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Nonpropagation of tachyon on the BTZ black hole in type 0B string theory. (English) Zbl 0987.81559

Summary: We obtain the BTZ black hole (\(\text{AdS}_3 \times X^3\)) as a non-dilatonic solution from type 0B string theory. Analyzing the s-wave perturbation around this black hole background, we show that the tachyon is not a propagating mode.

MSC:

81T30 String and superstring theories; other extended objects (e.g., branes) in quantum field theory
83C57 Black holes
83E30 String and superstring theories in gravitational theory

References:

[1] Polyakov, A. M., Int. J. Mod. Phys. A, 14, 645 (1999), hep-th/9809057 · Zbl 0931.81013
[2] I.R. Klebanov, A.A. Tseytlin, Nucl. Phys. B 546 (1999) 155, hep-th/9811035; Nucl. Phys. B 547 (1999) 143, hep-th/9812089.; I.R. Klebanov, A.A. Tseytlin, Nucl. Phys. B 546 (1999) 155, hep-th/9811035; Nucl. Phys. B 547 (1999) 143, hep-th/9812089.
[3] J.A. Minahan, JHEP 9901 (1999) 020, hep-th/9811156; JHEP 9904 (1999) 007, hep-th/9902074.; J.A. Minahan, JHEP 9901 (1999) 020, hep-th/9811156; JHEP 9904 (1999) 007, hep-th/9902074.
[4] L. Dixon, J. Harvey, Nucl. Phys. B 274 (1986) 93; N. Seiberg, E. Witten, Nucl. Phys. B 276 (1986) 272.; L. Dixon, J. Harvey, Nucl. Phys. B 274 (1986) 93; N. Seiberg, E. Witten, Nucl. Phys. B 276 (1986) 272.
[5] G. Ferretti, D. Martelli, hep-th/9811208; N. Nekrasov, S. Shatashvili, hep-th/9902110; M. Alishahiha, A. Brandhuber, Y. Oz, hep-th/9903186; O. Berman, G. Gaberdiel, hep-th/9906055; A. Armoni, B. Kol, hep-th/9906081; R. Blumenhagen, A. Font, D. Lust, hep-th/9906101; J.Y. Kim, hep-th/9906196.; G. Ferretti, D. Martelli, hep-th/9811208; N. Nekrasov, S. Shatashvili, hep-th/9902110; M. Alishahiha, A. Brandhuber, Y. Oz, hep-th/9903186; O. Berman, G. Gaberdiel, hep-th/9906055; A. Armoni, B. Kol, hep-th/9906081; R. Blumenhagen, A. Font, D. Lust, hep-th/9906101; J.Y. Kim, hep-th/9906196.
[6] Klebanov, I. R.; Tseytlin, A. A., JHEP, 9903, 015 (1999), hep-th/9901101
[7] M.S. Costa, hep-th/9903128.; M.S. Costa, hep-th/9903128.
[8] H.W. Lee, Y.S. Myung and Jin Young Kim, hep-th/9907024.; H.W. Lee, Y.S. Myung and Jin Young Kim, hep-th/9907024.
[9] I. Sachs, hep-th/9907201.; I. Sachs, hep-th/9907201.
[10] H.W. Lee, N.J. Kim, Y.S. Myung, hep-th/9805050.; H.W. Lee, N.J. Kim, Y.S. Myung, hep-th/9805050.
[11] C. Callan, S. Gubser, I. Klebanov, A. Tseytlin, Nucl. Phys. B 489 (1997) 65, het-th/9610172; I.R. Klebanov, M. Krasnitz, Phys. Rev. D 55 (1997) R3250.; C. Callan, S. Gubser, I. Klebanov, A. Tseytlin, Nucl. Phys. B 489 (1997) 65, het-th/9610172; I.R. Klebanov, M. Krasnitz, Phys. Rev. D 55 (1997) R3250.
[12] Lee, H. W.; Myung, Y. S.; Kim, J. Y., Phys. Rev. D, 58, 104006 (1998), hep-th/9708099
[13] C. Misner, K. Thorne, J. Wheeler, Gravitation, Freeman, San Francisco, 1973.; C. Misner, K. Thorne, J. Wheeler, Gravitation, Freeman, San Francisco, 1973.
[14] M. Banados, C. Teitelboim, A. Zanelli, Phys. Rev. Lett. 69 (1992) 1849; S. Carlip, Class. Quant. Grav. 12 (1995) 2853.; M. Banados, C. Teitelboim, A. Zanelli, Phys. Rev. Lett. 69 (1992) 1849; S. Carlip, Class. Quant. Grav. 12 (1995) 2853.
[15] Gregory, R.; Laflamme, R., Nucl. Phys. B, 428, 399 (1994) · Zbl 1037.83509
[16] Lee, H. W.; Myung, Y. S., Phys. Rev. D, 58, 104013 (1998), hep-th/9804095
[17] S. Chandrasekhar, The Mathematical Theory of Black Hole (Oxford Univ. Press, New York, 1983).; S. Chandrasekhar, The Mathematical Theory of Black Hole (Oxford Univ. Press, New York, 1983). · Zbl 0511.53076
[18] de Boer, J., Nucl. Phys. B, 548, 139 (1999), hep-th/9806104
[19] J. Maldacena, A. Strominger, JHEP 9812 (1998) 005, hep-th/9804085; K. Behrndt, D. Lüst, hep-th/9905180.; J. Maldacena, A. Strominger, JHEP 9812 (1998) 005, hep-th/9804085; K. Behrndt, D. Lüst, hep-th/9905180.
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