A new representation of theH-functions of radiative transfer |
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Authors: | Das Gupta S R |
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Institution: | (1) Johnson Space Center, Houston, TX, USA;(2) Lehigh University, Bethlehem, PA, USA;(3) National Aeronautics and Space Administration, Washington, DC, USA |
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Abstract: | The energetics involved in the formation of neutron stars in close binaries as a result of supernova explosions are considered. The gravitational binding energy of the neutron star must find proper outlets. The mass ejection and cosmic ray particles can carry away only a small fraction (up to a few per cent) of this energy. Most of the binding energy goes into rotational kinetic energy, gravitational radiation and neutrino emissions. A scenario is considered in which most of the gravitational binding energy goes into rotational kinetic energy and is, ultimately, radiated away as gravitational waves. |
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