Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies

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. 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.

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.

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.

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

Original

1903

Earlier work this paper cites.

P. Agrawal, F. Y. Cyr-Racine, D. Pinner and L. Randall, Rock ’n’ Roll solutions to the Hubble tension

Original

1904

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.

E. Ó. Colgáin and H. Yavartanoo, Testing the Swampland: H 0 H_{0} tension

Original

1905

Earlier work this paper cites.

T. Hamana et al

Original

1906

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.

P. Agrawal, G. Obied and C. Vafa, H 0 H_{0} tension, Swampland conjectures and the epoch of fading dark matter

Original

1906

Earlier work this paper cites.

N. Aghanim et al

Original

1907

Earlier work this paper cites.

L. Verde, T. Treu and A. Riess, Tensions between the Early and the Late Universe

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, New physics in light of the H 0 H_{0} tension: An alternative view

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. Handley, Curvature tension: evidence for a closed universe

Original

1908

Earlier work this paper cites.

L. Knox and M. Millea, Hubble constant hunter’s guide

Original

1908

Earlier work this paper cites.

T. Tröster et al

Original

1909

Earlier work this paper cites.

N. Arendse, R. J. Wojtak, A. Agnello, G. C. F. Chen, C. D. Fassnacht, D. Sluse, S. Hilbert, M. Millon, V. Bonvin and K. C. Wong, et al

Original

1909

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.

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 and J. Silk, Planck evidence for a closed Universe and a possible crisis for cosmology

Original

1911

Earlier work this paper cites.

L. A. Anchordoqui, I. Antoniadis, D. Lüst, J. F. Soriano and T. R. Taylor, H 0 H_{0} tension and the String Swampland

Original

1912

Earlier work this paper cites.

S. Weinberg, Goldstone bosons as fractional cosmic neutrinos

Original

1971

Earlier work this paper cites.

G. Steigman, D. N. Schramm and J. E. Gunn, Cosmological limits to the number of massive leptons

1977

Earlier work this paper cites.

C. Wetterich, Cosmology and the fate of dilatation symmetry

Original

1988

Earlier work this paper cites.

P. J. E. Peebles and B. Ratra, Cosmology with a time variable cosmological constant

1988

Earlier work this paper cites.

B. Ratra and P. J. E. Peebles, Cosmological consequences of a rolling homogeneous scalar field

1988

Earlier work this paper cites.

M. S. Morris, K. S. Thorne and U. Yurtsever, Wormholes, time machines, and the weak energy condition

1988

Earlier work this paper cites.

E. W. Kolb and M. S. Turner, The Early Universe

1990

Earlier work this paper cites.

A. Gelman and D. B. 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.

W. Hu and N. Sugiyama, Small scale cosmological perturbations: An Analytic approach

1996

Earlier work this paper cites.

R. R. Caldwell, R. Dave and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state

1998

Earlier work this paper cites.

L. Amendola, Coupled quintessence

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. G. Riess, The Expansion of the Universe is Faster than Expected,

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.

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.

H. Amirhashchi and A. K. Yadav, Interacting Dark Sectors in Anisotropic Universe: Observational Constraints and H 0 H_{0} Tension

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, Non-linear 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, Shedding light on dark matter-dark energy interactions

Original

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.

R. R. Caldwell, A phantom menace?

2002

Earlier work this paper cites.

G. Benevento, W. Hu and M. Raveri, Can late dark energy transitions raise the Hubble constant?

Original

2002

Earlier work this paper cites.

D. Comelli, M. Pietroni and A. Riotto, Dark energy and dark matter

2003

Earlier work this paper cites.

S. M. Carroll, M. Hoffman and M. Trodden, Can the dark energy equation-of-state parameter w w be less than − 1 -1 ?

2003

Earlier work this paper cites.

R. R. Caldwell, M. Kamionkowski and N. N. Weinberg, Phantom energy and cosmic doomsday

2003

Earlier work this paper cites.

J. C. Hill, E. McDonough, M. W. Toomey and S. Alexander, Early dark energy does not restore cosmological concordance

Original

2003

Earlier work this paper cites.

W. Yang, E. Di Valentino, O. Mena and S. Pan, Dynamical dark sectors and neutrino masses and abundances

Original

2003

Earlier work this paper cites.

E. Di Valentino, A. Melchiorri and J. Silk, Investigating Cosmic Discordance

Original

2003

Earlier work this paper cites.

U. Franca and R. Rosenfeld, Age constraints and fine tuning in VAMP models

2004

Earlier work this paper cites.

A. Gómez-Valent, V. Pettorino and L. Amendola, Update on coupled dark energy and the H 0 H_{0} tension

Original

2004

Earlier work this paper cites.

S. M. Carroll, A. De Felice and M. Trodden, Can we be tricked into thinking that w w is less than − 1 -1 ?

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.

K. Akita and M. Yamaguchi, A precision calculation of relic neutrino decoupling

Original

2005

Cited alongside, same era.

A. Gogoi, R. K. Sharma, P. Chanda and S. Das, Early mass-varying neutrino dark energy: Nugget formation and Hubble anomaly

Original

2005

Cited alongside, same era.

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

2005

Cited alongside, same era.

E. Di Valentino, S. Gariazzo, E. Giusarma and O. Mena, Robustness of cosmological axion mass limits

Original

2015

Later among the works it cites.

E. Di Valentino, E. Giusarma, M. Lattanzi, O. Mena, A. Melchiorri and J. Silk, Cosmological Axion and neutrino mass constraints from Planck 2015 temperature and polarization data

Original

2015

Later among the works it cites.

E. Aver, K. A. Olive and E. D. Skillman, The effects of He I λ \lambda 10830 on helium abundance determinations

Original

2015

Later among the works it cites.

J. Väliviita and E. Palmgren, Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data

Original

2015

Later among the works it cites.

S. Pan, S. Bhattacharya and S. Chakraborty, An analytic model for interacting dark energy and its observational constraints