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E. Dudas, L. Heurtier, and Y. Mambrini, “Generating X-ray lines from annihilating dark matter,” Phys.Rev
Original
1927
Earlier work this paper cites.
I. Y. Kobsarev, L. B. Okun, and I. Y. Pomeranchuk Sov. J. Nucl. Phys
1966
Earlier work this paper cites.
M. S. Chanowitz and S. R. Sharpe, “Spectrum of Gluino Bound States,” Phys. Lett. B
1983
Earlier work this paper cites.
E. D. Carlson, M. E. Machacek, and L. J. Hall, “Self-Interacting Dark Matter,” Astrophys. J
1992
Earlier work this paper cites.
J. L. Feng and J. Kumar, “The WIMPless Miracle: Dark-Matter Particles without Weak-Scale Masses or Weak Interactions,” Phys.Rev.Lett
Original
2008
Earlier work this paper cites.
J. L. Feng, H. Tu, and H.-B. Yu, “Thermal Relics in Hidden Sectors,” JCAP
Original
2008
Earlier work this paper cites.
J. Kang, M. A. Luty, and S. Nasri, “The Relic abundance of long-lived heavy colored particles,” JHEP
2008
Earlier work this paper cites.
L. E. Strigari, J. S. Bullock, M. Kaplinghat, J. D. Simon, M. Geha, et al
Original
2008
Earlier work this paper cites.
J. E. Juknevich, D. Melnikov, and M. J. Strassler, “A Pure-Glue Hidden Valley I. States and Decays,” JHEP
Original
2009
Earlier work this paper cites.
D. S. Alves, S. R. Behbahani, P. Schuster, and J. G. Wacker, “Composite Inelastic Dark Matter,” Phys.Lett
Original
2010
Earlier work this paper cites.
M. Lisanti and J. G. Wacker, “Parity Violation in Composite Inelastic Dark Matter Models,” Phys.Rev
Original
2010
Earlier work this paper cites.

Similar

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Original
2010
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J. L. Feng and Y. Shadmi, “WIMPless Dark Matter from Non-Abelian Hidden Sectors with Anomaly-Mediated Supersymmetry Breaking,” Phys.Rev
Original
2011
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J. L. Feng, V. Rentala, and Z. Surujon, “WIMPless Dark Matter in Anomaly-Mediated Supersymmetry Breaking with Hidden QED,” Phys.Rev
Original
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Cited alongside, same era.
S. Galli, F. Iocco, G. Bertone, and A. Melchiorri, “Updated CMB constraints on Dark Matter annihilation cross-sections,” Phys.Rev
Original
2011
Cited alongside, same era.
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Then

T. Higaki, K. S. Jeong, and F. Takahashi, “A Parallel World in the Dark,” JCAP
Original
2013
Later among the works it cites.
E. Bulbul, M. Markevitch, A. Foster, R. K. Smith, M. Loewenstein, et al
Original
2014
Closest in time.
M. Heikinheimo, A. Racioppi, M. Raidal, C. Spethmann, and K. Tuominen, “Physical Naturalness and Dynamical Breaking of Classical Scale Invariance,” Mod.Phys.Lett
Original
2014
Closest in time.
Y. Bai and P. Schwaller, “The Scale of Dark QCD,” Phys.Rev
Original
2014
Closest in time.
J. M. Cline, Z. Liu, G. D. Moore, and W. Xue, “Composite strongly interacting dark matter,” Phys. Rev. D
Original

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2014

SIMPle Dark Matter: Self-Interactions and keV Lines

Boddy, Kimberly K., Feng, Jonathan L., Kaplinghat, Manoj et al.

Understand

We consider a simple supersymmetric hidden sector: pure SU(N) gauge theory.

Dark matter is made up of hidden glueballinos with mass $m_X$ and hidden glueballs with mass near the confinement scale $\Lambda$.
For $m_X \sim 1\,\text{TeV}$ and $\Lambda \sim 100\,\text{MeV}$, the glueballinos freeze out with the correct relic density and self-interact through glueball exchange to resolve small-scale structure puzzles.
An immediate consequence is that the glueballino spectrum has a hyperfine splitting of order $\Lambda^2 / m_X \sim 10\,\text{keV}$.