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Abstract:

We show the kinematic equivalence between cosmological models driven by Dirac{Born{ Infeld (DBI) fields with constant proper velocity of the brane and exponential potential V = V0e-B, and interactive cosmological systems with modified holographic Ricci type uids as dark energy (DE) in at Friedmann-Robertson-Walker (FRW) cosmologies. © 2017 World Scientific Publishing Company.

Registro:

Documento: Artículo
Título:Kinematic equivalence between models driven by DBI field with constant γ and exotic holographic quintessence cosmological models
Autor:Forte, M.
Filiación:Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, 1428, Argentina
Palabras clave:DBI field; interacting dark energy; modified holographic Ricci
Año:2017
Volumen:32
Número:26
DOI: http://dx.doi.org/10.1142/S0217732317501401
Título revista:Modern Physics Letters A
Título revista abreviado:Mod. Phys. Lett. A
ISSN:02177323
CODEN:MPLAE
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02177323_v32_n26_p_Forte

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Citas:

---------- APA ----------
(2017) . Kinematic equivalence between models driven by DBI field with constant γ and exotic holographic quintessence cosmological models. Modern Physics Letters A, 32(26).
http://dx.doi.org/10.1142/S0217732317501401
---------- CHICAGO ----------
Forte, M. "Kinematic equivalence between models driven by DBI field with constant γ and exotic holographic quintessence cosmological models" . Modern Physics Letters A 32, no. 26 (2017).
http://dx.doi.org/10.1142/S0217732317501401
---------- MLA ----------
Forte, M. "Kinematic equivalence between models driven by DBI field with constant γ and exotic holographic quintessence cosmological models" . Modern Physics Letters A, vol. 32, no. 26, 2017.
http://dx.doi.org/10.1142/S0217732317501401
---------- VANCOUVER ----------
Forte, M. Kinematic equivalence between models driven by DBI field with constant γ and exotic holographic quintessence cosmological models. Mod. Phys. Lett. A. 2017;32(26).
http://dx.doi.org/10.1142/S0217732317501401