- Open Access
Extremal black hole with a unique ground state
Phys. Rev. D 113, 026010 – Published 13 January, 2026
DOI: https://doi.org/10.1103/n2p6-1ksm
Abstract
Recent computations in gravity suggest that nonsupersymmetric extremal black holes lack any sizeable ground state degeneracy. We confirm this for a D-brane description of nonsupersymmetric four-charge extremal black holes in string theory. The microscopic description comprises four stacks of D-branes wrapping various cycles of the internal six torus and intersecting at a point. The orientations of the stacks are such that supersymmetry is broken completely. We construct the low energy worldline Lagrangian for the brane system, which is seen to have 32 Goldstinos and 28 Goldstones. The Hamiltonian has a unique ground state, which carries a nonzero energy implying the absence of any truly extremal state. Our arguments rely on symmetry and hence should hold in the supergravity regime as well.
Physics Subject Headings (PhySH)
Article Text
Supplemental Material
References (42)
- D. N. Page, arXiv:hep-th/0012020.
- J. Preskill, P. Schwarz, A. D. Shapere, S. Trivedi, and F. Wilczek, Mod. Phys. Lett. A 06, 2353 (1991).
- J. M. Maldacena, J. Michelson, and A. Strominger, J. High Energy Phys. 02 (1999) 011.
- L. V. Iliesiu and G. J. Turiaci, J. High Energy Phys. 05 (2021) 145.
- A. Strominger and C. Vafa, Phys. Lett. B 379, 99 (1996).
- J. M. Maldacena, A. Strominger, and E. Witten, J. High Energy Phys. 12 (1997) 002.
- J. C. Breckenridge, D. A. Lowe, R. C. Myers, A. W. Peet, A. Strominger, and C. Vafa, Phys. Lett. B 381, 423 (1996).
- J. M. Maldacena, Phys. Rev. D 55, 7645 (1997).
- G. T. Horowitz, J. M. Maldacena, and A. Strominger, Phys. Lett. B 383, 151 (1996).
- K. Sfetsos and K. Skenderis, Nucl. Phys. B517, 179 (1998).
- J. M. Maldacena, Phys. Rev. D 57, 3736 (1998).
- J. M. Maldacena, Nucl. Phys. B477, 168 (1996).
- G. T. Horowitz, D. A. Lowe, and J. M. Maldacena, Phys. Rev. Lett. 77, 430 (1996).
- A. Dabholkar, Phys. Lett. B 402, 53 (1997).
- U. H. Danielsson, A. Guijosa, and M. Kruczenski, J. High Energy Phys. 09 (2001) 011.
- M. Cvetic and D. Youm, Nucl. Phys. B477, 449 (1996).
- M. Cvetic and A. A. Tseytlin, Nucl. Phys. B537, 381 (1999).
- M. Cvetic, H. Lu, and C. N. Pope, Nucl. Phys. B549, 194 (1999).
- S. R. Das, Phys. Rev. D 56, 3582 (1997).
- J.-G. Zhou, H. J. W. Muller-Kirsten, J. Q. Liang, and F. Zimmerschied, Nucl. Phys. B487, 155 (1997).
We thank Roberto Emparan for drawing our attention to this issue.
- R. Minasian, G. W. Moore, and D. Tsimpis, Commun. Math. Phys. 209, 325 (2000).
- R. Emparan and G. T. Horowitz, Phys. Rev. Lett. 97, 141601 (2006).
- A. Chowdhury, R. S. Garavuso, S. Mondal, and A. Sen, J. High Energy Phys. 10 (2014) 186.
- A. Chowdhury, R. S. Garavuso, S. Mondal, and A. Sen, J. High Energy Phys. 04 (2016) 082.
- T. Ortin, Phys. Lett. B 422, 93 (1998).
- E. G. Gimon, F. Larsen, and J. Simon, J. High Energy Phys. 01 (2008) 040.
- E. G. Gimon, F. Larsen, and J. Simon, J. High Energy Phys. 07 (2009) 052.
- D. Shih, A. Strominger, and X. Yin, J. High Energy Phys. 06 (2006) 037.
- T. Banks, W. Fischler, S. H. Shenker, and L. Susskind, Phys. Rev. D 55, 5112 (1997).
- E. Witten, Nucl. Phys. B460, 335 (1996).
E.g. for the D2 brane wrapping the 45 directions, will be the Wilson line along 45, whereas will be the transverse coordinates along 67,89. For the D6 branes all three scalars describe Wilson lines.
- P. Fayet and J. Iliopoulos, Phys. Lett. 51B, 461 (1974).
- See Supplemental Material at http://link.aps.org/supplemental/10.1103/n2p6-1ksm for F-term equations.
- J. Manschot and S. Mondal, Phys. Rev. D 107, L121903 (2023).
- F. Denef, J. High Energy Phys. 10 (2002) 023.
- I. Bena, M. Berkooz, J. de Boer, S. El-Showk, and D. Van den Bleeken, J. High Energy Phys. 11 (2012) 171.
- A. Sen, J. High Energy Phys. 08 (2009) 068.
- A. Dabholkar, J. Gomes, S. Murthy, and A. Sen, J. High Energy Phys. 04 (2011) 034.
- A. Sen, Gen. Relativ. Gravit. 43, 2171 (2011).
- K. Bringmann and S. Murthy, Commun. Num. Theor Phys. 7, 15 (2013).
- S. Mondal, SciPost Phys. 18, 103 (2025).