Gravitational collapse in Weyl integrable spacetimes

Details Gravitational collapse in Weyl integrable spacetimes Gravitational collapse in Weyl integrable spacetimes

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cqgra..16.3281s&link_type=abstract

Classical and Quantum Gravity, Volume 16, Issue 10, pp. 3281-3295 (1999).

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Spherically symmetric gravitational collapse in Weyl integrable spacetime is studied by some simplified models. The matter content is represented by a perfect fluid coupled with the geometric scalar field. A family of analytical solutions is found for a non-radiative collapsing nebulae of dust and the condition for black hole formation is established. Junction conditions with an exterior spacetime and the radiative collapse of a spherical star are also studied. In this case we find two classes of solutions with an exterior Vaidya spacetime: one with no internal heat flux while the other is obtained from a static initial condition.

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