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Time-dependent solutions of gravity.

Jones, Gregory Chapman.

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Time-dependent solutions of gravity.

Record Type:	Language materials, printed : Monograph/item
Title/Author:	Time-dependent solutions of gravity./
Author:	Jones, Gregory Chapman.
Description:	232 p.
Notes:	Adviser: Andrew Strominger.
Contained By:	Dissertation Abstracts International67-05B.
Subject:	Physics, Elementary Particles and High Energy. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3217775
ISBN:	9780542692925

Time-dependent solutions of gravity.
Jones, Gregory Chapman.

Time-dependent solutions of gravity. - 232 p.

Adviser: Andrew Strominger.

Thesis (Ph.D.)--Harvard University, 2006.

Fourth, we discuss the variety of S-branes, bubbles, and anti-bubbles obtainable from charged and spinning black holes in de Sitter and anti-de Sitter space.

ISBN: 9780542692925Subjects--Topical Terms:

1019488
Physics, Elementary Particles and High Energy.

Time-dependent solutions of gravity.
LDR:02994nam 2200325 a 45 001 954327
005 20110622
008 110622s2006 eng d
020 $a 9780542692925
035 $a (UMI)AAI3217775
035 $a AAI3217775
040 $a UMI $c UMI
100 1 $a Jones, Gregory Chapman. $3 1277798
245 1 0 $a Time-dependent solutions of gravity.
300 $a 232 p.
500 $a Adviser: Andrew Strominger.
500 $a Source: Dissertation Abstracts International, Volume: 67-05, Section: B, page: 2624.
502 $a Thesis (Ph.D.)--Harvard University, 2006.
520 $a Fourth, we discuss the variety of S-branes, bubbles, and anti-bubbles obtainable from charged and spinning black holes in de Sitter and anti-de Sitter space.
520 $a Third, we give the correct global description of the odd-dimensional S-Kerr universes: D = 5, 7,9,.... All but the first ( D = 5) yield a new instanton which can be used to describe the semiclassical decay of a simpler spacetime into the S-brane.
520 $a Several new solutions of Einstein gravity, Einstein-Maxwell, and supergravity are presented. The solutions are derived, often from known solutions via analytic continuation, or generating or transformation methods. Then their properties and global structure are understood. Finally, their role in quantum gravity and string theory is described.
520 $a First, we describe the card diagram which is used to describe all Weyl-type spacetimes, and can be generalized beyond known Weyl types to include a cosmological constant. Card diagrams are extensions of Weyl half-planes to include time-dependent regions, and display all regions and global structure of a spacetime. Card diagrams have enabled the author and his collaborators to easily understand global structure of spacetime where pictureless methods would result in verbosity, confusion, or error. Additionally, card diagrams teach us about the structure of gravitational equations, sources, and solutions of PDEs/BVPs.
520 $a Then, we look at solutions gotten from the black dihole geometry. We review the dihole wave, and the complicated S-dihole U -universes and E -universes. Scaling limits are discussed, and affine coordinates are emphasized for analyzing the complexified non-Killing 2-manifolds.
520 $a Lastly, we use these twisted bubbles in AdS5 to describe semiclassical decays of AdS5 orbifolds, and extend the Gibbons-Hawking thermodynamic formalism to the twisted case. We use card diagrams for AdS to argue the global structure in the Kerr AdS case, and find that a certain non-Killing event horizon remains present in the bubble spacetime for any a, b ≠ 0, so with a cosmological constant, the nonspinning case is highly nongeneric.
590 $a School code: 0084.
650 4 $a Physics, Elementary Particles and High Energy. $3 1019488
690 $a 0798
710 2 $a Harvard University. $3 528741
773 0 $t Dissertation Abstracts International $g 67-05B.
790 $a 0084
790 1 0 $a Strominger, Andrew, $e advisor
791 $a Ph.D.
792 $a 2006
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3217775