Gravitational collapse in brane-worlds revisited

Abstract This paper is dedicated to revisit the modifications caused by branes in the collapse of a stellar structure under the Snyder-Oppenheimer scheme. Due to the homogeneity and isotropy of the model, we choose study the case of a closed geometry described by k = 1, through the tool of dynamical...

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Veröffentlicht in:Revista mexicana de física 2016-06, Vol.62 (3), p.199-205
Hauptverfasser: García-Aspeitia, M.A., Ortiz, C., López-Domínguez, J.C., Hinojosa-Ruiz, S., Reyes-Ibarra, M.J.
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container_issue 3
container_start_page 199
container_title Revista mexicana de física
container_volume 62
creator García-Aspeitia, M.A.
Ortiz, C.
López-Domínguez, J.C.
Hinojosa-Ruiz, S.
Reyes-Ibarra, M.J.
description Abstract This paper is dedicated to revisit the modifications caused by branes in the collapse of a stellar structure under the Snyder-Oppenheimer scheme. Due to the homogeneity and isotropy of the model, we choose study the case of a closed geometry described by k = 1, through the tool of dynamical systems. We revisit the different components of the star and its evolution during the stellar collapse, paying particular attention to the non-local effects and the quadratic terms of the energy momentum tensor that come from branes corrections. In the same vein we realize a phase portrait together with a stability analysis with the aim of obtain information about the attractors or saddle points of the dynamical system under different initial conditions in the density parameters, remarking the parameters that come from branes contributions.
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title Gravitational collapse in brane-worlds revisited
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