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We show that the latest empirical constraints on cosmology, from a combination of DESI, CMB and supernova data, can be accounted for if a small component of dark matter has an evolving and oscillating equation of state within $-1<w<1$.
W. Hu, Structure formation with generalized dark matter , Astrophys. J. 506
1998
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, Perturbations in k-inflation , Phys. Lett. B 458
1999
Earlier work this paper cites.
P. Sikivie and Q. Yang, Bose-Einstein Condensation of Dark Matter Axions , Phys. Rev. Lett. 103
2009
Earlier work this paper cites.
2018
Cited alongside, same era.
N. J. Popławski, Non-particle dark matter from hubble parameter , The European Physical Journal C 79
2019
Cited alongside, same era.
Cited in the paper.
Cited in the paper.
Cited in the paper.
Cited in the paper.
D. Wang, Evidence for Dynamical Dark Matter , 2504.21481
Cited in the paper.
2021
Later among the works it cites.
2024
Later among the works it cites.
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