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Phys. Rev. D 55, 1788–1794 (1997)

Dimensionally continued Oppenheimer-Snyder gravitational collapse: Solutions in even dimensions

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Anderson Ilha
Departamento de Astrofísica, Observatório Nacional–CNPq, Rua General José Cristino 77, 20921 Rio de Janeiro, Brazil

José P. S. Lemos
Departamento de Astrofísica, Observatório Nacional–CNPq, Rua General José Cristino 77, 20921 Rio de Janeiro, Brazil
Departamento de Física, Instituto Superior Técnico, Av. Rovisco Pais 1, 1096 Lisboa, Portugal

Received 2 August 1996; published in the issue dated 15 February 1997

The extension of the general relativity theory to higher dimensions, so that the field equations for the metric remain of second order, is done through the Lovelock action. This action can also be interpreted as the dimensionally continued Euler characteristics of lower dimensions. The theory has many constant coefficients apparently without any physical meaning. However, it is possible, in a natural way, to reduce to two (the cosmological and Newton’s constant) these several arbitrary coefficients, yielding a restricted Lovelock gravity. In this process one separates theories in even dimensions from theories in odd dimensions. These theories have static black-hole solutions. In general relativity, black holes appear as the final state of gravitational collapse. In this work, gravitational collapse of a regular dust fluid in even-dimensional restricted Lovelock gravity is studied. It is found that black holes emerge as the final state for these regular initial conditions.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.55.1788
DOI:
10.1103/PhysRevD.55.1788
PACS:
97.60.Lf, 04.20.Jb