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Abstract:

We make a scalar representation of interactive models with cold dark matter and modified holographic Ricci dark energy through unified models driven by scalar fields with non-canonical kinetic term. These models are applications of the formalism of exotic k-essences generated by the global description of cosmological models with two interactive fluids in the dark sector and in these cases they correspond to the usual k-essences. The formalism is applied to the cases of constant potential in Friedmann–Robertson–Walker geometries. © 2016, The Author(s).

Registro:

Documento: Artículo
Título:Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
Autor:Forte, M.
Filiación:Departamento de Física, Facultad de ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, 1428, Argentina
Año:2016
Volumen:76
Número:12
DOI: http://dx.doi.org/10.1140/epjc/s10052-016-4572-0
Título revista:European Physical Journal C
Título revista abreviado:Eur. Phys. J. C
ISSN:14346044
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14346044_v76_n12_p_Forte

Referencias:

  • arXiv:astro-ph/9805201 A.G. Riess et al. [Supernova Search Team Collaboration], Astron. J. 116, 1009 (1998); arXiv:astro-ph/9812133 S. Perlmutter et al. [Supernova Cosmology Project Collaboration], Astrophys. J. 517, 565 (1999); Amanullah, R., (2010) Astrophys. J., 716, p. 712. , arXiv:1004.1711 [astro-ph.CO]
  • arXiv:astro-ph/0603449 D.N. Spergel et al. [WMAP Collaboration], Astrophys. J. Suppl. 170, 377 (2007); Weinberg, D.H., Mortonson, M.J., Eisenstein, D.J., Hirata, C., Riess, A.G., Rozo, E., (2013) Phys. Rep., 530, p. 87. , arXiv:1201.2434 [astro-ph.CO]
  • Percival, W.J., Cole, S., Eisenstein, D.J., Nichol, R.C., Peacock, J.A., Pope, A.C., Szalay, A.S., (2007) Mon. Not. R. Astron. Soc., 381, p. 1053. , arXiv:0705.3323 [astro-ph]
  • Zlatev, I., Wang, L.M., Steinhardt, P.J., (1999) Phys. Rev. Lett., 82, p. 896. , arXiv:astro-ph/9807002
  • Caldwell, R.R., Dave, R., Steinhardt, P.J., (1998) Phys. Rev. Lett., 80, p. 1582. , arXiv:astro-ph/9708069
  • Frieman, J.A., Hill, C.T., Stebbins, A., Waga, I., (1995) Phys. Rev. Lett., 75, p. 2077. , arXiv:astro-ph/9505060
  • Peebles, P.J.E., Ratra, B., (1988) Astrophys. J., 325, p. L17
  • Ratra, B., Peebles, P.J.E., (1988) Phys. Rev. D, 37, p. 3406
  • Armendariz-Picon, C., Mukhanov, V.F., Steinhardt, P.J., (2000) Phys. Rev. Lett., 85, p. 4438. , arXiv:astro-ph/0004134
  • Armendariz-Picon, C., Mukhanov, V.F., Steinhardt, P.J., (2001) Phys. Rev. D, 63, p. 103510. , arXiv:astro-ph/0006373
  • Copeland, E.J., Sami, M., Tsujikawa, S., (2006) Int. J. Mod. Phys. D, 15, p. 1753. , arXiv:hep-th/0603057
  • Chimento, L.P., (2004) Phys. Rev. D, 69, p. 123517. , arXiv:astro-ph/0311613
  • Chiba, T., (2002) Phys. Rev. D, 66, p. 063514. , arXiv:astro-ph/0206298
  • Tsujikawa, S., Sami, M., (2004) Phys. Lett. B, 603, p. 113. , arXiv:hep-th/0409212
  • Malquarti, M., Copeland, E.J., Liddle, A.R., Trodden, M., (2003) Phys. Rev. D, 67, p. 123503. , arXiv:astro-ph/0302279
  • Aguirregabiria, J.M., Chimento, L.P., Lazkoz, R., (2004) Phys. Rev. D, 70, p. 023509. , arXiv:astro-ph/0403157
  • Chimento, L.P., Forte, M.I., Lazkoz, R., (2005) Mod. Phys. Lett. A, 20, p. 2075. , arXiv:astro-ph/0407288
  • Chimento, L.P., Forte, M.I., (2006) Phys. Rev. D, 73, p. 063502. , arXiv:astro-ph/0510726
  • Armendariz-Picon, C., Lim, E.A., (2005) JCAP, 508, p. 007. , arXiv:astro-ph/0505207
  • Li, M., Zhang, X., (2003) Phys. Lett. B, 573, p. 20. , arXiv:hep-ph/0209093
  • Guo, Z.K., Piao, Y.S., Zhang, X.M., Zhang, Y.Z., (2005) Phys. Lett. B, 608, p. 177. , arXiv:astro-ph/0410654
  • Cai, Y.F., Saridakis, E.N., Setare, M.R., Xia, J.Q., (2010) Phys. Rep., 493, p. 1. , arXiv:0909.2776 [hep-th]
  • Feng, B., Wang, X.L., Zhang, X.M., (2005) Phys. Lett. B, 607, p. 35. , arXiv:astro-ph/0404224
  • Feng, B., Li, M., Piao, Y.S., Zhang, X., (2006) Phys. Lett. B, 634, p. 101. , arXiv:astro-ph/0407432
  • Chimento, L.P., Forte, M.I., Lazkoz, R., Richarte, M.G., (2009) Phys. Rev. D, 79, p. 043502. , arXiv:0811.3643 [astro-ph]
  • arXiv:gr-qc/9310026 G. ’t Hooft, Salamfest, pp. 0284–296 (1993); arXiv:hep-th/9806039 W. Fischler, L. Susskind; Aharony, O., Gubser, S.S., Maldacena, J.M., Ooguri, H., Oz, Y., (2000) Phys. Rep., 323, p. 183. , arXiv:hep-th/9905111
  • Bousso, R., (2002) Rev. Mod. Phys., 74, p. 825. , arXiv:hep-th/0203101
  • Bousso, R., (1999) JHEP, 9907, p. 004. , arXiv:hep-th/9905177
  • Hsu, S.D.H., (2004) Phys. Lett. B, 594, p. 13. , arXiv:hep-th/0403052
  • Amendola, L., (2000) Phys. Rev. D, 62, p. 043511. , arXiv:astro-ph/9908023
  • Mangano, G., Miele, G., Pettorino, V., (2003) Mod. Phys. Lett. A, 18, p. 831. , arXiv:astro-ph/0212518
  • del Campo, S., Herrera, R., Pavon, D., (2004) Phys. Rev. D, 70, p. 043540. , arXiv:astro-ph/0407047
  • Farrar, G.R., Peebles, P.J.E., (2004) Astrophys. J., 604, p. 1. , arXiv:astro-ph/0307316
  • Guo, Z.K., Cai, R.G., Zhang, Y.Z., (2005) JCAP, 505, p. 002. , arXiv:astro-ph/0412624
  • Guo, Z.K., Zhang, Y.Z., (2005) Phys. Rev. D, 71, p. 023501. , arXiv:astro-ph/0411524
  • Cai, R.G., Wang, A., (2005) JCAP, 503, p. 002. , arXiv:hep-th/0411025
  • Gumjudpai, B., Naskar, T., Sami, M., Tsujikawa, S., (2005) JCAP, 506, p. 007. , arXiv:hep-th/0502191
  • Curbelo, R., Gonzalez, T., Leon, G., Quiros, I., (2006) Class. Quantum Gravity, 23, p. 1585. , arXiv:astro-ph/0502141
  • Zimdahl, W., Pavon, D., (2001) Phys. Lett. B, 521, p. 133. , arXiv:astro-ph/0105479
  • Chimento, L.P., Jakubi, A.S., Pavon, D., Zimdahl, W., (2003) Phys. Rev. D, 67, p. 083513. , arXiv:astro-ph/0303145
  • Olivares, G., Atrio-Barandela, F., Pavon, D., (2005) Phys. Rev. D, 71, p. 063523. , arXiv:astro-ph/0503242
  • Szydlowski, M., Cosmological model with energy transfer (2006) Phys. Lett. B, 632, p. 1. , arXiv:astro-ph/0502034
  • Chimento, L., Forte, M.I., (2008) Phys. Lett. B, 666, p. 205. , arXiv:0706.4142 [astro-ph]
  • arXiv:1610.07441 M. Forte, [hep-th]; arXiv:1507.03658 M. Forte, Eur. Phys. J. C 76(1), 42 (2016) [gr-qc]; Granda, L.N., Oliveros, A., (2009) Phys. Lett. B, 671, p. 199. , arXiv:0810.3663 [gr-qc]
  • Nojiri, S., Odintsov, S.D., (2006) Gen. Relativ. Gravity, 38, p. 1285. , arXiv:hep-th/0506212
  • Li, M., (2004) Phys. Lett. B, 603, p. 1. , arXiv:hep-th/0403127
  • Chimento, L.P., Forte, M.I., Richarte, M.G., (2013) Mod. Phys. Lett. A, 28, p. 1250235. , arXiv:1106.0781 [astro-ph.CO]
  • arXiv:1301.2737 L.P. Chimento, M. Forte, M.G. Richarte, Eur. Phys. J. C 73(1), 2285 (2013) [gr-qc]; Pankunni, P., Mathew, T.K., (2014) Int. J. Mod. Phys. D, 23, p. 1450024. , arXiv:1309.3136 [astro-ph.CO]
  • arXiv:1412.5482 E.K. Li, Y. Zhang, J.L. Geng, Phys. Rev. D 90(8), 083534 (2014). doi:. [gr-qc]; arXiv:1511.00600 A. Pasqua, S. Chattopadhyay, R. Myrzakulov, [gr-qc]; Sharif, M., Jawad, A., (2012) Astrophys. Space Sci., 337, p. 789
  • del Campo, S., Fabris, J.C., Herrera, R., Zimdahl, W., (2011) Phys. Rev. D, 83, p. 123006. , arXiv:1103.3441 [astro-ph.CO]
  • arXiv:1508.07248 R.C.G. Landim, Int. J. Mod. Phys. D 25(04), 1650050 (2016) [hep-th]; Bamba, K., Capozziello, S., Nojiri, S., Odintsov, S.D., (2012) Astrophys. Space Sci., 342, p. 155. , arXiv:1205.3421 [gr-qc]
  • Granda, L.N., Oliveros, A., (2008) Phys. Lett. B, 669, p. 275. , arXiv:0810.3149 [gr-qc]
  • Zeldovich, Y.B., (1972) Mon. Not. R. Astron. Soc., 160, p. 1P
  • arXiv:1412.0743 P.H. Chavanis, Phys. Rev. D 92(10), 103004 (2015) [gr-qc]; S.W. Hawking, G.F.R. Ellis; Wald, (University of Chicago Press (1984) USA, p. 491
  • Bean, R., Dore, O., (2004) Phys. Rev. D, 69, p. 083503. , arXiv:astro-ph/0307100
  • M.S. Longair; (2010) Padmanabhan, , Cambridge University Press, Cambridge, UK
  • Coles, P., F. Lucchin, (Wiley (2002) Chichester, p. 492
  • Garriga, J., Mukhanov, V.F., (1999) Phys. Lett. B, 458, p. 219. , arXiv:hep-th/9904176
  • Babichev, E., Mukhanov, V., Vikman, A., (2008) JHEP, 802, p. 101. , arXiv:0708.0561 [hep-th]
  • Vikman, A., (2005) Phys. Rev. D, 71, p. 023515. , arXiv:astro-ph/0407107
  • Chimento, L.P., (2010) Phys. Rev. D, 81, p. 043525. , arXiv:0911.5687 [astro-ph.CO]
  • arXiv:gr-qc/0608031 N.J. Poplawski

Citas:

---------- APA ----------
(2016) . Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy. European Physical Journal C, 76(12).
http://dx.doi.org/10.1140/epjc/s10052-016-4572-0
---------- CHICAGO ----------
Forte, M. "Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy" . European Physical Journal C 76, no. 12 (2016).
http://dx.doi.org/10.1140/epjc/s10052-016-4572-0
---------- MLA ----------
Forte, M. "Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy" . European Physical Journal C, vol. 76, no. 12, 2016.
http://dx.doi.org/10.1140/epjc/s10052-016-4572-0
---------- VANCOUVER ----------
Forte, M. Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy. Eur. Phys. J. C. 2016;76(12).
http://dx.doi.org/10.1140/epjc/s10052-016-4572-0