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Volumn 62, Issue 6, 2000, Pages 1-8

Quantum (in)stability of dilatonic AdS backgrounds and the holographic renormalization group with gravity

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EID: 17244370843     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.62.064006     Document Type: Article
Times cited : (25)

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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (1999) Phys. Rev. Lett. , vol.83 , pp. 4922
    • Goldberger, W.D.1    Wise, M.B.2
  • 13
    • 0001610103 scopus 로고    scopus 로고
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 586
    • Arkani-Hamed, N.1    Dimopoulos, S.2    Dvali, G.3    Kaloper, N.4
  • 14
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (1999) Prog. Theor. Phys. , vol.102 , pp. 1181
    • Izawa, K.-I.1    Nomura, Y.2    Yanagida, T.3
  • 15
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Nucl. Phys. , vol.B567 , pp. 111
    • Dienes, K.R.1    Dudas, E.2    Gherghetta, T.3
  • 16
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 2080
    • Davoudiasl, H.1    Hewett, J.L.2    Rizzo, T.G.3
  • 17
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Phys. Rev. D , vol.61 , pp. 064003
    • Kim, H.B.1    Kim, H.D.2
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    • (2000) Phys. Lett. B , vol.475 , pp. 253
    • Behrndt, K.1    Cvetic, M.2
  • 19
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (1999) Prog. Theor. Phys. , vol.102 , pp. 1213
    • Hatanaka, H.1    Sakamoto, M.2    Tachibana, M.3    Takenaga, K.4
  • 20
    • 85037215741 scopus 로고    scopus 로고
    • E. Halyo, hep-th/9909127
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Phys. Rev. D , vol.62 , pp. 024011
    • Flanagan, E.E.1    Henry Tye, S.-H.2    Wasserman, I.3
  • 21
    • 0001851163 scopus 로고    scopus 로고
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 1080
    • Chamblin, A.1    Gibbons, G.W.2
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    • (to be published), hep-th/ 9909134
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • Phys. Rev. D
    • Dewolfe, O.1    Freedman, D.Z.2    Gubser, S.S.3    Karch, A.4
  • 23
    • 0001935913 scopus 로고    scopus 로고
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (1999) Phys. Lett. B , vol.468 , pp. 31
    • Kanti, P.1    Kogan, I.I.2    Olive, K.A.3    Pospelov, M.4
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    • (2000) Phys. Lett. B , vol.477 , pp. 285
    • Binetruy, P.1    Deffayet, C.2    Ellwanger, U.3    Langlois, D.4
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    • (2000) Phys. Rev. Lett. , vol.84 , pp. 2778
    • Garriga, J.1    Tanaka, T.2
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    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • Phys. Rev. D
    • Csaki, C.1    Graesser, M.2    Randall, L.3    Terning, J.4
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    • S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • (2000) Nucl. Phys , vol.B576 , pp. 106
    • Youm, D.1
  • 34
    • 0001851163 scopus 로고    scopus 로고
    • to be published
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • Phys. Rev. D
    • Charmousis, C.1    Gregory, R.2    Rubakov, V.A.3
  • 35
    • 0001851163 scopus 로고    scopus 로고
    • (to be published), hep-th/9912186
    • T. Nihei, Phys. Lett. B 465, 81 (1999); N. Kaloper, Phys. Rev. D 60, 123506 (1999); H. Verlinde, hep-th/9906182; D. J. H. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); I. Oda, Phys. Lett. B 480, 305 (2000); 472, 59 (2000); P.J. Steinhardt, ibid. 462, 41 (1999); W.D. Goldberger and M.B. Wise, Phys. Rev. Lett. 83, 4922 (1999); N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, ibid. 84, 586 (2000); K.-I. Izawa, Y. Nomura, and T. Yanagida, Prog. Theor. Phys. 102, 1181 (1999); K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B567, 111 (2000); H. Davoudiasl, J.L. Hewett, and T.G. Rizzo, Phys. Rev. Lett. 84, 2080 (2000); ; H.B. Kim and H.D. Kim, Phys. Rev. D 61, 064003 (2000); K. Behrndt and M. Cvetic, Phys. Lett. B 475, 253 (2000); H. Hatanaka, M. Sakamoto, M. Tachibana, and K. Takenaga, Prog. Theor. Phys. 102, 1213 (1999); E.E. Flanagan, S.-H. Henry Tye, and I. Wasserman, Phys. Rev. D 62, 024011 (2000); E. Halyo, hep-th/9909127; A. Chamblin and G.W. Gibbons, Phys. Rev. Lett. 84, 1080 (2000); O. DeWolfe, D.Z. Freedman, S.S. Gubser, and A. Karch, Phys. Rev. D (to be published), hep-th/ 9909134; P. Kanti, I.I. Kogan, K.A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); G. Aldazabal, L.E. Ibanez, and F. Quevedo, J. High Energy Phys. 01, 031 (2000); S. Chang and M. Yamaguchi, hep-ph/9909523; A. Chamblin, S.W. Hawking, and H.S. Reall, Phys. Rev. D 61, 065007 (2000); R. Kallosh, A. Linde, and M. Shmakova, J. High Energy Phys. 9911, 010 (1999); C. Grojean, J. Cline, and G. Servant, Nucl. Phys. B578, 259 (2000); K. Benakli and Y. Oz, Phys. Lett. B 472, 83 (2000); T. Shiromizu, K. Maeda, and M. Sasaki, Phys. Rev. D 62, 024012 (2000); P. Binetruy, C. Deffayet, U. Ellwanger, and D. Langlois, Phys. Lett. B 477, 285 (2000); J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000); C. Csaki, M. Graesser, L. Randall, and John Terning, Phys. Rev. D (to be published), hep-ph/9911406; C.P. Burgess, R.C. Myers, and F. Quevedo, hep-th/9911164; D. Youm, Nucl. Phys B576, 106 (2000); S. Nam, hep-th/9911237; D. Ida, gr-qc/9912002; P.H. Frampton and T.W. Kephart, hep-th/9912028; C. Charmousis, R. Gregory, and V.A. Rubakov, Phys. Rev. D (to be published); Z. Chacko and A.E. Nelson, ibid. (to be published), hep-th/9912186; M. Cvetic and J. Wang, ibid. 61, 124020 (2000); R. Maartens, D. Wands, B.A. Bassett, and I.P.C. Heard, ibid. 62, 041301 (2000); G.K. Leontaris and N.E. Mavromatos, ibid. 61, 124004 (2000); S. Chang, J. Hisano, H. Nakano, N. Okada, and M. Yamaguchi, ibid. (to be published), hep-ph/9912498; M. Cvetic, H. Lu, and C.N. Pope, hep-th/0001002; C. Csaki, J. Erlich, T.J. Hollowood, and Y. Shirman, hep-th/0001033; T. Chiba, Phys. Rev. D 62, 021502 (2000); K. Koyama and J. Soda, Phys. Lett. B 483, 432 (2000); K. Behrndt and S. Gukov, hep-th/0001082.
    • Phys. Rev. D
    • Chacko, Z.1    Nelson, A.E.2
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