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- W3121607205 abstract "In this paper, we address the implications when a homogeneous dust model is considered for a scenario of gravitational collapse in the context of Eddington-inspired Born-Infeld (EiBI) theory. In order to describe the dynamical evolution of the collapse, we present an effective equation, which constitutes the first order corrections, in EiBI coupling parameter $kappa$, to Einstein's field equations. The geometry outside the collapsing object is derived by imposing the standard Darmois-Israel junction conditions at the boundary surface of the dust. This induces an effective matter source in the outer region which gives rise to a non-singular, non-Schwarzschild geometry at the final state of the collapse. For this exterior geometry, we find the threshold of mass for the formation of the black hole. This provides a cut-off over $kappa$ as $|kappa|=5.1times10^{-97} ~kg^{-1}cdot m^3$." @default.
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- W3121607205 date "2017-03-13" @default.
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- W3121607205 title "The final state of gravitational collapse in Eddington-inspired Born-Infeld theory" @default.
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- W3121607205 doi "https://doi.org/10.1002/andp.201600415" @default.
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