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We study observational signatures of non-gravitational interactions between the dark components of the cosmic fluid, which can be either due to creation of dark particles from the expanding vacuum or an effect of the clustering of a dynamical dark energy.
1902
Earlier work this paper cites.
1907
Earlier work this paper cites.
1907
Earlier work this paper cites.
1908
Earlier work this paper cites.
1908
Earlier work this paper cites.
A. P. Billyard and A. A. Coley, “Interactions in scalar field cosmology,” Phys. Rev
2000
Earlier work this paper cites.
L. Amendola, “Coupled quintessence,” Phys. Rev
2000
Earlier work this paper cites.
J. Martin, A. Riazuelo and M. Sakellariadou, “Nonvacuum initial states for cosmological perturbations of quantum mechanical origin,” Phys. Rev. D 61, 083518 (2000)
2000
Earlier work this paper cites.
W. Zimdahl, D. Pavon, and L. P. Chimento, “Interacting quintessence,” Phys. Lett
2001
Earlier work this paper cites.
W. Zimdahl, D. J. Schwarz, A. B. Balakin and D. Pavon, “Cosmic anti-friction and accelerated expansion,” Phys. Rev. D 64, 063501 (2001)
2001
Earlier work this paper cites.
A. Y. Kamenshchik, U. Moschella and V. Pasquier, “An Alternative to quintessence,” Phys. Lett. B 511, 265 (2001)
2001
Earlier work this paper cites.
I. Wasserman, “On the degeneracy inherent in observational determination of the dark energy equation of state,” Phys. Rev. D 66, 123511 (2002)
2002
Earlier work this paper cites.
C. Rubano and P. Scudellaro, “Quintessence or phoenix?,” Gen. Rel. Grav. 34, 1931 (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, 043507 (2002)
2002
Earlier work this paper cites.
N. Bilic, G. B. Tupper and R. D. Viollier, “Unification of dark matter and dark energy: The Inhomogeneous Chaplygin gas,” Phys. Lett. B 535, 17 (2002)
2002
Earlier work this paper cites.
J. S. Alcaniz, D. Jain and A. Dev, “High - redshift objects and the generalized Chaplygin gas,” Phys. Rev. D 67, 043514 (2003)
2003
Earlier work this paper cites.
S. Dodelson, “Modern Cosmology,” Amsterdam, Netherlands: Academic Pr. (2003) 440 p
2003
Earlier work this paper cites.
A. Dev, D. Jain and J. S. Alcaniz, “Constraints on Chaplygin quartessence from the CLASS gravitational lens statistics and supernova data,” Astron. Astrophys. 417, 847 (2004)
2004
Earlier work this paper cites.
M. C. Bento, O. Bertolami and A. A. Sen, “The Revival of the unified dark energy - dark matter model?,” Phys. Rev. D 70, 083519 (2004)
2004
Earlier work this paper cites.
S. Cole et al
2005
Earlier work this paper cites.
M. Tegmark et al
2006
Earlier work this paper cites.
W. J. Percival et al
2007
Earlier work this paper cites.
J.-H. He and B. Wang, “Effects of the interaction between dark energy and dark matter on cosmological parameters,” JCAP
2008
Earlier work this paper cites.
J. Valiviita, E. Majerotto, and R. Maartens, “Instability in interacting dark energy and dark matter fluids,” JCAP
2008
Earlier work this paper cites.
M. Kunz, “The dark degeneracy: On the number and nature of dark components,” Phys. Rev. D 80, 123001 (2009)
2009
Cited alongside, same era.
S. del Campo, R. Herrera and D. Pavon, “Interacting models may be key to solve the cosmic coincidence problem,” JCAP 0901, 020 (2009)
2009
Cited alongside, same era.
I. L. Shapiro and J. Sola, “On the possible running of the cosmological ’constant’,” Phys. Lett. B 682, 105 (2009)
2009
Cited alongside, same era.
K. Koyama, R. Maartens and Y. S. Song, “Velocities as a probe of dark sector interactions,” JCAP 0910, 017 (2009)
2009
Cited alongside, same era.
K. A. Malik and D. Wands, “Cosmological perturbations,” Phys. Rept. 475, 1 (2009)
2009
Cited alongside, same era.
B. A. Reid et al
N. Aghanim et al
2016
Later among the works it cites.
C. Pigozzo, S. Carneiro, J. S. Alcaniz, H. A. Borges and J. C. Fabris, “Evidence for cosmological particle creation?,” JCAP 1605, no. 05, 022 (2016)
2016
Later among the works it cites.
R. F. vom Marttens, L. Casarini, W. Zimdahl, W. S. Hipólito-Ricaldi and D. F. Mota, “Does a generalized Chaplygin gas correctly describe the cosmological dark sector?,” Phys. Dark Univ. 15, 114 (2017)
2017
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2017
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2018
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2010
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W. Zimdahl, H. A. Borges, S. Carneiro, J. C. Fabris and W. S. Hipolito-Ricaldi, “Non-adiabatic perturbations in decaying vacuum cosmology,” JCAP 1104, 028 (2011)
2011
Cited alongside, same era.
D. Blas, J. Lesgourgues and T. Tram, “The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes,” JCAP 1107, 034 (2011)
2011
Cited alongside, same era.
D. Wands, J. De-Santiago and Y. Wang, “Inhomogeneous vacuum energy,” Class. Quant. Grav. 29, 145017 (2012)
2012
Cited alongside, same era.
J. S. Alcaniz, H. A. Borges, S. Carneiro, J. C. Fabris, C. Pigozzo and W. Zimdahl, “A cosmological concordance model with dynamical vacuum term,” Phys. Lett. B 716, 165 (2012)
2012
Cited alongside, same era.
H. A. Borges, S. Carneiro, J. C. Fabris and W. Zimdahl, “Non-adiabatic Chaplygin gas,” Phys. Lett. B 727, 37 (2013)
2013
Cited alongside, same era.
Y. Wang, D. Wands, L. Xu, J. De-Santiago and A. Hojjati, “Cosmological constraints on a decomposed Chaplygin gas,” Phys. Rev. D 87, no. 8, 083503 (2013)
2013
Cited alongside, same era.
F. D’Eramo, R. Z. Ferreira, A. Notari and J. L. Bernal, “Hot Axions and the H 0 H_{0} tension,” JCAP 1811, no. 11, 014 (2018)
2018
Later among the works it cites.
K. Bolejko, “Emerging spatial curvature can resolve the tension between high-redshift CMB and low-redshift distance ladder measurements of the Hubble constant,” Phys. Rev. D 97, no. 10, 103529 (2018)
2018
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E. Mörtsell and S. Dhawan, “Does the Hubble constant tension call for new physics?,” JCAP 1809, no. 09, 025 (2018)
2018
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M. Benetti, L. L. Graef and J. S. Alcaniz, “The H 0 H_{0} and σ 8 \sigma_{8} tensions and the scale invariant spectrum,” JCAP 1807, no. 07, 066 (2018)
2018
Later among the works it cites.
J. E. Gonzalez, H. H. B. Silva, R. Silva and J. S. Alcaniz, “Physical constraints on interacting dark energy models,” Eur. Phys. J. C 78, no. 9, 730 (2018)
2018
Later among the works it cites.
S. Carneiro, “The cosmological dark sector as a scalar σ \sigma -meson field,” Eur. Phys. J. C 78, no. 3, 183 (2018)
2018
Later among the works it cites.
S. Carneiro, “Can the cosmological dark sector be modeled by a single scalar field?,” Gen. Rel. Grav. 50, no. 9, 114 (2018)
2018
Later among the works it cites.
S. Carneiro and H. A. Borges, “Dynamical system analysis of interacting models,” Gen. Rel. Grav. 50, no. 10, 129 (2018)
2018
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D. M. Scolnic et al
2018
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R. J. Cooke, M. Pettini and C. C. Steidel, “One Percent Determination of the Primordial Deuterium Abundance,” Astrophys. J. 855, no. 2, 102 (2018)
2018
Later among the works it cites.
E. Di Valentino, A. Melchiorri, Y. Fantaye and A. Heavens, “Bayesian evidence against the Harrison-Zel’dovich spectrum in tensions with cosmological data sets,” Phys. Rev. D 98, no. 6, 063508 (2018)
2018
Later among the works it cites.
R. Aurich and S. Lustig, “On the concordance of cosmological data in the case of the generalized Chaplygin gas,” Astropart. Phys. 97, 118 (2018)
2018
Later among the works it cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” Astrophys. J. 876, no. 1, 85 (2019)
2019
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S. Carneiro, P. C. de Holanda, C. Pigozzo and F. Sobreira, “Is the H 0 H_{0} tension suggesting a fourth neutrino generation?,” Phys. Rev. D 100, no. 2, 023505 (2019)
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V. Poulin, T. L. Smith, T. Karwal and M. Kamionkowski, “Early Dark Energy Can Resolve The Hubble Tension,” Phys. Rev. Lett. 122, no. 22, 221301 (2019)
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L. L. Graef, M. Benetti and J. S. Alcaniz, “Primordial gravitational waves and the H0-tension problem,” Phys. Rev. D 99, no. 4, 043519 (2019)
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A. Cid, B. Santos, C. Pigozzo, T. Ferreira and J. Alcaniz, “Bayesian Comparison of Interacting Scenarios,” JCAP 1903, no. 03, 030 (2019)
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R. von Marttens, L. Casarini, D. F. Mota and W. Zimdahl, “Cosmological constraints on parametrized interacting dark energy,” Phys. Dark Univ. 23, 100248 (2019)
2019
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