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1992
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A. A. de Laix, R. J. Scherrer and R. K. Schaefer, Astrophys. J. 452
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T. Appelquist, P. S. Rodrigues da Silva and F. Sannino, Phys. Rev. D 60
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Z. y. Duan, P. S. Rodrigues da Silva and F. Sannino, Nucl. Phys. B 592
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M. Markevitch, A. H. Gonzalez, D. Clowe, A. Vikhlinin, L. David, W. Forman, C. Jones and S. Murray et al
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2015

SIMP model at NNLO in chiral perturbation theory

Hansen, Martin, Langaeble, Kasper, Sannino, Francesco

Understand

We investigate the phenomenological viability of a recently proposed class of composite dark matter models where the relic density is determined by 3 to 2 number-changing processes in the dark sector.

Here the pions of the strongly interacting field theory constitute the dark matter particles.
By performing a consistent next-to-leading and next-to-next-to-leading order chiral perturbative investigation we demonstrate that the leading order analysis cannot be used to draw conclusions about the viability of the model.
We further show that higher order corrections substantially increase the tension with phenomenological constraints challenging the viability of the simplest realisation of the strongly interacting massive particle (SIMP) paradigm.

Built on

J. Wess and B. Zumino, Phys. Lett. B 37
1971
Earlier work this paper cites.
E. Witten, Nucl. Phys. B 223
1983
Earlier work this paper cites.
E. Witten, Nucl. Phys. B 223
1983
Earlier work this paper cites.
E. D. Carlson, M. E. Machacek and L. J. Hall, Astrophys. J. 398
1992
Earlier work this paper cites.
A. A. de Laix, R. J. Scherrer and R. K. Schaefer, Astrophys. J. 452
1995
Earlier work this paper cites.
T. Appelquist, P. S. Rodrigues da Silva and F. Sannino, Phys. Rev. D 60
1999
Earlier work this paper cites.
Z. y. Duan, P. S. Rodrigues da Silva and F. Sannino, Nucl. Phys. B 592
2001
Earlier work this paper cites.
M. Markevitch, A. H. Gonzalez, D. Clowe, A. Vikhlinin, L. David, W. Forman, C. Jones and S. Murray et al
2004
Earlier work this paper cites.