2012
DOI: 10.1016/j.physletb.2012.04.001
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Interacting agegraphic dark energy model in tachyon cosmology coupled to matter

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Cited by 16 publications
(18 citation statements)
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“…Otherwise, in this paper we prove that the works [2][3][4][5]11] that use L m = P , or any of the specific linear combination of −ρ and P for the Lagrangian, are incompatible with the matter current conservation. Also, let us remark that it seems very unlikely that in the most general case -where the matter current conservation constraint is relaxed -the Lagrangian would reduce precisely to either L m = P or any of the specific linear combination of −ρ and P that is used in many works.…”
Section: Conclusion and Final Remarksmentioning
confidence: 75%
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“…Otherwise, in this paper we prove that the works [2][3][4][5]11] that use L m = P , or any of the specific linear combination of −ρ and P for the Lagrangian, are incompatible with the matter current conservation. Also, let us remark that it seems very unlikely that in the most general case -where the matter current conservation constraint is relaxed -the Lagrangian would reduce precisely to either L m = P or any of the specific linear combination of −ρ and P that is used in many works.…”
Section: Conclusion and Final Remarksmentioning
confidence: 75%
“…Also, let us remark that it seems very unlikely that in the most general case -where the matter current conservation constraint is relaxed -the Lagrangian would reduce precisely to either L m = P or any of the specific linear combination of −ρ and P that is used in many works. Therefore, we finally argue that one should be very cautious before considering any of the results of the works that used the results of Brown [6] in alternative theories of gravity without questioning the validity of its extrapolation to this type of models, as, for instance, in [2][3][4][5]11].…”
Section: Conclusion and Final Remarksmentioning
confidence: 94%
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“…Tachyon scalar field motivated from string theory is a especial scalar field which can explain the whole history of the Universe from inflation to late time acceleration [50][51][52][53][54][55][56][57][58][59]. The tachyon field reconstruction of HDE and ADE models has been studied separately in some works [60][61][62][63][64].…”
Section: Issn: 2641-886xmentioning
confidence: 99%
“…Also, before the nucleus decay neutrino was not a belongings as a part of that nucleus, already it is appeared at the moment of the nucleus decay, as a consequence of a process of the interaction with dark energy and dark matter as in [40][41][42][43].…”
Section: Commentmentioning
confidence: 99%