Particle Physics WS 2012/13 ( )

Similar documents
Particle Physics WS 2012/13 ( )

Particle Physics WS 2012/13 ( )

Standard Model of Particle Physics SS 2013

Lecture 6:Feynman diagrams and QED

Particle Physics WS 2012/13 ( )

Electroweak Physics. Krishna S. Kumar. University of Massachusetts, Amherst

PRECISION&MEASUREMENTS&

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

IX. Electroweak unification

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Experimental Aspects of Deep-Inelastic Scattering. Kinematics, Techniques and Detectors

Dr Victoria Martin, Spring Semester 2013

Lecture 3 (Part 1) Physics 4213/5213

Physics at Hadron Colliders

Introduction to Elementary Particle Physics I

Particle Physics Lecture 1 : Introduction Fall 2015 Seon-Hee Seo

The achievements of the CERN proton antiproton collider

Standard Model of Particle Physics SS 2013

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

PRECISION MEASUREMENTS

Deep Inelastic Scattering in Lepton-Hadron Collisions Probing the Parton Structure of the Nucleon with Leptons Basic Formalism (indep.

Electroweak Physics and Searches for New Physics at HERA

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1

The God particle at last? Astronomy Ireland, Oct 8 th, 2012

Search for New Physics at HERA

Search for a Z at an e + e - Collider Thomas Walker

Particle Physics. Michaelmas Term 2011 Prof Mark Thomson. Handout 5 : Electron-Proton Elastic Scattering. Electron-Proton Scattering

Intro to Nuclear and Particle Physics (5110)

4. The Standard Model

Standard Model of Particle Physics SS 2012

Discovery of the W and Z 0 Bosons

The God particle at last? Science Week, Nov 15 th, 2012

Higgs couplings and mass measurements with ATLAS. Krisztian Peters CERN On behalf of the ATLAS Collaboration

Higgs Searches at CMS

Modern physics 1 Chapter 13

Lecture 3. Experimental Methods & Feynman Diagrams

Particle Physics. Dr Victoria Martin, Spring Semester 2012 Lecture 10: QCD at Colliders

Search for physics beyond the SM in ep collisions at HERA

Introduction to Neutrino Physics. TRAN Minh Tâm

Part II Particle and Nuclear Physics Examples Sheet 1

Outline. Charged Leptonic Weak Interaction. Charged Weak Interactions of Quarks. Neutral Weak Interaction. Electroweak Unification

Interactions/Weak Force/Leptons

Higgs Searches and Properties Measurement with ATLAS. Haijun Yang (on behalf of the ATLAS) Shanghai Jiao Tong University

Interactions/Weak Force/Leptons

Standard Model of Particle Physics SS 2013

Lecture 4: Antiparticles

Collider overview and kinematics

Hadronic events in e + e -

Physics at the Fermilab Tevatron Collider. Darien Wood Northeastern University

PoS(Photon 2013)071. Anomalous gauge couplings in W/Z exclusive pair production at the LHC. E. Chapon. C. Royon. O. Kepka

Interactions and Fields

Test of T and CP Violation in Leptonic Decay of. Yung Su Tsai. Stanford University, Stanford, California ABSTRACT

OUTLINE. CHARGED LEPTONIC WEAK INTERACTION - Decay of the Muon - Decay of the Neutron - Decay of the Pion

A Measurement of the Induced polarization of electro-produced Λ(1116) with CLAS

Weak interactions, parity, helicity

e e Collisions at ELIC

Standard Model of Particle Physics SS 2012

Discovery of Pions and Kaons in Cosmic Rays in 1947

Upgrade of ATLAS and CMS for High Luminosity LHC: Detector performance and Physics potential

Question. Why are oscillations not observed experimentally? ( is the same as but with spin-1 instead of spin-0. )

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

Standard Model of Particle Physics SS 2013

Higgs cross-sections

Searches for (non-susy) Exotics at HERA

High Energy Physics. Lecture 9. Deep Inelastic Scattering Scaling Violation. HEP Lecture 9 1

QCD and deep inelastic scattering

Risultati dell esperimento ATLAS dopo il run 1 di LHC. C. Gemme (INFN Genova), F. Parodi (INFN/University Genova) Genova, 28 Maggio 2013

P-P PHYSICS AT LHC. W and Z produc1on. Data and MC comparison. Lecture 4

FYS3510 Subatomic Physics. Exam 2016

Feynman Diagrams. e + e µ + µ scattering

Z boson studies at the ATLAS experiment at CERN. Giacomo Artoni Ph.D Thesis Project June 6, 2011

Particle Physics: Introduction to the Standard Model

Quantum ElectroDynamics III

Some of the experimental origins of the Electroweak Theory. Peter Fisher MIT August 18, 2006

Recent results from rare decays

Lecture 8. CPT theorem and CP violation

Lecture 10: Weak Interaction. 1

Subatomic Physics: Particle Physics Study Guide

Experimental Tests of the Standard Model. Precision Tests of the Standard Model

Particle Physics: Problem Sheet 5

Physics 217 Solution Set #5 Fall 2016

Search for New Physics at HERA

Particle Physics (SH/IM)

Experimental verification of the Salaam-Weinberg model. Pásztor Attila, Eötvös University Experimental Particle Physics Student Seminar

Tutorial on Top-Quark Physics

Measurements with Polarized Hadrons

6-8 February 2017 Hotel do Mar Sesimbra. Hands on Neutrinos

Electroweak Physics at the Tevatron

1 Introduction. 1.1 The Standard Model of particle physics The fundamental particles

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:

Identification of the Higgs boson produced in association with top quark pairs in proton-proton

La ricerca dell Higgs Standard Model a CDF

arxiv: v1 [hep-ex] 5 Sep 2014

Particle Physics WS 2012/13 ( )

Particle Physics. Tommy Ohlsson. Theoretical Particle Physics, Department of Physics, KTH Royal Institute of Technology, Stockholm, Sweden

Decays and Scattering. Decay Rates Cross Sections Calculating Decays Scattering Lifetime of Particles

arxiv:hep-ph/ v1 24 Jul 1996

The W-mass Measurement at CDF

Elementary Particles, Flavour Physics and all that...

Weak interactions and vector bosons

Transcription:

Particle Physics WS 2012/13 (9.11.2012) Stephanie Hansmann-Menzemer Physikalisches Institut, INF 226, 3.101

QED Feyman Rules Starting from elm potential exploiting Fermi s gold rule derived QED Feyman Rules e p 1 e p 3 incoming electron u(p 1 ) incoming positron v(p 2 ) 1 st vertex p 2 p 4 e + e + -im = i q e v e p 2 outgoing electron u(p 3 ) outgoing positron v(p 4 ) γ μ u e (p 1 ) igμν q 2 iq e u e p 3 γ ν v e (p 4 ) 2 nd vertex fermion current propagator fermion current at 1 st vertex at 2 nd vertex 2

e p 1 p 2 Calculation of cross section e + e - μ + μ - Lecture 3, diff. cross-section in CMS: e + μ + μ p 3 p 4 dσ = 1 p f M dω 64 π 2 s p fi 2 i lowest order diagram M ~ e 2 ~α em (NU: e= 4πα; α ~ 1 137 ) -im = i q e v e p 2 p 1 = p 2 = p i p 3 = p 4 = p f s = (E 1 + E 2 ) 2 γ ξ u e (p 1 ) igξν q 2 iq μ u μ p 3 γ ν v μ (p 4 ) For unpolarized beam need to average over all possible initial helicity combinations. spin averaged matrix element < M 2 > = 1 4 ( M RL XX 2 + M RR XX 2 + M LL XX 2 + M LR XX 2 ) 3

Matrix Element Calculation Computation was done for limit E>>m; note, several helicity combinations vanished! 4 4 4 4 M(RL RL) 2 M(RL LR) 2 M(LR RL) 2 M(LR LR) 2 4

Differential Cross Section The cross section is obtained by averaging over the initial states and summing over all final states. (E>>m μ p f = p ) i = dσ dω = 1 4 = 1 64 π 2 s p f p i M fi 2 1 ( M(RL RL) 2 + M(LR LR) 2 + M(RL LR) 2 + M(LR RL) 2 ) 256 π 2 s 4πα 2 256 π 2 s (2(1+cosθ)2 + 2(1-cosθ) 2 ) dσ = α2 dω 4s (1+cos2 θ) Example: e + e - μ + μ, s = 29 GeV pure QED (α 3 ) calculation QED + Z contribution 5 5

Total Cross Section Total cross section obtained by intregrating over θ and φ using 1 + cos 2 θ dω = 2π (1 + cos 2 θ) dθ = 16π 3 total cross section for (e + e - μ + μ ): σ = 4πα2 3s Lowest order computation provides good description of data Very impressive result: from first principle computation we have reached a 1% precise result! 6

Helicity and Chirality = σ 0 0 σ = σ 1 σ 1 σ 2 σ 2 helicity operator: h = Σp [H,h] = 0 Helicity is a conserved quantity! σ 3 Helicity is not a LI quantity! σ 3 (p is not a LI) chirality operator: γ 5 = i γ 0 γ 1 γ 2 γ 3 = 0 I I 0 in Dirac representation [H,γ 5 ] 0 Chirality is not a conserved quantity! Chirality is however LI! only for E>>m : γ 5 ~ Σp LH chirality eigenstates LH helicity eigenstates RH chirality eigenstates RH helicity eigenstates For massive particles (not ultra relativisitc): helicity states are combination of chirality states! 7

Chirality Eigenstates Only certain combinations of chirality eigenstates take part in elm IA (property of vertex coupling) u L γ μ u L, u R γ μ u R Right handed particles with right handed particles Left handed particles with left handed particles v L γ μ v L, v R γ μ v R Right handed antiparticles with right handed antiparticles Left handed anti particles with left handed antiparticles u L γ μ v R, u R γ μ v L, v R γ μ u L v L γ μ u R Right handed particles with left handed antiparticles Left handed particles with right handed particles Left handed antiparticles right handed particles Right handed antiparticles left handed particles Coupling strength for left handed and right handed particles is the same in elm. IA! 8

Content of Today We do already have e + e + μ + μ + e μ + Calculate cross-section for related process exploiting symmetries and Mandelstam variables e + μ e + μ e e e + μ and e + e + e + e + e e e e + + μ μ e + e e + e + Test of first order QED computations in e + e - collisions at TASSO Luminosity measurements exploiting e + e + e + e + Discovery of τ lepton in e + e - collisions 9

Time and Space Structure of Feynman Diagrams general 4 prong diagram (several first order QED diagrams have this structure) a) Time like s channel process p A p B p c p D choose CMS system p A p c s =q 2 =(p A +p B ) 2 = (E A +E B ) 2 (p A +p B ) 2 (m A +m B ) 2 > 0 real photon: q 2 = E 2 - p 2 = 0 p B t p D q 2 >0 virtual photon b) Space like t channel process p A p c t =q 2 =(p C -p A ) 2 = (E C -E A ) 2 (p C p A ) 2 p B p D t choose A at rest and m A =m C : E C > m C t = E c2-2e c m A +m 2 A - p c2 = m C2 2E C m A + m A2 < 0 q 2 <0 virtual photon 10

b) u channel process p A p B p c p D Mandelstam variables u =q 2 =(p D -p A ) 2 < 0 q 2 <0 virtual photon Mandelstam variables: s = (p A +p B ) 2 = (p C +p D ) 2 t = (p C -p A ) 2 = (p D -p B ) 2 u = (p D -p A ) 2 = (p C -p B ) 2 t Total cross/section or any LI invariant diff. cross-section can only depend on scalar products of 4-momenta p A, p B, p C, p D. p i p j 10 scalars: p A p A, p A p B, p A p C, p A p D p B p B, p B p C, p B p D, p C p C, p C p D, p D p D p 2 i = E 2 i - p 2 i = m 2 i four constraints energy + momentum conservation: (p A +p B = p C +p D ) four constraints 2 independent scalars describe the process, usually 2 of Mandelstam variables are chosen 11

Lorentz Invariant Representation of X-Section <M fi > 2 = 1 4 M fi 2 e p 1 μ = 1 4 ( M(RL RL) 2 + M(LR LR) 2 + M(RL LR) 2 + M(LR RL) 2 ) p 3 = e4 4 (2(1+cosθ)2 + 2(1-cosθ) 2 ) [Θ in CMS, E >> m] p 2 e + μ + p 4 <M fi > 2 is LI, would be good to express it in form of LI quantities! In CMS: p 1 = (E,0,0,E) p 2 = (E,0,0,-E) p 3 = (E,E sinθ, 0, E cosθ) p 4 = (E, -E sinθ, 0, -E cosθ) (p i ±p j ) 2 = m i 2 + m j 2 ± 2p i p j ~ ±2p i p j E>>m p 3 μ e θ e + p 1 p 4 μ + π-θ x z p 2 p 1 p 2 = 2E 2 ~ ½ (p 1 +p 2 ) 2 = 1 2 s p 1 p 3 = E 2 (1+cosθ) ~ -½ (p 3 -p 1 ) 2 = - 1 2 t p 1 p 4 = E 2 (1-cosθ) ~ -½ (p 4 -p 1 ) 2 = - 1 2 u <M fi > 2 = 2e 4 t 2 +u 2 s 2 12

e - μ - e - μ - e - e + μ - μ + e μ + p 1 p 3 p 1 e - μ - e - μ - e e p 3 e + p 1 p 1 p 2 p μ 4 p 2 μ μ p 2 p 3 p 3 p 2 p 4 p 4 p 4 s = (p 1 +p 2 ) 2 t = (p 3 -p 1 ) 2 u = (p 4 -p 1 ) 2 (p 1 -p 3 ) 2 = t (-p 2 -p 1 ) 2 = s (p 4 -p 1 ) 2 = u <M fi > 2 = 2e 4 t2 +u 2 s 2 <M fi > 2 = 2e 4 s2 +u 2 t 2 13

e - μ - Scattering in CMS In CMS: p 1 = (E,0,0,E); p 2 = (E,0,0,-E); p 3 = (E,E sinθ, 0, E cosθ); p 4 = (E, -E sinθ, 0, -E cosθ) p 1 x s = 4E 2 z t = (p 3 -p 1 ) 2 e π-θ p 3 θ e μ p 2 ~ -2p 3 p 1 = -2E 2 (1-cosθ) u = (p 4 -p 1 ) 2 ~ -2p 4 p 1 = -2E 2 (1+cosθ) <M fi > 2 = 2e 4 s2 +u 2 t 2 = 2e 2 4 4+ 1+cosθ 1 cosθ 2 p 4 μ dσ = 1 p f <M dω 64 π 2 s p fi > 2 i = e4 8π 2 s 1+ 1 4 1+cosθ 2 1 cosθ 2 = e 4 8π 2 s 1+ 1 4 1+cosθ 2 4 sin 4 θ/2 sideremark: almost Rutherford, for Rutherford need non-relativisitc computation 14

Bhabha-Scattering e + e + e + e + M = M 2 M 1 e e + + e e e + e e + e + M 2 = M 1 2 + interference + M 2 2 same as for e - e + μ - μ + same as for e - e + e - e + dσ dω = e4 8π 2 s t 2 + u 2 s 2 + 2u 2 t + s 2 + u 2 2 t 2 15

Overview from Halz from Halzen and Martin 16

dσ dω Scatter Processes in e + e - Bhabha scattering: t+s channel e e e e Z e + e e + e - e + e + e + e + t-channel less sensitiv to contributions from Z exchange, even at larger energies. QED computation have precision of 10-4 Exploit forward region for luminosity measurements e + e γγ s-channel only e + e μ + μ- e μ+ e μ + exploited for luminosity measurements e + μ e + Z μ 17

Luminosity Determination at e + e - Machines Interaction rate: N IA = σ IA x L Number of observed events: N IA = σ IA x L dt = σ IA L dt σ IA : interaction cross-section L: luminosity, depends on machine parameters [cm 2 /s] L int = L dt [barn -1 ] L = 1 n B f n 1 n 2 4π σ x σ y n 1, n 2 : particles per bunch n B : number of buches f : revolution frequency σ x, σ y : beam size at IA point determination of delivered integrated luminosity from machine parameters not precise enough (± 5-10%) Instead a known reference process with known x-section is used to determine the integrated luminosity L int = N ref σ ref 18

Luminosity Determination at e + e - Machines Reference process for e + e - machines: small angle Bhabha scattering, precisely known, very high rate, very little background e + e + e - e - main detector L int = N(e+ e ) θ σ min < θ < θ max ref Luminosity monitors e.g. forward calorimeters Typical ranges for angles: 15 < θ < 35 (other standard candle Z μμ) 19

L3 Detector at LEP LEP: Large Electron Positron Collider, CERN, E CM = 90 GeV. SLUM: Silicon luminosity detector LCAL: Luminosity calorimeter collision center 20

Bhabha Scattering Event in LEP LCAL 21

Experimental Test of QED: Tasso Experiment PETRA: Positron-electron collider (DESY, Hamburg), E CM up to 35 GeV Started data taking in 1976, finished data taking in 1986 Tasso: Two Arm Spectrometer Solenoid [Tasso experiment is famous for discovery of the gluon] 22

How to test for possible deviations in e + e - e + e - ------ theory prediction (dominated by t-channel) data points Perfect agreement! - how to quantify perfect? Possible deviations from QED: Finite extension of lepton modified photon propagator Description and parametrization of deviation by form factor: F(q 2 ) = 1 ± 1 q 2 1 q 2 ± 1 q 2 Λ ± 2 q 2 q 2 2 Λ ± In this choice of form factor parameterization F(q 2 ) describes an add. massive photon which modify the propagator. Parameter Λ ± would correspond to the photon mass of add. photon. 23

How to test for possible deviations in e + e - e + e - dσ dω = e4 8π 2 s t 2 + u 2 s 2 F t 2 + 2u2 t 2 F t F s + s2 + u 2 t 2 F(s) 2 A fit to the Tasso data results in: Λ + > 435 GeV, Λ - > 590 GeV @ 95% CL In the space picture form factor correspond to modified Coulomb potential: 1 r 1 r (1 + e Λr ) extended charge For Λ > 500 GeV Point-like electron: < 0.197 fm/500 = 0.5 10-18 m 24

Test of QED in e + e - μ + μ - Total cross section Very good agreement σ(e+e- μ+μ-) = e4 3s (1 ± s s Λ ± 2) Λ ± > 250 GeV R μμ = σ exp σ th muon substructure < 10-18 m 25

Test of QED in e + e - μ + μ - Total cross-section in very good agreement, however angular distribution deviates from QED predictions effect of electroweak interference e μ + e μ + + e + μ e + Z μ backward region forward region A FB = σ F σ B σ F + σ B Due to interference effect of EW contribution already seen at s = 30 GeV! 26

Discovery of the Tau Lepton 1975 M. L. Perl, leader of Mark-I experiment at SLAC Nobel prize 1995 SPEAR: Standford-positron-electron-accelerator ring E CM up to 8 GeV Mark-I experiment 27

Discovery of the Tau Meson physics process: e + e - τ + τ Signature in experiment: e + e - e ± μ + 2 undetected particles e + v τ ν e μ - v μ ν τ + CC in e+e- collisions we know the initial 4 momenta, thus we can check for missing energy in the final state

Mark-I experiment μ e

Discovery of the Tau Lepton signature: e + e - e ± μ + 2 undetected particles Background process: e + e - e + e and e + e - μ + μ with one leg in the final state mis/identified as electron/muon respectively; cut on θ copl >20 reduced this background significantly e + e - μ + μ - e + e - Very rare decay, cross check: look for same sign e - μ - and e + μ + combinations hadron mis-id background (h: hadron) e + e - μ + h - X, e + e - h + e - X, e + e - h + h - X 4.7 ± 1.5 background candidates from these sources 24 signal candidates clear signal, not compatible with background fluctuations 30

Discovery of the Tau Lepton M m : missing energy M i : invariant mass of (e,μ) No resonance observed, thus at least 2 missing particles in final state threshold behaviour indicates mass of tau particle 2m τ ~ 4 GeV

Measurement of Tau Mass Later measurement at BESS (1994):

Point like nature of τ Particle As for e+e- μ+μ- 1 st order QED prediction of total cross-section for e + e - τ + τ - in wonderful agreement (differential cross-section suffers from interference with Z exchange diagram) Λ± > 200 GeV another point like (elementary) particle 33

Summary Two add. variables (beside all masses and 4 momenta of initial particles) are required to describe scatter process A+B C +D. E.g. use 2 out of 3 (LI) Mandelstam variables Symmetry arguments can be used to relate cross-section of different scatter process (technical: swap of Mandelstam variables in cross-section formular) First order QED correction describe well the total cross section in data (for e + e - e + e -, e + e - μ + μ -, e + e - τ + τ - ) This is mainly related to the strong supression of higher order diagrams α ~1/137 Differential cross-section is affected by interference with Z exchange diagram (can be computed as well) Next time :continue test of QED in e + e - scattering hadronic resonances in e + e - scattering higher order corrections and renormalization (running coupling constants) 34