Published September 1986 | Version v1
Journal article Metadata-only

Observational manifestations of pion stars

Creators

  • 1. Erevan State Univ.

Description

It is shown that for nuclearlike superdense cosmic objects - pion stars - the Kelvin cooling time is due solely to the photon energy loss channel and is much shorter than for ordinary neutron stars. Specific nuclear processes taking place on the surface of such objects in the presence of matter accretion may lead to the occurrence of γ pulsars

Additional details

Publishing Information

Journal Title
Astrophysics (Engl. Transl.)
Journal Volume
24
Journal Issue
2
Series
Astrophysics (Engl. Transl.).
Journal Page Range
176-179
ISSN
0004-6396
CODEN
ATPYA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
18034094
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COOLING; COSMIC PIONS; DENSITY; ENERGY LOSSES; NUCLEAR REACTIONS; PHOTONS; REMOTE SENSING; STAR EVOLUTION; STAR MODELS; STARS; TIME DEPENDENCE
Descriptors DEC
BOSONS; COSMIC RADIATION; ELEMENTARY PARTICLES; HADRONS; IONIZING RADIATIONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MESONS; PHYSICAL PROPERTIES; PIONS; PSEUDOSCALAR MESONS; RADIATIONS; SECONDARY COSMIC RADIATION

Optional Information

Notes
Cover-to-cover translation of Astrofizika (USSR).