Abstract
The spectrum of the linearized equations of IIB supergravity above the Klebanov-Strassler background solution is investigated. It is shown that the spectrum of a scalar particle minimally interacting with the background is degenerate with the spectrum of the graviton (traceless spin-2 mode), and this spectrum is studied in detail. The results are generalized to the more general case of the solution that is known in the literature as a baryonic branch.
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References
S. Ferrara and B. Zumino, Nucl. Phys. B 87, 207 (1975).
G. Veneziano and S. Yankielowicz, Phys. Lett. B 113B, 231 (1982).
I. Campos et al. (DESY-Munster Collab.), Eur. Phys. J. C 11, 507 (1999), hep-lat/9903014; F. Farchioni et al. (DESY-Munster-Roma Collab.), Eur. Phys. J. C 23, 719 (2002), hep-lat/0111008; R. Peetz, F. Farchioni, C. Gebert, and G. Munster, Nucl. Phys. (Proc. Suppl.) 119, 912 (2003), hep-lat/0209065.
G. M. Shore, Nucl. Phys. B 222, 446 (1983); G. R. Farrar, G. Gabadadze, and M. Schwetz, Phys. Rev. D 58, 015009 (1998), hep-th/9711166; D. G. Cerdeno, A. Knauf, and J. Louis, Eur. Phys. J. C 31, 415 (2003), hep-th/0307198.
P. I. Pronin and K. V. Stepanyantz, hep-th/9902163.
J. M. Maldacena, Adv. Theor. Math. Phys. 2, 231 (1998) [Int. J. Theor. Phys. 38, 1113 (1999)], hep-th/9711200.
S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Nucl. Phys. B 636, 99 (2002), hep-th/0204051; E. Witten, Adv. Theor. Math. Phys. 2, 253 (1998), hep-th/9802150].
I. R. Klebanov and M. J. Strassler, J. High Energy Phys. 0008, 052 (2000), hep-th/0007191.
P. Candelas and X. C. de la Ossa, Nucl. Phys. B 342, 246 (1990).
A. Butti, M. Grana, R. Minasian, et al., J. High Energy Phys. 0503, 069 (2005), hep-th/0412187.
S. S. Gubser, I. R. Klebanov, and A. A. Tseytlin, Nucl. Phys. B 499, 217 (1997), hep-th/9703040; R. C. Brower, S. D. Mathur, and C. I. Tan, Nucl. Phys. B 574, 219 (2000), hep-th/9908196; N. R. Constable and R. C. Myers, J. High Energy Phys. 9910, 037 (1999), hep-th/9908175.
J. H. Schwarz, Nucl. Phys. B 226, 269 (1983).
G. Papadopoulos and A. A. Tseytlin, Class. Quantum Grav. 18, 1333 (2001), hep-th/0012034.
M. Krasnitz, hep-th/0011179.
E. Caceres and R. Hernandez, Phys. Lett. B 504, 64 (2001), hep-th/0011204; X. Amador and E. Caceres, J. High Energy Phys. 0411, 022 (2004), hep-th/0402061.
N. S. Bakhvalov, N. P. Zhidkov, and G. M. Kobel’kov, Numerical Methods, 4th ed. (Fizmatlit, Moscow, 2003) [in Russian].
J. M. Maldacena and C. Nuñez, Phys. Rev. Lett. 86, 588 (2001), hep-th/0008001.
A. H. Chamseddine and M. S. Volkov, Phys. Rev. Lett. 79, 3343 (1997), hep-th/9707176; A. H. Chamseddine and M. S. Volkov, Phys. Rev. D 57, 6242 (1998), hepth/9711181.
A. Dymarsky, I. R. Klebanov, and N. Seiberg, J. High Energy Phys. 0601, 155 (2006), hep-th/0511254.
H. Firouzjahi and S. H. Tye, J. High Energy Phys. 0601, 136 (2006), hep-th/0512076.
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Original Russian Text © A.Ya. Dymarsky, D.G. Melnikovv, 2006, published in Pis’ma v Zhurnal Éksperimental’noĭ i Teoreticheskoĭ Fiziki, 2006, Vol. 84, No. 7, pp. 440–444.