoparametric Concept
UNIVERSITY OF CALIFORNIA BERKELEY Dpartmnt of Civil Enginring Spring 06 Structural Enginring, Mchanics and Matrials Profssor: S. Govindj Nots on D isoparamtric lmnts Isoparamtric Concpt Th isoparamtric
More informationLecture 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 informationINTRODUCTION TO AUTOMATIC CONTROLS INDEX LAPLACE TRANSFORMS
adjoint...6 block diagram...4 clod loop ytm... 5, 0 E()...6 (t)...6 rror tady tat tracking...6 tracking...6...6 gloary... 0 impul function...3 input...5 invr Laplac tranform, INTRODUCTION TO AUTOMATIC
More informationDeepak Rajput
Q Prov: (a than an infinit point lattic is only capabl of showing,, 4, or 6-fold typ rotational symmtry; (b th Wiss zon law, i.. if [uvw] is a zon axis and (hkl is a fac in th zon, thn hu + kv + lw ; (c
More informationBasic Polyhedral theory
Basic Polyhdral thory Th st P = { A b} is calld a polyhdron. Lmma 1. Eithr th systm A = b, b 0, 0 has a solution or thr is a vctorπ such that π A 0, πb < 0 Thr cass, if solution in top row dos not ist
More informationThe 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 informationTESTING A SPIN-2 MEDIATOR IN DECAYS
TESTING A SPIN- MEDIATOR IN b s DECAYS BAZENA MEIC Thortical Physics Division Rudjr Boskovic Institut, Zagrb arxiv 1801.07115 in collaboration with Svjtlana Fajfr & Monalisa Patra (IJS, jubljana Windows
More informationEigenvalue Distributions of Quark Matrix at Finite Isospin Chemical Potential
Tim: Tusday, 5: Room: Chsapak A Eignvalu Distributions of Quark Matri at Finit Isospin Chmical Potntial Prsntr: Yuji Sasai Tsuyama National Collg of Tchnology Co-authors: Grnot Akmann, Atsushi Nakamura
More informationSchrodinger 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 informationMagnetic Neutron Scattering and Spin-Polarized Neutrons
agntic Nutron Scattring and Spin-Polarizd Nutrons Physical origin: potntial of magntic dipol momnt of th nutron in magntic fild gnratd by lctron spins and orbital momnts in th solid. µ n µ H Spcializ to
More informationPHYSICS 489/1489 LECTURE 16: WEAK INTERACTION OF HADRONS
PHYSICS 489/1489 LECTURE 16: WEAK INTERACTION OF HADRONS ANNOUNCEMENTS Problem Set 3 e on Friay 1700 No cla next Teay No office hor Monay, Teay Sorry! Pleae feel free to en me email abot qetion, etc. or
More informationWhy 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 informationRefer to Chapter 8 Kaon system Oscillations and CKM mixing matrix Neutrinos
Chaptr 1 Rfr to Chaptr 8 Kaon systm Oscillations and CKM mixing matrix Nutrinos " # K 1 = 1 $ K K " # K = 1 $ K K C K = K ; C K = K P K = K ; P K = K % ' & % ' & K andk ar not ignstats of CP : CP K = K
More informationExam 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 informationConstituents of the Atom
1 Constitunts of th Atom To b know th constitunts of th atom with thir masss and chargs To b abl to calculat th spcific charg of th constitunts To b abl to xplain what isotops and ions ar Th Nuclar Modl
More informationThe 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 informationElements 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 informationPlasma notes: Ohm s Law and Hall MHD by E. Alec Johnson, October, 2007.
1 Plama not: Ohm Law and Hall MHD by E. Alc Johnon, Octobr, 2007. 1 Boltzmann quation Th Boltzmann quation for pci i an volution quation for particl dnity in pha pac. Pha pac i a collction of coordinat
More informationDavisson 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 informationBackground: 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 informationChapter. 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 informationEE243 Advanced Electromagnetic Theory Lec # 23 Scattering and Diffraction. Reading: Jackson Chapter , lite
Applid M Fall 6, Nuruthr Lctur #3 Vr /5/6 43 Advancd lctromagntic Thory Lc # 3 cattring and Diffraction calar Diffraction Thory Vctor Diffraction Thory Babint and Othr Principls Optical Thorm ading: Jackson
More informationMaxwellian Collisions
Maxwllian Collisions Maxwll ralizd arly on that th particular typ of collision in which th cross-sction varis at Q rs 1/g offrs drastic siplifications. Intrstingly, this bhavior is physically corrct for
More informationelectron -ee mrw o center of atom CLASSICAL ELECTRON THEORY Lorentz' classical model for the dielectric function of insulators
CLASSICAL ELECTRON THEORY Lorntz' claical odl for th dilctric function of inulator In thi odl th lctron ar aud to b bound to th nuclu ith forc obying Hook la. Th forc ar aud to b iotropic and daping can
More informationBrief 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 informationsurface 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 information6. 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[ ] 1+ lim G( s) 1+ s + s G s s G s Kacc SYSTEM PERFORMANCE. Since. Lecture 10: Steady-state Errors. Steady-state Errors. Then
SYSTEM PERFORMANCE Lctur 0: Stady-tat Error Stady-tat Error Lctur 0: Stady-tat Error Dr.alyana Vluvolu Stady-tat rror can b found by applying th final valu thorm and i givn by lim ( t) lim E ( ) t 0 providd
More informationQuasi-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 informationFinite element discretization of Laplace and Poisson equations
Finit lmnt discrtization of Laplac and Poisson quations Yashwanth Tummala Tutor: Prof S.Mittal 1 Outlin Finit Elmnt Mthod for 1D Introduction to Poisson s and Laplac s Equations Finit Elmnt Mthod for 2D-Discrtization
More informationTREATMENT OF THE PLASMA NONLINEAR ABSORPTION LAW AT LINEARLY POLARIZED LASER RADIATION OF RELATIVISTIC INTENSITIES. A. G.
Armnian Journal of Physics, 15, vol. 8, issu, pp. 64-7 TREATMENT OF THE PLASMA NONLINEAR ABSORPTION LAW AT LINEARLY POLARIZED LASER RADIATION OF RELATIVISTIC INTENSITIES A. G. Ghazaryan Cntr of Strong
More informationIntroduction 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 informationSPH4U Electric Charges and Electric Fields Mr. LoRusso
SPH4U lctric Chargs an lctric Fils Mr. LoRusso lctricity is th flow of lctric charg. Th Grks first obsrv lctrical forcs whn arly scintists rubb ambr with fur. Th notic thy coul attract small bits of straw
More informationModeling with first order equations (Sect. 2.3).
Moling with first orr quations (Sct. 2.3. Main xampl: Salt in a watr tank. Th xprimntal vic. Th main quations. Analysis of th mathmatical mol. Prictions for particular situations. Salt in a watr tank.
More informationNonlinear reduced Braginskii equations with ion thermal dynamics in toroidal plasma
Nonlinar ruc Braginkii quation with ion thrmal ynamic in toroial plama A. Zilr a) Max-Planck-Intitut für Plamaphyik, EURATOM Aoation, 85748 Garching, Grmany J. F. Drak an B. Rogr Intitut for Plama Rarch,
More informationY 0. Standing Wave Interference between the incident & reflected waves Standing wave. A string with one end fixed on a wall
Staning Wav Intrfrnc btwn th incint & rflct wavs Staning wav A string with on n fix on a wall Incint: y, t) Y cos( t ) 1( Y 1 ( ) Y (St th incint wav s phas to b, i.., Y + ral & positiv.) Rflct: y, t)
More information22/ 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 informationSection 11.6: Directional Derivatives and the Gradient Vector
Sction.6: Dirctional Drivativs and th Gradint Vctor Practic HW rom Stwart Ttbook not to hand in p. 778 # -4 p. 799 # 4-5 7 9 9 35 37 odd Th Dirctional Drivativ Rcall that a b Slop o th tangnt lin to th
More informationIntroduction 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 informationElectrochemistry L E O
Rmmbr from CHM151 A rdox raction in on in which lctrons ar transfrrd lctrochmistry L O Rduction os lctrons xidation G R ain lctrons duction W can dtrmin which lmnt is oxidizd or rducd by assigning oxidation
More informationA new idea to search for charged lepton flavor violation using a muonic atom
Journal of Physics: Confrnc Sris OPEN ACCESS A nw ida to sarch for chargd lpton flavor violation using a muonic atom To cit this articl: Jo Sato 2014 J. Phys.: Conf. Sr. 485 012036 Rlatd contnt - Sarch
More informationAlpha 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