what do we study nucleosynthesis builds nuclei up to he nuclear force…nuclear physics universe too...
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What do we study
Nucleosynthesis builds nuclei up to HeNuclear Force…Nuclear Physics
Universe too hot for electrons to bindE-M…Atomic (Plasma) Physics
E/M Plasma
Too hot for quarks to bind!!!Too hot for quarks to bind!!!Standard Model (N/P) Physics
Quark-Gluon
Plasma??
Too hot for nuclei to bindNuclear/Particle (N/P) Physics Hadron
Gas
SolidLiquidGas
Today’s Cold UniverseGravity…Newtonian/General Gravity…Newtonian/General
RelativityRelativity
Structure of matter in the Universe
scale ~ 10-15 m
scale ~ 10-10 m
Huge scale Iron
Wood
3
1
3
1
3
1
3
2
3
2
3
2
UniverseGravitational
Electromagnetic
Strong
Leptons: electron, muon, etc
Current building block
Quarks are Confined inside Particles
Strong Interaction (QCD)
•Strong interaction is mediated by gluons
•Both gluons and quarks has “color” charge.
• V(r) = -kV(r) = -k11/r + k/r + k22rr, , kk22 1 GeV / 1 GeV / fm, constant force.fm, constant force.
Electromagnetic Interaction
• Force (r) ~ 1/r2
• Two charges can be broken apart and set free
As two quarks are pulling away, energy increase. Color string fragment into new pairs of quark. Single quarks are confined inside particles. When energy is high enough, it forms a jet.
How to Liberate Quarks and Gluons
Increase Temperature and/or Pressure
Bayon (pressure)pressure
Water molecule is liberated with high T and P
Librated Quarks and Gluons
1,500,000,000,000 K~100,000 times higher temperature than the center of our sun.
One Way to Increase Temperature or Pressure
Small “Bang”
Heavy alien object hits the heavy earth
Tremendous kinetic energy converted into tremendous heat and pressure.
One (Nuclear Physicist’) Way to Increase Temperature or Pressure
Mini “Bang”
Heavy (Au) Nuclei hits the heavy (Au) Nuclei
Tremendous kinetic energy converted into tremendous heat
One (Real Nuclear Physicist’) Way to Increase Temperature or Pressure
Mini “Bang”
Heavy Nuclei hits the heavy Nuclei
Tremendous kinetic energy converted into tremendous heat
Different Stage after the Collision
• Right before the collision.
• Instantly (< 1 fm/c) after the collision. Highest energy density (15GeV/fm3).
• After ~1fm, system thermalized, i.e. thermal equilibrium. Temperature is the same everywhere.
Hadron continue to interact with each other elastically. Hadron is not changed but the momentum distribution does. At Kinetic freezout, the elastic interaction between hadrons stop. Hadron spree out and detected by the experiment
System continue the expension and cool down. Quarks and gluons start to fragment into hadrons. The particle ratio kept on changing due to the chemical reactions. At the point of Chemical Freezout, the chemical reaction ceased
What are the probes.
• soft hadron: Pions, kions, protons, etc
•coming from the fragmentation process after chemical freezout.
•To study their behavior (cross section, correlation, suppression, etc) can leads to the estimation of the QGP properties, e.g. temperature, pressure, energy density.
• Penetrating probes: direct photons, jet, heavy flavor, etc
•Coming from the QGP, i.e. before the chemical freezout. Directly bring the information of the QGP properties.
What are Detected
Detector in Rphi plane
particle tracks
beambeam
• collision vertex
• particle momentum (px, py, pz) right after the collsion through bending curvature in the magnet field.
• particle energy (photon, no bending in the magnet field).
• particle species identification through, e.g. energy loss (dE/dx) and particle speed (time of flight), cerenkov radiation, etc.
Take what is necessary: trigger
target
trigger
• soft hadron production ……………………………..…………… Minimum-bias trigger
• Direct photons ………………………………………..…………… photon trigger
• High pT particles (belong to jet). ………………………………….. High pt trigger
•J/psi, D meson production. ………………….…………………… J/psi, D meson trigger
• ………………………..
• One can take all the collision events with enough resources.
• Not every collision is interesting.
• heavy flavor, photon are very rare.
What is needed for the result to be publishable
The result, in principle, need to be independent of a specific experiment.
An experiment is specific in it:
• detector acceptance (Accp):
•N (accepted by the detector)/N (produced from the collision).
•Detector efficiency (Eff).
• HV trip, construction flaw. The efficiency < 100%
•Experiment trigger efficiency (Trg_eff).
•Trigger always biased,
•e.g. photon trigger: only accept events with hits above a certain energy.
pT
accp
x
y
pT
Trg_eff
Example of Publishable Results.
• cross section (σ): a Lorentz invariant measure of the probability of interactions. It has dimension of area (unit cm2 or barn )
• σ x L = N(events), where L is the luminosity, i.e. the intensity of the beams
effTrgEffAccp
photonN
Nppphoton
collision _
)(1)()(
How to Study QGP
• Nuclei is made of protons and neutrons: p+p collision is a natural reference (note: QGP may have already been produced by p+p collisions: ask Rolf and Brijesh)
• Behavior Quarks and gluons in a static nuclei is different from that in proton.
• Cold nuclear effect, or initial state nuclear effect, i.e. before collisions
• p(d)+Au can quantify this effect.
• New matter is produced after the collisions ( hot or final state effect).
time
p+p
d+Au
Au+Au
Study QGP in different Centrality
Most Central events (highest multiplicity), e.g. top 5% central, i.e. 5% of the events with largest multiplicity
Mid Central events
Most Peripheral events
From most central to most peripheral event, the collision is more like a p+p collisions.
One can also collision smaller size of nuclear, e.g. Cu+Cu, Si+Si, instead of Au+Au to gain more luminosity.
N_coll: 8 N_part: 6
Centrality can be quantified by the number of collisions (N_coll) and number of participants (N_part) through the glauber model calculation with
Ways to Reveal the QGP properties---RAA
• nuclear modification factor (RAA):
)__()(
)(
tsparticipanorcollisionsNppyield
AuAuyieldRAA
)__()(
)(
tparticipanorcollisionsNppyield
AudyieldRdA
RAA ( or RdA)
No medium effect
Au + Au Experiment (200GeV) d + Au Control Experiment (200GeV)
Preliminary DataFinal Data
Cronin enhancement: parton pT smearing from random kick before collisions (i.e. initial state effect)
Energy loss: parton loss lots of energy (dE/dx = ???GeV/fm) through bremsstrahlung when pass through the new state of matter (final state effect)
coneRWays to Reveal the QGP properties---Jet correlation
Calculate angle between two jet particles
trigger
Adler et al., PRL90:082302 (2003), STAR
near-side
away-side
Energy dissipated when parton pass through opaque medium. How?
Particle ratio is determined by Temperature and chemical potential
• abundances in hadrochemical equilibrium
Ways to Reveal the QGP properties---particle ratio
1
1
2 /3
3
22
Tmp
hhBh
e
pdVgN
lesantipartic and
,.......,,,,,,,,,, DdpKKh
>= critical temperature
A Movie of Glass Bead Show Liquid Behavior
http://www-news.uchicago.edu/releases/07/071106.liquids.shtml
Decreasing the number of glass beads in the cross section of the jet changes the behavior of the granular stream after hitting the target from liquid-like pattern to one that looks like fireworks. This latter pattern is more characteristic of how individual particles would behave after hitting a wall.
A Movie of Glass Bead Show Liquid Behavior
http://www-news.uchicago.edu/releases/07/071106.liquids.shtml
More Materials
• RHIC white paper: for physics understanding– J. Adams et al., Nucl. Phys. A 757, 102 (2005); K. Adcox et al., Nucl. Phys. A
757, 184 (2005) ; I. Arsene et al., Nucl. Phys. A 757, 1 (2005); B. B. Back et al., Nucl. Phys. A 757, 28 (2005).
• CERN detector and analysis brief book: For nice explanation of jargon in this field. – http://physics.web.cern.ch/Physics/DataAnalysis/BriefBook/
– http://physics.web.cern.ch/Physics/ParticleDetector/BriefBook/