Field theoretic interpretations of interacting dark energy scenarios and recent observations

M. Martinelli, N. B. Hogg, S. Peirone, M. Bruni and D. Wands, Constraints on the interacting vacuum–geodesic CDM scenario,

Original

1902

Earlier work this paper cites.

M. Asghari, J. Beltrán Jiménez, S. Khosravi and D. F. Mota, On structure formation from a small-scales-interacting dark sector,

Original

1902

Earlier work this paper cites.

A. Paliathanasis, S. Pan and W. Yang, Dynamics of nonlinear interacting dark energy models,

Original

1903

Earlier work this paper cites.

S. Pan, W. Yang, C. Singha and E. N. Saridakis, Observational constraints on sign-changeable interaction models and alleviation of the H 0 H_{0} tension,

Original

1903

Earlier work this paper cites.

S. Kumar, R. C. Nunes and S. K. Yadav, Dark sector interaction: a remedy of the tensions between CMB and LSS data,

Original

1903

Earlier work this paper 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 Λ \Lambda CDM,

Original

1903

Earlier work this paper cites.

W. Yang, S. Pan, E. Di Valentino, B. Wang and A. Wang, Forecasting Interacting Vacuum-Energy Models using Gravitational Waves,

Original

1904

Earlier work this paper cites.

N. Zhang, Y. B. Wu, J. N. Chi, Z. Yu and D. F. Xu, Diagnosing the interacting Tsallis Holographic Dark Energy models,

Original

1905

Earlier work this paper cites.

W. Yang, S. Vagnozzi, E. Di Valentino, R. C. Nunes, S. Pan and D. F. Mota, Listening to the sound of dark sector interactions with gravitational wave standard sirens,

Original

1905

Earlier work this paper cites.

W. Yang, O. Mena, S. Pan and E. Di Valentino, Dark sectors with dynamical coupling,

Original

1906

Earlier work this paper cites.

S. Savastano, L. Amendola, J. Rubio and C. Wetterich, Primordial dark matter halos from fifth forces,

Original

1906

Earlier work this paper cites.

S. Pan, W. Yang, E. Di Valentino, E. N. Saridakis and S. Chakraborty, Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the H 0 H_{0} tension,

Original

1907

Earlier work this paper cites.

N. Aghanim et al

Original

1907

Earlier work this paper cites.

E. Di Valentino, A. Melchiorri, O. Mena and S. Vagnozzi, Interacting dark energy after the latest Planck, DES, and H 0 H_{0} measurements: an excellent solution to the H 0 H_{0} and cosmic shear tensions,

Original

1908

Earlier work this paper cites.

E. Di Valentino, A. Melchiorri, O. Mena and S. Vagnozzi, Non-minimal dark sector physics and cosmological tensions,

Original

1910

Earlier work this paper cites.

W. Yang, S. Pan, R. C. Nunes and D. F. Mota, Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release,

Original

1910

Earlier work this paper cites.

R. von Marttens, L. Lombriser, M. Kunz, V. Marra, L. Casarini and J. Alcaniz, Dark degeneracy I: Dynamical or interacting dark energy?,

Original

1911

Earlier work this paper cites.

G. Papagiannopoulos, P. Tsiapi, S. Basilakos and A. Paliathanasis, Dynamics and cosmological evolution in Λ \Lambda -varying cosmology,

Original

1911

Earlier work this paper cites.

V. F. Mukhanov, H. A. Feldman and R. H. Brandenberger, Theory of cosmological perturbations,

1992

Earlier work this paper cites.

A. Gelman and D. Rubin, Inference from iterative simulation using multiple sequences,

1992

Earlier work this paper cites.

C. Wetterich, The cosmon model for an asymptotically vanishing time-dependent cosmological constant,

1995

Earlier work this paper cites.

C. P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges,

1995

Earlier work this paper cites.

R. E. Kass and A. E. Raftery, Bayes factors

1995

Earlier work this paper cites.

S. M. Carroll, Quintessence and the rest of the world,

1998

Earlier work this paper cites.

L. Amendola, Coupled quintessence,

2000

Earlier work this paper cites.

A. P. Billyard and A. A. Coley, Interactions in scalar field cosmology,

2000

Earlier work this paper cites.

A. Lewis, A. Challinor and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models,

2000

Earlier work this paper cites.

A. Nunes, J. P. Mimoso and T. C. Charters, Scaling solutions from interacting fluids,

2001

Earlier work this paper cites.

D. Tocchini-Valentini and L. Amendola, Stationary dark energy with a baryon dominated era: Solving the coincidence problem with a linear coupling,

2002

Earlier work this paper cites.

A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach,

2002

Earlier work this paper cites.

L. Amendola and C. Quercellini, Tracking and coupled dark energy as seen by WMAP,

2003

Earlier work this paper cites.

E. Elizalde, S. Nojiri and S. D. Odintsov, Late-time cosmology in (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up,

2004

Earlier work this paper cites.

R. G. Cai and A. Wang, Cosmology with interaction between phantom dark energy and dark matter and the coincidence problem,

2005

Earlier work this paper cites.

S. Nojiri, S. D. Odintsov and S. Tsujikawa, Properties of singularities in (phantom) dark energy universe,

2005

Earlier work this paper cites.

B. Feng, X. L. Wang and X. M. Zhang, Dark energy constraints from the cosmic age and supernova,

2005

Cited alongside, same era.

J. D. Barrow and T. Clifton, Cosmologies with energy exchange,

2006

Cited alongside, same era.

E. J. Copeland, M. Sami and S. Tsujikawa, Dynamics of dark energy,

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,

2006

Cited alongside, same era.

S. Capozziello, S. Nojiri and S. D. Odintsov, Unified phantom cosmology: Inflation, dark energy and dark matter under the same standard,

2006

Cited alongside, same era.

S. del Campo, R. Herrera and D. Pavón, Toward a solution of the coincidence problem,

G. Cognola, R. Myrzakulov, L. Sebastiani, S. Vagnozzi and S. Zerbini, Covariant Hor̆ava-like and mimetic Horndeski gravity: cosmological solutions and perturbations,

Original

2016

Later among the works it cites.

H. Gil-Marín et al

Original

2016

Later among the works it cites.

C. van de Bruck, J. Mifsud and J. Morrice, Testing coupled dark energy models with their cosmological background evolution,

Original

2017

Later among the works it cites.

S. Pan and G. S. Sharov, A model with interaction of dark components and recent observational data,

Original

2017

Later among the works it cites.

G. S. Sharov, S. Bhattacharya, S. Pan, R. C. Nunes and S. Chakraborty, A new interacting two fluid model and its consequences,