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The value of Hubble constant inferred from Planck measurements of anisotropies in the cosmic microwave background is at $4.4\sigma$ tension with direct astronomical measurements at low redshifts.
1903
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1903
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1904
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1905
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1906
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1906
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L. Verde, T. Treu and A. G. Riess, Tensions between the early and the late universe
1907
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V. V. Flambaum and I. B. Samsonov, Ultralight dark photon as a model for early universe dark matter
1908
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A. Desai, K. R. Dienes and B. Thomas, Constraining dark-matter ensembles with supernova data
1909
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S. Weinberg, Goldstone bosons as fractional cosmic neutrinos
1971
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G. Steigman, D.N. Schramm and J.E. Gunn, Cosmological limits to the number of massive leptons
1977
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E. W. Kolb and M. S. Turner, The Early Universe
1990
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G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P.D. Serpico, Relic neutrino decoupling including flavor oscillations
2005
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2011
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L. A. Anchordoqui and H. Goldberg, Neutrino cosmology after WMAP 7-year data and LHC first Z’ bounds
2012
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2012
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2012
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2012
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2017
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2018
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2018
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2018
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2018
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2013
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T. D. Jacques, L. M. Krauss and C. Lunardini, Additional light sterile neutrinos and cosmology
2013
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C. Brust, D. E. Kaplan and M. T. Walters, New light species and the CMB
2013
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2015
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2015
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2016
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2016
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2016
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2018
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F. D’Eramo, R. Z. Ferreira, A. Notari and J. L. Bernal, Hot axions and the H 0 H_{0} tension
2018
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M. Tanabashi et al
2018
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2019
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2019
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2019
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2019
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