Structure of the black hole nucleus

Details Structure of the black hole nucleus Structure of the black hole nucleus

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cqgra...5l.201p&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 5, Dec. 1, 1988, p. L201-L205. Research supported by Fonds pour la Formatio

Astronomy and Astrophysics

Astrophysics

55

Astrophysics, Black Holes (Astronomy), Gravitational Collapse, Stellar Cores, Stellar Structure, Perturbation Theory, Polarization Characteristics, Space-Time Functions

Scientific paper

This letter explores different possibilities for the nuclear structure of a black hole formed by a collapse with zero angular momentum. If the stress induced by vacuum polarization along the axes of the 3-cylinders (r = constant) is a tension rather than a pressure, the space-time geometry could be self-regulatory and describable semiclassically down to radii of a few Planck units. The nucleus would then appear as an open string of roughly constant sub-Planckian density, with a thickness of about 10 to the -20th cm for a solar-mass black hole.

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