Vibrating-dust spheres in the Reissner-Nordstrom metric

Details Vibrating-dust spheres in the Reissner-Nordstrom metric Vibrating-dust spheres in the Reissner-Nordstrom metric

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ncimb..76...28d&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 76 B, July 11, 1983, p. 28-34. Sponsorship: Consiglio Nazionale delle Ricerche.

Physics

1

Gravitational Collapse, Reissner-Nordstrom Solution, Stellar Models, Stellar Oscillations, Charged Particles, Polarization (Charge Separation), Red Shift, Stable Oscillations, Stellar Evolution, Stellar Radiation

Scientific paper

Consideration is given to the collapse of a charged dust sphere with a charge Q larger than the mass M (both in geometrized units). It is shown that the outcome of collapse is most likely a stable, vibrating configuration. The period of the vibrations is of the order of 10,000 per s for masses of the order of a solar mass. Optically such an object shows a quasi-steady redshift which can be very large when Q is close to M.

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