Built on

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.
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.
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.
J. D. Barrow and G. Kittou, Non-linear interactions in cosmologies with energy exchange,
Original
1907
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.
S. Vagnozzi, Cosmological searches for the neutrino mass scale and mass ordering,
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.
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.
E. Di Valentino, A. Melchiorri, O. Mena and S. Vagnozzi, Nonminimal dark sector physics and cosmological tensions,
Original
1910
Earlier work this paper cites.
M. Asgari et al
Original
1910
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.
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.
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.
W. Yang, E. Di Valentino, S. Pan, S. Basilakos and A. Paliathanasis, Metastable dark energy models in light of Planck 2018: Alleviating the H 0 H_{0} tension,
Original
2001
Earlier work this paper cites.
S. Pan, G. S. Sharov and W. Yang, Field theoretic interpretations of interacting dark energy scenarios and recent observations,
Original
2001
Earlier work this paper cites.
S. Pan, J. de Haro, W. Yang and J. Amorós, Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds,
Original
2001
Earlier work this paper cites.
W. Yang, E. Di Valentino, O. Mena, S. Pan and R. C. Nunes, All-inclusive interacting dark sector cosmologies,
Original
2001
Earlier work this paper cites.
S. Pan, W. Yang and A. Paliathanasis, Nonlinear interacting cosmological models after Planck 2018 legacy release and the H 0 H_{0} tension,
Original
2002
Earlier work this paper cites.
M. Lucca and D. C. Hooper, Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions,
Original
2002
Earlier work this paper cites.

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A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach,
2002
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2003
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S. Hagstotz, P. F. de Salas, S. Gariazzo, M. Gerbino, M. Lattanzi, S. Vagnozzi, K. Freese and S. Pastor, Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches,
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Then

P. F. de Salas and S. Pastor, Relic neutrino decoupling with flavour oscillations revisited,
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2016
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S. Pan and G. S. Sharov, A model with interaction of dark components and recent observational data,
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2017
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C. van de Bruck, J. Mifsud and J. Morrice, Testing coupled dark energy models with their cosmological background evolution,
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2017
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A. Mukherjee and N. Banerjee, In search of the dark matter dark energy interaction: a kinematic approach,
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2020

Dynamical Dark sectors and Neutrino masses and abundances

Yang, Weiqiang, Di Valentino, Eleonora, Mena, Olga et al.

Understand

We investigate generalized interacting dark matter-dark energy scenarios with a time-dependent coupling parameter, allowing also for freedom in the neutrino sector.

The models are tested in the phantom and quintessence regimes, characterized by an equation of state $w_x<-1$ and $w_x>-1$, respectively.
Our analyses show that for some of the scenarios the existing tensions on the Hubble constant $H_0$ and on the clustering parameter $S_8$ can be significantly alleviated.
The relief is either due to \textit{(a)} a dark energy component which lies within the phantom region; or \textit{(b)} the presence of a dynamical coupling in quintessence scenarios.

Built on

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.
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.
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.
J. D. Barrow and G. Kittou, Non-linear interactions in cosmologies with energy exchange,
Original
1907
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.
S. Vagnozzi, Cosmological searches for the neutrino mass scale and mass ordering,
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.
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.
E. Di Valentino, A. Melchiorri, O. Mena and S. Vagnozzi, Nonminimal dark sector physics and cosmological tensions,
Original
1910
Earlier work this paper cites.
M. Asgari et al
Original
1910
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.
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.
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.
W. Yang, E. Di Valentino, S. Pan, S. Basilakos and A. Paliathanasis, Metastable dark energy models in light of Planck 2018: Alleviating the H 0 H_{0} tension,
Original
2001
Earlier work this paper cites.
S. Pan, G. S. Sharov and W. Yang, Field theoretic interpretations of interacting dark energy scenarios and recent observations,
Original
2001
Earlier work this paper cites.
S. Pan, J. de Haro, W. Yang and J. Amorós, Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds,
Original
2001
Earlier work this paper cites.
W. Yang, E. Di Valentino, O. Mena, S. Pan and R. C. Nunes, All-inclusive interacting dark sector cosmologies,
Original
2001
Earlier work this paper cites.
S. Pan, W. Yang and A. Paliathanasis, Nonlinear interacting cosmological models after Planck 2018 legacy release and the H 0 H_{0} tension,
Original
2002
Earlier work this paper cites.
M. Lucca and D. C. Hooper, Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions,
Original
2002
Earlier work this paper cites.

Similar

A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach,
2002
Cited alongside, same era.
L. Amendola and C. Quercellini, Tracking and coupled dark energy as seen by WMAP,
2003
Cited alongside, same era.
S. Hagstotz, P. F. de Salas, S. Gariazzo, M. Gerbino, M. Lattanzi, S. Vagnozzi, K. Freese and S. Pastor, Bounds on light sterile neutrino mass and mixing from cosmology and laboratory searches,
Original
2003
Cited alongside, same era.
D. Pavón and W. Zimdahl, Holographic dark energy and cosmic coincidence,
2005
Cited alongside, same era.
G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P. D. Serpico, Relic neutrino decoupling including flavor oscillations,
2005
Cited alongside, same era.

Then

P. F. de Salas and S. Pastor, Relic neutrino decoupling with flavour oscillations revisited,
Original
2016
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.
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.
A. Mukherjee and N. Banerjee, In search of the dark matter dark energy interaction: a kinematic approach,
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,

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

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

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,

2007

Cited alongside, same era.

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