Published 1976 | Version v1
Report Restricted

Physics of neutron stars

Creators

Description

Work on the equation of state of dense matter and the consequences of this for neutron stars are briefly reviewed for the conventional theories. Then the significance of the pion condensation which is likely to occur in neutron stars is discussed; pressure effects, cooling rates, and supernova explosions are addressed. 10 figures

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
14 p.
Report number
COO--3001-148

Conference

Title
Spring meeting of the American Physical Society.
Dates
26 Apr 1976.
Place
Washington, District of Columbia, United States of America (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
8282429
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COOLING; EQUATIONS OF STATE; EXPLOSIONS; MASS; NEUTRON STARS; NUCLEAR MATTER; PHASE TRANSFORMATIONS; PIONS MINUS; PRESSURE DEPENDENCE; SUPERNOVAE
Descriptors DEC
ANTIMATTER; ANTIMESONS; ANTIPARTICLES; BOSONS; ELEMENTARY PARTICLES; EQUATIONS; HADRONS; MATTER; MESONS; PIONS; PSEUDOSCALAR ANTIMESONS; PSEUDOSCALAR MESONS; STARS

Optional Information

Notes
Available from NTIS. $3.50.
Secondary number(s)
CONF-760431--3.