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2017

Is Self-Interacting Dark Matter Undergoing Dark Fusion?

McDermott, Samuel D.

Understand

We suggest that two-to-two dark matter fusion may be the relaxation process that resolves the small-scale structure problems of the cold collisionless dark matter paradigm.

In order for the fusion cross section to scale correctly across many decades of astrophysical masses from dwarf galaxies to galaxy clusters, we require the fractional binding energy released to be greater than v^n ~ [10^{-(2-3)}]^n, where n=1,2 depends on local dark sector chemistry.
The size of the dark-sector interaction cross sections must be sigma ~ 0.1-1 barn, moderately larger than for Standard Model deuteron fusion, indicating a dark nuclear scale Lambda ~ O(100 MeV).
Dark fusion firmly predicts constant sigma v below the characteristic velocities of galaxy clusters.

Built on

H. A. Bethe and C. Longmire, Phys. Rev. 77
1950
Earlier work this paper cites.
G. Baym, H. A. Bethe, and C. Pethick, Nucl. Phys. A175
1971
Earlier work this paper cites.
F. D. Mackie and G. Baym, Nucl. Phys. A285
1977
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. Kaplinghat, L. Knox, and M. S. Turner, Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
L. Hui, Phys. Rev. Lett. 86
2001
Earlier work this paper cites.
J. F. Beacom, N. F. Bell, and G. D. Mack, Phys. Rev. Lett. 99
2007
Earlier work this paper cites.
D. P. Finkbeiner and N. Weiner, Phys. Rev. D76
2007
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.
J. P. Huchra, L. M. Macri, K. L. Masters, T. H. Jarrett, P. Berlind, M. Calkins, A. C. Crook, R. Cutri, P. Erdogdu, E. Falco, T. George, C. M. Hutcheson, O. Lahav, J. Mader, J. D. Mink, N. Martimbeau, S. Schneider, M. Skrutskie, S. Tokarz, and M. Westover, (2011) , 1108.0669
Original
2011
Earlier work this paper cites.
M. McCullough and L. Randall, JCAP 1310
Original
2013
Earlier work this paper cites.