Properties of nuclear matter from subtheshold strangeness production
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Transcript of Properties of nuclear matter from subtheshold strangeness production
Properties of nuclear matter from subtheshold strangeness production
Christoph Hartnack, Helmut Oeschler, Jörg AichelinSubatech Nantes and TH Darmstadt
Outline:● Subthreshold production, optical potential● Spectra, temperatures and KN rescattering● Azimuthal distribution and the KN potential● Scaling laws and the nuclear equation of state● Conclusion
Calculations performed with IQMD, a semiclassical, microscopic N-body model with quantum features for the description of HICs on an event-by-event basis
Subthreshold kaon production•Production of kaons at energies below the kinetic threshold for K production in elementary pp collisions
•Fermi momenta may contribute in energy
•Multistep processes can cumulate the energy needed for kaon production
•Importance of resonances (especially the) for storing energy
•Short livetime of resonance favors early production at high densities
•Sensitivity to in-medium effects and nuclear equation of state
Time-evolution & kaon production
K+: early, multistep induced product. when baryon density is highest
K-: prod. later when pion density is highest, strangeness exchange
0fm/c
4fm/c
8fm/c
12fm/c
16fm/c
20fm/c
In medium effects on kaons•KN-Rescattering,
absorption for K-
•Optical potential: repulsive for K+, attractive for K-
Penalizes K+ production at high densities but favors K- production at high densities
Effects yields but also dynamics
Parametrization from Schaffner-Bielich RMF results
Au-data: Foerster et al, KaoS
Ni-data: Uhlig et al., KaoSKN pot
No Pot
Can we reveal the KN potential from K+ yields?
Visible difference between calculations with and without KN potential on a log-scale. KN-pot yields less kaons, but incertainties on induced cross sections discourage a preliminary conclusion.
K- production dominated by strangeness exchange
BB+B
+Y+BY
Direct channels BB, B enhanced by K- potential, similar forexchange channels Y+BY. The K+ potential penalizes hyperon production and compensates in the dominant channels Y+BY.
BB+B+Y+BY
Spectra: slopes dominated by KN-rescattering
K+
K-
Rescattering potential
Strong enhancement of the slope from initial to final mom.
Slight effects: enhancement (K+) or reduction (K-)
K+ rescatter
Collision number
High K+ rescattering less K- rescattering
Temperatures of K+
IQMD results with KN-rescattering are in good agreement with KaoS data
K+ heated up by coll. with expanding nucl.medium
K- show systematically lower temperatures.
Reason: less rescattering, diff. potentials?
KaoS
A.Förster et al. PRC75(2007) 024906
Azimuthal distributions
Azimuthal distributions are effected by rescattering and by the optical potential.
While the rescattering acts in the same direction for K+ and K- the optical potential gives opposite effects for K+ and K-
Azimuthal distribution fitted with
a (1+v1 cos() + 2 v2cos(2))
KaoS and FOPI see opposite signs of v2 for K+ and K-
Ni+Ni 1.93 GeV,
F. Uhlig et al, KaoS
Excitation function of v2 for K+
Rescattering and optical potential are needed to describe the v2 of kaons.
The effects of the optical potential become dominant with respect to the effect of rescattering when going down in beam energy.
This is in agreement with calculations of Li&Ko who found a strong potential effect for Au+Au 1 GeV/A.
Comparison of v1(y0) to FOPI data
Preliminary data from FOPI (Kim et al. ) favor an optical potential less strong than implemented by us
The original idea of measuring the eos
•Eos describes the energy needed to compress nuclear matter
•A hard eos requires more energy for a given density than a soft one
•For a given density and a given available energy a soft eos leaves more thermal energy to the system than a hard eos
•R.Stock: This thermal energy could be measured by regarding pion production
At which density can we measure the eos?
Different densities are reached for hard and soft eos. A soft eos yields higher densities than a hard eos.
The differences in compressional energy and thus in thermal energy become less. The pion number is not sensitive enough. Pions come out late due to reabsorption in dense matter
Kaons might be an interesting probe. However the effects of the optical potential and incertainties of the cross section do not allow a direct measure of the eos from kaon yields.
The solution: ratios Au/C
Data: Ch.Sturm et al.
RQMD: Ch. Fuchs
Robust against changes of cross sections, optical potential, Delta lifetimes, etc.
KaoS data support soft eos
IQMD supports this
Symbols: KaoS data
Lines IQMD
Au: central versus peripheralDifferent cross sections and potential parameters may change the global yield. However, the parameter for the increase of the kaon yield N with the number A of participating nucleons (raising with centrality)
N(K)=N0 Adepends on the eos.
central
peripheral
A soft eos yields higher values than a hard eos.
Determination of the eos from
soft hard
The relation between the compression modulus and is monotonously falling.
KaoS data (Förster et al.) favor a value below 200 MeV, i.e. a soft eos.
C.H. et al. PRL 96 (2006) 012302
KaoS:Förster et al.
Same for Au/C ratio
Another scaling systematics: system size
2 independent observables ( centrality scaling and system size scaling) confirm soft eos
System size, Kaos Data
Apart in Au+Au from KaoS agrees with that
Scaling with system size in inclusive A+A events
Kaons and density isomers•Could reveal density isomers by a sudden rise in the excitation function of kaons - KaoS might measure it
Density isomers yield up to factors of 10 in K+ production
A 2ndminimum would yield a sudden factor of 10 in the kaon yield 600
800MeV
C.H. et al. PRL 72 (1994) 3767
Effect related to subthreshold prod.
A density isomer would have needed the strong raise indicated by the arrows.
IQMD calculations using a KN optical potential and a soft eos are consistent with KaoS data on Au+Au and C+C of Sturm et al.
For higher densities/beam energies we need other particles produced below threshold
KaoS DATA: no isomer up to 30
Conclusions
• Kaon spectra reveal strong rescattering of kaons with the surrounding nuclear matter
• Comparison of flow variables supports the existence of KN optical potential
• Scaling laws of the kaon production claim strongly for a soft equation of state
• The KaoS measurements (which can be continued by eos data) contradict the existence of density isomers at moderate densities
Effect of the potential: penalty reimbursed
Kaons with did not undergo collisions:
No KN potential : final=initial
•Initial distributions show a difference of calculations with KN-pot and without pot at all energies. This is due to the penalty paid at the production.
•In the final state the kaons regain the paid penalty and the curves of both calculations become rather close
Only at small energies a lack remains stemming from those kaons which failed to be produced due to the penalty.
KN collisions change the spectra
Most kaons underwent many collisions before leaving.
They show a significant enhancement of the slope.
At the time before the freeze out of the kaons (about 12-20 fm/c) the nucleonic system is still hot and expanding. The kaons carry the temperature of that expansion phase.
initial
Comparison to data for K-
Less rescattering for the K- yield smaller temperature than for K+
Comparison of spectra for K+
Temperature: centrality dependence
Temperature and collisions
Maxwellian Demon
Au+Au 1.5 GeV azimuthal distribution
For Au+Au at 1.5 GeV weneeded both potential and rescattering to reproduce the results of Foerster et al.
Influence on v2(pT) at midrapidity
Again opposite effect on K+ an K- useful for balancing the effect of rescattering
FOPI and KaoS see opposite signs of v2 for K+ and K-
V2:pT dependence
Polar distributions
Polar distribution: rescattering and potential
Excitation function of K+
A observation which is robust
versus effects of production cross sections, KN-potential, -lifetime
NTsushimaN=.75 NN
Going down in beam energy
A soft eos yields 1.4 at E=0.8 AGeV, a hard eos yields 1.2
Limits for lower E: no asymptotic yield for peripheral collisions
System size dependence
1.8
1.5
Einc
1.2
1.0
0.8
0.6
A soft eos obtains higher kaon yields for heavy systems
KaoS: PRC in preparation
A mixture of both
NC=0 has a visible fraction to the yield, shows a taller rapidity distribution and strongly negative flow.
For NC>2 a positive flow and a wider y-distribution is observed
The potential shifts to negative flow
NC=0: initial shadowing boosted by potential to strong neg. flow
NC>2: initial bias, enhanced by scattering, reduced by potential
Initial vs final Pot vs. NoPot
Final flow a superposition of different flows
Initial flow: bias for having collisions or notFinal flow: visible shift from the potential
Rescattering enhances potential effect
For NC=0 the initial flow is invertedRescattering adds up more positive flow