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Could the Presence of Dark Matter Affect the Neutrino Flux?

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Abstract

In the framework of the Standard Model minimal hypercolor extension, scattering of cosmic leptons and protons off two-component Dark Matter with neutrino generation is considered. Possible neutrino flux changes and accelerating of Dark Matter objects are estimated.

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REFERENCES

  1. C. Kilic, T. Okui, and R. Sundrum, J. High Energy Phys. 2010, 18 (2010); arXiv: 0906.0577.

    Article  Google Scholar 

  2. O. Antipin, M. Redi, and A. Strumia, J. High Energy Phys. 2015, 157 (2015); arXiv: 1410.1817.

    Article  Google Scholar 

  3. R. Pasechnik, V. Beylin, V. Kuksa, and G. Vereshkov, Phys. Rev. D 88, 075009 (2013); arXiv: 1304.2081.

    Article  ADS  Google Scholar 

  4. V. Beylin, M. Bezuglov, V. Kuksa, and N. Volchanskiy, Adv. High Energy Phys. 2017, 1 (2017). https://doi.org/10.1155/2017/1765340

    Article  Google Scholar 

  5. V. Beylin, M. Y. Khlopov, V. Kuksa, and N. Volchanskiy, Symmetry 11, 587 (2019); arXiv: 1904.12013.

  6. C. Cai, H.-H. Zhang, and G. Cacciapaglia, J. High Energy Phys. 2019, 130 (2019); arXiv: 1805.07619.

  7. Z. Han and W. Skiba, Phys. Rev. D 72, 035005 (2005); hep-ph/0506206.

    Article  ADS  Google Scholar 

  8. S. Gopalakrishna, T. S. Mukherjee, and S. Sadhukhan, Phys. Rev. D 94, 015034 (2016); arXiv: 1512.05731.

  9. M. Vysotskii, Y. Kogan, and M. Shifman, Sov. J. Nucl. Phys. 42, 318 (1985).

    Google Scholar 

  10. J. Verbaarschot, in Proceedings of the Latin-American School of Physics 35th Elaf on Supersymmetries in Physics and Its Applications, Ed. by R. B. Bijker, O. Castanos, D. Fernandez, H. Morales-Técotl, L. Urrutia, and C. Villarreal, AIP Conf. Proc. 744, 277 (2004); hep-th/0410211.

  11. Y. Bai and R. J. Hill, Phys. Rev. D 82, 111701 (2010); arXiv: 1005.0008.

    Article  ADS  Google Scholar 

  12. O. Antipin, M. Redi, A. Strumia, and E. Vigiani, J. High Energy Phys. 2015, 39 (2015); arXiv: 1503.08749.

  13. M. Aoki, M. Duerr, J. Kubo, and H. Takano, Phys. Rev. D 86, 076015 (2012); arXiv: 1207.3318.

    Article  ADS  Google Scholar 

  14. A. Ahmed, M. Duch, B. Grzadkowski, and M. Iglicki, Eur. Phys. J. C 78, 905 (2018); arXiv: 1710.01853.

  15. V. Beylin, M. Bezuglov, V. Kuksa, E. Tretyakov, and A. Yagozinskaya, Int. J. Mod. Phys. A 34, 1950040 (2019); arXiv: 1810.00372.

  16. L. Roszkowski, E. M. Sessolo, and S. Trojanowski, Rep. Prog. Phys. 81, 066201 (2018); arXiv: 1707.06277.

  17. J. M. Gaskins, Contemp. Phys. 57, 496 (2016); arXiv: 1604.00014.

  18. G. Arcadi, M. Dutra, P. Ghosh, M. Lindner, Y. Mambrini, M. Pierre, S. Profumo, and F. S. Queiroz, Eur. Phys. J. C 78, 203 (2018); arXiv: 1703.07364.

  19. D. Gaggero and M. Valli, Adv. High Energy Phys. 2018, 23 (2018).

    Article  Google Scholar 

  20. M. Gorchtein, S. Profumo, and L. Ubaldi, Phys. Rev. D 82, 083514 (2010); arXiv: 1008.2230.

    Article  ADS  Google Scholar 

  21. S. Profumo and L. Ubaldi, J. Cosmol. Astropart. Phys. 2011, 020 (2011); arXiv: 1106.4568.

  22. V. Beylin, M. Bezuglov, V. Kuksa, and E. Tretiakov, Symmetry 12, 708 (2020).

    Article  Google Scholar 

  23. V. I. Kuksa and N. I. Volchanskiy, Centr. Eur. J. Phys. 11, 182 (2013); arXiv: 1109.1541.

  24. V. S. Berezinsky, V. I. Dokuchaev, and Y. N. Eroshenko, J. Cosmol. Astropart. Phys. 2013, 059 (2013); arXiv: 1308.6742.

  25. A. Tasitsiomi and A. V. Olinto, Phys. Rev. D 66, 083006 (2002); astro-ph/0206040.

    Article  ADS  Google Scholar 

  26. E. Richard, K. Okumura, K. Abe, Y. Haga, Y. Hayato, M. Ikeda, K. Iyogi, J. Kameda, Y. Kishimoto, M. Miura, et al., Phys. Rev. D 94, 052001 (2016); arXiv: 1510.08127.

  27. H. M. Niederhausen, Y. Xu, and IceCube Collab., in Proceedings of the 35th International Cosmic Ray Conference ICRC2017, PoS 301, 968 (2017).

  28. A. Kochanov, S. Sinegovskiy, T. Sinegovskaya, and A. Morozova, Soln.-Zemn. Fiz., No. 1, 3 (2015).

  29. Z.-H. Lei, J. Tang, and B.-L. Zhang, arXiv: 2008.07116 (2020); arXiv: 2008.07116.

  30. J. Kopp, J. Liu, and X.-P. Wang, J. High Energy Phys. 2015, 105 (2015); arXiv: 1503.02669.

  31. D. Kim, J.-C. Park, and S. Shin, Phys. Rev. Lett. 119, 161801 (2017); arXiv: 1612.06867.

  32. J. B. Dent, B. Dutta, J. L. Newstead, and I. M. Shoemaker, Phys. Rev. D 101, 116007 (2020); arXiv: 1907.03782.

  33. S. Forte, Acta Phys. Polon. B 41, 2859 (2010); arXiv: 1011.5247.

    Google Scholar 

  34. J. Jaeckel and W. Yin, J. Cosmol. Astropart. Phys. 2021, 044 (2021); arXiv: 2007.15006.

  35. L. A. Fusco and F. Versari, Eur. Phys. J. Plus 135, 624 (2020); arXiv: 1912.10778.

  36. K.-H. Kampert and A. A. Watson, Eur. Phys. J. H 37, 359 (2012); arXiv: 1207.4827.

    Article  Google Scholar 

  37. X. Bai, B. Y. Bi, X. J. Bi, Z. Cao, S. Z. Chen, Y. Chen, A. Chiavassa, X. H. Cui, Z. G. Dai, D. della Volpe, et al., arXiv: 1905.02773 (2019).

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ACKNOWLEDGMENTS

V.B. acknowledges V. Kuksa and M. Khlopov for fruitful discussions and important comments, M. Bezuglov and E. Tretiakov for the help in numerical analysis.

Funding

V.B. acknowledges the support from the Russian Science Foundation (project no. 18-12-00213-P).

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Authors and Affiliations

  1. Southern Federal University, Rostov-on-Don, Russia

    V. A. Beylin

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  1. V. A. Beylin
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Correspondence to V. A. Beylin.

Additional information

Paper presented at the Fourth Zeldovich meeting, an international conference in honor of Ya.B. Zeldovich held in Minsk, Belarus, on September 7–11, 2020. Published by the recommendation of the special editors: S.Ya. Kilin, R. Ruffini, and G.V. Vereshchagin.

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Beylin, V.A. Could the Presence of Dark Matter Affect the Neutrino Flux?. Astron. Rep. 65, 906–910 (2021). https://doi.org/10.1134/S1063772921100036

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