Built on

J. J. Heckman, C. Lawrie, L. Lin, J. Sakstein, and G. Zoccarato, Pixelated Dark Energy
Original
1901
Earlier work this paper cites.
C. Desgrange, A. Heinesen, and T. Buchert, Dynamical spatial curvature as a fit to type Ia supernovae
Original
1902
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
Original
1902
Earlier work this paper cites.
M. Raveri, Reconstructing Gravity on Cosmological Scales
Original
1902
Earlier work this paper cites.
F. Gerardi, M. Martinelli, and A. Silvestri, Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
Original
1902
Earlier work this paper cites.
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.
R. D’Agostino, Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
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.
A. Diaz Rivero, V. Miranda, and C. Dvorkin, Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
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.
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.
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.
X. Li, A. Shafieloo, V. Sahni, and A. A. Starobinsky, Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
Original
1904
Earlier work this paper cites.
W. Yang, S. Pan, A. Paliathanasis, S. Ghosh, and Y. Wu, Observational constraints of a new unified dark fluid and the H 0 H_{0} tension
Original
1904
Earlier work this paper cites.
C. Li, X. Ren, M. Khurshudyan, and Y.-F. Cai, Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
Original
1904
Earlier work this paper cites.
F. K. Anagnostopoulos, D. Benisty, S. Basilakos, and E. I. Guendelman, Dark energy and dark matter unification from dynamical space time: observational constraints and cosmological implications
Original
1904
Earlier work this paper cites.
R. E. Keeley, S. Joudaki, M. Kaplinghat, and D. Kirkby, Implications of a transition in the dark energy equation of state for the H 0 H_{0} and σ 8 \sigma_{8} tensions
Original
1905
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension
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.
S. D. Odintsov and V. K. Oikonomou, Unification of Inflation with Dark Energy in f ⁡ ( R ) f(R) Gravity and Axion Dark Matter
Original
1905
Earlier work this paper cites.
M. Martinelli and I. Tutusaus, CMB tensions with low-redshift H 0 H_{0} and S 8 S_{8} measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
Original
1906
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky, and C. Umilta, Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, Late time transitions in the quintessence field and the H 0 H_{0} tension
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.
M. Archidiacono, D. C. Hooper, R. Murgia, S. Bohr, J. Lesgourgues, and M. Viel, Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman- α \alpha
Original
1907
Earlier work this paper cites.
L. Kazantzidis and L. Perivolaropoulos, Is gravity getting weaker at low z? Observational evidence and theoretical implications
Original
1907
Earlier work this paper cites.
S. Nesseris, D. Sapone, and S. Sypsas, Evaporating primordial black holes as varying dark energy
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.
S. Pan, W. Yang, E. Di Valentino, A. Shafieloo, and S. Chakraborty, Reconciling H 0 H_{0} tension in a six parameter space?
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, Revisiting a negative cosmological constant from low-redshift data
Original
1907
Earlier work this paper cites.
Y.-F. Cai, M. Khurshudyan, and E. N. Saridakis, Model-independent reconstruction of f ⁡ ( T ) f(T) gravity from Gaussian Processes
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. Nakamura, R. Kase, and S. Tsujikawa, Coupled vector dark energy
Original
1907
Earlier work this paper cites.
Y.-L. Kim, Y. Kang, and Y.-W. Lee, Environmental Dependence of Type Ia Supernova Luminosities from the YONSEI Supernova Catalog
Original
1908
Earlier work this paper cites.
L. Xiao, L. Zhang, R. An, C. Feng, and B. Wang, Fractional Dark Matter decay: cosmological imprints and observational constraints
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
Original
1908
Earlier work this paper cites.
S. Ghosh, R. Khatri, and T. S. Roy, Dark Neutrino interactions phase out the Hubble tension
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
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.
M. Benetti, W. Miranda, H. A. Borges, C. Pigozzo, S. Carneiro, and J. S. Alcaniz, Looking for interactions in the cosmological dark sector
Original
1908
Earlier work this paper cites.
W. Handley, Curvature tension: evidence for a closed universe
Original
1908
Earlier work this paper cites.
J. Solà Peracaula, A. Gomez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, Brans–Dicke Gravity with a Cosmological Constant Smoothes Out Λ \Lambda CDM Tensions
Original
1909
Earlier work this paper cites.
M. Escudero and S. J. Witte, A CMB Search for the Neutrino Mass Mechanism and its Relation to the H 0 H_{0} Tension
Original
1909
Earlier work this paper cites.
S.-F. Yan, P. Zhang, J.-W. Chen, X.-Z. Zhang, Y.-F. Cai, and E. N. Saridakis, Interpreting cosmological tensions from the effective field theory of torsional gravity
Original
1909
Earlier work this paper cites.
R. Kase and S. Tsujikawa, Scalar-Field Dark Energy Nonminimally and Kinetically Coupled to Dark Matter
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, O. Mena, and S. Vagnozzi, Nonminimal dark sector physics and cosmological tensions
Original
1910
Earlier work this paper cites.
M. Hogas, F. Torsello, and E. Mörtsell, On the Stability of Bimetric Structure Formation
Original
1910
Earlier work this paper cites.
G. Efstathiou and S. Gratton, A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps
Original
1910
Earlier work this paper cites.
M. J. Childress, C. Wolf, and H. J. Zahid, Ages of Type Ia Supernovae Over Cosmic Time
Original
1911
Earlier work this paper cites.
S. Vagnozzi, L. Visinelli, O. Mena, and D. F. Mota, Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early dark energy from massive neutrinos – a natural resolution of the Hubble tension
Original
1911
Earlier work this paper cites.
M. Aljaf, D. Gregoris, and M. Khurshudyan, Phase space analysis and singularity classification for linearly interacting dark energy models
Original
1911
Earlier work this paper cites.
G. Cheng, Y. Ma, F. Wu, J. Zhang, and X. Chen, Testing interacting dark matter and dark energy model with cosmological data
Original
1911
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.
Y. Kang, Y.-W. Lee, Y.-L. Kim, C. Chung, and C. H. Ree, Early-type Host Galaxies of Type Ia Supernovae. II. Evidence for Luminosity Evolution in Supernova Cosmology
Original
1912
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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
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N. Frusciante, S. Peirone, L. Atayde, and A. De Felice, Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
Original
1912
Earlier work this paper cites.
O. Akarsu, J. D. Barrow, L. A. Escamilla, and J. A. Vazquez, Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant
Original
1912
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C. Brans and R. H. Dicke, Mach’s principle and a relativistic theory of gravitation
1961
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C. Wetterich, Cosmology and the Fate of Dilatation Symmetry
Original
1988
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B. Ratra and P. J. E. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field
1988
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A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences
1992
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R. R. Caldwell, R. Dave, and P. J. Steinhardt, Cosmological imprint of an energy component with general equation of state
1998
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Supernova Search Team
1998
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R. Tripp, A Two-parameter luminosity correction for type Ia supernovae
1998
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S. M. Carroll, Quintessence and the rest of the world
1998
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P. J. E. Peebles and A. Vilenkin, Quintessential inflation
1999
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Supernova Cosmology Project
1999
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G. Efstathiou, Constraining the equation of state of the universe from distant type Ia supernovae and cosmic microwave background anisotropies
1999
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A. Lewis, A. Challinor, and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models
2000
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L. Amendola, Coupled quintessence
2000
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A. Yu. Kamenshchik, U. Moschella, and V. Pasquier, An Alternative to quintessence
2001
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S. Nadathur, W. J. Percival, F. Beutler, and H. Winther, Testing low-redshift cosmic acceleration with large-scale structure
Original
2001
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M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter
2001
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G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?
Original
2001
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S. Pan, G. S. Sharov, and W. Yang, Field theoretic interpretations of interacting dark energy scenarios and recent observations
Original
2001
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W. Yang, E. Di Valentino, O. Mena, S. Pan, and R. C. Nunes, All-inclusive interacting dark sector cosmologies
Original
2001
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M. C. Bento, O. Bertolami, and A. A. Sen, Generalized Chaplygin gas, accelerated expansion and dark energy matter unification
2002
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K. Freese and M. Lewis, Cardassian expansion: A Model in which the universe is flat, matter dominated, and accelerating
2002
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B. M. Rose, D. Rubin, A. Cikota, S. Deustua, S. Dixon, A. Fruchter, D. O. Jones, A. G. Riess, and D. M. Scolnic, No Evidence for Type Ia Supernova Luminosity Evolution: Evidence for Dark Energy is Robust
Original
2002
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H. B. Sandvik, J. D. Barrow, and J. Magueijo, A simple cosmology with a varying fine structure constant
2002
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T. Damour, F. Piazza, and G. Veneziano, Runaway dilaton and equivalence principle violations
2002
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R. Jimenez and A. Loeb, Constraining cosmological parameters based on relative galaxy ages
2002
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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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C. Krishnan, E. O. Colgáin, Ruchika, A. A. Sen, M. M. Sheikh-Jabbari, and T. Yang, Is there an early Universe solution to Hubble tension?
Original
2002
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Similar

R. D’Agostino and R. C. Nunes, Measurements of H 0 H_{0} in modified gravity theories: The role of lensed quasars in the late-time Universe
Original
2002
Cited alongside, same era.
G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?
Original
2002
Cited alongside, same era.
M. Lucca and D. C. Hooper, Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
Original
2002
Cited alongside, same era.
N. B. Hogg, M. Bruni, R. Crittenden, M. Martinelli, and S. Peirone, Latest evidence for a late time vacuum – geodesic CDM interaction
Original
2002
Cited alongside, same era.
G. Efstathiou and S. Gratton, The evidence for a spatially flat Universe

Then

E. Aubourg et al., Cosmological implications of baryon acoustic oscillation measurements
Original
2015
Later among the works it cites.
A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden, and M. Manera, The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15
Original
2015
Later among the works it cites.
M. Moresco, Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ \sim 2
Original
2015
Later among the works it cites.
R. C. Nunes and S. Pan, Cosmological consequences of an adiabatic matter creation process
Original
2016
Later among the works it cites.
H. Campbell, M. Fraser, and G. Gilmore, How SN Ia host-galaxy properties affect cosmological parameters

Beyond the bibliography

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

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Reading the bibliography…

2020

Soundness of Dark Energy properties

Di Valentino, Eleonora, Gariazzo, Stefano, Mena, Olga et al.

Understand

Type Ia Supernovae (SNeIa) used as standardizable candles have been instrumental in the discovery of cosmic acceleration, usually attributed to some form of dark energy (DE).

Recent studies have raised the issue of whether intrinsic SNeIa luminosities might evolve with redshift.
While the evidence for cosmic acceleration is robust to this possible systematic, the question remains of how much the latter can affect the inferred properties of the DE component responsible for cosmic acceleration.
This is the question we address in this work.

Built on

J. J. Heckman, C. Lawrie, L. Lin, J. Sakstein, and G. Zoccarato, Pixelated Dark Energy
Original
1901
Earlier work this paper cites.
C. Desgrange, A. Heinesen, and T. Buchert, Dynamical spatial curvature as a fit to type Ia supernovae
Original
1902
Earlier work this paper cites.
C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions
Original
1902
Earlier work this paper cites.
M. Raveri, Reconstructing Gravity on Cosmological Scales
Original
1902
Earlier work this paper cites.
F. Gerardi, M. Martinelli, and A. Silvestri, Reconstruction of the Dark Energy equation of state from latest data: the impact of theoretical priors
Original
1902
Earlier work this paper cites.
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.
R. D’Agostino, Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
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.
A. Diaz Rivero, V. Miranda, and C. Dvorkin, Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
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.
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.
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.
X. Li, A. Shafieloo, V. Sahni, and A. A. Starobinsky, Revisiting Metastable Dark Energy and Tensions in the Estimation of Cosmological Parameters
Original
1904
Earlier work this paper cites.
W. Yang, S. Pan, A. Paliathanasis, S. Ghosh, and Y. Wu, Observational constraints of a new unified dark fluid and the H 0 H_{0} tension
Original
1904
Earlier work this paper cites.
C. Li, X. Ren, M. Khurshudyan, and Y.-F. Cai, Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
Original
1904
Earlier work this paper cites.
F. K. Anagnostopoulos, D. Benisty, S. Basilakos, and E. I. Guendelman, Dark energy and dark matter unification from dynamical space time: observational constraints and cosmological implications
Original
1904
Earlier work this paper cites.
R. E. Keeley, S. Joudaki, M. Kaplinghat, and D. Kirkby, Implications of a transition in the dark energy equation of state for the H 0 H_{0} and σ 8 \sigma_{8} tensions
Original
1905
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension
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.
S. D. Odintsov and V. K. Oikonomou, Unification of Inflation with Dark Energy in f ⁡ ( R ) f(R) Gravity and Axion Dark Matter
Original
1905
Earlier work this paper cites.
M. Martinelli and I. Tutusaus, CMB tensions with low-redshift H 0 H_{0} and S 8 S_{8} measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
Original
1906
Earlier work this paper cites.
M. Rossi, M. Ballardini, M. Braglia, F. Finelli, D. Paoletti, A. A. Starobinsky, and C. Umilta, Cosmological constraints on post-Newtonian parameters in effectively massless scalar-tensor theories of gravity
Original
1906
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson, Late time transitions in the quintessence field and the H 0 H_{0} tension
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.
M. Archidiacono, D. C. Hooper, R. Murgia, S. Bohr, J. Lesgourgues, and M. Viel, Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman- α \alpha
Original
1907
Earlier work this paper cites.
L. Kazantzidis and L. Perivolaropoulos, Is gravity getting weaker at low z? Observational evidence and theoretical implications
Original
1907
Earlier work this paper cites.
S. Nesseris, D. Sapone, and S. Sypsas, Evaporating primordial black holes as varying dark energy
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.
S. Pan, W. Yang, E. Di Valentino, A. Shafieloo, and S. Chakraborty, Reconciling H 0 H_{0} tension in a six parameter space?
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson, Revisiting a negative cosmological constant from low-redshift data
Original
1907
Earlier work this paper cites.
Y.-F. Cai, M. Khurshudyan, and E. N. Saridakis, Model-independent reconstruction of f ⁡ ( T ) f(T) gravity from Gaussian Processes
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. Nakamura, R. Kase, and S. Tsujikawa, Coupled vector dark energy
Original
1907
Earlier work this paper cites.
Y.-L. Kim, Y. Kang, and Y.-W. Lee, Environmental Dependence of Type Ia Supernova Luminosities from the YONSEI Supernova Catalog
Original
1908
Earlier work this paper cites.
L. Xiao, L. Zhang, R. An, C. Feng, and B. Wang, Fractional Dark Matter decay: cosmological imprints and observational constraints
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin, Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
Original
1908
Earlier work this paper cites.
S. Ghosh, R. Khatri, and T. S. Roy, Dark Neutrino interactions phase out the Hubble tension
Original
1908
Earlier work this paper cites.
L. Knox and M. Millea, Hubble constant hunter’s guide
Original
1908
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.
M. Benetti, W. Miranda, H. A. Borges, C. Pigozzo, S. Carneiro, and J. S. Alcaniz, Looking for interactions in the cosmological dark sector
Original
1908
Earlier work this paper cites.
W. Handley, Curvature tension: evidence for a closed universe
Original
1908
Earlier work this paper cites.
J. Solà Peracaula, A. Gomez-Valent, J. de Cruz Pérez, and C. Moreno-Pulido, Brans–Dicke Gravity with a Cosmological Constant Smoothes Out Λ \Lambda CDM Tensions
Original
1909
Earlier work this paper cites.
M. Escudero and S. J. Witte, A CMB Search for the Neutrino Mass Mechanism and its Relation to the H 0 H_{0} Tension
Original
1909
Earlier work this paper cites.
S.-F. Yan, P. Zhang, J.-W. Chen, X.-Z. Zhang, Y.-F. Cai, and E. N. Saridakis, Interpreting cosmological tensions from the effective field theory of torsional gravity
Original
1909
Earlier work this paper cites.
R. Kase and S. Tsujikawa, Scalar-Field Dark Energy Nonminimally and Kinetically Coupled to Dark Matter
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, O. Mena, and S. Vagnozzi, Nonminimal dark sector physics and cosmological tensions
Original
1910
Earlier work this paper cites.
M. Hogas, F. Torsello, and E. Mörtsell, On the Stability of Bimetric Structure Formation
Original
1910
Earlier work this paper cites.
G. Efstathiou and S. Gratton, A Detailed Description of the CamSpec Likelihood Pipeline and a Reanalysis of the Planck High Frequency Maps
Original
1910
Earlier work this paper cites.
M. J. Childress, C. Wolf, and H. J. Zahid, Ages of Type Ia Supernovae Over Cosmic Time
Original
1911
Earlier work this paper cites.
S. Vagnozzi, L. Visinelli, O. Mena, and D. F. Mota, Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden, Early dark energy from massive neutrinos – a natural resolution of the Hubble tension
Original
1911
Earlier work this paper cites.
M. Aljaf, D. Gregoris, and M. Khurshudyan, Phase space analysis and singularity classification for linearly interacting dark energy models
Original
1911
Earlier work this paper cites.
G. Cheng, Y. Ma, F. Wu, J. Zhang, and X. Chen, Testing interacting dark matter and dark energy model with cosmological data
Original
1911
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E. Di Valentino, A. Melchiorri, and J. Silk, Planck evidence for a closed Universe and a possible crisis for cosmology
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