Navegar

Colección

Datos Estadísticas

Artículo

Este artículo es de Acceso Abierto y puede ser descargado en su versión final desde nuestro repositorio
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

We find the group of symmetry transformations generated by interacting fluids in spatially flat Friedmann-Robertson-Walker (FRW) spacetime which links cosmologies with the same scale factor (identity) or with scale factors a and a-1 (duality). There exists a duality between contracting and superaccelerated expanding scenarios associated with (phantom) cosmologies. We investigate the action of this symmetry group on self-interacting minimally (conformally) coupled quintessence and k-essence cosmologies. © 2005 Elsevier B.V. All rights reserved.

Registro:

Documento: Artículo
Título:Interacting fluids generating identical, dual and phantom cosmologies
Autor:Chimento, L.P.
Filiación:Departamento de Física, Facultad de Ciencias Exactas Y Naturales, Pabellón I, 1428 Buenos Aires, Argentina
Año:2006
Volumen:633
Número:1
Página de inicio:9
Página de fin:13
DOI: http://dx.doi.org/10.1016/j.physletb.2005.11.027
Título revista:Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Título revista abreviado:Phys Lett Sect B Nucl Elem Part High-Energy Phys
ISSN:03702693
CODEN:PYLBA
PDF:https://bibliotecadigital.exactas.uba.ar/download/paper/paper_03702693_v633_n1_p9_Chimento.pdf
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v633_n1_p9_Chimento

Referencias:

  • Chimento, L.P., (2002) Phys. Rev. D, 65, p. 063517
  • Padmanabhan, T., Choudhury, T.R., (2002) Phys. Rev. D, 66, p. 081301
  • Chimento, L.P., Lazkoz, R., (2003) Phys. Rev. Lett., 91, p. 301
  • García, A.A., García-Quiroz, A., Cataldo, M., Del Campo, S., (2004) Phys. Rev. D, 69, p. 041302
  • Chimento, L.P., Lazkoz, R., (2005) Int. J. Mod. Phys. D, 14, p. 587. , astro-ph/0405518
  • Barreiro, T., Sen, astro-ph/0408185A.A; Da̧browski, M.P., Stachowiak, T., Szydłowski, M., (2003) Phys. Rev. D, 68, p. 103519
  • Lidsey, gr-qc/0405055J.E; Da̧browski, M.P., Stachowiak, hep-th/0411199T; Caldwell, R.R., (2002) Phys. Lett. B, 545, p. 23
  • Hannestad, S., Mörstell, E., (2002) Phys. Rev. D, 66, p. 063508
  • Doran, M., Jaeckel, J., (2002) Phys. Rev. D, 66, p. 043519
  • Frampton, P.H., Takahashi, T., (2003) Phys. Lett. B, 557, p. 135
  • Carroll, S.M., Hoffman, M., Trodden, M., (2003) Phys. Rev. D, 68, p. 023509
  • Melchiorri, A., Mersini, L., Odman, C.J., Trodden, M., (2003) Phys. Rev. D, 68, p. 043509
  • Nojiri, S., Odintsov, S., (2003) Phys. Lett. B, 571, p. 1
  • Liu, D.J., Li, X.Z., (2003) Phys. Rev. D, 68, p. 067301
  • Piao, Y.S., Zhou, E., (2003) Phys. Rev. D, 68, p. 083515
  • Nojiri, S., Odintsov, S.D., (2003) Phys. Lett. B, 562, p. 147
  • Singh, P., Sami, M., Dadhich, N., (2003) Phys. Rev. D, 68, p. 023522
  • Hao, J.G., Li, X.Z., (2003) Phys. Rev. D, 68, p. 083514
  • González-Díaz, P.F., (2004) Phys. Lett. B, 586, p. 1
  • Elizalde, E., Quiroga Hurtado, J., (2004) Mod. Phys. Lett. a, 19, p. 29
  • Feinstein, A., Jhingan, S., (2004) Mod. Phys. Lett. a, 19, p. 457
  • Li, X.Z., Hao, hep-th/0303093J.G; Stefancic, astro-ph/0310904H; Johri, astro-ph/0311293V.B; Piao, Y.S., Zhou, astro-ph/0401231E; Calcagni, hep-ph/0402126G; Nojiri, S., Odintsov, astro-ph/0403622S.D; Hao, J.G., Li, astro-ph/0404154X.Z; Guo, Z.K., Piao, Y.S., Zhang, Y.Z., (2004) Phys. Lett. B, 594, p. 247
  • Piazza, F., Tsujikawa, hep-th/0405054S; Wu, P.X., Yu, astro-ph/0407424H.W; Piao, Y.S., Zhang, Y.Z., (2004) Phys. Rev. D, 70, p. 043516
  • Guo, Z.K., Cai, R.G., Zhang, astro-ph/0412624Y.Z; Babichev, E., Dokuchaev, V., Eroshenko, Yu., (2004) Phys. Rev. Lett., 93, p. 021102
  • Guo, Z.K., Piao, Y.S., Zhang, X.M., Zhang, Y.Z., (2005) Phys. Lett. B, 608, p. 177
  • Guo, Z.K., Zhang, Y.Z., (2005) Phys. Rev. D, 71, p. 023501
  • Parampreet, gr-qc/0502086S; Curbelo, R., Gonzalez, T., Quiros, astro-ph/0502141I; Piao, Y.S., (2005) Phys. Lett. B, 606, p. 245
  • Onemli, V.K., Woodard, R.P., (2002) Class. Quantum Grav., 19, p. 4607
  • Onemli, V.K., Woodard, R.P., (2004) Phys. Rev. D, 70, p. 107301
  • Chimento, L.P., Jakubi, A.S., Pavon, D., (2004) Phys. Rev. D, 69, p. 083511
  • Caldwell, R.R., (2002) Phys. Lett. B, 545, p. 23
  • Gibbons, hep-th/0302199G.W; Barrow, J., (2004) Class. Quantum Grav., 21, p. 79
  • Aguirregabiria, J.M., Chimento, L.P., Lazkoz, astro-ph/0411258R; Chimento, L.P., (2004) Phys. Rev. D, 69, p. 123517
  • Chimento, L.P., Pavon, gr-qc/0505096D

Citas:

---------- APA ----------
(2006) . Interacting fluids generating identical, dual and phantom cosmologies. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 633(1), 9-13.
http://dx.doi.org/10.1016/j.physletb.2005.11.027
---------- CHICAGO ----------
Chimento, L.P. "Interacting fluids generating identical, dual and phantom cosmologies" . Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 633, no. 1 (2006) : 9-13.
http://dx.doi.org/10.1016/j.physletb.2005.11.027
---------- MLA ----------
Chimento, L.P. "Interacting fluids generating identical, dual and phantom cosmologies" . Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, vol. 633, no. 1, 2006, pp. 9-13.
http://dx.doi.org/10.1016/j.physletb.2005.11.027
---------- VANCOUVER ----------
Chimento, L.P. Interacting fluids generating identical, dual and phantom cosmologies. Phys Lett Sect B Nucl Elem Part High-Energy Phys. 2006;633(1):9-13.
http://dx.doi.org/10.1016/j.physletb.2005.11.027