Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen...

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Relativistic equation of state at subnuclear densities in the Thomas-Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th Oct. 2014 KIAA at Peking University, Beijing, China Z. W. Zhang and H. Shen, Astrophys. J. 788, 185 (2014).

Transcript of Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen...

Page 1: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Relativistic equation of state at subnuclear densities in the Thomas-Fermi approximation

Zhaowen ZhangSupervisor: H. Shen

Nankai University

20th-22th Oct. 2014

KIAA at Peking University, Beijing, ChinaZ. W. Zhang and H. Shen, Astrophys. J. 788, 185 (2014).

Page 2: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Motivation

Methods

Results

Conclusion

Background

Page 3: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Background

Supernova explosions Neutron star formations

• Equation of state(EOS) of nuclear matter is very important in understanding many astrophysical phenomena:

Lots of the EOS investigations focused on the case of zero temperature or high density for uniform matter.

Page 4: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Background

G. Shen C. J. Horowitz S. Teige. PhysRevC, 82, 015806 (2010)

• The EOS for the core-collapse supernova simulations covers wide ranges of temperature, proton fraction, and baryon density.

T=1 MeV

T=3.16 MeV

T=6.31 MeV T=10 MeV

Page 5: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Background

Lattimer–Swesty Compressible liquid-drop model

Lattimer, J. M., & Swesty, F. D. Nucl. Phys. A, 535, 331 (1991)

• Some famous nuclear EOSs

H. Shen etc. Parameterized Thomas–Fermi approximation

Shen, H., Toki, H., Oyamatsu, K., & Sumiyoshi, K. Prog. Theor. Phys., 100, 1013 (1998)

G. Shen & Horowitz etc. Relativistic mean field theory

G. Shen C. J. Horowitz S. Teige. PhysRevC, 83, 035802 (2011)

Page 6: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Background

Parameterized Thomas–Fermi approximation

• Nucleon distribution function

• Gradient energy

F0 = 70 MeV fm5 is determined by reproducing the binding energies and charge radii of finite nuclei.

in ou t

3

t ou

out

,

,

1 0i

ii

i C

t

i i ii

i

rr R

n r

R r R

n n nR

n

2

3

cellce 0ll ng

pnE r n d rF r

Page 7: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Motivation

• Self-consistent Thomas–Fermi approximation

Nucleon distribution and gradient energy are calculated self-consistently.

Both droplet and bubble configurations are considered.

bubbledroplet uniform matter

• In present work, we compare and examine the difference between PTF and STF.

Page 8: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Methods• Lagrangian density

Equations of motion

3

,

2 2 3 42 3

223

2

RMF

1

2

1 1 1 1

2 2 3 41 1 1

4 2 41 1 1

4 2 4

ai a i

i p n

e e e

a a a a

i M g g g e A

i m e A

m g g

W W m c

R R m F F

L

0

30 0A A

Mean field approach

2 2 2 32 3

2 2 33

2

2

23

s

v

c

m g g g

A e

n

m c g n

m g

n

n

Page 9: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Methods

• Distribution functionFermi–Dirac distribution

• Chemical potential

Wigner–Seitz cell

• Wigner–Seitz cell

BCC

22 0

( ) (1

) )( k kii ifn r d r rkk f

2 *2

2 *2

1

1 exp /

1

1 exp /

ki

i

ki

i

fk M T

fk M T

*M M g

p p

n n

g g eA

g g

BCC WSV V

Page 10: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Methods

• Thermodynamic quantities

Entropy density

Free energy

Energy density

2 2 *22

, 0

2 2 2 3 42 3

2 2 2 43

2 2 2

2

1

1 1 1 1( )

2 2 3 41 1 1

( )2 2 41 1

( )2 21

( )2

k ki i

i p n

p n

p n

p e

dkk k M f f

m g g

m c g n n

m g n n

A eA n n

ò

22

, 0

1ln 1 ln 1

ln 1 ln 1

k k k ki i i i

i p n

k k k ki i i i

s dkk f f f f

f f f f

cell cell cellF E TS

Page 11: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Methods• Calculation

T Yp ρB RWS

μi σ0(r) ω0(r) ρ0(r)

Nucleon distribution ni(r)

σ(r) ω(r) ρ(r) A(r)

ni(r) converge

Ecell Scell Fcell

Minimizing Fcell by changing RWS

Thermodynamically favored state

YES

NO

M mσ mω mρ gσ

938.0 511.19777 783.0 770.0 10.02892

gω gρ g2 (fm-1) g3 c3

12.61394 4.63219 -7.23247 0.61833 71.30747

TM1 Parameter set

Y. Sugahara and H. Toki, Nucl. Phys. A, 579, 557 (1994)

different initial fields lead to different configuration

Page 12: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Results

Strong Yp dependence

T=1

T=10

Bubble appearance

Delay the transition to uniform matter

• Free energy & Entropy

Small difference

Page 13: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Results

T=1 T=10

ρB

• The densities at the center are lower in the STF.• The cell radius Rc of STF is larger.• More free nucleons exist outside the nuclei at T = 10 MeV.

• Nucleon distribution

Page 14: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Results• Numbers & Fractions

T=1

T=10

Nuclei fractionNeutron gas fractionProton gas fraction

cell

cell

/( ) /( ) /

A d B

n n C B

p p C B

X A NX V n R NX V n R N

T=1

T=10

Cause by difference of nucleon distribution

More nucleons can drip out of the nuclei

Ad

Zd

Ad

Zd

XA

XA

Xn

Xn

Xp

Dominant

Page 15: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Results

T=1 T=10

Yp =0.3

Yp =0.5

• Neutron chemical potential

• The results of droplet are almost identical for STF and PTF.• The sudden jumps caused by the different Coulomb potential of bubble and droplet.

Page 16: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Results

T=1 T=10

Yp =0.3

Yp =0.5

• Proton chemical potential

• The difference of STF and PTF may be caused by the Coulomb and surface energies.• Proton is directly effected by Coulomb interaction.

Page 17: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Conclusion

Outlook

1. More pasta phases could be considered in STF.2. Alpha particles will be included in the future.

Page 18: Relativistic equation of state at subnuclear densities in the Thomas- Fermi approximation Zhaowen Zhang Supervisor: H. Shen Nankai University 20th-22th.

Thank you!