Published January 1980 | Version v1
Journal article Metadata-only

Simulation of pulsar behavior in a low-temperature laboratory /Review/

Creators

  • 1. Akademiia Nauk Gruzinskoi SSR, Institut Fiziki, Tiflis, Georgian SSR

Description

The results are given of an experimental study of the properties of superfluid He II in a regime of nonstationary rotation. On the basis of an analysis of the experimental data it is shown that the features of pulsar rotation (abrupt glitches in the angular velocity, oscillations of the angular velocity, and prolonged relaxation processes) can be explained under the assumption of superfluidity of a neutron liquid in the pulsars

Additional details

Publishing Information

Journal Title
Astrophysics (Engl. Transl.)
Journal Volume
15
Journal Issue
3
Series
Astrophysics (Engl. Transl.).
Journal Page Range
353-361
ISSN
0004-6396

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
14759757
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ANGULAR VELOCITY; HELIUM ISOTOPES; PULSARS; RELAXATION TIME; ROTATION; STAR MODELS; SUPERFLUIDITY; TIME DEPENDENCE
Descriptors DEC
COSMIC RADIO SOURCES; MATHEMATICAL MODELS; VELOCITY

Optional Information

Notes
Translated from Astrofizika; 15: 533-547(Jul-Sep 1979). Cover-to-cover translation of Astrofizika (USSR).