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• W2334585369 abstract "The purpose of this paper is to extend the analysis presented in Goswami et al. [Phys. Rev. Lett. 96, 031302 (2006)] by means of investigating how a specific type of loop (quantum) effect can alter the outcome of gravitational collapse. To be more concrete, a particular class of spherically symmetric spacetime is considered with a tachyon field $ensuremath{phi}$ and a barotropic fluid constituting the matter content; the tachyon potential $V(ensuremath{phi})$ is assumed to be of the form ${ensuremath{phi}}^{ensuremath{-}2}$. Within inverse triad corrections, we then obtain, for a semiclassical description, several classes of analytical as well as numerical solutions. Moreover, we identify a subset whose behavior corresponds to an outward flux of energy, thus avoiding either a naked singularity or a black hole formation." @default.
• W2334585369 created "2016-06-24" @default.
• W2334585369 creator A5029988402 @default.
• W2334585369 creator A5048646658 @default.
• W2334585369 creator A5056144801 @default.
• W2334585369 creator A5077811935 @default.
• W2334585369 date "2013-01-24" @default.
• W2334585369 modified "2023-09-25" @default.
• W2334585369 title "Semiclassical collapse with tachyon field and barotropic fluid" @default.
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• W2334585369 doi "https://doi.org/10.1103/physrevd.87.024042" @default.
• W2334585369 hasPublicationYear "2013" @default.
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