Does gravitational radiation limit the angular velocities of superfluid neutron stars

Details Does gravitational radiation limit the angular velocities of superfluid neutron stars Does gravitational radiation limit the angular velocities of superfluid neutron stars

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...444..804l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 444, no. 2, p. 804-809

Astronomy and Astrophysics

Astrophysics

69

Angular Velocity, Gravitational Effects, Gravitational Waves, Mathematical Models, Neutron Stars, Stellar Rotation, Superfluidity, Boundary Conditions, Dissipation, Gravity Anomalies, Hydrodynamics, Stellar Oscillations, Temperature Gradients

Scientific paper

The gravitational radiation instability which limits the rotation rates of normal neutron stars is studied using superfluid hydrodynamics and dissipation mechanisms. The influences of these superfluid effects on this instability are evaluated using simple analytical solutions to the superfluid pulsation equations. The superfluid dissipation mechanism 'mutual friction' overwhelmingly suppresses the graviational radiation instability according to these estimates. Thus, gravitational radiation does not limit the angular velocities of superfluid neutron stars.

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