The exploration of cosmological scenarios that incorporate a blend of variable modified Chaplygin gas and tachyonic fluid within the context of higher-dimensional theories of gravity represents a highly specialized and intricate area of study within the domains of theoretical physics and cosmology. In this paper, we have explored a five-dimensional cosmological model, taking into account the presence of Chaplygin gas and tachyonic fluid. Our study involves an investigation into various physical and kinematic properties of this model.
REFERENCES
1.
S.
Perlmutter
, et al, (1998
). Discovery of a supernova explosion half the age of the universe
. Nature
, 391
, 51
.2.
S.
Riess
, et al, (2004
). Type Ia Supernova discoveries at z> 1 from the Hubble space telescope: Evidence for past deceleration and constraints on dark energy evolution
. Astrophys.J.
, 607
, 665
.3.
D.
Miller
, et al, (1999
). A Measurement of the angular power spectrum of the cosmic microwave background from l=100 to 400
”. Astrophys. J
, 524
, L1
.4.
S.
Briddle
, et al, (2003
). Precision cosmology? Not just yet…
Science
, 299
, 1532
.5.
S.
Spergel
, et al,(2003
). First-Year Wilkinson microwave anisotropy probe (WMAP)* observations: Determination of cosmological parameters
. Astrophys. J. Suppl.
, 148
, 175
.6.
C.
Wetterich
, (1988
). Cosmology and the fate of dilatation symmetry
. Nucl. Phys. B
, 302
, 668
.7.
R. R.
Caldwell
, (2002
). A phantom menace? Cosmological consequences of a dark energy component with the super-negative equation of state
. Phys. Lett. B
, 545
, 23
.8.
B.
Feng
, X. L.
Wang
and X. M.
Zhang
, (2005
). Dark energy constraints from the cosmic age and supernova
. Phys. Lett. B
, 607
, 35
.9.
Y. F.
Cai
, H.
Li
, Y. S.
Piao
and X. M.
Zhang
, (2007
). Cosmic duality in quintom universe
, Phys. Lett. B
, 646
, 141
.10.
Y. F.
Cai
, M. Z.
Li
, J. X.
Lu
, Y. S.
Piao
, T. T. Qiuand X. M.
Zhang
, (2007
). A string-inspired quintom model of dark energy
. Phys. Lett. B
, 651
, 1
.11.
Y. F.
Cai
, E. N.
Saridakis
, M. R.
Setare
and J. Q.
Xia
, (2010
), Quintom cosmology: theoretical implications and observations
. Phys. Rep.
, 493
, 1
.12.
Y. F.
Cai
and J.
Wang
, (2008
). Dark energy model with spinor matter and its quintom scenario
. Class. Quantum Gravity
, 25
, 165014
.13.
M.R.
Setare
, J.
Sadeghi
and A. R.
Amani
, (2009
). Interacting Tachyon dark energy in a non-flat universe
. Phys. Lett. B
, 673
, 241
.14.
M.R.
Setare
, (2007
). Holographic Chaplygin gas model
. Phys. Lett. B
, 648
, 329
.15.
M. R.
Setare
,(2007a
). Holographic Tachyon model of dark energy
. Phys. Lett. B
,653
, 116
.16.
M.R.
Setare
, (2009
). Holographic Chaplygin DGP cosmologies
. Int. J. Mod. Phys. D
, 18
, 419
.17.
N.
Afshordi
, D.J.H.
Chung
and G.
Geshnizjani
, (2007
). Causal field theory with an infinite speed of sound
. Phys. Rev. D
, 75
, 083513
.18.
19.
M.
Makler
, et al, (2003
). Constraints on the generalized Chaplygin gas from supernovae observations
. Phys. Lett. B
, 555
, 1
.20.
H.
Sandvik
, et al, (2004
). The end of unified dark matter?
Phys. Rev. D
, 69
, 123524
.21.
Z. H.
Zhu
, (2004
). Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
. Astron. Astrophys.
, 423
, 421
.22.
M.C.
Bento
, O.
Bertolami
and A. A.
Sen
, (2003
). WMAP constraints on the generalized Chaplygin gas model
. Phys. Lett. B
, 575
, 172
.23.
N.
Bilic
, G. B.
Tupper
and R. D.
Viollier
, (2002
). Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
. Phys. Lett. B
, 535
, 17
.24.
D.
Bazeia
, (1999
). Galileo’s invariant system and the motion of relativistic d-branes
. Phys. Rev. D
, 59
, 085007
.25.
M.R.
Setare
, (2007b
). Interacting holographic generalized Chaplygin gas model
. Phys. Lett. B
, 654
, 1
.26.
M.R.
Setare
, (2007c
). Interacting generalized Chaplygin gas model in the non-flat universe
. Eur. Phys. J. C
, 52
, 689
.27.
U.
Debnath
, A.
Banerjee
and S.
Chakraborty
, (2004
). Role of modified Chaplygin gas in the accelerated universe
. Class. Quantum Gravity
, 21
, 5609
.28.
S. M.
Noorbakhsh
and M.
Ghominejadwe
, (2013
). Interaction between Tachyon dark energy and modified Chaplygin gas
. Astrophys. Space Sc.
, 348
, 221
.29.
M.
Khurshudyan
, (2018
), Can an interacting varying Chaplygin gas and tachyonic matter accelerate the universe?
Int. J. Geom. Methods in Mod. Phys.
09
1850155
.30.
H.
Benaoum
, (2022
), Accelerated Universe from Modified Chaplygin Gas and Tachyonic Fluid
, Universe
, 8
(7
), 340
.31.
M.
Khurshudyan
, (2013a
). Interaction between generalized varying Chaplygin gas and Tachyonic fluid
. arXiv:1301.1021 [gr-qc].32.
M.
Khurshudyan
, (2013b
). Interaction between variable Chaplygin gas and Tachyonic matter
. arXiv:1301.4990 [gr-qc].33.
34.
U.
Alam
, V.
Sahni
, T. D.
Saini
, A. A.
Starobinsky
, (2004
). Is there supernova evidence for dark energy metamorphosis?
Mon. Not. R. Astron. Soc.
, 354
, 275
.
This content is only available via PDF.
© 2024 Author(s). Published under an exclusive license by AIP Publishing.
2024
Author(s)
You do not currently have access to this content.