Cosmic D- and DF-strings from D3 anti-D 3: Black Strings and BPS Bound - INSPIRE

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Cosmic D- and DF-strings from D3 anti-D 3: Black Strings and BPS Bound

Taekyung Kim
(
- Sungkyunkwan U.
)
,
Yoonbai Kim
(
- Sungkyunkwan U.
)
,
Bumseok Kyae
(
- Korea Inst. Advanced Study, Seoul
)
,
Jungjai Lee
(
- Daejin U.
)

Dec, 2006

23 pages

Published in:

Phys.Rev.D 77 (2008) 065027

e-Print:

hep-th/0612285 [hep-th]

DOI:

10.1103/PhysRevD.77.065027

Report number:

KIAS-P06067

View in:

ADS Abstract Service

reference search7 citations

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Abstract:

We study D- and DF-strings from D3

{\bar {\rm D}}3

in the context of Dirac-Born-Infeld type effective field theory. In the presence of an electric flux from a transverse direction, gravitating thick D-string solutions form a spatial manifold,

{\rm S}^{2}\times {\rm R}^{1}

, and straight D-strings stretched along the R

{}^{1}

direction are located at the south and north poles of the two-sphere. There is a horizon along its equator and then the structure of black strings is supported. We also discuss systematic derivation of the BPS bounds for thin parallel D- and DF-strings in both flat and curved spacetime. The BPS sum rule is obtained for arbitrarily-separated multi-string configuration under a Gaussian type tachyon potential and, at the site of each thin BPS D(F)-string, the pressure does not vanish but is finite. For the conical geometry induced by thin BPS D- and DF-strings, we find that there exists maximum deficit angle

\pi

.

11.27.+d
04.40.-b
Born-Infeld model
membrane model: D-brane
membrane model: p-brane
p-brane: 3
effective action
flux: electric
string model
soliton: BPS

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