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Studies of the high density behavior of nuclear symmetry energy by using the triton-3He relative and differential flows. Gao-Chan Yong IMP, China Collaborators: Bao-An Li, Lie-Wen Chen,Zhi-Gang Xiao,Ming Zhang, Xun-Chao Zhang Aug. 24, IWND09. EoS of nuclear matter. - PowerPoint PPT Presentation
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Studies of the high density behavior of nuclear symmetry energy by using the
triton-3He relative and differential flows
Gao-Chan YongIMP, China
Collaborators: Bao-An Li, Lie-Wen Chen,Zhi-Gang Xiao,Ming Zhang, Xun-
Chao ZhangAug. 24, IWND09
EoS of nuclear matter
pn
pn2sym ,)(E)0,(E),(E
B.A. Li , L.W. Chen, Che Ming Ko, Phys. Rep. 464, 113 (2008).
W.G. Lynch, et al., arXiv: 090.0412, [nucl-ex]
poorly known especially at high densitiesConstraints at high densities have been extracted
HF with a modified Gogny force:HF with a modified Gogny force:
0 1 2 30
20
40
60
80x= -2
x= 0
x= 1
Esy
m(
)/M
eV
/0
MDI interaction
C.B. Das, S. Das Gupta, C. Gale and B.A. Li, PRC 67, 034611 (2003)
)(xUU Single particle potential
soft
stiff
X is induced to mimic
different symmetry energies
Related probes
①Single/double /
②Single/double n-p differential flow
③Squeezed-out n/p
④Hard photon emissions Phys. Lett. B661 (2008) 82
Phys. Lett. B650 (2007) 344
Phys. Rev. C74 (2006) 064617
Phys. Rev. C73 (2006) 034603
Ratio_neutron-rich / Ratio_neutron_deficient
Flow_neutron-rich / Flow_neutron_deficient
Nucleons emitted perpendicular to the reaction plane
Photon_neutron-rich / Photon_neutron_deficient
For more : Tsang, Lynch, Di toro, Q.Li, Y.X. Zhang, et al.
Phase space Coalescence after-burner+Coulomb after-burner
1, R_0=3 fm, P_0=263 MeV/c,
2, our predictions on the Au+Au@200MeV/nucleon
Z=1,Z=2 flows are consistent with the experimental data.
Li,Q: arXiv:0808.0624
Yields of triton and 3He
132Sn+124Sn@400MeV/A, b=5 fm
(1) The yields are not sensitive to
the symmetry energy.
(2) More tritons are produced than
the 3He.
(3) both mostly at mid-rapidities
from the participant ragion.
arXiv: 0906.0939
Ratio of triton and 3He yields
(1) The (n/p)_free/ (n/p)_bound is
higher/lower than the (n/p)_system
due to isospin fractionation.
(2) t/3He ratio is much higher than the
(n/p)_free, maybe due to Coulomb.
(3) All are insensitive to the symmetry
energy.
Triton and 3He flows
(1) 3He clusters show a stronger flow than triton clusters, due to the stronger Coulomb force
(2) 3He flow shows more effects of symmetry energy than the triton flow.
(3) Both are insensitive to the symmetry energy
n-p differential and relative flows
Hep
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To reduce the isoscalar potential while enlarge the isovector potential
Neutrons are hard to probe delicately,
it is thus necessary to see cluster’s flow
t-3He differential and relative flows
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To reduce the isoscalar potential while enlarge the isovector potential
n-p differential and relative flows
(1)The larger symmetry energy effects
at positive rapidities are due to the
more neutron-rich of projectile.
(2) n-p relative flow:
F(x = 1) = -53 MeV/c,
F(x = -1) = -25 MeV/c,
(3) n-p differential flow:
F(x = 1) = 20 MeV/c,
F(x = -1) = 36 MeV/c,
t-3He differential and relative flows(1)The triton-3He relative flow is very
sensitive to the symmetry energy
than the triton-3He differential flow
(2) The larger slope of the 3He flow cause the triton-3He relative flow shows a negative slope at mid-rapidity.
(3) The The triton-3He differential flow is dominated by triton clusters, thus exhibit a positive slope at mid-rapidity.
(3) t-3He relative flow:
F(x = 1) = -74 MeV/c,
F(x = -1) = -22 MeV/c,
(4) t-3He differential flow:
F(x = 1) = 21 MeV/c,
F(x = -1) = 42 MeV/c,
(5) Similar behavior to the n-p flow !Not very sensitive to the R_0,P_0