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We consider a phenomenological model of dark matter with an equation-of-state $w$ that is negative and changing at late times.
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2009
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2012
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2012
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2012
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L. Xu and Y. Chang, Equation of state of dark matter after Planck data, Phys. Rev. D 88
2013
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A. Lewis, Efficient sampling of fast and slow cosmological parameters, Phys. Rev. D87
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2014
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2014
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2015
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A. Kovács, The part and the whole: voids, supervoids, and their ISW imprint, MNRAS 475
2018
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2019
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P. Shah, P. Lemos, and O. Lahav, A buyer’s guide to the Hubble constant, A&A Rev. 29
2021
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2021
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2022
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L. Perivolaropoulos and F. Skara, Challenges for Λ \Lambda CDM: An update, New A Rev. 95
2022
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