Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy...

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Yingxun Zhang 张张张 Constraints on the density dependence of symmetry energy 十十十十十十十十十十十十十十十十十十十十十十十十十十十十十十 USTC 十十 11/6/2009 合合合Zhuxia Li 合合合合 () , M.B.Tsan g , P.Danielewicz, W.G.Lynch • China Institute of Atom ic Energy, 张张张张张张张张张张 • JINA, NSCL/MSU Motivation and Strategies on Stud y the density dependence of symm etry energy Brief introduction on ImQMD mod el Constraints on the density depend ence of symmetry energy from the ImQMD model Summary and outlook Outline
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Page 1: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Yingxun Zhang 张英逊

Constraints on the density dependence of symmetry energy

十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会USTC , 合肥, 11/6/2009

合作者: Zhuxia Li (李祝霞) , M.B.Tsang , P.Danielewicz, W.G.Lynch

• China Institute of Atomic Energy, 中国原子能科学研究院• JINA, NSCL/MSU

Motivation and Strategies on Study the density dependence of symmetry energy

Brief introduction on ImQMD model

Constraints on the density dependence of symmetry energy from the ImQMD model

Summary and outlook

Outline

Page 2: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Motivation and strategies on study the density dependence of symmetry energy

• Symmetry energy and the density dependence of symmetry energy

In asymmetric nuclear matter, the EOS

Esym():the density dependence of symmetry energy

E/A(,) = E/A(,0) + Esym() 2 + O(4) ;

= (n- p)/ (n+ p) = (N-Z)/A

E/A(,) = E/A(,0) + Esym() 2 + O(4) ;

= (n- p)/ (n+ p) = (N-Z)/A

It is a fundamental properties of nuclear matter, and is very important for understanding • neutron-rich HICs process• nuclear structure• thickness of the neutron skins,..• properties of NS, …. (Lie-Wen’s Talk)

Page 3: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Danielewicz, Lacey, Lynch, Science 298,1592 (2002)

E/A(,) = E/A(,0) + 2Esym() ; = (n- p)/ (n+ p) = (N-Z)/AE/A(,) = E/A(,0) + 2Esym() ; = (n- p)/ (n+ p) = (N-Z)/A

Equation of State of Nuclear Matter

1

10

100

1 1.5 2 2.5 3 3.5 4 4.5 5

symmetric matter

RMF:NL3AkmalFermi gasFlow ExperimentKaons ExperimentFSU Au

P (M

eV/f

m-3

)

/0

因此非对称核物质状态方程的确定依赖于对称能密度依赖形式的确定

集体流以及 Kaon 凝聚的实验数据对于 1 ~ 50 的对称核物质状态方程给出了约束 对称能密度依赖形式有很大的不确定性 !

Page 4: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

我们的工作主要是利用丰中子核中能重离子碰撞的方法对于低密区对称能密度依赖形式的约束

• Low densities (<0):– Isoscaling of fragments – Isospin diffusion– n/p spectra and flows; R(n/p), R(t/

3He)– Fragment isotopic distributions, R

(N/Z)– Correlation function, C(q)– Neutron, proton radii, E1 collective

modes.

• High densities (>0) – Neutron/proton, t/3He spectra and

flows; C(q) + vs. - production (Z.G.Xiao tal

k), k, hyperon production.

Observables to probe Esym()Why HICs ?

(BA Li, Tsang, Danielewciz, LW Chen, QFLi, YX Zhang, ZG Xiao…… )

Page 5: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

而对于中能重离子碰撞:包含各种复杂碎块的产生。

data

ImQMD 能够较好的重现中能区重离子碰撞的特点。

ImQMD

T.X.Liu.et.al., PRC76,034603

利用 ImQMD 模型的计算结果与 MSU/NSCL 的 Sn+Sn@50AMeV 中心以及擦边碰撞下的实验数据比较,获取低于饱和密度时对称能密度依赖形式的信息;研究碎块发射对于观测量的影响

Page 6: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Brief introduction on the ImQMD model

the mean fields acting on nucleon wavepackets are derived from Skyrme potential energy density functional

• Microscopic dynamics n-body transport model,• nucleon is represented by a Gauss WF

potential energy density functional:

3/5

0

3/82

0

2

0

,2

00

1

0

2

)(2

)]([212

gCgg

u spn

isosursur

• Change the symmetry potential in the transport model by varying the

主要改进与发展:

Page 7: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Parameters in Vloc are obtained from standard Skyrme interactions parameters

Phase space constraint for considering Pauli principle

The occupation number in cubic of h3 should be small than 1(Pauli principle)

1if

freenp

mednp )/1( 0free

ppnnmed

ppnn ,0, )/1(

freeppnnnp )(, Cugnon, et al., Nucl.Instr.Meth.Phys. B111, 215(1996)

Isospin dependent nucleon-nucleon cross sections are adopted, the medium corrections are

Energy density functional from Momentum dependent interaction

Page 8: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

• 成功的描述中能重离子碰撞的一些基本特点描述1) multifragmentation

Zhang, Li, PRC71(2005)24606

不同反应系统

不同入射能量下 ( <400AMeV)

Page 9: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

2) Stopping and flow observables

集体流与直接流的激发函数

阻止能力

ImQMD

ImQMD

Zhang, Li, PRC74,014602

Zhang, Li, PRC74,014602

Page 10: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Constraints on the density dependence of symmetry energy with multi-observables from ImQMD model

1), the density dependence of symmetry energy with the interaction in ImQMD

ImQMD

对称能密度依赖形式

Page 11: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

2) The n/p ratios of emitted nucleons and the influence of cluster emission

• more pre-equilibrium neutrons get emitted from the neutron rich 124Sn+124Sn system

• relatively more pre-equilibrium neutrons are also emitted in the calculations with softer symmetry energy

b=2fm

kp

knpn dEdM

dEdMR

/

//

YX Zhang, et al, PLB664(2008)145

对称势特点:

•中子排斥

•质子吸引

• n/p ratio is related to the stiffness of symmetry potential at subsaturation density (BALi, PRL(1997))

Page 12: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

•Significant cluster and sequential decay effects are at low energy!

• Over the whole energy range for both free and coalescence-invariant DR(n/p) the data seem closer to the gi=0.5 calculation

• For very small gi, the system completely disintegrated, DR decreases and approaches the limit of reaction system. the double ratio values peak around i~0.7.

• By comparing with data, the i=[0.4,1.05] within <2

DR(n/p)=Rn/p(124)/Rn/p(112)

Detailed comparison with data by varying i

MBTsang,YXZhang et.al., PRL102(2009) i

symE 03/2

0 /5.17/5.12

YX Zhang, P.Danielewicz, et al, PLB664(2008)145

Page 13: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

3) The isospin transport ratio and isospin diffusion and the influence of cluster emission

No isospin diffusion between symmetric systems

Isospin diffusion occurs only in asymmetric systems A+B, and diffusion ability depends on the symmetry energy.

124124

112112

124112

Ri = 1

Ri = -1

Ri=(2X-XAA-XBB)/(XAA-XBB)

同位旋扩散的能力由同位旋转移之比来量度

In absence of isospin diffusion R=1 or R=-1, R~0 for isospin equilibrium

•Theory: X is the , the isospin asymmetry of projectile residues• Exp: X is the isoscaling parameter ,•There is linear relationship between and , So, Ri()=Ri()

Page 14: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Tsang,YX Zhang, et.al., PRL102,122701(2009)

• Cluster emission effects make Ri larger for Ri ((Zmax>20))• The differences between Ri() and Ri(d(Zmax>20)) reflect the isospin diffusion mechanism for peripheral collisions. Isospin diffusion mainly occurs around neck region.

X= from heaviest fragments with Z>20

• Fast equilibration occurs for soft symmetry energy

• within 2uncertainties, gamma_i=[0.4,1.0]

X= from projectile residues with relevant rapidity

Page 15: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

4) The rapidity distribution of R7

))(/)(ln( 777 BeYLiYX

• Ri increase with rapidity increasing

• with 2s uncertainties, gamma_i=[0.45,0.95]

)( 77 XRR

利用 ImQMD 分析三种观测量,确定出在 2 的不确定度内 i 的范围是[0.45,0.95], Cs=35.2MeV

Page 16: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

Summary and Outlook

• The cluster emission play important roles on the isospin sensitive observables at intermediate energy HICs.

• The consistent constraints on the density dependence of symmetry energy at subsaturation density can be obtained from three observables, DR(n/p) ratios, Ri and R7 with ImQMD model.

• more observables and accurate data are needed in future in order to reduce the uncertainties on constraints on the density dependence of symmetry energy and reduce the uncertainties of the transport model.

Page 17: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

与其他模型的比较

The results overlap with recent constraints obtained from giant dipole resonances, pygmy dipole resonance, and mass data.

SMF, Wotler, arXiv:0712.2187

...183

2

0

0

0

0

BsymB

osym

KLSE

symB

sym PE

LB

00

33

0

Page 18: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

中低能重离子输运理论中不确定性的来源:

• 平均场、动量相关势,核子有效质量

• 介质中核子-核子散射截面

• 泡里阻塞的处理

• ……

Page 19: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

International workshop on simulations of low and intermediate energy HICs

ECT*, Italy, 2009

Same EOS, Same cross section different results!

Page 20: Yingxun Zhang 张英逊 Constraints on the density dependence of symmetry energy 十三届全国中高能核物理大会暨第七届全国中高能核物理专题研讨会 USTC ,

• 输运模型计算上的一些技术细节同样会导致很大的不确定性 如: test part 波包宽度、如何抽取初始核,……

• 需要更多、精确的实验数据来减少输运理论的不确定型。

• 输运模型本身还需进一步的发展。

谢谢!