Gravitational Radiation of Relativistic n = 1 Polytropes

Details Gravitational Radiation of Relativistic n = 1 Polytropes Gravitational Radiation of Relativistic n = 1 Polytropes

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap.....48..505s&link_type=abstract

Astrophysics, Volume 48, Issue 4, pp.505-513

Astronomy and Astrophysics

Astrophysics

Gravitation: Relativistic Polytrope

Scientific paper

The gravitational radiation of n = 1 polytropes undergoing quasiradial pulsations is examined. The intensity of the gravitational radiation and the gravitational wave amplitudes are calculated for polytropic models of white dwarfs and neutron stars when the energy of rotation of the object serves as the source of the radiated energy. Calculations of h0 show that objects with a polytropic equation of state can describe the expected gravitational radiation from white dwarfs and neutron stars. The gravitational radiation of polytropic models of galactic nuclei and quasars is also examined. These objects can create a high enough background of gravitational radiation at frequencies of 10-8 10-11 Hz for gravitational wave detectors operating in this frequency range.

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