2 4 Se p 20 08 Ricci flows , wormholes and critical phenomena
نویسنده
چکیده
We study the evolution of wormhole geometries under Ricci flow using numerical methods. Depending on values of initial data parameters, wormhole throats either pinch off or evolve to a monotonically growing state. The transition between these two behaviors exhibits a from of critical phenomena reminiscent of that observed in gravitational collapse. Similar results are obtained for initial data that describe space bubbles attached to asymptotically flat regions. Our numerical methods are applicable to “matter-coupled” Ricci flows derived from conformal invariance in string theory.
منابع مشابه
ar X iv : 0 80 8 . 08 80 v 1 [ gr - q c ] 6 A ug 2 00 8 Ricci flows , wormholes and critical phenomena
We study the evolution of wormhole geometries under Ricci flow using numerical methods. Depending on values of initial data parameters, wormhole throats either pinch off or evolve to a monotonically growing state. The transition between these two behaviors exhibits a from of critical phenomena reminiscent of that observed in gravitational collapse. Similar results are obtained for initial data ...
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متن کاملar X iv : 0 80 8 . 24 81 v 2 [ he p - th ] 1 6 O ct 2 00 8 MIFP - 08 - 21 USTC - ICTS - 08 - 14 AdS
We obtain a large class of smooth Lorentzian p-brane wormholes in supergravities in various dimensions. They connect two asymptotically flat spacetimes. In cases where there is no dilaton involved in the solution, the wormhole can connect an AdSn × Sm in one asymptotic region to a flat spacetime in the other. We obtain explicit examples for (n,m) = (4, 7), (7, 4), (5, 5), (3, 3), (3, 2). These ...
متن کاملar X iv : 0 80 8 . 24 81 v 1 [ he p - th ] 1 8 A ug 2 00 8 MIFP - 08 - 21 USTC - ICTS - 08 - 14 AdS
We obtain a large class of smooth Lorentzian p-brane wormholes in supergravities in various dimensions. They connect two asymptotically flat spacetimes. In cases where there is no dilaton involved in the solution, the wormhole can connect an AdSn × Sm in one asymptotic region to a flat spacetime in the other. We obtain explicit examples for (n,m) = (4, 7), (7, 4), (5, 5), (3, 3), (3, 2). These ...
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تاریخ انتشار 2008