Newborn hot neutron stars

Ignazio Bombaci; Madappa Prakash; Manju Prakash; Paul J. Ellis; James M. Lattimer; Gerald E. Brown

doi:10.1016/0375-9474(94)00736-7

Newborn hot neutron stars

Ignazio Bombaci
, Madappa Prakash
, Manju Prakash
, Paul J. Ellis
, James M. Lattimer
, Gerald E. Brown

Physics and Astronomy

Stony Brook University
University of Minnesota Twin Cities

Research output: Contribution to journal › Article › peer-review

36 Scopus citations

Abstract

The structure of newborn hot neutron stars is compared with that of cold catalyzed configurations. The role of the nuclear equation of state on the structural changes is investigated and some of the astrophysical consequences are briefly discussed.

Original language	English
Pages (from-to)	623-628
Number of pages	6
Journal	Nuclear Physics, Section A
Volume	583
Issue number	C
DOIs	https://doi.org/10.1016/0375-9474(94)00736-7
State	Published - Feb 6 1995

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title = "Newborn hot neutron stars",

abstract = "The structure of newborn hot neutron stars is compared with that of cold catalyzed configurations. The role of the nuclear equation of state on the structural changes is investigated and some of the astrophysical consequences are briefly discussed.",

author = "Ignazio Bombaci and Madappa Prakash and Manju Prakash and Ellis, \{Paul J.\} and Lattimer, \{James M.\} and Brown, \{Gerald E.\}",

year = "1995",

month = feb,

day = "6",

doi = "10.1016/0375-9474(94)00736-7",

language = "English",

volume = "583",

pages = "623--628",

journal = "Nuclear Physics, Section A",

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T1 - Newborn hot neutron stars

AU - Bombaci, Ignazio

AU - Prakash, Madappa

AU - Prakash, Manju

AU - Ellis, Paul J.

AU - Lattimer, James M.

AU - Brown, Gerald E.

PY - 1995/2/6

Y1 - 1995/2/6

N2 - The structure of newborn hot neutron stars is compared with that of cold catalyzed configurations. The role of the nuclear equation of state on the structural changes is investigated and some of the astrophysical consequences are briefly discussed.

AB - The structure of newborn hot neutron stars is compared with that of cold catalyzed configurations. The role of the nuclear equation of state on the structural changes is investigated and some of the astrophysical consequences are briefly discussed.

UR - https://www.scopus.com/pages/publications/0001059161

U2 - 10.1016/0375-9474(94)00736-7

DO - 10.1016/0375-9474(94)00736-7

M3 - Article

AN - SCOPUS:0001059161

SN - 0375-9474

VL - 583

SP - 623

EP - 628

JO - Nuclear Physics, Section A

JF - Nuclear Physics, Section A

IS - C

ER -

Newborn hot neutron stars

Abstract

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