Mass limits for non-degenerate white dwarfs

Gerd Schmidt; Hans Thomas Elze; Johann Rafelski

doi:10.1016/0375-9474(81)90586-8

Mass limits for non-degenerate white dwarfs

Gerd Schmidt
, Hans Thomas Elze
, Johann Rafelski

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

1 Scopus citations

Abstract

We obtain the dependence of the upper mass limit of white dwarf stars on the specific entropy per electron. For non-degenerate stars significantly larger masses are found. Stellar collapse as an entropy-producing process can therefore have a self-stabilizing influence on the stellar evolution.

Original language	English (US)
Pages (from-to)	527-532
Number of pages	6
Journal	Nuclear Physics, Section A
Volume	364
Issue number	2-3
DOIs	https://doi.org/10.1016/0375-9474(81)90586-8
State	Published - 1981
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/0375-9474(81)90586-8

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title = "Mass limits for non-degenerate white dwarfs",

abstract = "We obtain the dependence of the upper mass limit of white dwarf stars on the specific entropy per electron. For non-degenerate stars significantly larger masses are found. Stellar collapse as an entropy-producing process can therefore have a self-stabilizing influence on the stellar evolution.",

author = "Gerd Schmidt and Elze, \{Hans Thomas\} and Johann Rafelski",

year = "1981",

doi = "10.1016/0375-9474(81)90586-8",

language = "English (US)",

volume = "364",

pages = "527--532",

journal = "Nuclear Physics, Section A",

issn = "0375-9474",

publisher = "Elsevier B.V.",

number = "2-3",

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TY - JOUR

T1 - Mass limits for non-degenerate white dwarfs

AU - Schmidt, Gerd

AU - Elze, Hans Thomas

AU - Rafelski, Johann

PY - 1981

Y1 - 1981

N2 - We obtain the dependence of the upper mass limit of white dwarf stars on the specific entropy per electron. For non-degenerate stars significantly larger masses are found. Stellar collapse as an entropy-producing process can therefore have a self-stabilizing influence on the stellar evolution.

AB - We obtain the dependence of the upper mass limit of white dwarf stars on the specific entropy per electron. For non-degenerate stars significantly larger masses are found. Stellar collapse as an entropy-producing process can therefore have a self-stabilizing influence on the stellar evolution.

UR - https://www.scopus.com/pages/publications/33744626523

UR - https://www.scopus.com/pages/publications/33744626523#tab=citedBy

U2 - 10.1016/0375-9474(81)90586-8

DO - 10.1016/0375-9474(81)90586-8

M3 - Article

AN - SCOPUS:33744626523

SN - 0375-9474

VL - 364

SP - 527

EP - 532

JO - Nuclear Physics, Section A

JF - Nuclear Physics, Section A

IS - 2-3

ER -

Mass limits for non-degenerate white dwarfs

Abstract

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