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Similar

F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, L. Campbell et al., The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant , Mon. Not. Roy. Astron. Soc. 416
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2011
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M. Boylan-Kolchin, J. S. Bullock and M. Kaplinghat, Too big to fail? The puzzling darkness of massive Milky Way subhaloes , Mon. Not. Roy. Astron. Soc. 415
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2011
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M. Archidiacono, E. Calabrese and A. Melchiorri, The Case for Dark Radiation , Phys. Rev. D84
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2011
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D. Blas, J. Lesgourgues and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes , JCAP 07
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2011
Cited alongside, same era.
N. Weiner and I. Yavin, How Dark Are Majorana WIMPs? Signals from MiDM and Rayleigh Dark Matter , Phys. Rev. D 86

Then

M. Archidiacono, S. Bohr, S. Hannestad, J. H. Jørgensen and J. Lesgourgues, Linear scale bounds on dark matter–dark radiation interactions and connection with the small scale crisis of cold dark matter , JCAP 1711
Original
2017
Later among the works it cites.
J. B. Muñoz and A. Loeb, Constraints on Dark Matter-Baryon Scattering from the Temperature Evolution of the Intergalactic Medium , JCAP 1711
Original
2017
Later among the works it cites.
S. Tulin and H.-B. Yu, Dark Matter Self-interactions and Small Scale Structure , Phys. Rept. 730
Original
2018
Later among the works it cites.
R. Barkana, Possible interaction between baryons and dark-matter particles revealed by the first stars , Nature 555
Original
2018
Later among the works it cites.
J. B. Munoz and A. Loeb, A small amount of mini-charged dark matter could cool the baryons in the early Universe , Nature 557

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2020

Cosmological constraints on multi-interacting dark matter

Becker, Niklas, Hooper, Deanna C., Kahlhoefer, Felix et al.

Understand

The increasingly significant tensions within $\Lambda$CDM, combined with the lack of detection of dark matter (DM) in laboratory experiments, have boosted interest in non-minimal dark sectors, which are theoretically well-motivated and inspire new search strategies for DM.

Here we consider, for the first time, the possibility of DM having simultaneous interactions with photons, baryons, and dark radiation (DR).
We have developed a new and efficient version of the Boltzmann code CLASS that allows for one DM species to have multiple interaction channels.
With this framework we reassess existing cosmological bounds on the various interaction coefficients in multi-interacting DM scenarios.