Scaling from Jupiter to pulsars and mass spectrum of pulsars

Details Scaling from Jupiter to pulsars and mass spectrum of pulsars Scaling from Jupiter to pulsars and mass spectrum of pulsars

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...260..353f&link_type=abstract

Astrophysical Journal, Part 1, vol. 260, Sept. 1, 1982, p. 353-361. Research supported by Johns Hopkins University;

Astronomy and Astrophysics

Astrophysics

3

Energy Dissipation, Jupiter Atmosphere, Mass Spectra, Planetary Mass, Pulsars, Scaling Laws, Angular Velocity, Energetic Particles, Inertia, Neutron Stars, Particle Acceleration, Radii, Similitude Law, Stellar Models, Stellar Rotation

Scientific paper

Following the principle of similitude, the energy loss of Jupiter was scaled through the acceleration of high energy particles to that of Crab pulsar. The agreement suggests a classification scheme for all pulsars in which the pulsar angular velocity and its decrease with time are related to the pulsar moment of inertia divided by its radius and its mass is determined according to neutron star models. The mass spectrum of 194 pulsars is found to be approximately 1/sq m.

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