Phantom cosmologies and fermions
Form invariance transformations can be used for constructing phantom cosmologies starting with conventional cosmological models. In this work we reconsider the scalar field case and extend the discussion to fermionic fields, where the 'phantomization' process exhibits a new class of possib...
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2008
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Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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LEADER | 04297caa a22006257a 4500 | ||
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001 | PAPER-5972 | ||
003 | AR-BaUEN | ||
005 | 20230518203539.0 | ||
008 | 190411s2008 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-43049093393 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
100 | 1 | |a Chimento, L.P. | |
245 | 1 | 0 | |a Phantom cosmologies and fermions |
260 | |c 2008 | ||
270 | 1 | 0 | |m Chimento, L. P.; Departamento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina; email: chimento@df.uba.ar |
506 | |2 openaire |e Política editorial | ||
504 | |a Chimento, L.P., (2002) Phys. Rev., 65 (6), p. 063517 | ||
504 | |a Aguirregabiria, J.M., Chimento, L.P., Jakubi, A.S., Lazkoz, R., (2003) Phys. Rev., 67 (8), p. 083518 | ||
504 | |a Chimento, L.P., Lazkoz, R., (2003) Phys. Rev. Lett., 91 (21), p. 211301 | ||
504 | |a Aguirregabiria, J.M., Chimento, L.P., Lazkoz, R., (2004) Phys. Rev., 70 (2), p. 023509 | ||
504 | |a Chimento, L.P., Lazkoz, R., (2005) Int. J. Mod. Phys., 14, p. 587 | ||
504 | |a Chimento, L.P., (2006) Phys. Lett., 633 (1), p. 9 | ||
504 | |a Caldwell, R.R., (2002) Phys. Lett., 545 (1-2), p. 23 | ||
504 | |a Caldwell, R.R., Kamionkowski, M., Weinberg, N.N., (2003) Phys. Rev. Lett., 91 (7), p. 071301 | ||
504 | |a Gonzalez-Diaz, P.F., (2003) Phys. Rev., 68 (2), p. 021303 | ||
504 | |a Johri, V.B., (2004) Phys. Rev., 70 (4), p. 041303 | ||
504 | |a Singh, P., Sami, M., Dadhich, N., (2003) Phys. Rev., 68 (2), p. 023522 | ||
504 | |a Li, X.-Z., Hao, J.-G., (2004) Phys. Rev., 69 (10), p. 107303 | ||
504 | |a Dabrowski, M.P., Stachowiak, T., Szydlowski, M., (2003) Phys. Rev., 68 (10), p. 103519 | ||
504 | |a Obukhov, Y.N., (1993) Phys. Lett., 182 (2-3), p. 214 | ||
504 | |a Saha, B., Shikin, G.N., (1997) Gen. Rel. Grav., 29 (9), p. 1099 | ||
504 | |a Saha, B., (2001) Phys. Rev., 64 (12), p. 123501 | ||
504 | |a Armendariz-Picon, C., Greene, P.B., (2003) Gen. Rel. Grav., 35 (9), p. 1637 | ||
504 | |a Saha, B., Boyadjiev, T., (2004) Phys. Rev., 69 (12), p. 124010 | ||
504 | |a Saha, B., (2006) Phys. Rev., 74 (12), p. 124030 | ||
504 | |a Ribas, M.O., Devecchi, F.P., Kremer, G.M., (2005) Phys. Rev., 72 (12), p. 123502 | ||
504 | |a Cataldo, M., Chimento, L.P., (2005); Chimento, L.P., Pavon, D., (2006) Phys. Rev., 73 (6), p. 063511 | ||
504 | |a Chimento, L.P., Zimdahl, W., (2006); Cai, Y.F., Li, H., Piao, Y.S., Zhang, X., (2007) Phys. Lett., 646 (4), p. 141 | ||
504 | |a Veneziano, G., (1991) Phys. Lett., 265 (3-4), p. 287 | ||
504 | |a Chimento, L.P., Lazkoz, R., (2006) Class. Quantum Grav., 23 (9), p. 3195 | ||
520 | 3 | |a Form invariance transformations can be used for constructing phantom cosmologies starting with conventional cosmological models. In this work we reconsider the scalar field case and extend the discussion to fermionic fields, where the 'phantomization' process exhibits a new class of possible accelerated regimes. As an application we analyze the cosmological constant group for a fermionic seed fluid. © 2008 IOP Publishing Ltd. |l eng | |
593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina | ||
593 | |a Departamento de Física, Universidade Federal Do Paran, Caixa Postal 19044, 81531-990 Curitiba, Brazil | ||
700 | 1 | |a Devecchi, F.P. | |
700 | 1 | |a Forte, M. | |
700 | 1 | |a Kremer, G.M. | |
773 | 0 | |d 2008 |g v. 25 |k n. 8 |p Classical Quantum Gravity |x 02649381 |w (AR-BaUEN)CENRE-326 |t Classical and Quantum Gravity | |
856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-43049093393&doi=10.1088%2f0264-9381%2f25%2f8%2f085007&partnerID=40&md5=0e7b220ccd2257a937d31373d6491d82 |y Registro en Scopus |
856 | 4 | 0 | |u https://doi.org/10.1088/0264-9381/25/8/085007 |y DOI |
856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_02649381_v25_n8_p_Chimento |y Handle |
856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02649381_v25_n8_p_Chimento |y Registro en la Biblioteca Digital |
961 | |a paper_02649381_v25_n8_p_Chimento |b paper |c PE | ||
962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
963 | |a VARI | ||
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