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We exploit the gauge-invariant formalism to analyse the perturbative behaviour of two cosmological models based on the generalized Chaplygin gas describing both dark matter and dark energy in the present Universe.
Lifshitz E M, On the gravitational stability of the expanding universe
1946
Earlier work this paper cites.
Brillouin L 1960 Wave propagation and group velocity
1960
Earlier work this paper cites.
Lifshitz E M and Khalatnikov I M, Investigations in relativistic cosmology
1963
Earlier work this paper cites.
Bardeen J M, Gauge–invariant cosmological perturbation
1980
Earlier work this paper cites.
Erdelyi A, Magnus W, Oberhettinger F and Tricomi F G 1981 Higher Transcendental Functions
1981
Earlier work this paper cites.
Solov’eva L V and Starobinsky A A, Gravitational instability of a two–component medium in an expanding universe
1985
Earlier work this paper cites.
Kofman L A and Starobinsky A A, Cosmological constant and large-scale anisotropy of the relic background radiation
1985
Earlier work this paper cites.
Bardeen J M, Bond J R, Kaiser N and Szalay A S The statistics of peaks of gaussian random fields
1986
Earlier work this paper cites.
Peebles P J E and Ratra B, Cosmology with a time variable cosmological constant
1988
Earlier work this paper cites.
Wetterich C, Cosmology and the fate of dilatation symmetry
1988
Earlier work this paper cites.
Mukhanov V F, Feldman H A and Brandenberger R H, Theory of cosmological perturbation
1992
Earlier work this paper cites.
Sugiyama N, Cosmic background anisotropies in CDM cosmology
1995
Earlier work this paper cites.
Caldwell R R, Dave R and Steinhardt P J, Cosmological imprint of an energy component with general equation of state
1998
Earlier work this paper cites.
Starobinsky A A, How to determine an effective potential for a variable cosmological term
1998
Earlier work this paper cites.
Perlmutter S et al
1999
Earlier work this paper cites.
Peacock J A 1999 Cosmological Physics
1999
Earlier work this paper cites.
Parker L and Raval A, Non-perturbative effects of vacuum energy on the recent expansion of the universe
1999
Cited alongside, same era.
Sahni V and Starobinsky A A, The case for a positive cosmological Lambda–term
2000
Cited alongside, same era.
Kamenshchik A Y, Moschella U and Pasquier V, An alternative to quintessence
2001
Cited alongside, same era.
Bilic N, Tupper G B and Viollier R D, Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
2002
Cited alongside, same era.
Bento M C, Bertolami O and Sen A A, Generalized Chaplygin gas, accelerated expansion, and dark-energy-matter unification
2002
Cited alongside, same era.
Tegmark M et al
2002
Cited alongside, same era.
Gorini V, Kamenshchik A, Moschella U, Pasquier V and Starobinsky A, Stability properties of some perfect fluid cosmological models
2005
Later among the works it cites.
Sahni V and Starobinsky A A, Reconstructing dark energy
2006
Later among the works it cites.
Zhang H and Zhu Z, Interacting Chaplygin gas
2006
Later among the works it cites.
Wu P and Yu H, Generalized Chaplygin gas model: constraints from Hubble parameter versus redshift data
2007
Closest in time.
Wu P and Yu H, Constraints on the unified dark energy – dark matter model from latest observational data
2007
Closest in time.
Davis T et al
2007
Closest in time.
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Riess A G et al
2003
Cited alongside, same era.
Gorini V, Kamenshchik A Y and Moschella U, Can the Chaplygin gas be a plausible model for dark energy?
2003
Cited alongside, same era.
Bean R and Dorè O, Are Chaplygin gas serious contenders for the dark energy?
2003
Cited alongside, same era.
Beca L M G, Avelino P P, de Carvalho J P M and Martins C J A P, Role of baryons in unified dark matter models
2003
Cited alongside, same era.
Reis R R R, Waga I, Calvao M O and Joras S E, Entropy perturbations in quartessence Chaplygin models
2003
Cited alongside, same era.
Carturan D and Finelli F, Cosmological effects of a class of fluid dark energy models
2003
Cited alongside, same era.
Alam U, Sahni V and Starobinsky A A, Exploring the properties of dark energy using type Ia supernova and other datasets
2007
Closest in time.
Melchiorri A, Pagano L and Randolfi S, When did cosmic acceleration start?
2007
Closest in time.
2007
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Riess A G et al
2007
Closest in time.
Daly R A and Djorgovsky S G, The acceleration history of the Universe and properties of dark energy
2007
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Wang Y and Mukherjee P, Observational constraints on dark energy and cosmic curvature
2007
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Kang J U, Vanchurin V and Winitzki S, Attractor scenarios and superluminal signals in k-essence cosmology
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Bertacca D and Bartolo N, ISW effect in the unified dark matter scalar field cosmologies: an analytical approach
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