Thermal Friction as a Solution to the Hubble and Large-Scale Structure Tensions

C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré, Neutrino puzzle: Anomalies, interactions, and cosmological tensions, Phys. Rev. D 101

Original

1902

Earlier work this paper cites.

P. W. Graham, D. E. Kaplan, and S. Rajendran, Relaxation of the Cosmological Constant, Phys. Rev. D 100

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, Astrophys. J. 876

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, (2019), arXiv:1904.01016 [astro-ph.CO]

Original

1904

Earlier work this paper cites.

S. Alexander and E. McDonough, Axion-Dilaton Destabilization and the Hubble Tension, Phys. Lett. B 797

Original

1904

Earlier work this paper cites.

M. Park, C. D. Kreisch, J. Dunkley, B. Hadzhiyska, and F.-Y. Cyr-Racine, Λ \Lambda CDM or self-interacting neutrinos: How CMB data can tell the two models apart, Phys. Rev. D 100

Original

1904

Earlier work this paper cites.

M.-X. Lin, G. Benevento, W. Hu, and M. Raveri, Acoustic Dark Energy: Potential Conversion of the Hubble Tension, Phys. Rev. D 100

Original

1905

Earlier work this paper cites.

L. Verde, T. Treu, and A. G. Riess, Tensions between the Early and the Late Universe, Nature Astron. 3

Original

1907

Earlier work this paper cites.

W. L. Freedman et al. , The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch 10.3847/1538-4357/ab2f73 (2019), arXiv:1907.05922 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

N. Aghanim et al. (Planck), Planck 2018 results. V. CMB power spectra and likelihoods, Astron. Astrophys. 641

Original

1907

Earlier work this paper cites.

C. D. Huang, A. G. Riess, W. Yuan, L. M. Macri, N. L. Zakamska, S. Casertano, P. A. Whitelock, S. L. Hoffmann, A. V. Filippenko, and D. Scolnic, Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant 10.3847/1538-4357/ab5dbd (2019), arXiv:1908.10883 [astro-ph.CO]

Original

1908

Earlier work this paper cites.

M. J. Reid, D. W. Pesce, and A. G. Riess, An Improved Distance to NGC 4258 and its Implications for the Hubble Constant, Astrophys. J. Lett. 886

Original

1908

Earlier work this paper cites.

W. Yuan, A. G. Riess, L. M. Macri, S. Casertano, and D. Scolnic, Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant, Astrophys. J. 886

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, Phys. Rev. D 101

Original

1908

Earlier work this paper cites.

L. Knox and M. Millea, Hubble constant hunter’s guide, Phys. Rev. D 101

Original

1908

Earlier work this paper cites.

M. M. Ivanov, M. Simonović, and M. Zaldarriaga, Cosmological Parameters from the BOSS Galaxy Power Spectrum, JCAP 05

Original

1909

Earlier work this paper cites.

F. Niedermann and M. S. Sloth, New early dark energy, Phys. Rev. D 103

Original

1910

Earlier work this paper cites.

K. V. Berghaus, P. W. Graham, and D. E. Kaplan, Minimal Warm Inflation, JCAP 03

Original

1910

Earlier work this paper cites.

A. Lewis, GetDist: a Python package for analysing Monte Carlo samples, (2019), arXiv:1910.13970 [astro-ph.IM]

Original

1910

Earlier work this paper cites.

J. Sakstein and M. Trodden, Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension, Phys. Rev. Lett. 124

Original

1911

Earlier work this paper cites.

K. V. Berghaus and T. Karwal, Thermal Friction as a Solution to the Hubble Tension, Phys. Rev. D 101

Original

1911

Earlier work this paper cites.

A. Gelman and D. B. Rubin, Inference from Iterative Simulation Using Multiple Sequences, Statist. Sci. 7

1992

Earlier work this paper cites.

A. Berera, Warm inflation, Phys. Rev. Lett. 75

1995

Earlier work this paper cites.

A. Berera and L.-Z. Fang, Thermally induced density perturbations in the inflation era, Phys. Rev. Lett. 74

1995

Earlier work this paper cites.

C.-P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges, Astrophys. J. 455

1995

Earlier work this paper cites.

A. Berera, M. Gleiser, and R. O. Ramos, A First principles warm inflation model that solves the cosmological horizon / flatness problems, Phys. Rev. Lett. 83

1999

Earlier work this paper cites.

A. Berera, Warm inflation at arbitrary adiabaticity: A Model, an existence proof for inflationary dynamics in quantum field theory, Nucl. Phys. B 585

2000

Earlier work this paper cites.

D. W. Pesce et al. , The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints, Astrophys. J. Lett. 891

Original

2001

Earlier work this paper cites.

G. Ye and Y.-S. Piao, Is the Hubble tension a hint of AdS phase around recombination?, Phys. Rev. D 101

Original

2001

Earlier work this paper cites.

W. L. Freedman, B. F. Madore, T. Hoyt, I. S. Jang, R. Beaton, M. G. Lee, A. Monson, J. Neeley, and J. Rich, Calibration of the Tip of the Red Giant Branch (TRGB) 10.3847/1538-4357/ab7339 (2020), arXiv:2002.01550 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

G. Benevento, W. Hu, and M. Raveri, Can Late Dark Energy Transitions Raise the Hubble constant?, Phys. Rev. D 101

Original

2002

Earlier work this paper cites.

J. C. Hill, E. McDonough, M. W. Toomey, and S. Alexander, Early dark energy does not restore cosmological concordance, Phys. Rev. D 102

Original

2003

Earlier work this paper cites.

N. Blinov and G. Marques-Tavares, Interacting radiation after Planck and its implications for the Hubble Tension, JCAP 09

Original

2003

Earlier work this paper cites.

A. Chudaykin, D. Gorbunov, and N. Nedelko, Combined analysis of Planck and SPTPol data favors the early dark energy models, JCAP 08

Original

2004

Cited alongside, same era.

M. Braglia, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, and K. Koyama, Unified framework for early dark energy from α \alpha -attractors, Phys. Rev. D 102

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, Astrophys. J. 915

Original

2005

Cited alongside, same era.

J. Torrado and A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, JCAP 05

Original

2005

Cited alongside, same era.

M. M. Ivanov, E. McDonough, J. C. Hill, M. Simonović, M. W. Toomey, S. Alexander, and M. Zaldarriaga, Constraining Early Dark Energy with Large-Scale Structure, Phys. Rev. D 102

W. L. Freedman, Cosmology at a Crossroads, Nature Astron. 1

Original

2017

Later among the works it cites.

S. Alam et al. (BOSS), The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Mon. Not. Roy. Astron. Soc. 470

Original

2017

Later among the works it cites.

E. Krause et al. (DES), Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses, (2017), arXiv:1706.09359 [astro-ph.CO]

Original

2017

Later among the works it cites.

G. E. Addison, D. J. Watts, C. L. Bennett, M. Halpern, G. Hinshaw, and J. L. Weiland, Elucidating Λ \Lambda CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy, Astrophys. J. 853

Original

2018

Later among the works it cites.