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The discrepancy in measurements of the Hubble constant indicates new physics in dark energy, dark matter, or both.
1903
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1903
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E. Ó Colgáin and H. Yavartanoo, Testing the Swampland: H 0 H_{0} tension
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L. Verde, T. Treu and A. G. Riess, Tensions between the early and the late universe
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S. Vagnozzi, New physics in light of the H 0 H_{0} tension: an alternative view
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1912
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G. Benevento, W. Hu and M. Raveri, Can late dark energy transitions raise the Hubble constant?
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D. Cremades, L. E. Ibañez and F. Marchesano, Yukawa couplings in intersecting D-brane models
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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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R. Blumenhagen, M. Cvetič, P. Langacker and G. Shiu, Toward realistic intersecting D-brane models
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M. Laine and Y. Schroder, Quark mass thresholds in QCD thermodynamics
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R. Blumenhagen, B. Kors, D. Lüst and S. Stieberger, Four-dimensional string compactifications with D-branes, orientifolds and fluxes
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2014
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2014
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2015
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2015
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2008
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2009
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2009
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2009
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2010
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2011
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2011
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2015
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2016
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2016
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2017
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2017
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S. Kumar and R. C. Nunes, Echo of interactions in the dark sector
2017
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E. Di Valentino, A. Melchiorri and O. Mena, Can interacting dark energy solve the H 0 H_{0} tension?
2017
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2018
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2018
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2018
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D. Baumann, Primordial cosmology
2018
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M. Tanabashi et al
2018
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2018
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2018
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2018
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M. Raveri, W. Hu and S. Sethi, Swampland conjectures and late-time cosmology
2019
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