Built on

C. Wetterich, “The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’,” Astron. Astrophys. 301
1995
Earlier work this paper cites.
L. Randall and R. Sundrum, “A Large mass hierarchy from a small extra dimension,” Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
L. Amendola, “Scaling solutions in general nonminimal coupling theories,” Phys. Rev. D60
1999
Earlier work this paper cites.
L. Amendola, “Coupled quintessence,” Phys. Rev. D62
2000
Earlier work this paper cites.
G. N. Felder, L. Kofman, and A. Starobinsky, “Caustics in tachyon matter and other Born-Infeld scalars,” JHEP 09
2002
Earlier work this paper cites.
A. V. Frolov, L. Kofman, and A. A. Starobinsky, “Prospects and problems of tachyon matter cosmology,” Phys. Lett. B545
2002
Earlier work this paper cites.
L. Amendola and C. Quercellini, “Tracking and coupled dark energy as seen by WMAP,” Phys. Rev. D68
2003
Earlier work this paper cites.
L. Amendola, C. Quercellini, D. Tocchini-Valentini, and A. Pasqui, “Constraints on the interaction and selfinteraction of dark energy from cosmic microwave background,” Astrophys. J. 583
2003
Earlier work this paper cites.
L. Amendola, “Linear and non-linear perturbations in dark energy models,” Phys. Rev. D69
2004
Earlier work this paper cites.
T. Koivisto, “Growth of perturbations in dark matter coupled with quintessence,” Phys. Rev. D72
2005
Earlier work this paper cites.
R. Mainini and S. Bonometto, “Mass functions in coupled Dark Energy models,” Phys. Rev. D74
2006
Earlier work this paper cites.
C. P. Burgess, “Introduction to Effective Field Theory,” Ann. Rev. Nucl. Part. Sci. 57
2007
Earlier work this paper cites.

Similar

R. Bean, E. E. Flanagan, I. Laszlo, and M. Trodden, “Constraining Interactions in Cosmology’s Dark Sector,” Phys. Rev. D78
Original
2008
Cited alongside, same era.
R. Bean, E. E. Flanagan, and M. Trodden, “The Adiabatic Instability on Cosmology’s Dark Side,” New J. Phys. 10
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2008
Cited alongside, same era.
R. Bean, E. E. Flanagan, and M. Trodden, “Adiabatic instability in coupled dark energy-dark matter models,” Phys. Rev. D78
Original
2008
Cited alongside, same era.
V. Pettorino and C. Baccigalupi, “Coupled and Extended Quintessence: theoretical differences and structure formation,” Phys. Rev. D77
Original
2008
Cited alongside, same era.
G. La Vacca, J. R. Kristiansen, L. P. L. Colombo, R. Mainini, and S. A. Bonometto, “Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?,” JCAP 0904

Then

M. Baldi, “Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation,” Mon. Not. Roy. Astron. Soc. 411
Original
2011
Later among the works it cites.
V. Pettorino, L. Amendola, C. Baccigalupi, and C. Quercellini, “Constraints on coupled dark energy using CMB data from WMAP and SPT,” Phys. Rev. D86
Original
2012
Later among the works it cites.
V. Salvatelli, A. Marchini, L. Lopez-Honorez, and O. Mena, “New constraints on Coupled Dark Energy from the Planck satellite experiment,” Phys. Rev. D88
Original
2013
Later among the works it cites.
V. Pettorino, “Testing modified gravity with Planck: the case of coupled dark energy,” Phys. Rev. D88
Original
2013
Later among the works it cites.
C. de Rham and R. H. Ribeiro, “Riding on irrelevant operators,” JCAP 1411

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2017

Field Theories and Fluids for an Interacting Dark Sector

Gonzalez, Mariana Carrillo, Trodden, Mark

Understand

We consider the relationship between fluid models of an interacting dark sector, and the field theoretical models that underlie such descriptions.

This question is particularly important in light of suggestions that such interactions may help alleviate a number of current tensions between different cosmological datasets.
We construct consistent field theory models for an interacting dark sector that behave exactly like the coupled fluid ones, even at the level of linear perturbations, and can be trusted deep in the nonlinear regime.
As a specific example, we focus on the case of a Dirac, Born-Infeld (DBI) field conformally coupled to a quintessence field.

Built on

C. Wetterich, “The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’,” Astron. Astrophys. 301
1995
Earlier work this paper cites.
L. Randall and R. Sundrum, “A Large mass hierarchy from a small extra dimension,” Phys. Rev. Lett. 83
1999
Earlier work this paper cites.
L. Amendola, “Scaling solutions in general nonminimal coupling theories,” Phys. Rev. D60
1999
Earlier work this paper cites.
L. Amendola, “Coupled quintessence,” Phys. Rev. D62
2000
Earlier work this paper cites.
G. N. Felder, L. Kofman, and A. Starobinsky, “Caustics in tachyon matter and other Born-Infeld scalars,” JHEP 09
2002
Earlier work this paper cites.
A. V. Frolov, L. Kofman, and A. A. Starobinsky, “Prospects and problems of tachyon matter cosmology,” Phys. Lett. B545
2002
Earlier work this paper cites.
L. Amendola and C. Quercellini, “Tracking and coupled dark energy as seen by WMAP,” Phys. Rev. D68
2003
Earlier work this paper cites.
L. Amendola, C. Quercellini, D. Tocchini-Valentini, and A. Pasqui, “Constraints on the interaction and selfinteraction of dark energy from cosmic microwave background,” Astrophys. J. 583
2003
Earlier work this paper cites.
L. Amendola, “Linear and non-linear perturbations in dark energy models,” Phys. Rev. D69
2004
Earlier work this paper cites.
T. Koivisto, “Growth of perturbations in dark matter coupled with quintessence,” Phys. Rev. D72
2005
Earlier work this paper cites.
R. Mainini and S. Bonometto, “Mass functions in coupled Dark Energy models,” Phys. Rev. D74
2006
Earlier work this paper cites.
C. P. Burgess, “Introduction to Effective Field Theory,” Ann. Rev. Nucl. Part. Sci. 57
2007
Earlier work this paper cites.