Scale-Invariant Scalar Field Dark Matter Through the Higgs-Portal
425
observed properties for the corresponding value of the DM mass although it will be
very difficult to probe it in the laboratory in the near future.
References
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425
observed properties for the corresponding value of the DM mass although it will be
very difficult to probe it in the laboratory in the near future.
References
1. C. Cosme, J.G. Rosa, O. Bertolami, J. High Energy Phys. 1805, 129 (2018). https://doi.org/10.
1007/JHEP05(2018)129. [arXiv:1802.09434 [hep-ph]]
2. C. Cosme, J.G. Rosa, O. Bertolami, Phys. Lett. B 781, 639 (2018). https://doi.org/10.1016/j.
physletb.2018.04.062. [arXiv:1709.09674 [hep-ph]]
3. A. Riotto, ICTP Lect. Notes Ser. 14, 317 (2003). [hep-ph/0210162]
4. E. Bulbul, M. Markevitch, A. Foster, R.K. Smith, M. Loewenstein, S.W. Randall, Astrophys.
J. 789, 13 (2014). https://doi.org/10.1088/0004-637X/789/1/13. [arXiv:1402.2301 [astroph.CO]]
5. A. Boyarsky, O. Ruchayskiy, D. Iakubovskyi, J. Franse, Phys. Rev. Lett. 113, 251301 (2014).
https://doi.org/10.1103/PhysRevLett.113.251301. [arXiv:1402.4119 [astro-ph.CO]]
6. A. Boyarsky, J. Franse, D. Iakubovskyi, O. Ruchayskiy, Phys. Rev. Lett. 115, 161301 (2015).
https://doi.org/10.1103/PhysRevLett.115.161301. [arXiv:1408.2503 [astro-ph.CO]]
7. N. Cappelluti, et al., (2017). arXiv:1701.07932 [astro-ph.CO]
8. T. Higaki, K.S. Jeong, F. Takahashi, Phys. Lett. B 733, 25 (2014). https://doi.org/10.1016/j.
physletb.2014.04.007. [arXiv:1402.6965 [hep-ph]]
9. J. Jaeckel, J. Redondo, A. Ringwald, Phys. Rev. D 89, 103511 (2014). https://doi.org/10.1103/
PhysRevD.89.103511. [arXiv:1402.7335 [hep-ph]]
10. E. Dudas, L. Heurtier, Y. Mambrini, Phys. Rev. D 90, 035002 (2014). https://doi.org/10.1103/
PhysRevD.90.035002. [arXiv:1404.1927 [hep-ph]]
11. F.S. Queiroz, K. Sinha, Phys. Lett. B 735, 69 (2014). https://doi.org/10.1016/j.physletb.2014.
06.016. [arXiv:1404.1400 [hep-ph]]
12. J. Heeck, D. Teresi, (2017). arXiv:1706.09909 [hep-ph]
13. O. Ruchayskiy, et al., Mon. Not. Roy. Astron. Soc. 460(2), 1390 (2016). https://doi.org/10.
1093/mnras/stw1026. [arXiv:1512.07217 [astro-ph.HE]]