TY - JOUR

T1 - Open string tachyon in supergravity solution

AU - Kobayashi, Shinpei

AU - Asakawa, Tsuguhiko

AU - Matsuura, So

N1 - Funding Information:
The authors would like to thank K. Ohta, H. Kawai, T. Tada, M. Hayakawa, M. Sakagami and Y. Tsubo for helpful discussions. S.K. is also grateful to D. Ida for useful comments and advice. S.K. would also like to express his appreciation to Y. Himemoto for deep suggestions and continuous encouragement. This work of T.A. and S.M. is supported by Special Postdoctoral Researchers Program at RIKEN.

PY - 2005/5/20

Y1 - 2005/5/20

N2 - We study the tachyon condensation of the DD̄-brane system with a constant tachyon vev in the context of classical solutions of the Type II supergravity. We find that the general solution with the symmetry ISO(1, p) x SO(9-p) (the three-parameter solution) includes the extremal black p-brane solution as an appropriate limit of the solution by fixing one of the three parameters (c1). Furthermore, we compare the long distance behavior of the solution with the massless modes of the closed strings from the boundary state of the DD̄-brane system with a constant tachyon vev. We find that we must fix c1 to zero and only two parameters are needed to express the tachyon condensation of the DD̄-brane system. This means that the parameter c1 does not correspond to the tachyon vev of the DD̄-brane system.

AB - We study the tachyon condensation of the DD̄-brane system with a constant tachyon vev in the context of classical solutions of the Type II supergravity. We find that the general solution with the symmetry ISO(1, p) x SO(9-p) (the three-parameter solution) includes the extremal black p-brane solution as an appropriate limit of the solution by fixing one of the three parameters (c1). Furthermore, we compare the long distance behavior of the solution with the massless modes of the closed strings from the boundary state of the DD̄-brane system with a constant tachyon vev. We find that we must fix c1 to zero and only two parameters are needed to express the tachyon condensation of the DD̄-brane system. This means that the parameter c1 does not correspond to the tachyon vev of the DD̄-brane system.

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U2 - 10.1142/S0217732305017354

DO - 10.1142/S0217732305017354

M3 - Article

AN - SCOPUS:20844441633

VL - 20

SP - 1119

EP - 1134

JO - Modern Physics Letters A

JF - Modern Physics Letters A

SN - 0217-7323

IS - 15

ER -