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).

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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!