Incompressibility of Hot Asymmetrical Nuclear Matter: Lowest Order Constrained Variational Approach. - INSPIRE

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Incompressibility of Hot Asymmetrical Nuclear Matter: Lowest Order Constrained Variational Approach.

M. Modarres
(
- Shiraz U.
)
,
G.H. Bordbar
(
- Shiraz U.
)

Nov, 1998

6 pages

Published in:

Phys.Rev.C 58 (1998) 2781-2786

DOI:

10.1103/PhysRevC.58.2781

View in:

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Abstract: (APS)

The isothermal and isentropic incompressibility of asymmetrical nuclear matter are investigated in the framework of the lowest order constrained variational method. Various phenomenological nucleon-nucleon interactions, namely, the Reid, the Δ-Reid, and the new Argonne potentials are used. It is found that the temperature as well as the asymmetry parameter reduce the incompressibility of asymmetrical nuclear matter. The pressure is calculated along isentropic paths. It is shown that the equation state is much harder than the one usually assumed in the hydrodynamical simulations of supernova collapse. Various discussions are made in connection with the problem of supernova explosions and other many-body model calculations.

References(26)

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COMPRESSION EFFECTS IN RELATIVISTIC NUCLEUS NUCLEUS COLLISIONS

et al.

- Phys.Rev.Lett. 49 (1982) 1236-1239
•
DOI:
- 10.1103/PhysRevLett.49.1236

Circumstantial Evidence for a Stiff Nuclear Equation of State

J.J. Molitoris
(
- Michigan State U.
)
,
D. Hahn
(
- Michigan State U.
)
,
Horst Stoecker
(
- Michigan State U.
)

- Nucl.Phys.A 447 (1986) 13C-26C,
- Nucl. Phys. A447 ( 1986) 13C-26C
•
DOI:
- 10.1016/0375-9474(86)90595-6

- Phys.Rept. 137 137

A Guide to microscopic models for intermediate-energy heavy ion collisions

G.F. Bertsch
(
- Michigan State U.
)
,
S. Das Gupta
(
- McGill U.
)

- Phys.Rept. 160 (1988) 189-233
•
DOI:
- 10.1016/0370-1573(88)90170-6

Direct URCA process in neutron stars

J.M. Lattimer
(
- SUNY, Stony Brook
)
,
M. Prakash
(
- SUNY, Stony Brook
)
,
C.J. Pethick
(
- Nordita and
- Illinois U., Urbana
)
,
P. Haensel
(
- Warsaw, Copernicus Astron. Ctr.
)

- Phys.Rev.Lett. 66 (1991) 2701-2704
•
DOI:
- 10.1103/PhysRevLett.66.2701

Composition and structure of protoneutron stars

Madappa Prakash
(
- SUNY, Stony Brook and
- Santa Barbara, KITP
)
,
Ignazio Bombaci
(
- SUNY, Stony Brook
)
,
Manju Prakash
(
- SUNY, Stony Brook and
- Santa Barbara, KITP
)
,
Paul J. Ellis
(
- Santa Barbara, KITP and
- Minnesota U.
)
,
James M. Lattimer
(
- SUNY, Stony Brook
)

et al.

- Phys.Rept. 280 (1997) 1-77
•
e-Print:
- nucl-th/9603042
•
DOI:
- 10.1016/S0370-1573(96)00023-3

Equation of state in the gravitational collapse of stars

- Nucl.Phys.A 324 (1979) 487-533
•
DOI:
- 10.1016/0375-9474(79)90596-7

Supernova mechanisms

H.A. Bethe
(
- Cornell U., LNS
)

- Rev.Mod.Phys. 62 (1990) 801-866
•
DOI:
- 10.1103/RevModPhys.62.801

LOCV Calculation of Nuclear Matter with Phenomenological two-nucleon Interaction Operators.

G.H. Bordbar
(
- Shiraz U.
)
,
M. Modarres
(
- Shiraz U.
)

- J.Phys.G 23 (1997) 1631
•
DOI:
- 10.1088/0954-3899/23/11/011

Lowest Order Constrained Variational Calculation for Asymmetrical Nuclear Matter with the New Argonne Potential.

G.H. Bordbar
(
- Shiraz U.
)
,
M. Modarres
(
- Shiraz U.
)

- Phys.Rev.C 57 (1998) 714-721
•
DOI:
- 10.1103/PhysRevC.57.714

Local phenomenological nucleon-nucleon potentials

Roderick V. Reid, Jr.
(
- MIT, LNS and
- Cornell U., LNS
)

- Annals Phys. 50 (1968) 411-448
•
DOI:
- 10.1016/0003-4916(68)90126-7

- J.Phys.G 4 1085

PHENOMENOLOGICAL TWO NUCLEON INTERACTION OPERATOR

- Nucl.Phys.A 359 (1981) 331-348,
- Nucl. Phys. A359 ( 1981) 331-348
•
DOI:
- 10.1016/0375-9474(81)90240-2

- Phys.Rev.Lett. 29 1207

An Accurate nucleon-nucleon potential with charge independence breaking

Robert B. Wiringa
(
- Argonne, PHY
)
,
V.G.J. Stoks
(
- Flinders U.
)
,
R. Schiavilla
(
- Jefferson Lab and
- Old Dominion U.
)

- Phys.Rev.C 51 (1995) 38-51
•
e-Print:
- nucl-th/9408016
•
DOI:
- 10.1103/PhysRevC.51.38

LOCV CALCULATIONS WITH A SELFCONSISTENT TREATMENT OF ISOBARS

M. Modarres
(
- Manchester U. and
- Daresbury
)
,
J.M. Irvine
(
- Manchester U. and
- Daresbury
)

- J.Phys.G 5 (1979) 511-526
•
DOI:
- 10.1088/0305-4616/5/4/016

- J.Phys.G 5 7

- J.Phys.G 23 923

Hot and cold, nuclear and neutron matter

- Nucl.Phys.A 361 (1981) 502-520
•
DOI:
- 10.1016/0375-9474(81)90649-7

- J.Phys.G 19 1349

The incompressibility of hot asymmetric nuclear matter

I. Bombaci
(
- SUNY, Stony Brook
)
,
T.T.S. Kuo
(
- SUNY, Stony Brook
)
,
U. Lombardo
(
- Catania U. and
- INFN, Catania
)

- Phys.Lett.B 311 (1993) 9-14
•
DOI:
- 10.1016/0370-2693(93)90524-L

- Phys.Rept. 242 165

- Astron.Astrophys. 182 L34

Type II supernovae in 12 M(sun) and 15 M(sun) stars: The equation of state and general relativity

E. Baron
(
- SUNY, Stony Brook and
- Brookhaven
)
,
J. Cooperstein
(
- SUNY, Stony Brook and
- Brookhaven
)
,
S. Kahana
(
- SUNY, Stony Brook and
- Brookhaven
)

- Phys.Rev.Lett. 55 (1985) 126-129
•
DOI:
- 10.1103/PhysRevLett.55.126

- Mod.Phys.Lett. 5 1071

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