We present a short discussion of the Neutrino-4 experimental results and the results of other experiments searching for the sterile neutrino. We estimated the contribution of the sterile neutrino with parameters \(\Delta m_{{14}}^{2} \approx 7.3{\kern 1pt} \) eV2 and \({{\sin }^{2}}2{{\theta }_{{14}}} \approx 0.36\) obtained in the Neutrino-4 experiment to the energy density of the Universe. We address the contradiction between the measured sterile neutrino parameters and the constraints on the sterile neutrino from cosmology. With this article, we want to draw attention to the problem of the contradiction between experiment and theory, in order to inspire the search for theoretical models that include a sterile neutrino with mass in the region of several eV, and to the necessity to sufficiently increase the precision of the experiment.
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REFERENCES
A. Aguilar, L. B. Auerbach, R. L. Burman, et al. (LSND Collab.), Phys. Rev. D 64, 112007 (2001); hep-ex/0104049. https://doi.org/10.1103/PhysRevD.64.112007
A. A. Aguilar-Arevalo, B. C. Brown, L. Bugel, et al. (MiniBooNE Collab.), Phys. Rev. Lett. 121, 221801 (2018); arXiv: 1805.12028. https://doi.org/10.1103/PhysRevLett.121.221801
G. Mention, M. Fechner, T. Lasserre, T. Mueller, D. Lhuillier, M. Cribier, and A. Letourneau, Phys. Rev. D 83, 073006 (2011); arXiv: 1101.2755. https://doi.org/10.1103/PhysRevD.83.073006
C. Giunti and Th. Lasserre, Ann. Rev. Nucl. Part. Sci. 69, 163 (2019); arXiv: 1901.08330. https://doi.org/10.1146/annurev-nucl-101918-023755
W. Hampel, G. Heusser, J. Kiko, et al. (GALLEX Collab.), Phys. Lett. B 420, 114 (1998). https://doi.org/10.1016/S0370-2693(97)01562-1
J. N. Abdurashitov, V. N. Gavrin, S. V. Girin, et al. (SAGE Collab.), Phys. Rev. C 59, 2246 (1999). https://doi.org/10.1103/PhysRevC.59.2246
V. V. Barinov, B. T. Cleveland, S. N. Danshin, et al. (BEST Collab.), Phys. Rev. C 105, 065502 (2022); ar-Xiv: 2201.07364. https://doi.org/10.1103/PhysRevC.105.065502
A. Serebrov and R. Samoilov, JETP Lett. 112, 199 (2020). https://doi.org/10.1134/S0021364020160122
A. P. Serebrov, R. M. Samoilov, V. G. Ivochkin, et al. (Neutrino-4 Collab.), Phys. Rev. D 104, 032003 (2021). https://doi.org/10.1103/PhysRevD.104.032003
A. P. Serebrov, R. M. Samoilov, and M. E. Chaikov-skii, arXiv: 2112.14856.
M. Aker, K. Altenmueller, A. Beglarian, et al. (K-ATRIN Collab.), Phys. Rev. Lett. 126, 091803 (2021); arXiv: 2011.05087. https://doi.org/10.1103/PhysRevLett.126.091803
M. Aker, A. Beglarian, J. Behrens, et al. (The KATRIN Collab.), Nat. Phys. 18, 160 (2022); arXiv: 2105.08533. https://doi.org/10.1038/s41567-021-01463-1
S. S. Gershtein, E. P. Kuznetsov, and V. A. Ryabov, Phys. Usp. 40, 773 (1997). https://doi.org/10.1070/PU1997v040n08ABEH000272
D. S. Gorbunov and V. A. Rubakov, Introduction to the Theory of the Early Universe: Hot Big Bang Theory, 2nd ed. (World Scientific, NJ, 2017). https://doi.org/10.1142/7874
D. Notzold and G. Raffelt, Nucl. Phys. B 307, 924 (1988). https://doi.org/10.1016/0550-3213(88)90113-7
A. D. Dolgov, Phys. Rep. 370, 333 (2002); arXiv: hep-ph/0202122 https://doi.org/10.1016/S0370-1573(02)00139-4
R. Barbieri and A. D. Dolgov, Nucl. Phys. B 349, 743 (1991). https://doi.org/10.1016/0550-3213(91)90396-F
N. Aghanim, Y. Akrami, M. Ashdown, et al. (Planck Collab.), Astron. Astrophys. 641, A6 (2020). https://doi.org/10.1051/0004-6361/201833910
E. Giusarma, S. Vagnozzi, Sh. Ho, S. Ferraro, K. Freese, R. Kamen-Rubio, and K.-B. Luk, Phys. Rev. D 98, 123526 (2018); arXiv: 1802.08694. https://doi.org/10.1103/PhysRevD.98.123526
R. C. Nunes and A. Bonilla, Mon. Not. R. Astron. Soc. 473, 4404 (2018); arXiv: 1710.10264. https://doi.org/10.1093/mnras/stx2661
B. D. Fields, K. A. Olive, T.-H. Yeh, and C. Young, J. Cosmol. Astropart. Phys., No. 03, 010 (2020); arXiv: 1912.01132.https://doi.org/10.1088/1475-7516/2020/03/010
Erratum: J. Cosmol. Astropart. Phys., No. 11, E02 (2020).
V. V. Barinov, R. A. Burenin, D. S. Gorbunov, and R. A. Krivonos, Phys. Rev. D 103, 063512 (2021). https://doi.org/10.1103/PhysRevD.103.063512
B. M. Roach, S. Rossland, K. C. Y. Ng, K. Perez, J. F. Beacom, B. W. Grefenstette, Sh. Horiuchi, R. Krivonos, and D. R. Wik, arXiv: 2207.04572v2.
M. Aker, M. Balzer, D. Batzler, et al. (KATRIN Collab.), arXiv: 2203.08059v2.
A. D. Dolgov, Nucl. Phys. B 610, 411 (2001); arXiv: hep/0102125. https://doi.org/10.1016/S0550-3213(01)00323-6
R. Abbasi, M. Ackermann, J. Adams, et al. (IceCube Collab.), arXiv: 2204.00612.
ACKNOWLEDGMENTS
We are grateful to V.A. Rubakov, A.D. Dolgov, and Z.G. Berezhiani for advice and comments on the theoretical aspects of this work and to the colleagues at the Petersburg Nuclear Physics Institute and at the Institute for Nuclear Research, Russian Academy of Sciences for useful discussions in seminars.
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The work was supported by the Russian Science Foundation, project no. 20-12-00079.
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Serebrov, A.P., Samoilov, R.M., Chaikovskii, M.E. et al. Result of the Neutrino-4 Experiment and the Cosmological Constraints on the Sterile Neutrino (Brief Review). Jetp Lett. 116, 669–682 (2022). https://doi.org/10.1134/S002136402260224X
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DOI: https://doi.org/10.1134/S002136402260224X