47
HIM-2009-9-26 Instability and Phase Transition in Asymmetric Nuclei Kyung Hee University Suk-Joon Lee

HIM-2009-9-26 Instability and Phase Transition in Asymmetric Nuclei Kyung Hee University Suk-Joon Lee

Embed Size (px)

Citation preview

HIM-2009-9-26

Instability and Phase Transition in Asymmetric

Nuclei

Kyung Hee UniversitySuk-Joon Lee

Thermalized nuclear systemMedium energy heavy-ion collision RIB - AsymmetricNeutron star Short range repulsive and long range attractive Saturation, Phase transitionTow component system: 3-d of , , T He, Binary alloyPhase diagram; surface in 3-d of P, T, y or densitySymmetry energy Second order transition, Isospin fractionationCoulomb energy Beta stability line , Asymmetric phase diagramFinite system Surface energyVelocity dependent interaction Effective mass

3

3

NZ

np /py

S.J. LeeA.Z. MekjianPRC56,2621(1997)

S.J.LeeA,Z,MekjianPRC45,1284(192)

H. Mueller and B,D. Serot, PRC.52, 2072 (1995)

J. Xu, L.W. Chen, B.A, Li,and H.L. MaPRC77, 014302(2008)

),()()(

),()()(Im

),()(

),()(

1

1

1

1),(),(

3

3

2

23

2

32

2

2]),([

2

~

2*

2

prfpi

pdrrJ

prfp

pdrrj

prfp

pdr

prfpdr

eheh

prfh

prf

qiqi

iq

qiqi

iq

qqi

iq

qqi

iq

m

pprqqq

qq

qq

)()()(),(),(

),(

rprprhprf

Hprh

UHHHHHHH

qqqqq

BKBJCSB

Thermodynamic Variables

qq

q

qqqqp

qq

qqqqq

qq

q

qq

qq

Kqq

qqqiiqq

ipi

qii

PETS

fpdfp

pdfpd

ffffpdh

S

EEEE

E

EfpdfppdP

333

~~~~3

3

*

33

3

1ln1ln

3

2

Momentum conservation:

0333

rdfppdrddt

d

jq

iq

ji PP

002

2

2

2

q

q

q

q

qq

PP

0y

P

Coexistence ; Gibbs conditions

Spinodal

Critical point

Equal concentration or extremum of

0y

and at )(myy

TPy ,|)(

0,

Ty

P

0,

TP

q

y

For mechanical instability:

For chemical instability:

at same T but not necessarily jq

iq

dPdd

PTSE

nnpp

nnpp

/p

np

y

),,( TPyq

3/23/10222

222211

222

11

22

2211

2

22

11

223

233

220

200

22112

21

1

22

4

3

4

2

1

2

1

4

1

21

21

4

1

2

1

2

13

16

1

21

213

16

1

2

1

21

12

2

1

21

2

2

1

2

1

4

1

21

21

4

1

22

V

rCReCCH

jjxtxtjx

tx

tH

Cxtxt

xt

xtH

HHHxxt

xxt

xtxtx

tx

t

mmH

SpC

npj

Snp

S

jSCnp

np

nnpp

nn

pp

Skyrme Hamiltonian

Single particle energy

2

2

2

2

*3

2

2

)(),(

),(

)()(),()(

)(),()()(

),(

pEp

pETT

EETT

prprhrrd

rprhrp

HHpHprh

qqq

Fq

qqq

qq

qq

Fqqqqqq

qqqq

qqq

q

Helmholtz Free Energy

EEEE

EP

TTTETTS

TSEF

qq

q

qq

qq

Kqq

qqqqq

qKqq

*

*

3

2

),(),(3

5),(

''

'

3 0

qq q

q

qq

qq

qq

nnpp

ST

EE

TSErd

At low T or high density(nearly degenerated Fermi

gas)

UEE

EP

EETT

Tm

mTS

Tm

Em

Em

Tm

mm

pT

qq

q

qq

Kqq

qq

qqq

qq

q

q

qq

qKqq

Kqq

qq

qqq

Fqq

*

3/123/4

24

2*23/22

*

2

3/123/4

24

2*23/5

3/22*

2

*

2

3/223/4

24

2*23/2

3/22

*

2

*

2

3

2

),(

6

26

2

63

56

5

322

63

6

22

At high T or low density, small(nearly nondegenerated Fermi gas)

3

Tm

TTTTS

Tm

E

m

p

qq

q

qqqqq

qq

qqqqqq

qKq

qqqqqqqq

q

Fqq

*2

33

23

2/5

3

2/5*

2*

3333

*

2

/2

422ln

2

5

3

2

8

1

2

11

2

3

2

22

1ln

22

11ln

2

1,

21

213

33

313

3

001330

0

23

2/52

*

2211

23

2/52

*2

21

1

33

2

22

1

122)1(

2

1

122

1

12

2

1)2(

21

1221

2

12

2

3

2

1

2

1

4

1

2

12

2

3

21

21

4

1

22ln

Spqpp

qq

q

qq

qq

qq

qq

q

qq

qq

q

CCC

xt

xt

xt

xtxtx

t

mTxtxt

mT

xt

xt

TT

)1()1(

2

1

22

1

2)1(

21

1221

2

222

1

2

3

2222

5

2

5

2

23

320

0233200

23*23

Sp

qq

qq

qqq

q

qq

q

q

CC

xt

xtxtxt

m

mT

TTP

S.J. LeeA.Z. MekjianPRC79,044323(2009)

S.J. LeeA.Z. MekjianPRC63,044605(2001)

S.J. LeeA.Z. MekjianPRC68,14608(2003)

S.J. LeeA.Z. MekjianPLB580,137(2004)

S.J. LeeA.Z. MekjianPRC77,054612(2008)

Thick: insideThin; outside

Summary

• Surface tension: lower pressure of coexistence binodal surface (toward P=0)

• Coulomb interaction: Shrink binodal region and mechanical and chemical instability region, move LEC to lower than 0.5, cross of curves in y for different P, asymmetric pair of LG at higher , two pairs meet together with lowest P at

• Symmetry energy: for and for , larger symmetry energy make higher pressure and narrower coexistence loop, loops are closer to , tend to restore symmetry of loops

• Value of for LEC is somewhat insensitive to nuclear force, value of pressure is more sensitive

Ey p

Eyy

Ey

LG yy Eyy LG yy Eyy

Ey

Ey

• Mechanical instability loop is inside of chemical instability boundary and tangent at - diffusive chemical transition occurs even in mechanically stable region

• Chemical instability loop is inside of coexistence loop and tangent to it at their maxima in P

• At , all curves coincide in -T plot, phase transition behaves same as one component system

• For , neutron diffusion is important, while proton diffusion for

• Momentum dependent isoscalar makes pressure higher while isovector momentum dependent term makes much lower for given density and y

• Momentum dependent isoscalar makes loops smaller while momentum dependent isovector term makes loops more larger

Ey

Ey

Eyy Eyy

• Momentum dependent isoscalar makes coexistence loop closer to while momentum dependent isovector term makes loop away

• Momentum dependent term lower the height of coexistence loop at proton rich side while it remains similar at neutron rich side

• Momentum dependent isovector term has opposite and larger effect than isoscalar momentum dependent term

• Isovector term make symmetry energy smaller and thus loops become more asymmetric

• For SLy4 left coexistence loop of lower proton fraction is more pronounced than right loop of high proton fraction, isoscalar and isovector have same sign

• SLy4 loop at higher y is narrower in y than loop for SKM(m*=m)

• Symmetry energy has important role in coexistence

Ey

• Surface tension; lower pressure of coexistence binodal surface (to P=0)• Coulomb interaction; shrink binodal loop, cross of chemical potential curves in y for diffe

rent P at near y=0.5, move LEC to smaller yE than 0.5 for symmetric system, asymmetric pair of L-G at higher y > yE, two pairs meet together with lowest P at yE

• Value of yE is somewhat insensitive to nuclear force, pressure is more sensitive• Symmetry energy; Larger y in gas and smaller y in liquid for y > yE, opposite for y < yE • Nonlinear density dependence of symmetry energy• Coulomb shrink chemical & mechanical instability region• Mechanical is inside of chemical and tangent at yE, diffusive chemical transition occurs

even in mechanically stable region, same at yE• Chemical is inside of coexitence and tangent to it at maxima• At yE, peak in chemical instability and binodal surface coincide, • For y.ne.yE In T vs rho, paks for chemical instability and coexistence coincide, but peak

of mrchanical or spinodal instability is below of others• At y = yE, phase transition behaves same as one component system keeping y=yE in bot

h phase• For y < yE, neutron diffusion is important, while proton diffusion for y < yE• Momentum dependence increase pressure at given density• Momentum dependence make smaller boundaries• Reduce height of coexistence loop at proton rich side and remain similar at neutron rich

side, increase lowest pressure of coexistence curve• Largest and smallest y in coexitence loops shifted toward yE

• For SLy4 left coexistence loop of lower proton fraction is more pronounced than right loop of high proton fraction, isoscalar and isovector have same sighn

• For SKM(m*=m) right loop is more pronounced than left loop, isoscalar term raises pressure of loop on neutron rich side while isovector lowers due to opposite sighn of force

• SLy4 loop at higher y is narrower in y than loop for SKM(m*=m), SLy4 has higher symmetry energy

• Higher left loop means liquid and gas can coexist at higher pressurewith more neutron rich gas and lesser rich neutron liquid for left loop

• Narroing of coexistence loop brings yG and yL closer together thereby reducing proton fraction differece in gas and liquid phase

• Momentum dependent isovector term has opposite and larger effect than isoscalar momentum dependent term

• Isovector tem make symmetry energy smaller and thus loops become more adsymmetric

• Pressure for given rho, y, T becomes larger by isoscalar term while it becomes smaller by isovectoer term

• Symmetry energy terms tend to restore dymmetry of loops• Loops for SKM(m*=m) with both isoscalar and isovector terms have smallest sy

mmetry energy, has cut at y=0• Loops for SLy4 with largestsymmetry energy, are closer to its yE than SKM(m*=

m)

For Skyme Hamiltonian of

),(

)(),(

),(),,(

222

*

**

22

*

2

qq

qqmqmqmqqKq

qqKnKpqqq

U

baE

UEEH

qqq

qq

qqm

pprqqq

qqqq

qq

eheh

prfh

prf

prfp

pdjprfp

pd

prfpd

*

2

2

2]),([

2

~

2

32

23

3

1

1

1

1),(),(

),(),,(

),(

Momentum Independent Interaction

For Consistency

03

5

),(

''

'*''

'

'

' '2

2

qq

q

q

q

Kq

q

q

q

qq

q

q q

Fq

qqq

TEE

ST

EpETT