ultra-peripheral collisions at rhic spencer klein, lbnl for the star collaboration
DESCRIPTION
Ultra-peripheral Collisions at RHIC Spencer Klein, LBNL for the STAR Collaboration. Ultra-peripheral Collisions: What and Why Vector meson interferometry STAR Results: Au + Au --> Au + Au + r 0 r 0 production with nuclear excitation Direct p + p - production & interference - PowerPoint PPT PresentationTRANSCRIPT
Ultra-peripheral Collisions at RHICSpencer Klein, LBNL
for the STAR Collaboration
Ultra-peripheral Collisions: What and Why
Vector meson interferometry
STAR Results:
Au + Au --> Au + Au + 0
0 production with nuclear excitation
Direct +- production & interference
e+e- pairs
2001 Plans - STAR, PHENIX, PHOBOS
Conclusions
Coherent Interactions b > 2RA;
no hadronic interations <b> ~ 40 fermi
Ions are sources of fields photons
Z2
Pomerons or mesons (mostly f0) A 2 (bulk) A 4/3 (surface)
Fields couple coherently to ions P < h/RA, ~30 MeV/c for heavy ions
P|| < h/RA ~ 3 GeV/c at RHIC
large cross sections Enormous variety of reactions
Au
Au
Coupling ~ nuclear form factor
, P, or meson
Specific Channels Vector meson production
A -- > ’, , , J/,… A Production cross sections --> (VN) Vector meson spectroscopy (, , ,…) Wave function collapse Multiple vector meson production
Electromagnetic particle production
leptons,mesons Strong Field QED
Z ~ 0.6 meson spectroscopy
~ charge content of scalar/tensor mesons particles without charge (glueballs) won’t be seen
Mutual Coulomb excitation (GDR & higher) Luminosity measurement, impact parameter tag
Production occurs in/near one ion
VM
e+e-, qq,...s
Z ~ 0.6; is N > 1?
Exclusive 0 Production
One nucleus emits a photon The photon fluctuates to a qq pair The pair scatters elastically from the other nucleus
also Photon- meson contribution qq pair emerges as a vector meson is large: 380 mb for with Au at 130 GeV/nucleon
5% of hadronic cross section 120 Hz production rate at full RHIC energy/luminosity
10% of hadronic cross section , , , * rates > 5 Hz J/’, *, *, all copiously produced, a challenge
Au
Au
0
Interference 2 indistinguishable possibilities
Interference!! Similar to pp bremsstrahlung
no dipole moment, so no dipole radiation
2-source interferometer separation b
,, , J/ are JPC = 1- -
Amplitudes have opposite signs ~ |A1 - A2eip·b|2
b is unknown For pT << 1/<b>
destructive interference
No Interference
Interference
pT (GeV/c)
y=0
Entangled Waveforms VM are short lived
decay before traveling distance b Decay points are separated in space-time
no interference OR
the wave functions retain amplitudes for all possible decays, long after the decay occurs
Non-local wave function non-factorizable: +- + -
Example of the Einstein-Podolsky-Rosen paradox
e+
e-
J/
+
-
J/
b
(transverse view)
+
Multiple meson production P(0) ~ 1% at b=2RA
w/ Poisson distribution P(00) ~ (1%)2/2 at b=2RA ~ 106 00 /year
Identical state enhancement (ala HBT) for production from same ion (away from y=0) p < h/RA
Like production coherence reqt. Large fraction of pairs
Stimulated decays?
b (fermi)
P(b
)
Looking further ahead…. A --> ccX, bbX, ttX (at LHC)
sensitive to gluon structure function high rates leptons/mass peak/separated vertex. backgrounds from grazing hadronic ints.
Double-Pomeron interactions in AA prolific glueball source narrow range of b
small to moderate cross sections harder pT spectrum
experimental signature? Double-Pomeron interactions in pp
pT is different for qq mesons vs. exotica? Tag pomeron momenta with Roman pots
Production occurs in one ion
QQ-->open charm
Transverse view: anarrow range of impact parameters
g
glueballs
Triggering Strategies Ultra-peripheral final states
1-6 charged particles low pT
rapidity gaps small b events
‘tagged’ by nuclear breakup
Nuclear Excitation
Nuclear excitation ‘tag’s small b Multiple Interactions probable
P(0, b=2R) ~ 1% P(2EXC, b=2R) ~ 30%
Factorization appears valid EXC
useful for triggering select small b for interference studies
Au* decay via neutron emission
)()( 022 bPbbPd EXC
Au
Au
P
Au*
Au*
(1+)0
Preliminary
Experimental Studies Exclusive Channels
0 and nothing else 2 charged particles net charge 0
Coherent Coupling pT < 2h/RA ~100 MeV/c
back to back in transverse plane
Nuclear breakup possible Backgrounds:
incoherent photonuclear interactions
grazing nuclear collisions beam gas
Peripheral Trigger & Data Collection Level 0 - prototype, circa 2000
hits in opposing CTB quadrants Rate 20-40 /sec
Level 3 (online reconstruction) vertex position, multiplicity Rate 1-2 /sec
7 hours of data ~ 30,000 events Backgrounds
cosmic rays beam gas upstream interactions out-of-time events
Exclusive 0 2 track vertex
vertex in diamond non-coplanar, < 3 rad
reject cosmic rays track dE/dx consistent with No neutrons in ZDC peak for pT < 100 MeV/c
asymmetric M peak and model background
matches pairs from higher multiplicity events scaled up by 2.1 flat/phase space in pT
mostly at low M()
0 PT
M()
Preliminary
‘Minimum Bias’ Dataset Trigger on >1 neutron signal
in both zero degree calorimeters
~800,000 triggers Event selection same as
peripheral but no ZDC cuts
and model background phase space in pT
small
0 PT
M()
Preliminary
Direct + - production
Direct + - is independent of energy The two processes interfere
1800 phase shift at M(0) changes + - lineshape
good data with p (HERA + fixed target) + - fraction should decrease as A rises
-
+
-
A -- > 0A -- > + - A
+
A -- > + - A
0
0 lineshape
Data
Fit
0
+-
Fit all data to 0 + +-
interference is significant+- fraction is high (background?)
ZEUS p --> (0 + +- )p
Set =0 for STAR
STAR Au --> (0 + +- )Au
Preliminary
P (GeV/c)
A peek at --> e+e-
‘Minimum bias dataset Select electrons by dE/dx
in region p< 140 MeV/c Select identified pairs pT peaked at 1/<b>
Eve
nts
Pt (GeVc)
dE/d
x (k
eV/c
m)
Blue - all particlesred - e+ e- pairs
e
Preliminary
2001 RHIC - higher luminosity, energy, longer run
larger cross sections STAR
improved triggering trigger in parallel with central collisions program 10-100X ‘topological’ data
expanded solid angle (FTPC, MWC,…) 10X minimum bias data
PHOBOS “interest in pursuing it, but will require major trigger reconfiguration
and enhancements before we can get serious data”
Coherent Peripheral Collisions in PHENIX
Study coherent two-photon and photonuclear interactions in coincidence with mutual Coulomb excitation of the nuclei. • Two central tracking arms ||0.35, = 290°• Global detectors (used for triggering): Zero-Degree Calorimeters, Beam-Beam Counters Trigger: Level 1 – ZDC coincidence, BBC veto
Level 2 – 1-5 tracks (hits) in each tracking arm
Goals for 2001: Observe 0 production in the reaction Au+Au Au*+Au*+0; 0 +- ,
A total integrated Au+Au luminosity of 300 b-1
should give a sample of about 20,000 0 ’s, Study the factorization of 0 production and Coulomb excitation, Try to see the 2-source interference in 0 production.
Physics Recap RHIC is a high luminosity and A collider Coherent events have distinctive kinematics Ultra-peripheral collisions allow for many studies
Measurement of (VA) Vector meson spectroscopy A measurement of the 0 pT spectrum can test if particle
decay triggers wave function collapse multiple vector meson production Strong field QED tests Studies of charge content of glueball candidates
Conclusions STAR has observed three peripheral collisions processes
Au + Au -- > Au + Au + 0
Au + Au -- > Au* + Au* + 0
Au + Au -- > Au* + Au* + e+e-
Interference between 0 and direct is seen Next year: higher energy, more luminosity, more data, more
experiments, more detector subsystems, ... More channels, cross sections, pT spectra,...
Ultra-peripheral collisions is in it’s infancy It works!!! come back next year!