Multidimensional cosmological solutions of the Friedman type in dilaton gravity
Teoretičeskaâ i matematičeskaâ fizika, Tome 123 (2000) no. 1, pp. 163-176 Cet article a éte moissonné depuis la source Math-Net.Ru

Voir la notice de l'article

Generalized Friedman-type cosmological solutions (spatially homogeneous and isotropic) are obtained and classified in a $D$-dimensional dilaton gravitational model with the central charge deficit $\Lambda$.
@article{TMF_2000_123_1_a13,
     author = {E. G. Vorontsova and G. S. Sharov},
     title = {Multidimensional cosmological solutions of the {Friedman} type in dilaton gravity},
     journal = {Teoreti\v{c}eska\^a i matemati\v{c}eska\^a fizika},
     pages = {163--176},
     year = {2000},
     volume = {123},
     number = {1},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/TMF_2000_123_1_a13/}
}
TY  - JOUR
AU  - E. G. Vorontsova
AU  - G. S. Sharov
TI  - Multidimensional cosmological solutions of the Friedman type in dilaton gravity
JO  - Teoretičeskaâ i matematičeskaâ fizika
PY  - 2000
SP  - 163
EP  - 176
VL  - 123
IS  - 1
UR  - http://geodesic.mathdoc.fr/item/TMF_2000_123_1_a13/
LA  - ru
ID  - TMF_2000_123_1_a13
ER  - 
%0 Journal Article
%A E. G. Vorontsova
%A G. S. Sharov
%T Multidimensional cosmological solutions of the Friedman type in dilaton gravity
%J Teoretičeskaâ i matematičeskaâ fizika
%D 2000
%P 163-176
%V 123
%N 1
%U http://geodesic.mathdoc.fr/item/TMF_2000_123_1_a13/
%G ru
%F TMF_2000_123_1_a13
E. G. Vorontsova; G. S. Sharov. Multidimensional cosmological solutions of the Friedman type in dilaton gravity. Teoretičeskaâ i matematičeskaâ fizika, Tome 123 (2000) no. 1, pp. 163-176. http://geodesic.mathdoc.fr/item/TMF_2000_123_1_a13/

[1] E. S. Fradkin, A. A. Tseytlin, Phys. Lett. B, 158 (1985), 316 ; C. G. Callan, D. Friedan, E. J. Martinec, M. J. Perry, Nucl. Phys. B, 262 (1985), 593 ; C. Lovelace, Phys. Lett. B, 135 (1984), 75 ; Nucl. Phys. B, 273 (1986), 413 | DOI | MR | Zbl | DOI | MR | DOI | MR | DOI | MR

[2] M. Grin, Dzh. Shvarts, E. Vitten, Teoriya superstrun, T. 1, Mir, M., 1990 | MR

[3] C. G. Callan, S. B. Giddings, J. A. Harvey, A. Strominger, Phys. Rev. D, 45 (1992), R1005 ; E-print hep-th/9111056 | DOI | MR

[4] G. W. Gibbons, M. J. Perry, Int. J. Mod. Phys. D, 1 (1992), 335 ; E-print hep-th/9204090 | DOI | MR | Zbl

[5] H. Pelzer, T. Strobl, Class. Q Grav., 15 (1998), 3803 ; E-print gr-qc/9805059 | DOI | MR | Zbl

[6] D. Bailin, A. Love, Phys. Lett. B, 163 (1985), 135 ; D. Bailin, A. Love, D. Wong, Phys. Lett. B, 165 (1985), 270 ; K. Maeda, Phys. Rev. D, 35 (1987), 471 ; A. R. Liddle, R. G. Moorhouse, A. B. Henriques, Nucl. Phys. B, 311 (1989), 719 | DOI | MR | DOI | MR | DOI | MR | DOI

[7] R. C. Myers, Phys. Lett. B, 199 (1987), 371 ; I. Antoniadis, C. Bachas, J. Ellis, D. V. Nanopoulos, Phys. Lett. B, 211 (1988), 393 ; Nucl. Phys. B, 328 (1989), 117 ; Phys. Lett. B, 257 (1991), 278 | DOI | MR | DOI | MR | DOI | MR | DOI | MR

[8] M. Mueller, Nucl. Phys. B, 337 (1990), 37 | DOI | MR

[9] G. Veneziano, Phys. Lett. B, 265 (1991), 287 | DOI | MR

[10] A. A. Tseytlin, Mod. Phys. Lett. A, 6 (1991), 1721 | DOI | MR | Zbl

[11] A. A. Tseytlin, Int. J. Mod. Phys. D, 1 (1992), 223 ; E-print hep-th/9203033 | DOI | MR | Zbl

[12] A. A. Tseytlin, C. Vafa, Nucl. Phys. B, 372 (1992), 443 ; ; A. A. Tseytlin, Class. Q Grav., 9 (1992), 979 ; E-print hep-th/9109048E-print hep-th/9112004 | DOI | MR | DOI | MR

[13] M. Gasperini, G. Veneziano, Astropart. Phys., 1 (1993), 317 ; E-print hep-th/9211021 | DOI

[14] M. Gasperini, G. Veneziano, Mod. Phys. Lett. A, 8 (1993), 3701 ; E-print hep-th/9309023 | DOI | MR | Zbl

[15] J. A. Casas, J. García-Bellido, M. Quirós, Nucl. Phys. B, 361 (1991), 713 ; J. García-Bellido, M. Quirós, Nucl. Phys. B, 385 (1992), 558 | DOI | MR | DOI | MR

[16] R. Brustein, G. Veneziano, Phys. Lett. B, 329 (1994), 429 ; E-print hep-th/9403060 | DOI

[17] S. Behrndt, S. Förste, Nucl. Phys. B, 430 (1994), 441 ; E-print hep-th/9403179 | DOI | MR | Zbl

[18] E. J. Copeland, A. Lahiri, D. Wands, Phys. Rev. D, 50 (1994), 4868 ; E-print hep-th/9406216 | DOI

[19] R. Easther, K. Maeda, Phys. Rev. D, 54 (1996), 7572 ; E-print hep-th/9605173 | DOI

[20] R. Easther, K. Maeda, D. Wands, Phys. Rev. D, 53 (1996), 4247 ; E-print hep-th/9509074 | DOI

[21] N. Kaloper, R. Madden, K. A. Olive, Nucl. Phys. B, 452 (1995), 677 ; ; Phys. Lett. B, 371 (1996), 34 ; E-print hep-th/9506027E-print hep-th/9510117 | DOI | DOI | MR

[22] E. J. Copeland, R. Easther, D. Wands, Phys. Rev. D, 56 (1997), 874 ; E-print hep-th/9701082 | DOI

[23] T. Barreiro, B. de Carlos, E. J. Copeland, Phys. Rev. D, 58 (1998), 083513 ; E-print hep-th/9805005 | DOI

[24] J. Ellis, K. Enqvist, D. V. Nanopoulos, M. Quiros, Nucl. Phys. B, 277 (1986), 231 ; K. Maeda, M. D. Pollack, Phys. Lett. B, 173 (1986), 251 ; K. A. Olive, Phys. Rep., 190 (1990), 307 | DOI | DOI | DOI

[25] G. S. Sharov, TMF, 101:3 (1994), 458 | MR | Zbl

[26] E. Witten, Phys. Rev. D, 44 (1991), 314 ; S. Kar, Phys. Rev. D, 55 (1997), 4872 ; M. O. Katanaev, W. Kummer, H. Liebl, Phys. Rev. D, 53 (1996), 5609 ; E-print gr-qc/9511009 | DOI | MR | Zbl | DOI | MR | DOI | MR