Built on

E. D. Carlson, M. E. Machacek, and L. J. Hall, Astrophys. J. 398
1992
Earlier work this paper cites.
R. A. Flores and J. R. Primack, Astrophys. J. 427
1994
Earlier work this paper cites.
J. McDonald, Phys. Rev. D50
1994
Earlier work this paper cites.
A. A. Starobinsky and J. Yokoyama, Phys. Rev. D50
1994
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk, and S. D. M. White, Astrophys. J. 490
1997
Earlier work this paper cites.
A. A. Klypin, A. V. Kravtsov, O. Valenzuela, and F. Prada, Astrophys. J. 522
1999
Earlier work this paper cites.
M. Markevitch, A. H. Gonzalez, D. Clowe, A. Vikhlinin, L. David, W. Forman, C. Jones, S. Murray, and W. Tucker, Astrophys. J. 606
2004
Earlier work this paper cites.
S. W. Randall, M. Markevitch, D. Clowe, A. H. Gonzalez, and M. Bradac, Astrophys. J. 679
Original
2008
Earlier work this paper cites.
F. L. Bezrukov and M. Shaposhnikov, Phys. Lett. B659
Original
2008
Earlier work this paper cites.
W. J. G. de Blok, Adv. Astron. 2010
Original
2010
Earlier work this paper cites.
L. J. Hall, K. Jedamzik, J. March-Russell, and S. M. West, JHEP 1003
Original
2010
Earlier work this paper cites.
M. Boylan-Kolchin, J. S. Bullock, and M. Kaplinghat, Mon. Not. Roy. Astron. Soc. 415
Original
2011
Earlier work this paper cites.
X. Chu, T. Hambye, and M. H. G. Tytgat, JCAP 1205
Original
2012
Earlier work this paper cites.
M. Rocha, A. H. G. Peter, J. S. Bullock, M. Kaplinghat, S. Garrison-Kimmel, J. Onorbe, and L. A. Moustakas, Mon. Not. Roy. Astron. Soc. 430
Original
2013
Earlier work this paper cites.
A. H. G. Peter, M. Rocha, J. S. Bullock, and M. Kaplinghat, Mon. Not. Roy. Astron. Soc. 430
Original
2013
Earlier work this paper cites.
M. Viel, G. D. Becker, J. S. Bolton, and M. G. Haehnelt, Phys. Rev. D88
Original
2013
Earlier work this paper cites.
E. Bulbul, M. Markevitch, A. Foster, R. K. Smith, M. Loewenstein, and S. W. Randall, Astrophys. J. 789
Original
2014
Earlier work this paper cites.
A. Boyarsky, O. Ruchayskiy, D. Iakubovskyi, and J. Franse, Phys. Rev. Lett. 113
Original
2014
Earlier work this paper cites.

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Original
2014
Cited alongside, same era.
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Original
2014
Cited alongside, same era.
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Original
2014
Cited alongside, same era.
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Original
2014
Cited alongside, same era.
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Original
2014
Cited alongside, same era.

Then

A. Merle, A. Schneider, and M. Totzauer, (2015), arXiv:1512.05369 [hep-ph]
Original
2015
Later among the works it cites.
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Original
2015
Later among the works it cites.
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Original
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Later among the works it cites.
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Later among the works it cites.
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Original
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2016

Observational Constraints on Decoupled Hidden Sectors

Heikinheimo, Matti, Tenkanen, Tommi, Tuominen, Kimmo et al.

Understand

We consider an extension of the Standard Model with a singlet sector consisting of a real (pseudo)scalar and a Dirac fermion coupled with the Standard Model only via the scalar portal.

We assume that the portal coupling is weak enough for the singlet sector not to thermalize with the Standard Model allowing the production of singlet particles via the freeze-in mechanism.
If the singlet sector interacts with itself sufficiently strongly, it may thermalize within itself, resulting in dark matter abundance determined by the freeze-out mechanism operating within the singlet sector.
We investigate this scenario in detail.