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Gravitational Waves and Neutron Stars

Published online by Cambridge University Press:  12 April 2016

Bernard F. Schutz
Bernard F. Schutz*
Affiliation:
Albert Einstein Institute, Potsdam, Germany Cardiff University, Wales, UKschutz@aei-potsdam.mpg.de

Abstract

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The first generation of laser-interferomteric gravitational wave observatories will make intensive searches for gravitational radiation from spinning neutron stars. Sensitivity to a number of possible sources, including the Crab pulsar, will be better than any existing observational limits, and will improve dramatically over the next decade. This paper reviews these developments and expectations, and discusses ways in which pulsar radio astronomers and gravitational wave astronomers can benefit from one another’s work.

Type
Part 11. The Future – Where to go?
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 727 - 732
Copyright
Copyright © Astronomical Society of the Pacific 2000

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