Is cooling of a neutron star due to gravitational radiation

Details Is cooling of a neutron star due to gravitational radiation Is cooling of a neutron star due to gravitational radiation

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..115r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 1, Jan. 1983, p. 115-125.

Astronomy and Astrophysics

Astrophysics

1

Gravitational Waves, Neutron Stars, Stellar Models, Stellar Temperature, Cooling, Lattices, Mathematical Models

Scientific paper

On the basis of a calculation of gravitational radiation emission by a linear chain, a preliminary estimate is given of the thermal gravitational radiation of lattice structures. Suggesting this as a possible cooling mechanism for neutron stars, it is found that the interior of young neutron stars with lattice structure would be cooled down within extremely short times. The gravitational radiation emission for the linear chain is calculated for the case of thermal excitation; a transition is made to a three-dimensional lattice by transferring the result of the linear chain in a plausible manner. Since the free vibrations of a finite three-dimensional lattice are unknown, this way is seen as the only possible one for estimating the gravitational radiation produced by the thermal phonons of a real crystal.

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