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Abstract:

A duality transformation that interrelates expanding and contracting cosmological models is shown to single out a duality invariant, interacting two-component description of any irrotational, geodesic and shear-free cosmic medium with vanishing three-curvature scalar. We have applied this feature to a system of matter and radiation, to a mixture of dark matter and dark energy, to minimal and conformal scalar fields, and to an enlarged Chaplygin gas model of the cosmic substratum. We have extended the concept of duality transformations to cosmological perturbations and demonstrated the invariance of adiabatic pressure perturbations under these transformations. © 2008 World Scientific Publishing company.

Registro:

Documento: Artículo
Título:Duality invariance and cosmological dynamics
Autor:Chimento, L.P.; Zimdahl, W.
Filiación:Departamento de Física, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina
Departamento de Física, Universidade Federal Do Espírito Santo, CEP29075-910 Vitória, Espírito Santo, Brazil
Palabras clave:Cosmology; Duality; Phantom
Año:2008
Volumen:17
Número:12
Página de inicio:2229
Página de fin:2254
DOI: http://dx.doi.org/10.1142/S0218271808013820
Título revista:International Journal of Modern Physics D
Título revista abreviado:Int. J. Mod. Phys. D
ISSN:02182718
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02182718_v17_n12_p2229_Chimento

Referencias:

  • Wands, D., (2002) Class. Quant. Grav, 19, p. 3403
  • Finelli, F., Brandenberger, R., (2002) Phys. Rev. D, 65, p. 103522
  • Durrer, R., Vernizzi, F., (2002) Phys. Rev. D, 66, p. 083503
  • Gordon, C., Turok, N., (2003) Phys. Rev. D, 67, p. 123508
  • Gasperini, M., Veneziano, G., (2003) Phys. Rep, 373, p. 1
  • Martin, J., Peter, P., (2003) Phys. Rev. D, 68, p. 103517
  • Boyle, L.A., Steinhardt, P.J., Turok, N., (2004) Phys. Rev. D, 70, p. 023504. , arXiv:hep-th/0403026
  • Piao, Y.S., Zhang, Y.Z., (2004) Phys. Rev. D, 70, p. 043516
  • Piao, Y.S., (2005) Phys. Lett. B, 606, p. 245
  • Lidsay, J.A., (2004) Phys. Rev. D, 70, p. 041302. , arXiv:gr-qc/0405055
  • Veneziano, G., (1991) Phys. Lett. B, 265, p. 287
  • Tseytlin, A.A., (1991) Mod. Phys. Lett. A, 6, p. 1721
  • Sen, A., (1991) Phys. Lett. B, 271, p. 295
  • Gasperini, M., arXiv:hep-th/9907067; Kolb, E.W., Turner, M.S., (1998) The Early Universe, , Addison Wesley
  • Zimdahl, W., Pavón, D., (1994) Mon. Not. R. Astron. Soc, 266, p. 872
  • Chimento, L.P., Pavón, D., (2006) Phys. Rev. D, 73, p. 063511
  • Wetterich, C., (1988) Nucl. Phys. B, 302, p. 668
  • Wetterich, C., (1995) Astron. Astrophys, 301, p. 321
  • Amendola, L., (2000) Phys. Rev. D, 62, p. 043511
  • Zimdahl, W., Pavón, D., Chimento, L.P., (2001) Phys. Lett. B, 521, p. 133
  • Chimento, L.P., (2003) Phys. Rev. D, 67, p. 083513
  • Amendola, L., (2004) Phys. Rev. D, 69, p. 103524
  • R.-G. Cai and A. Wang, J. Cosmol. Astropart. Phys. 03 (2005) 002; Z.-K. Guo, R.-G. Cai and Y.-Z. Zhang, J. Cosmol. Astropart. Phys. 05 (2005) 002; Berger, M.S., Shojaei, H., (2006) Phys. Rev. D, 74, p. 043530. , arXiv:astro-ph/0606408
  • Cai, Y., (2007) Phys. Lett. B, 646, p. 141. , arXiv:gr-qc/0609039
  • Xia, J.-Q., (2006) Phys. Rev. D, 73, p. 063521
  • S. Nesseris and L. Perivolaropoulos, J. Cosmol. Astropart. Phys. 01 (2007) 018 [arXiv:astro-ph/0610092]; Faraoni, V., (2003) Phys. Rev. D, 68, p. 063508
  • Gunzig, E., (2001) Phys. Rev. D, 63, p. 067301
  • Faraoani, V., (1996) Phys. Rev. D, 53, p. 6813
  • Gonzalez-Diaz, P.F., (2003) Phys. Rev. D, 68, p. 021303
  • Chimento, L.P., Lazkoz, R., (2006) Class. Quant. Grav, 23, pp. 3195-3204
  • Bento, M.C., Bertolami, O., Sen, A.A., (2002) Phys. Rev. D, 66, p. 043507
  • Chimento, L.P., (2004) Phys. Rev. D, 69, p. 123517
  • Chimento, L.P., (2003) Phys. Rev. D, 67, p. 083513
  • Bento, M.C., Bertolami, O., Sen, A.A., (2004) Phys. Rev. D, 70, p. 083519
  • Zimdahl, W., Fabris, J.C., (2005) Class. Quant. Grav, 22, p. 4311
  • Liddle, A.R., Lyth, D.H., (2000) Cosmological Inflation and Large-Scale Structure, , Cambridge University Press, Cambridge
  • Bardeen, J.M., Steinhardt, P.J., Turner, M.S., (1983) Phys. Rev. D, 28, p. 679
  • Lyth, D.H., (1985) Phys. Rev. D, 31, p. 1792
  • García-Bellido, J., Wands, D., (1996) Phys. Rev. D, 53, p. 5437
  • Wands, D., (2000) Phys. Rev. D, 62, p. 043527
  • Dvali, G., Gruzinov, A., Zaldarriaga, M., (2004) Phys. Rev. D, 69, p. 083505
  • S. Matarrese and A. Riotto, J. Cosmol. Astropart. Phys. 0308 (2003) 007; Lyth, D.H., Ungarelli, C., Wands, D., (2003) Phys. Rev. D, 67, p. 023503
  • Zimdahl, W., (2005) Int. J. Mod. Phys. D, 14, p. 2319

Citas:

---------- APA ----------
Chimento, L.P. & Zimdahl, W. (2008) . Duality invariance and cosmological dynamics. International Journal of Modern Physics D, 17(12), 2229-2254.
http://dx.doi.org/10.1142/S0218271808013820
---------- CHICAGO ----------
Chimento, L.P., Zimdahl, W. "Duality invariance and cosmological dynamics" . International Journal of Modern Physics D 17, no. 12 (2008) : 2229-2254.
http://dx.doi.org/10.1142/S0218271808013820
---------- MLA ----------
Chimento, L.P., Zimdahl, W. "Duality invariance and cosmological dynamics" . International Journal of Modern Physics D, vol. 17, no. 12, 2008, pp. 2229-2254.
http://dx.doi.org/10.1142/S0218271808013820
---------- VANCOUVER ----------
Chimento, L.P., Zimdahl, W. Duality invariance and cosmological dynamics. Int. J. Mod. Phys. D. 2008;17(12):2229-2254.
http://dx.doi.org/10.1142/S0218271808013820