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Abstract:

In this work we illustrate how form-invariance transformations (FITs) can be used to construct phantom and complementary tachyon cosmologies from standard tachyon field universes. First we show how these transformations act on the Hubble expansion rate, and the energy density and pressure of the tachyon field. Then we use the FIT to generate three different families of the tachyon field. In other words, the FIT generates new cosmologies from a known "seed" one; in particular, we apply the FIT to the ordinary tachyon field to obtain two types of tachyon species, denoted as the phantom and complementary tachyons. We see that the FIT allows us to pass from a nonstable cosmology to a stable one and vice versa. Finally, as an example, we apply the transformations to an inverse-square potential, V φ-2, and generate the extended tachyon field. © 2014 American Physical Society.

Registro:

Documento: Artículo
Título:Extended tachyon field using form invariance symmetry
Autor:Sánchez G., I.E.
Filiación:Departamento de Matemática, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina
Año:2014
Volumen:90
Número:2
DOI: http://dx.doi.org/10.1103/PhysRevD.90.027308
Título revista:Physical Review D - Particles, Fields, Gravitation and Cosmology
Título revista abreviado:Phys Rev D Part Fields Gravit Cosmol
ISSN:15507998
CODEN:PRVDA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v90_n2_p_SanchezG

Referencias:

  • Padmanabhan, T., (2002) Phys. Rev. D, 66, p. 021301. , PRVDAQ 0556-2821 10.1103/PhysRevD.66.021301
  • Feinstein, A., Power-law inflation from the rolling tachyon (2002) Physical Review D, 66 (6), p. 063511. , DOI 10.1103/PhysRevD.66.063511
  • Abramo, L.R.W., Finelli, F., (2003) Phys. Lett. B, 575, p. 165. , PYLBAJ 0370-2693 10.1016/j.physletb.2003.09.065
  • Campuzano, C., Del Campo, S., Herrera, R., Curvaton reheating in tachyonic inflationary models (2006) Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 633 (2-3), pp. 149-154. , DOI 10.1016/j.physletb.2005.11.058, PII S0370269305017314
  • Chattopadhyay, S., Debnath, U., Chattopadhyay, G., (2008) Astrophys. Space Sci., 314, p. 41. , APSSBE 0004-640X 10.1007/s10509-007-9732-0
  • Del Campo, S., Herrera, R., Toloza, A., (2009) Phys. Rev. D, 79, p. 083507. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.083507
  • Jain, R.K., Chingangbam, P., Sriramkumar, L., (2011) Nucl. Phys., B852, p. 366. , NUPBBO 0550-3213 10.1016/j.nuclphysb.2011.07.003
  • Aguirregabiria, J.M., Lazkoz, R., (2004) Phys. Rev. D, 69, p. 123502. , PRVDAQ 0556-2821 10.1103/PhysRevD.69.123502
  • Aguirregabiria, J.M., Chimento, L.P., Lazkoz, R., Phantom k-essence cosmologies (2004) Physical Review D, 70 (2), p. 023509. , DOI 10.1103/PhysRevD.70.023509
  • Calcagni, G., Liddle, A.R., Tachyon dark energy models: Dynamics and constraints (2006) Physical Review D - Particles, Fields, Gravitation and Cosmology, 74 (4), p. 043528. , http://oai.aps.org/oai?verb=GetRecord&Identifier=oai:aps.org: PhysRevD.74.043528&metadataPrefix=oai_apsmeta_2, DOI 10.1103/PhysRevD.74.043528
  • Chimento, L.P., Forte, M., Kremer, G.M., Ribas, M.O., (2010) Gen. Relativ. Gravit., 42, p. 1523. , GRGVA8 0001-7701 10.1007/s10714-009-0924-5
  • Bagla, J.S., Jassal, H.K., Padmanabhan, T., Cosmology with tachyon field as dark energy (2003) Physical Review D, 67 (6), p. 063504. , DOI 10.1103/PhysRevD.67.063504
  • Guo, Z.K., Zhang, Y.Z., J. Cosmol. Astropart. Phys., 2004 (8), p. 010. , JCAPBP 1475-7516 10.1088/1475-7516/2004/08/010
  • Copeland, E.J., Garousi, M.R., Sami, M., Tsujikawa, S., (2005) Phys. Rev. D, 71, p. 043003. , PRVDAQ 1550-7998 10.1103/PhysRevD.71.043003
  • De Souza, R.C., Kremer, G.M., (2014) Phys. Rev. D, 89, p. 027302. , PRVDAQ 1550-7998 10.1103/PhysRevD.89.027302
  • Sen, A., J. High Energy Phys., 2002 (4), p. 048. , JHEPFG 1029-8479 10.1088/1126-6708/2002/04/048
  • Sen, A., J. High Energy Phys., 2002 (7), p. 065. , JHEPFG 1029-8479 10.1088/1126-6708/2002/07/065
  • Sen, A., (2002) Mod. Phys. Lett. A, 17, p. 1797. , MPLAEQ 0217-7323 10.1142/S0217732302008071
  • Sen, A., J. High Energy Phys., 1999 (10), p. 008. , JHEPFG 1029-8479 10.1088/1126-6708/1999/10/008
  • Garousi, M.R., (2000) Nucl. Phys., B584, p. 284. , NUPBBO 0550-3213 10.1016/S0550-3213(00)00361-8
  • Garousi, M.R., J. High Energy Phys., 2003 (5), p. 058. , JHEPFG 1029-8479 10.1088/1126-6708/2003/05/058
  • Bergshoeff, E.A., De Roo, M., De Wit, T.C., Eyras, E., Panda, S., J. High Energy Phys., 2000 (5), p. 009. , JHEPFG 1029-8479 10.1088/1126-6708/2000/05/009
  • Kutasov, D., Niarchos, V., Tachyon effective actions in open string theory (2003) Nuclear Physics B, 666 (1-2), pp. 56-70. , DOI 10.1016/S0550-3213(03)00498-X, PII S055032130300498X
  • Gibbons, G.W., (2002) Phys. Lett. B, 537, p. 1. , PYLBAJ 0370-2693 10.1016/S0370-2693(02)01881-6
  • Mukohyama, S., (2002) Phys. Rev. D, 66, p. 024009. , PRVDAQ 0556-2821 10.1103/PhysRevD.66.024009
  • Kofman, L., Linde, A., J. High Energy Phys., 2002 (7), p. 004. , JHEPFG 1029-8479 10.1088/1126-6708/2002/07/004
  • Sami, M., (2003) Mod. Phys. Lett. A, 18, p. 691. , MPLAEQ 0217-7323 10.1142/S021773230300968X
  • Mazumdar, A., Panda, S., Perez-Lorenzana, A., Assisted inflation via tachyon condensation (2001) Nuclear Physics B, 614 (1-2), pp. 101-116. , DOI 10.1016/S0550-3213(01)00410-2, PII S0550321301004102
  • Piao, Y.-S., Cai, R.-G., Zhang, X., Zhang, Y.-Z., Assisted tachyonic inflation (2002) Physical Review D, 66 (12), p. 121301. , DOI 10.1103/PhysRevD.66.121301
  • Cline, J.M., Firouzjahi, H., Martineau, P., J. High Energy Phys., 2002 (11), p. 041. , JHEPFG 1029-8479 10.1088/1126-6708/2002/11/041
  • Guo, Z.-K., Piao, Y.-S., Cai, R.-G., Zhang, Y.-Z., Inflationary attractor from tachyonic matter (2003) Physical Review D, 68 (4), p. 043508. , DOI 10.1103/PhysRevD.68.043508
  • Nojiri, S., Odintsov, S.D., (2003) Phys. Lett. B, 571, p. 1. , PYLBAJ 0370-2693 10.1016/j.physletb.2003.08.013
  • Elizalde, E., Lidsey, J.E., Nojiri, S., Odintsov, S.D., (2003) Phys. Lett. B, 574, p. 1. , PYLBAJ 0370-2693 10.1016/j.physletb.2003.08.074
  • Steer, D.A., Vernizzi, F., (2004) Phys. Rev. D, 70, p. 043527. , PRVDAQ 1550-7998 10.1103/PhysRevD.70.043527
  • Gorini, V., Kamenshchik, A., Moschella, U., Pasquier, V., Tachyons, scalar fields, and cosmology (2004) Physical Review D, 69 (12), p. 123512. , DOI 10.1103/PhysRevD.69.123512
  • Paul, B.C., Sami, M., Note on inflation with a tachyon rolling on the Gauss-Bonnet brane (2004) Physical Review D, 70 (2), p. 027301. , DOI 10.1103/PhysRevD.70.027301
  • Raul Abramo, L., Finelli, F., Pereira, T.S., Constraining Born-Infeld models of dark energy with CMB anisotropies (2004) Physical Review D, 70 (6), p. 063517. , DOI 10.1103/PhysRevD.70.063517
  • Calcagni, G., Tsujikawa, S., (2004) Phys. Rev. D, 70, p. 103514. , PRVDAQ 1550-7998 10.1103/PhysRevD.70.103514
  • Chimento, L.P., Extended tachyon field, Chaplygin gas, and solvable fc-essence cosmologies (2004) Physical Review D, 69 (12), p. 123517. , DOI 10.1103/PhysRevD.69.123517
  • Shi, S.-G., Piao, Y.-S., Qiao, C.-F., J. Cosmol. Astropart. Phys., 2009 (4), p. 027. , JCAPBP 1475-7516 10.1088/1475-7516/2009/04/027
  • Rangdee, R., Gumjudpai, B., (2014) Astrophys. Space Sci., 349, p. 975. , APSSBE 0004-640X 10.1007/s10509-013-1680-2
  • Novosyadlyj, B., arXiv:1311.0227; Gieres, F., Kibler, M., Lucchesi, C., Piguet, O., (1998), Symmetries in Physics, edited by, (Editions Frontieres, Gif sur Yvette, France); Green, M.B., Schwartz, J.H., Witten, E., (1987) Superstring Theory, , (Cambridge University Press, Cambridge, England);
  • Polchinski, J., (1998) String Theory, Vol. I-II, , (Cambridge University Press, Cambridge, England)
  • Veneziano, G., (1991) Phys. Lett. B, 265, p. 287. , PYLBAJ 0370-2693 10.1016/0370-2693(91)90055-U
  • Tseytlin, A.A., (1991) Mod. Phys. Lett. A, 6, p. 1721. , MPLAEQ 0217-7323 10.1142/S021773239100186X
  • Chimento, L.P., Symmetry and inflation (2002) Physical Review D, 65 (6), p. 063517. , DOI 10.1103/PhysRevD.65.063517
  • Chimento, L.P., Interacting fluids generating identical, dual and phantom cosmologies (2006) Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 633 (1), pp. 9-13. , DOI 10.1016/j.physletb.2005.11.027, PII S0370269305016904
  • Chimento, L.P., Lazkoz, R., Unified phantom cosmologies (2005) International Journal of Modern Physics D, 14 (3-4), pp. 587-598. , DOI 10.1142/S021827180500616X, PII S021827180500616X
  • Chimento, L.P., Richarte, M.G., Sánchez, I.E., (2013) Mod. Phys. Lett. A, 28, p. 1250236. , MPLAEQ 0217-7323 10.1142/S0217732312502367
  • Chimento, L.P., Forte, M., Lazkoz, R., Richarte, M.G., (2009) Phys. Rev. D, 79, p. 043502. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.043502
  • Charters, T., Mimoso, J.P., J. Cosmol. Astropart. Phys., 2010 (8), p. 022. , JCAPBP 1475-7516 10.1088/1475-7516/2010/08/022
  • Gibbons, G.W., (1987) Nucl. Phys., B292, p. 784. , NUPBBO 0550-3213 10.1016/0550-3213(87)90670-5
  • Barrow, J.D., Ellis, G.F.R., Maartens, R., Tsagas, C.G., (2003) Classical Quantum Gravity, 20, pp. L155. , CQGRDG 0264-9381 10.1088/0264-9381/20/11/102

Citas:

---------- APA ----------
(2014) . Extended tachyon field using form invariance symmetry. Physical Review D - Particles, Fields, Gravitation and Cosmology, 90(2).
http://dx.doi.org/10.1103/PhysRevD.90.027308
---------- CHICAGO ----------
Sánchez G., I.E. "Extended tachyon field using form invariance symmetry" . Physical Review D - Particles, Fields, Gravitation and Cosmology 90, no. 2 (2014).
http://dx.doi.org/10.1103/PhysRevD.90.027308
---------- MLA ----------
Sánchez G., I.E. "Extended tachyon field using form invariance symmetry" . Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 90, no. 2, 2014.
http://dx.doi.org/10.1103/PhysRevD.90.027308
---------- VANCOUVER ----------
Sánchez G., I.E. Extended tachyon field using form invariance symmetry. Phys Rev D Part Fields Gravit Cosmol. 2014;90(2).
http://dx.doi.org/10.1103/PhysRevD.90.027308