Impact of lepton asymmetry and sterile neutrinos on Primordial Nucleosynthesis
Schepkin A.A.1, Kurichin O.A.1, Ivanchik A.B.1
1Ioffe Institute, St. Petersburg, Russia
Email: alexander.shchepkin5@gmail.com

PDF
The ratio is defined between the number of additional relativistic degrees of freedom, Δ Neff, and parameter of lepton asymmetry of neutrino, ξ, in the epoch of the Primordial Nucleosynthesis (PN), when the theoretically predicted value of abundance of the primordial 4He, Yp, agrees with the value defined from the observations. It is shown that the presence of the light fully or partially thermalized sterile neutrinos does not contradict the observational data on PN at value ξ~0.05, which might be generated in the early Universe within the existing models of leptogenesis and resonant neutrino oscillations. Keywords: early Universe, Primordial Nucleosynthesis, sterile neutrinos, lepton asymmetry.
  1. T. Asaka, M. Shaposhnikov. Phys. Lett. B, 631, 151 (2005). DOI: 10.1016/j.physletb.2005.09.070
  2. D.S. Gorbunov. Physics Uspekhi, 57 (5), 503 (2014). DOI: 10.3367/UFNr.0184.201405i.0545
  3. P.A. Chernikov, A.V. Ivanchik. Astron. Lett., 48 (12), 689 (2022). DOI: 10.1134/S1063773722110056
  4. D.S. Gorbunov, V.A. Rubakov. Vvedenie v teoriyu ranney Vselennoy. Teoriya goryachego Bolshogo Vzryva (LENAND, M., 2016), ed. 3-rd, Vol. 1. ISBN: 978-5-9710-1679-3
  5. B.D. Fields. JCAP, 03, 010 (2020). DOI: 10.1088/1475-7516/2020/03/010
  6. Planck Collaboration, A\&A, 641, A6 (2020). DOI: 10.1051/0004-6361/201833910
  7. S. Gariazzo et al., JCAP, 07, 014 (2019). DOI: 10.1088/1475-7516/2019/07/014
  8. A.P. Serebrov, R.M. Samoilov, M.E. Chaikovskii, O.M. Zherebtsov. JETP Lett., 116 (10), 669 (2022). DOI: 10.1134/S002136402260224X
  9. L. Canetti, M. Drewes, T. Frossard, M. Shaposhnikov. Phys. Rev. D, 87, 093006 (2013). DOI: 10.1103/PhysRevD.87.093006
  10. A.D. Dolgov. Nucl. Phys. B, 610, 411 (2001). DOI: 10.1016/S0550-3213(01)00323-6
  11. S. Weinberg. Cosmology (Oxford University Press, 2008), ISBN: 978-0-19-852682-7
  12. R.V. Wagoner, W.A. Fowler, F. Hoyle. ApJ, 148, 3 (1967). DOI: 10.1086/149126
  13. O. Seto, Y. Toda. Phys. Rev. D, 104, 063019 (2021). DOI: 10.1103/PhysRevD.104.063019
  14. O.A. Kurichin, P.A. Kislitsyn, V.V. Klimenko, S.A. Balashev, A.V. Ivanchik. MNRAS, 502 (2), 3045 (2021). DOI: 10.1093/mnras/stab215

Подсчитывается количество просмотров абстрактов ("html" на диаграммах) и полных версий статей ("pdf"). Просмотры с одинаковых IP-адресов засчитываются, если происходят с интервалом не менее 2-х часов.

Дата начала обработки статистических данных - 27 января 2016 г.

Publisher:

Ioffe Institute

Institute Officers:

Director: Sergei V. Ivanov

Contact us:

26 Polytekhnicheskaya, Saint Petersburg 194021, Russian Federation
Fax: +7 (812) 297 1017
Phone: +7 (812) 297 2245
E-mail: post@mail.ioffe.ru