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Dynamics of colliding branes and black brane production

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arxiv gr-qc/0702138 v2 pith:XQSRQEKS submitted 2007-02-26 gr-qc astro-phhep-phhep-th

Dynamics of colliding branes and black brane production

classification gr-qc astro-phhep-phhep-th
keywords collidingdomainwallsblackbranebranescollisionsdynamics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the dynamics of colliding domain walls including self-gravity. The initial data is set up by applying a BPS domain wall in five-dimensional supergravity, and we evolve the system determining the final outcome of collisions. After a collision, a spacelike curvature singularity covered by a horizon is formed in the bulk, resulting in a black brane with trapped domain walls. This is a generic consequence of collisions, except for non-relativistic weak field cases, in which the walls pass through one another or multiple bounces take place without singularity formation. These results show that incorporating the self-gravity drastically changes a naive picture of colliding branes.

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  1. Kink collisions in a two-dimensional gravity model

    hep-th 2026-07 conditional novelty 6.0

    In a 2D dilaton-gravity model, stronger gravity shifts kink-antikink bounce windows to higher speeds and narrows them, leaves a lasting contraction of the conformal scale, and produces no curvature singularity in the ...