the nucleus at a trillion degrees david morrison brookhaven national laboratory
TRANSCRIPT
The nucleus at a The nucleus at a trillion degreestrillion degrees
David MorrisonDavid Morrison
Brookhaven National LaboratoryBrookhaven National Laboratory
Where can we find it?Where can we find it?
early universe … tough. very tough.early universe … tough. very tough. high energy nuclear collisions.high energy nuclear collisions.
creates only very small quantities of stuffcreates only very small quantities of stuff the created stuff is the created stuff is veryvery short-lived short-lived requires a big acceleratorrequires a big accelerator requires complex detectorsrequires complex detectors tough … but doabletough … but doable
quarkshadrons
mesons baryons
pions,kaons,
...
protons,neutrons,
...
nucleons
protons neutrons
partons
quarks gluons
Some terminologySome terminology
High energy nuclear collisionHigh energy nuclear collision
contracted by effects of special relativity
impact parameter
Aftermath of a collisionAftermath of a collision
As seen by STAR experiment at RHIC
End-on view of high energy gold-gold
collision
• more than 5000 particles• you only see the charged particles here (there are also lots of neutral particles)• your eye doesn’t really see particle momenta, correlations, distributions
QuickTime™ and aSorenson Video decompressorare needed to see this picture.
Corona: 106 K
Center: 107 K
Surface: 6000 KSolar and Heliospheric Observatory (SOHO) satellite
Planck distributiondescribes intensityas a function of thewavelength of theemitted radiation
“Blackbody” radiation is the spectrum of radiation
emitted by an object attemperature T
E p
inte
nsity
transverse momentum
Systematic Errors not shown
Phobos Preliminary
Determining temperatureDetermining temperature
From transverse momentum
distribution deduce temperature of about 120 MeV
Energy densityEnergy density
A typical approachA typical approach use calorimeters to measure energy emitted use calorimeters to measure energy emitted
from collisionfrom collision estimate the volume of the collisionestimate the volume of the collision
obtain energy densities ranging up to obtain energy densities ranging up to several GeV/fmseveral GeV/fm33
Energy density in highest energy head-on Au+Au collisions – more than 5 GeV/fm3
Calorimeters in PHENIXCalorimeters in PHENIX
5 GeV/fm5 GeV/fm33. Is that a lot?. Is that a lot?Last year, the U.S. used about 100 quadrillion BTUs of energy:
At 5 GeV/fm3, this would fit in a volume of:
Or, in other words, in a box of the following dimensions:
Chemical equilibriumChemical equilibrium
2H2O + energy 2H2 + O2
time
conc
entr
atio
n of
O2
equilibrium concentration will depend on intensive quantities: T, p
t1 t2
Not just your usual quarksNot just your usual quarks
Not exactly the way I think of them …
Ordinary matter made of up and down quarks
Chemical equilibriumChemical equilibrium
With enough time, forward and reverse reactions will drive system to chemical equilibrium. Abundances will only depend on temperature and chemical potential.
One way to dig even deeperOne way to dig even deeper
hadron
hadron possible for “knock-possible for “knock-
on” collisions of on” collisions of partonspartons
seen in high-energy seen in high-energy physics experiments physics experiments since mid-1970’ssince mid-1970’s
a real particle physics a real particle physics phenomenon that can phenomenon that can be used to probe the be used to probe the trillion degree material trillion degree material we createwe create
Force between two quarksForce between two quarks
Compare to gravitational force at Earth’s surface
Quarks exert 16 metric tons of force on each other!
quark quarkgluons
A “jet” of particlesA “jet” of particles
as connection as connection between quarks between quarks breaks up, most of breaks up, most of the motion stays the motion stays close to direction of close to direction of the original quarksthe original quarks
the fragmented bits the fragmented bits appear as “normal” appear as “normal” subatomic particlessubatomic particles pions, kaons, …pions, kaons, …
kaon
pion
pion
pion
An algorithmAn algorithm a way to locate the a way to locate the
running of the bulls in running of the bulls in Pamplona, Spain:Pamplona, Spain:
1.1. start by finding one high-start by finding one high-momentum bullmomentum bull
2.2. look others moving in look others moving in roughly the same directionroughly the same direction
3.3. if the bull density is high, if the bull density is high, you might reconsider the you might reconsider the place you’ve chosen to place you’ve chosen to standstand
The next step is simple: just replace “bull” by “particle”
Case study: opacity of fogCase study: opacity of fog
““is this thing on?”is this thing on?” if you detect one if you detect one beam, at least know beam, at least know the source is onthe source is on
intensity of the “other” intensity of the “other” beam tells you a lotbeam tells you a lot
Pedestal&flow subtracted
angle away from initial high momentum particle
inte
nsity
same direction opposite direction
The matter we make …The matter we make …
is fantastically hotis fantastically hot has incredible energy densityhas incredible energy density only exists for an instant, but shows many signs only exists for an instant, but shows many signs
of equilibriumof equilibrium some properties are more straightforward to some properties are more straightforward to
explain in language of partonsexplain in language of partons very, very “sticky” – partons lose lots of energy very, very “sticky” – partons lose lots of energy
trying to get through ittrying to get through it being studied in dozens of ways – lots of new being studied in dozens of ways – lots of new
results anticipated at Quark Matter ‘04!results anticipated at Quark Matter ‘04!
Heavy-Ion Physics(materia in extremis)