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The Effect of Neutrino Mass in Cosmology

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Astrophysics Aims and scope

The influence of the small neutrino mass on the properties of the cosmological neutrino gas and on the evolution of the universe is estimated. The characteristics of the equilibrium neutrino gas are first calculated and the temperatures up to which to which they can be regarded as ultrarelativistic for different neutrino masses are found. The evolution of cosmological neutrinos of any type are traced for different neutrino masses. The red shifts neutrinos remain ultrarelativistic are determined. The effective temperature of the neutrino gas and the effect of neutrino mass on the rate of expansion of the universe are determined.

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References

  1. W. Pauli, Letter to a physicist’s gathering at Tübingen, December 4 (1930), reproduced in L. M. Brown, Physics Today 31, 9 (1978).

    Google Scholar 

  2. F. Reines and C. L. Cowan, Phys. Rev. 92, 830 (1953).

    Article  ADS  Google Scholar 

  3. F. Reines and C. L. Cowan, Phys. Rev. 113, 273 (1959).

    Article  ADS  Google Scholar 

  4. W. Pauli, in: V. F. Weisskopf, ed., Aufsätse und Vorträge über Physik und Erkenntnistheorie, Vieweg, Braunschweig (1961), p. 156.

    Chapter  Google Scholar 

  5. Wu Tsyan-sui, in: Theoretical Physics in the Twentieth Century. A Memorial Volume to Wolfgang Pauli, Interscience Publishers, Cambridge, USA (1960), p. 249.

  6. Donglian Xu for IceCube collaboration. Nuclear and Particle Physics Proceedings 287, 139 (2017).

  7. Y. Fukuda, et al., Phys. Rev. Lett. 81, 1562 (1998).

    Article  ADS  Google Scholar 

  8. Q. R. Ahmad, et al., (SNO Collaboration), Phys. Rev. Lett. 87, 071301 (2001).

  9. Q. R. Ahmad, et al., Phys. Rev. Lett. 89, 011301 (2002).

    Article  ADS  Google Scholar 

  10. Ya. B. Zeldovich and M. Yu. Khlopov, UFN 135, 45 (1981).

    Article  Google Scholar 

  11. M. Gerbino and M. Lattanzi, arXiv:astro-ph/1712.07109.

  12. Sai Wang and Dong-Mei Xia, arXiv:astro-ph/1707.00588.

  13. S. Gariazzo, arXiv:astro-ph/1601.01475.

  14. D. Boriero, D. T. Schwatz, and H. Velten, Flavour composition and entropy increase of cosmological neutrinos after decoherence, JCAP in press. arXiv:astro-ph1704.06139.

  15. A. Abada, G. Arcadi, V. Domcke, et al., arXiv:astro-ph/1709.00415.

  16. R. Ruggeri, E. Castorina, C. Carbone, et al., arXiv:astro-ph/1712.02334.

  17. M. Zennaro, J. Bel, J. Dossett, et al., arXiv:astro-ph/1712.02886.

  18. G. Rossi, arXiv:astro-ph/1712.00230.

  19. R. C. Nunes and A. Bonilla, arXiv:astro-ph/1710.10264.

  20. A. Upadhye, Neutrino mass and dark energy constraints from redshift-space distortions, arXiv:astro-p/1707.09354.

  21. L. D. Landau and E. M. Lifshitz, Theoretical Physics in 10 vols., Vol. V, Statistical Physics, part 1 [in Russian], Nauka, Moscow (1995).

    Google Scholar 

  22. G. Hinshaw, et al., Astrophys. J. Suppl. Ser. 208, article id. 19 (2013).

  23. R. Alpher, J. W. Follin, and R. C. Herman, Phys. Rev. 92, 1347 (1953).

    Article  ADS  Google Scholar 

  24. Ya. B. Zeldovich and I. D. Novikov, Structure and Evolution of the Universe [in Russian], Nauka, Moscow (1975).

    Google Scholar 

Download references

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Correspondence to D. I. Nagirner.

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Translated from Astrofizika, Vol. 62, No. 1, pp. 131-149 (February 2019)

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Nagirner, D.I., Turichina, D.G. The Effect of Neutrino Mass in Cosmology. Astrophysics 62, 108–128 (2019). https://doi.org/10.1007/s10511-019-09568-5

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  • DOI: https://doi.org/10.1007/s10511-019-09568-5

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