Ultrarelativistic Heavy-Ions

Similar documents
1 The pion bump in the gamma reay flux

QGP Physics from Fixed Target to LHC

Lorentz invariant scattering cross section and phase space

Units. In this lecture, natural units will be used:

Relativistic Kinematics

Lecture 3. Experimental Methods & Feynman Diagrams

Ultra-Relativistic Heavy Ion Physics (FYSH551), May 31, 2013 Jan Rak and Thorsten Renk

2 Feynman rules, decay widths and cross sections

Inelastic scattering

Lecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2

1. Kinematics, cross-sections etc

Classical Scattering

Rutherford Backscattering Spectrometry

I. Elastic collisions of 2 particles II. Relate ψ and θ III. Relate ψ and ζ IV. Kinematics of elastic collisions

Heavy Ion Physics Lecture 3: Particle Production

Applied Nuclear Physics (Fall 2006) Lecture 19 (11/22/06) Gamma Interactions: Compton Scattering

Stefano Carignano 12/2010. Phenomenology of particle production in pp collisions

CHAPTER 2 ELECTRON-PROTON COLLISION

Problem Set # 2 SOLUTIONS

Properties of the S-matrix

2. Special Relativity (SR) explicit Lorentz transformations Particles with m > 0 can always be seen as boosted from their rest frame

Studying Nuclear Structure

Physic 492 Lecture 16

Massachusetts Institute of Technology Department of Physics. Final Examination December 17, 2004

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson V October 1, 2015

Coulomb Sum Rule. Huan Yao Feb 16,2010. Physics Experiment Data Analysis Summary Collaboration APS April Meeting

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

Elastic and inelastic cross section measurements with the ATLAS detector

2. Passage of Radiation Through Matter

NEW EXACT AND PERTURBTIVE SOLUTIONS OF RELATIVISTIC HYDRO A COLLECTION OF RECENT RESULTS

Investigation of jet quenching and elliptic flow within a pqcd-based partonic transport model

Measurements of the total and inelastic pp cross section with the ATLAS detector at 8 and 13 TeV

Physics with Tagged Forward Protons using the STAR Detector at RHIC. The Relativistic Heavy Ion Collider The pp2pp Experiment STAR 2009

FIRST MEASUREMENTS OF PROTON-PROTON ELASTIC SCATTERING AND TOTAL CROSS-SECTION AT THE LHC BY TOTEM

Monte Carlo radiation transport codes

Concept of Luminosity

Particles and Deep Inelastic Scattering

Spacetime and 4 vectors

Predictions for 5.02A TeV Pb+Pb Collisions from A Multi-Phase Transport Model

Calculating cross-sections in Compton scattering processes

Elliptic flow. p y. Non-central collision of spherical nuclei or central collision of deformed nuclei. Overlapping zone is of almond shape

Accelerators and Colliders

Introduction to particle physics Lecture 2: Special relativity

Coulomb Sum Rule. Huan Yao Advisor: Zein-Eddine Meziani Work support DOE Grant: DE-FG02-94ER40844

Pomeron Intercept and Slope: the QCD connection

The special theory of relativity

Investigation of jet quenching and elliptic flow within a pqcd-based partonic transport model

Accelerator Physics Homework #3 P470 (Problems: 1-5)

Fall Quarter 2010 UCSB Physics 225A & UCSD Physics 214 Homework 1

PHYS 5012 Radiation Physics and Dosimetry

1 Tensors and relativity

A Brief Introduction to Relativistic Quantum Mechanics

Introduction to Elementary Particle Physics I

Lecture 8. CPT theorem and CP violation

PHY-494: Applied Relativity Lecture 5 Relativistic Particle Kinematics

arxiv:nucl-th/ v1 3 Jul 1996

Vector meson photoproduction in ultra-peripheral p-pb collisions measured using the ALICE detector

Figure 1: Grad, Div, Curl, Laplacian in Cartesian, cylindrical, and spherical coordinates. Here ψ is a scalar function and A is a vector field.

Radiative Correction Introduction. Hanjie Liu Columbia University 2017 Hall A&C Analysis meeting

Particle Interactions in Detectors

Elastic Scattering. R = m 1r 1 + m 2 r 2 m 1 + m 2. is the center of mass which is known to move with a constant velocity (see previous lectures):

Particle collisions and decays

Amplitude Analysis An Experimentalists View. K. Peters. Part II. Kinematics and More

Conservation of Linear Momentum : If a force F is acting on particle of mass m, then according to Newton s second law of motion, we have F = dp /dt =

Special Relativity. Chapter The geometry of space-time

Studies on the definition of inelastic Non-Single Diffractive events

Einstein Toolkit Workshop. Joshua Faber Apr

Jets and Diffraction Results from HERA

Lecture 3 Cross Section Measurements. Ingredients to a Cross Section

Pomeron Intercept and Slope: are they related?

Phys 622 Problems Chapter 6

Dr Victoria Martin, Spring Semester 2013

Quantum fields close to black hole horizons

Using Electron Scattering Superscaling to predict Charge-changing Neutrino Cross Sections in Nuclei

Measuring Inclusive Cross Sections in Hall C

Frigyes Nemes (Eötvös University) on behalf of the TOTEM collaboration

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

A study of φ-meson spin alignment with the AMPT model

PHYS1015 MOTION AND RELATIVITY JAN 2015 EXAM ANSWERS

Global Properties of Nucleus Nucleus Collisions

Quantum Field Theory Spring 2019 Problem sheet 3 (Part I)

Coulomb Corrections in Quasielastic Scattering off Heavy Nuclei

Radiative Processes in Astrophysics

Compound Nucleus Reactions

Measurement of Charged Particle Spectra in Deep-Inelastic ep Scattering at HERA

Single Particle Motion

Donie O Brien Nigel Buttimore

Overthrows a basic assumption of classical physics - that lengths and time intervals are absolute quantities, i.e., the same for all observes.

Inclusive distributions at the LHC as predicted from the DPMJET-III model with chain fusion

Eikonal method for halo nuclei

Database for Imaging and Transport with Energetic Neutral Atoms (ENAs)

GLAUBER MODEL FOR HEAVY ION COLLISIONS FROM LOW ENERGIES TO HIGH ENERGIES. P. Shukla. Nuclear Physics Division

arxiv: v3 [hep-ph] 14 Nov 2017

Decay rates and Cross section. Ashfaq Ahmad National Centre for Physics

Multi Lepton events at HERA

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

Proton-lead measurements using the ATLAS detector

Examples. Figure 1: The figure shows the geometry of the GPS system

Physics 214 UCSD Lecture 7 Halzen & Martin Chapter 4

Outline: Introduction and Motivation

Transcription:

Kinematics November 11, 2010 / GSI

Outline Introduction 1 Introduction 2 3 3

Notation Introduction A parallel to z-axis (beam): A A = A A transverse to z-axis: A = A A A = A Transverse mass: m = m 2 + p 2 m is invariant under Lorentz transformations along z-axis p = γ(p + vε) ε = m 2 + p 2 ε = γ(ε + vp ) γ = 1/ 1 v 2 p = p

Four vectors Introduction p µ = (p 0, p x, p y, p z ) (p 0, p) on shell = (ε, p) contravariant p µ = (p 0, p) covariant A µ B µ = A 0 B 0 A B four-vector product p 2 = p µ p µ = p0 2 p 2 on shell = ε 2 p 2 four-vector squared p 2 > 0 p 2 < 0 time like space like

Lorentz invariance (ε ) 2 ( p ) 2 = (ε) 2 ( p) 2 : p 2 Lorentz invariant m 2 Lorentz invariant Exponential spectra: dn m dm e m /λ p < 1 2 GeV λ: inverse slope parameter (apparent temperature) typical value λ 200 MeV ( ) λ 1 = d dm log dn m dm useful concept if dependence on m weak

Rapidity Introduction [ ] ( ) y = 1 2 log E+p p E p = arctanh E = arctanhv E = m 2 + p 2 = m 2 + p2 Rapidity is additive under Lorentz transformations along z-axis v = p E = tanh y p m = sinh y E m = cosh y To determine y in an experiment, need particle ID!

Pseudorapidity [ ] η = 1 2 log p +p = log [cot(θ/2)] = log [tan(θ/2)] p p Need only to measure angle θ p = p cosh η p = p sinh η sin θ = 1/ cosh η For m 0 (or for p ) η = y In general: dn dηd 2 p = p E dn dyd 2 p

CM frame Introduction In CM frame y η 0 central rapidity region (mid rapidity region) y = y P, y = y T projectile and target rapidity regions Central rapidity region: newly created particles, or original particles that have suffered several collisions dn dηd 2 p η=0 = p dn m dyd 2 p y=0 p = 0 p m = v < 1 dn/dη dn/dy (flattening of dn/dη)

Invariant cross section p = γ(p + vε) dp = γ(dp + vdε) = γ(1 + v p ε )dp ε = γ(ε + vp ) = γ(1 + v p ε )ε dp ε = dp ε Lorentz invariant ε dσ d 3 p = ε dσ = dσ d 2 p dp p dεd 2 Ω Invariant cross section

System expanding from a point (explosion) Ballistic trajectories: z = vt t v=z/t v=c Particle at (z, t) has velocity v = z/t Particle distribution g(z, t) = density of particles at (z, t) Change variables (z, t) (v, τ), τ = t 2 z 2 (proper time) f (v, τ) = g(z, t) Lorentz transformation f (v, τ) = f (v, τ) z τ = τ Rapidity: v = tanh y, y 1 = y 1 + y boost

If over a range in y τ t v=z/t f (y, τ) = f (τ) f is boost invariant In p p and A A collisions at very high energy, expect boost invariant dn/dy dn dyd 2 p = F(p ) ( y < y scaling < y beam ) If y scaling >> 1 a large range of Lorentz frames where system looks identical L.T. by V = v 2 : (v 2 t, t) (0, τ 2 ), τ 2 = t 1 (v 2 ) 2 z

Assumptions i) object created in inelastic collision interacts with the same σ inel ii) nuclei travel on straight lines Eikonal approximation classical approximation to angular momentum Elastic scattering amplitude f (s, t) = 1 2ip l (2l + 1) [ e 2iδ l 1 ] P l (cos θ) p 1 p 2 Mandelstam variables s = (p 1 + p 2 ) 2 t = (p 1 p 1 )2 p 1 p 2

Identical particles, CM frame s = 4(m 2 + p 2 ) 2t s 4m 2 = cos θ 1 Semiclassical approximation Large l, small θ pb = l + 1 2 P l (cos θ) 0 0 dφ 2π ei(2l+1) sin θ/2 cos φ dφ ei q b 2π

l + 1 2 pb l (l + 1 2 ) p2 db b f (s, t) = ip [ ] 2π d 2 b e i q b 1 e iχ(s, b) χ(s, b) = 2δ(s, b) Optical theorem σ tot = 4π p Im f (s, t = 0) = 2 d 2 b [ 1 Re e iχ] Elastic scattering Integrate over angles dω d 2 q p 2 (forward peaked) σ el = d 2 q 4π d 2 b d 2 b e i q b [ 1 e iχ] [ e i q b 1 e iχ ] 2 σ el = d 2 b 1 e iχ 2 σ in = σ tot σ el = d 2 b (1 e iχ 2)