Gravitational radiation from primordial solitons and soliton-star binaries

Details Gravitational radiation from primordial solitons and soliton-star binaries Gravitational radiation from primordial solitons and soliton-star binaries

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63.1199g&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 63, Sept. 18, 1989, p. 1199-1202. Research supported by DOE and NASA.

Astronomy and Astrophysics

Astrophysics

13

Binary Stars, Gravitational Waves, Quantum Chromodynamics, Solitary Waves, Stellar Gravitation, Astronomical Models, Background Radiation, Black Holes (Astronomy), Nuclear Astrophysics, Stochastic Processes

Scientific paper

The possibility that both the formation of nontopological solitons in a primordial second-order phase transition and binary systems of soliton stars could generate a stochastic gravitational-wave background is examined. The present contribution of gravitational radiation to the energy density of the universe from these processes is estimated for a number of different models. The detectability of such contributions from the timing measurements of the millisecond pulsar and spaceborne laser interferometry is briefly discussed and compared to other cosmological and local sources of background gravitational waves.

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