Black holes in supergravity: the non-BPS branch

Eric G. Gimon; Finn Larsen; Joan Simon

doi:10.1088/1126-6708/2008/01/040

Black holes in supergravity: the non-BPS branch

Eric G. Gimon, Finn Larsen, Joan Simon

School of Mathematics

Research output: Contribution to journal › Article › peer-review

Abstract

We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. In particular, we determine the ground state energy as a function of charges and moduli. We find that the mass of the non-BPS black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a non-zero gap above the BPS bound.

Original language	English
Article number	040
Number of pages	29
Journal	Journal of High Energy Physics
Volume	2008
Issue number	01
DOIs	https://doi.org/10.1088/1126-6708/2008/01/040
Publication status	Published - 15 Jan 2008

Keywords / Materials (for Non-textual outputs)

hep-th
Black Holes
D-branes
Black Holes in String Theory

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10.1088/1126-6708/2008/01/040

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abstract = "We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. In particular, we determine the ground state energy as a function of charges and moduli. We find that the mass of the non-BPS black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a non-zero gap above the BPS bound.",

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AU - Larsen, Finn

AU - Simon, Joan

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PY - 2008/1/15

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N2 - We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. In particular, we determine the ground state energy as a function of charges and moduli. We find that the mass of the non-BPS black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a non-zero gap above the BPS bound.

AB - We construct extremal, spherically symmetric black hole solutions to 4D supergravity with charge assignments that preclude BPS-saturation. In particular, we determine the ground state energy as a function of charges and moduli. We find that the mass of the non-BPS black hole remains that of a marginal bound state of four basic constituents throughout the entire moduli space and that there is always a non-zero gap above the BPS bound.

KW - hep-th

KW - Black Holes

KW - D-branes

KW - Black Holes in String Theory

U2 - 10.1088/1126-6708/2008/01/040

DO - 10.1088/1126-6708/2008/01/040

M3 - Article

SN - 1126-6708

VL - 2008

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

IS - 01

M1 - 040

ER -

Black holes in supergravity: the non-BPS branch

Abstract

Keywords / Materials (for Non-textual outputs)

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