Nonsingular solutions for S-branes - INSPIRE

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Nonsingular solutions for S-branes

Gregory Jones
(
- Harvard U.
)
,
Alexander Maloney
(
- SLAC and
- Stanford U., Phys. Dept.
)
,
Andrew Strominger
(
- Harvard U.
)

Mar, 2004

21 pages

Published in:

Phys.Rev.D 69 (2004) 126008

e-Print:

hep-th/0403050 [hep-th]

DOI:

10.1103/PhysRevD.69.126008

Report number:

SLAC-PUB-10324

View in:

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Abstract:

Exact, non-singular, time-dependent solutions of Maxwell-Einstein gravity with and without dilatons are constructed by double Wick rotating a variety of static, axisymmetric solutions. This procedure transforms arrays of charged or neutral black holes into s-brane (spacelike brane) solutions, i.e. extended, short-lived spacelike defects. Along the way, new static solutions corresponding to arrays of alternating-charge Reissner-Nordstrom black holes, as well as their dilatonic generalizations, are found. Their double Wick rotation yields s-brane solutions which are periodic in imaginary time and potential large-N duals for the creation/decay of unstable D-branes in string theory.

04.50.+h
04.20.Jb
11.25.Uv
Einstein-Maxwell equation: solution
dilaton
membrane model: S-brane
black hole
boundary condition
numerical calculations

References(35)

Figures(0)

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Roberto Emparan
(
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)

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