probing high density eos of neutron rich matter in heavy
TRANSCRIPT
Probing high density EOS of neutron rich
matter in heavy ion collisions
Y. Leifels for the FOPI and ASY-EOS collaborations GSI Helmholtzzentrum für Schwerionenforschung GmbH Darmstadt
XXVII Texas Symposium on
Relativistic Astrophysics
Dallas, December 8-13, 2013
transient state non-equilibrium, dynamical system thermal pressure, temperature and creation
of particles access to properties
microscopic transport models
Heavy ion collisions are unique tool to create states of high
density in the laboratory
Y. Leifels – Texas 2013 2
IQMD C. Hartnack
Central collisions
W. Cassing et al.
A. LeFevre et al.
Equation of state of nuclear/neutron matter
Y. Leifels – Texas 2013 3
Fuchs and Wolter, EPJA 30 (2006)
nuclear-many-body theory
/)(
)(O)(E)0,(E),(E
pn
4
sym
2
asymmetry parameter
Esym
E(,
)
(
MeV
)
Demorest et al. doi:10.1038/nature09466
Mass – Radius relation of neutron stars
0
2
22 )0T,(A/E
9
Compression modulus of E(,0)
Symmetry energy
Y. Leifels – Texas 2013 4
Fuchs and Wolter, EPJA 30 (2006)
0
d
)(dE3L
sym
0
slope
parameter
L small soft
SE bending over super soft
L large hard
=1.5
=0.5
used as:
Esym
= Esympot+Esym
kin
= 22 MeV·(ρ/ρ0)γ+12 MeV·(ρ/ρ0)
2/3
Testing pressure differences – Collective flow
Y. Leifels – Texas 2013 5
Elliptic flow v2
Side flow v1
P.
Da
nie
lew
icz e
t a
l. S
cie
nce
29
8,
15
92
(2
00
2)
Elliptic flow v2
Fourier expansion of azimuthal
distribution
protons
Au+Au
Elliptic flow
~d
dN
1 + 2v1cos() + 2v2cos(2)
parameterization of shape:
Elliptic flow at intermediate energies
Y. Leifels – Texas 2013 6
Au+Au
400A MeV
1.5A GeV
W. R
eis
do
rf et a
l, Nu
cl. P
hys. A
87
6 (2
01
2) 1
1.5A GeV
2)0(
2220
)0(
2
2220n2
Yvv)Y(v
vvv
beam energy (AGeV) v
2n
sensitive to EOS over a large
energy range
protons and light clusters
-v2
-v2
A. L
eF
evre
et a
l.
200 MeV
380 MeV
Constraining Esym - Elliptic flow of isospin pairs
Y. Leifels – Texas 2013 7
Experimental approach:
vary N/Z of collision system
(radioactive beams)
look at isospin pairs as probes
n/p 3He/3H π -π + K0/K+
observables: production ratios,
differences/ratios of spectra and
flows
neutron elliptic flow larger with a
‘hard’ density dependence of SE
→ investigate v2,n/v2,p or (v2,n-v2,p)
UrQMD: Qingfeng Li et al. / Y. Leifels
Data. W. Reisdorf et al.
-v2
-v2
Neutron/hydrogen elliptic flow in Au+Au collisions
Y. Leifels – Texas 2013 8
neutron squeeze-out in Au+Au collisions:
Y. Leifels et al., PRL 71, 963 (1993)
LAND 1 LAND 2
Forward Wall for
centrality and
reaction-plane
orientation
SB: shadow bar
for background
measurement
Large Area
Neutron Detector
acceptance:
in pt vs rapidity
Neutron/hydrogen elliptic flow
Y. Leifels – Texas 2013 9
Conclusion out of all available data:
n/p and n/H
by varying input parameters to the
model:
elastic NN cross sections
L = 85±40 MeV
intermediate
Au+Au
400A MeV
SE used in UrQMD model calculations P. Russotto et al. PLB 267 (2010)
P. Russotto et al., PLB 267 (2010)
v2
Neutron/hydrogen elliptic flow
Y. Leifels – Texas 2013 10
400A MeV
Towards model independence
Tested stability of results:
soft vs. hard 190<K<280 MeV
density dependence of sNN,elastic
asymmetry dependence of sNN,elastic
optical potential
momentum dependence of isovector
potential
Cozma et al. (Tübingen-QMD) :
L = 106±46 MeV
Russotto et al. (UrQMD):
L = 85±40 MeV
ruling out particular hard or soft Esym
statistics unsatisfactory
other observables?
M.D. Cozma et al., arXiv:1305.5417
P. Russotto et al., PLB 267 (2010)
Cozma et al.
Russotto et al.
The ASY-EOS experiment at GSI
Y. Leifels – SFAIR 2013 11 11
LAND CHIMERA
studied reactions: 197Au + 197Au @ 400 A MeV 96Ru + 96Ru @ 400 A MeV 96Zr + 96Zr @ 400 A MeV
CHIMERA, ALADIN Tof-wall,
μ-ball, for impact parameter
orientation and modulus
Testing density differences - The π-/π+ ratio
Y. Leifels – Texas 2013 12
Data described by various models with
stiff (or soft) density dependences of
the symmetry energy
Ferini et al. RMF stiffer for ratio up
Xiao et al. IBUU softer “
Feng & Jin ImIQMD stiffer “
Xie et al. ImIBL softer “
Data: W. Reisdorf et al., NPA 781 (2007)
Calculations: Z. Xiao et al, Phys. Rev. Lett. 102, 062502 (2009)
Au + Au central
Summary and conclusions
Y. Leifels – Texas 2013 13
At ~ (2-3)ρ0 , Ebeam=0.2 – 2 AGeV
multitude of experimental data help to
constrain the various input parameters to the
microscopic transport models
EOS of symmetric matter, in-medium
cross sections...
data support a soft Skyrme type EOS
P. Danielewicz et al., Science 298, 1592 (2002)
Symmetry energy at supra-saturation densities
very few data points at supra saturation densities
elliptic flow data
ratios or differences reduces influence of uncertainties in model
parameters
available data consistent with L~100+/- 45 MeV – new results soon
slightly harder than experiments at lower densities/astrophysical
observations
promising pion observables, but no consistent description
more data WITH radioactive beam will be available soon
Texas 2013 – Yvonne Leifels
New projects at radioactive beam facilities
RAON
SFAIR 2013 – Yvonne Leifels
The FOPI collaboration
A. Andronic, R. Averbeck, Z. Basrak, N. Bastid, M.L. Benabderramahne, M. Berger, P. Bühler,
R. Caplar, M. Cargnelli, M. Ciobanu, P. Crochet, I. Deppner, P. Dupieux, M. Dzelalija, L. Fabbietti, J. Frühauf,
F. Fu, P. Gasik, O. Hartmann, N. Herrmann, K.D. Hildenbrand, B. Hong, T.I. Kang, J. Keskemeti, Y.J. Kim, M.
Kis, M. Kirejczyk, R. Münzer, P. Koczon, M. Korolija, R. Kotte, A. Lebedev, K.S. Lee, Y. Leifels, A. LeFevre, P.
Loizeau, X. Lopez, M. Marquardt, J. Marton, M. Merschmeyer, M. Petrovici, K. Piasecki, F. Rami, V.
Ramillien, A. Reischl, W. Reisdorf, M.S. Ryu, A. Schüttauf, Z. Seres, B. Sikora, K.S. Sim, V. Simion,
K. Siwek-Wilczynska, K. Suzuki, Z. Tyminski, J. Weinert, K. Wisniewski, Z. Xiao, H.S. Xu,
J.T. Yang, I. Yushmanov, V. Zimnyuk, A. Zhilin, Y. Zhang, J. Zmeskal
and J. Aichelin, E. Bratkovskaya, W. Cassing, C. Hartnack, T.Gaitanos, Q. Li, D. Cozma
IPNE Bucharest, Romania, ITEP Moscow, Russia CRIP/KFKI Budapest, Hungary, Kurchatov Institute
Moscow, Russia, LPC Clermont-Ferrand, France, Korea University, Seoul, Korea, GSI Darmstadt, Germany, IReS Strasbourg, France, FZ Rossendorf, Germany, Univ. of Heidelberg, Germany, Univ. of Warsaw, Poland, RBI Zagreb, Croatia, IMP Lanzhou, China, SMI Vienna, Austria, TUM, Munich, Germany + P. Kienle (TUM),
T.Yamazaki(RIKEN)
SFAIR 2013 – Yvonne Leifels
Thank you
Star clusters young and old Chris Hetlage
APOD 2006, September 10
NUSYM 2013 – Yvonne Leifels FOPI
ASY-EOS
HADES
FOPI
KAOS
Inside IQMD
Y. Leifels – ASTRO 2013 20
after the convolution of the Skyrme type potentials supplemented by momentum dependent interactions (mdi) for infinite saturated nuclear matter at equilibrium
Testing density – Kaon production below threshold
Y. Leifels – SFAIR 2013 21
Independent on models and
details of the input (cross
sections, in medium
potentials etc.)
Testing densities at 2-3 ρ0
Data: C. Sturm et al., PRL 86 (2001) 39
IQMD: C. Hartnack et al., PRL96:012302,2006
RQMD: C. Fuchs et al., PRL 86 (2001) 1974
KAOS
Summary and conclusions
Y. Leifels – Texas 2013 22
At ~ (2-3)ρ0 data is consistent with a
soft Skyrme type EOS for symmetric
matter
confirmed for two different
observables within the same model,
which is describing reasonably well
all reaction data in this energy regime
absolute value may still model
dependent
more data will available at higher
densities with CBM@FAIR or NICA
In the relevant density regime soft
Skyrme type EOS follows closely the
A18+UIX+δν EOS of Akmal,
Pandharipande, Ravenhall
Phys. Rev. C, 58 (1998) 1804
Summary and conclusions
Y. Leifels – Texas 2013 23
Symmetry energy at supra-saturation densities
very few data points at supra saturation densities (experiments at GSI)
elliptic flow data
consistent with L~100+/- 45 MeV
slightly harder than experiments at lower densities/astrophysical
observations
pion ratio, but no consistent description, new experimental efforts at the
radioactive beam facility at RIKEN
more data WITH radioactive beams will be available soon
V2np
Bao-An Li, NUSYM 2013
Parameterization of
shape:
Elliptic flow of light clustered
Y. Leifels – Texas 2013 24
2)0(
2220
)0(
2
2220n2
Yvv)Y(v
vvv
A. L
eF
evre
et a
l, Nu
cl. P
hys. A
87
6 (2
01
2) 1
observable sensitive
to EOS over a large
energy range
protons and light
clustered
Soft EOS favored
Masses of neutron stars
Y. Leifels – ASTRO 2013 25
htt
p:/
/ww
w.s
tella
rco
llap
se
.org
/nsm
asse
s
Heaviest Neutron Stars
Name: J1614-2230
Mass: (1.976 0.04) M
P. Demorest et al. 2010
Shapiro delay
Name: J0348+0432
Mass: (2.01 0.04) M
J. Antoniadis et al. 2013
White dwarf spectroscopy
main sequence
neutron star binaries
white dwarf
neutron star binaries
double
neutron star binaries
X-Ray
optical binaries
What else?
Y. Leifels – ASTRO 2013 26
Hyperon production and propagation
YN and YY interaction in dense medium
Hypernuclei production
K-N interaction in dense medium
In-medium effects as a function of momentum and
density
“Hot” cluster formation
Phase transitions (QGP), new phases (SCC...)
Phase diagram of nuclear matter
Y. Leifels – ASTRO 2013 27
compression
heat
Z/N
Maximum compression reached at FAIR energies
Y. Leifels – FAIR Detectors 28
SIS 100/ 300
SIS AGS CERN SPS
optimum production of
baryons with strange quarks
maximum compression
in heavy-ion collisions
threshold for
strange quarks
threshold for
antiprotons
threshold for
charm quarks
1 10 100
ion energy [GeV/u]
nu
cle
ar
ma
tte
r d
en
sity (
blu
e c
urv
e)
Re
l.p
rod
uction
of str
an
ge
qu
ark
s (
red
cu
rve
)
To be determined:
Temperature
Pressure
Density
Observables:
Particle production
Flow of bulk matter
Production of D0, D±
, , e+e- or μ+μ-