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In this paper, after reconstructing the redshift evolution of the Hubble function by adopting Gaussian process techniques, we estimate the best-fit parameters for some flat Friedmann cosmological models based on a Modified Chaplygin Gas interacting with dark matter.
1903
Earlier work this paper cites.
1905
Earlier work this paper cites.
1906
Earlier work this paper cites.
1906
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
1910
Earlier work this paper cites.
1911
Earlier work this paper cites.
1912
Earlier work this paper cites.
1931
Earlier work this paper cites.
R. G. Cai and Q. Su, “On the Dark Sector Interactions,” Phys. Rev. D 81
1943
Earlier work this paper cites.
D. J. Gross and F. Wilczek, “Ultraviolet Behavior of Nonabelian Gauge Theories,” Phys. Rev. Lett. 30
1973
Earlier work this paper cites.
H. D. Politzer, “Reliable Perturbative Results for Strong Interactions?,” Phys. Rev. Lett. 30
1973
Earlier work this paper cites.
R. D. Peccei and H. R. Quinn, “Constraints imposed by CP conservation in the presence of pseudoparticles,” Phys. Rev. D 16
1977
Earlier work this paper cites.
J. R. Bond, G. Efstathiou and J. Silk, “Massive Neutrinos and the Large Scale Structure of the Universe,” Phys. Rev. Lett. 45
1980
Earlier work this paper cites.
R. M. Wald, General Relativity
1984
Earlier work this paper cites.
J. D. Barrow, “String-Driven Inflationary and Deflationary Cosmological Models,” Nucl. Phys. B 310
1988
Earlier work this paper cites.
C. Wetterich, “Cosmology and the Fate of Dilatation Symmetry,” Nucl. Phys. B 302
1988
Earlier work this paper cites.
B. Ratra and P. J. E. Peebles, “Cosmological Consequences of a Rolling Homogeneous Scalar Field,” Phys. Rev. D 37
1988
Earlier work this paper cites.
W. H. Press, B. P. Flannery, S. A. Teukolsky, W. T. Vetterling, “ Numerical Recipes in C: The Art of Scientific Computing
1992
Earlier work this paper cites.
V. F. Mukhanov, H. A. Feldmann, and R. H. Brandenberger, “Theory of cosmological perturbations,” Phys. Rep. 215
1992
Earlier work this paper cites.
P. J. E. Peebles, Principles of physical cosmology
1993
Earlier work this paper cites.
S. Dodelson and L. M. Widrow, “Sterile-neutrinos as dark matter,” Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
S. Dodelson and L. M. Widrow, “Sterile-neutrinos as dark matter,” Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
C. Wetterich, “The Cosmon model for an asymptotically vanishing time dependent cosmological constant,” Astron. Astrophys. 301
1995
Earlier work this paper cites.
J. Polchinski, String theory. Vol. 2: Superstring theory and beyond
1998
Earlier work this paper cites.
W. Hu, “Structure formation with generalized dark matter,” Astrophys. J. 506
1998
Earlier work this paper cites.
U. Seljak and M. Zaldarriaga, “Direct signature of an evolving gravitational potential from the cosmic microwave background,” Phys. Rev. D 60
1999
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour and V. F. Mukhanov, “k - inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, “Perturbations in k-inflation,” Phys. Lett. B 458
1999
Earlier work this paper cites.
F. Takayama and M. Yamaguchi, “Gravitino dark matter without R-parity,” Phys. Lett. B 485
2000
Earlier work this paper cites.
N. Arkani-Hamed, L. J. Hall, C. F. Kolda and H. Murayama, “A New perspective on cosmic coincidence problems,” Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
T. Chiba, T. Okabe and M. Yamaguchi, “Kinetically driven quintessence,” Phys. Rev. D 62
2000
Earlier work this paper cites.
A. Y. Kamenshchik, U. Moschella and V. Pasquier, “An Alternative to quintessence,” Phys. Lett. B 511
2001
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. G. Steinhardt, “Essentials of k k -essence,” Phys. Rev. D 63
2001
Earlier work this paper cites.
H. B. Benaoum, “Accelerated universe from modified Chaplygin gas and tachyonic fluid,” arXiv:0205140 [hep-th] (2002)
2002
Earlier work this paper cites.
M. C. Bento, O. Bertolami and A. A. Sen, “Generalized Chaplygin gas, accelerated expansion and dark energy matter unification,” Phys. Rev. D 66
2002
Earlier work this paper cites.
H. Stephani, D. Kramer, M. MacCallum, C. Hoensealers, E. Herlt, Exact Solutions of Einstein’s Field Equations
2002
Earlier work this paper cites.
R. R. Caldwell, “A Phantom menace?,” Phys. Lett. B 545
2002
Earlier work this paper cites.
M. B. Hoffman, “Cosmological constraints on a dark matter - dark energy interaction,” (2003), arXiv:0307350 [astro-ph]
2003
Earlier work this paper cites.
D. Hooper and L. T. Wang, “Possible evidence for axino dark matter in the galactic bulge,” Phys. Rev. D 70
2004
Earlier work this paper cites.
R. Fardon, A. E. Nelson and N. Weiner, “Dark energy from mass varying neutrinos,” JCAP 0410
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, “Chameleon fields: Awaiting surprises for tests of gravity in space,” Phys. Rev. Lett. 93
2004
Earlier work this paper cites.
J. Khoury and A. Weltman, “Chameleon cosmology,” Phys. Rev. D 69
2004
Earlier work this paper cites.
U. Debnath, A. Banerjee and S. Chakraborty, “Role of Modified Chaplygin Gas in Accelerated Universe,” Class. Quantum Grav. 21
2004
Earlier work this paper cites.
R. Cai and A. Wang, “Cosmology with interaction between phantom dark energy and dark matter and the coincidence problem,” JCAP 03
2005
Cited alongside, same era.
R. D. Peccei, “Neutrino models of dark energy,” Phys. Rev. D 71
2005
Cited alongside, same era.
X. J. Bi, B. Feng, H. Li and X. Zhang, “Cosmological evolution of interacting dark energy models with mass varying neutrinos,” Phys. Rev. D 72
2005
Cited alongside, same era.
S. Nojiri, S. D. Odintsov and S. Tsujikawa, “Properties of singularities in (phantom) dark energy universe,” Phys. Rev. D 71
2005
Cited alongside, same era.
J. D. Barrow and T. Clifton, “Cosmologies with energy exchange,” Phys. Rev. D 73
2006
Cited alongside, same era.
2014
Later among the works it cites.
2014
Later among the works it cites.
2014
Later among the works it cites.
W. Yang and L. Xu, “Testing coupled dark energy with large scale structure observation,” JCAP 08
2014
Later among the works it cites.
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S. Capozziello, S. Nojiri and S. Odintsov, “Unified phantom cosmology: Inflation, dark energy and dark matter under the same standard,” Phys. Lett. B 632
2006
Cited alongside, same era.
S. Nojiri and S. D. Odintsov, “Unifying phantom inflation with late-time acceleration: Scalar phantom-non-phantom transition model and generalized holographic dark energy,” Gen. Rel. Grav. 38
2006
Cited alongside, same era.
S. Nojiri, S. D. Odintsov and H. Stefancic, “On the way from matter-dominated era to dark energy universe,” Phys. Rev. D 74
2006
Cited alongside, same era.
L. Amendola, G. Camargo Campos and R. Rosenfeld, “Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data,” Phys. Rev. D 75
2007
Cited alongside, same era.
R. D. Peccei, “The Strong CP problem and axions,” Lect. Notes Phys. 741
2008
Cited alongside, same era.
2008
Cited alongside, same era.
2008
Cited alongside, same era.
2014
Later among the works it cites.
2014
Later among the works it cites.
R. C. Nunes and E. M. Barboza, Dark matter-dark energy interaction for a time-dependent EoS parameter, Gen. Rel. Grav. 46 (2014) 1820, [1404.1620]
2014
Later among the works it cites.
2014
Later among the works it cites.
2014
Later among the works it cites.
2014
Later among the works it cites.
2014
Later among the works it cites.
F. Iocco, M. Pato and G. Bertone, “Evidence for dark matter in the inner Milky Way,” Nature Phys. 11
2015
Later among the works it cites.
2015
Later among the works it cites.
2015
Later among the works it cites.
J. -B. Chen, Z. -Q. Liu, and L. Xing, “Cosmological constraints on the variable modified Chaplygin gas model by using MCMC approach,” IJMPD 24
2015
Later among the works it cites.
2015
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
W. Yang, H. Li, Y. Wu and J. Lu, “Cosmological constraints on coupled dark energy,” JCAP 10
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
M. J. Zhang and J. Q. Xia, “Test of the cosmic evolution using Gaussian processes,” JCAP 1612
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
2016
Later among the works it cites.
S. Kumar, and R. C. Nunes, “Echo of interactions in the dark sector,” Phys. Rev. D 96
2017
Later among the works it cites.
2017
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2017
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2017
Later among the works it cites.
2017
Later among the works it cites.
2017
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L. Amendola, J. Rubio and C. Wetterich, “Primordial black holes from fifth forces,” Phys. Rev. D 97
2018
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2018
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2018
Later among the works it cites.
2018
Later among the works it cites.
2019
Later among the works it cites.
J. Mifsud and C. van de Bruck, “An interacting dark sector and the implications of the first gravitational-wave standard siren detection on current constraints,” Mon. Not. Roy. Astron. Soc. 487
2019
Later among the works it cites.
2019
Later among the works it cites.
2019
Later among the works it cites.
H. Li, W. Yang, L. Gai, “Astronomical bounds on the modified Chaplygin gas as a unified dark fluid model,” A&A 623
2019
Later among the works it cites.
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