Hot Dense Matter and Stellar Collapse - INSPIRE

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Hot Dense Matter and Stellar Collapse

D.Q. Lamb
(
- Illinois U., Urbana
)
,
J.M. Lattimer
(
- Illinois U., Urbana
)
,
C.J. Pethick
(
- Illinois U., Urbana
)
,
D.G. Ravenhall
(
- Illinois U., Urbana
)

Dec 4, 1978

3 pages

Published in:

Phys.Rev.Lett. 41 (1978) 1623-1626

DOI:

10.1103/PhysRevLett.41.1623

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Abstract: (APS)

We calculate the equation of state for hot dense matter and discuss implications for stellar collapse.

References(8)

Figures(0)

- Astrophys.J. 213 213

Supernova Explosion and Neutral Currents of Weak Interaction

K. Sato
(
- Kyoto U.
)

- Prog.Theor.Phys. 54 (1975) 1325-1338
•
DOI:
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Neutrino Trapping During Gravitational Collapse of Stars

W.David Arnett
(
- Chicago U., EFI
)

- Astrophys.J. 218 (1977) 815
•
DOI:
- 10.1086/155738

Neutron star matter

- Nucl.Phys.A 175 (1971) 225-271
•
DOI:
- 10.1016/0375-9474(71)90281-8

Neutron star matter at high temperatures and densities. I - Bulk properties of nuclear matter

- Astrophys.J. 223 (1978) 314
•
DOI:
- 10.1086/156265

Nuclear Surface Energy and Neutron-Star Matter

D.G. Ravenhall
(
- Illinois U., Urbana
)
,
C.D. Bennett
(
- Illinois U., Urbana
)
,
C.J. Pethick
(
- Illinois U., Urbana
)

- Phys.Rev.Lett. 28 (1972) 978-981
•
DOI:
- 10.1103/PhysRevLett.28.978

- Phys.Rev. 8 3096

- Astrophys.J. 225 L19