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2018

Forecast on lepton asymmetry from future CMB experiments

Bonilla, Alexander, Nunes, Rafael C., Abreu, Everton M. C.

Understand

We consider a cosmological lepton asymmetry in the form of neutrinos and impose new expected sensitivities on such asymmetry through the degeneracy parameter ($\xi_{\nu}$) by using some future CMB experiment configurations, such as CORE and CMB-S4.

Taking the default scenario with three neutrino states, we find $\xi_{\mu} = 0.05 \pm 0.10 \, (\pm \, 0.04)$, from CORE (CMB-S4) at 95 percent CL, respectively.
Also, within this scenario, we evaluate the neutrino mass scale, obtaining that the normal hierarchy mass scheme is privileged.
Our results are an update concerning on the cosmological lepton asymmetry and the neutrino mass scale within this context, from which can bring a perspective on the null hypothesis for $\xi_{\nu}$ (and its effects on $\Delta N_{\rm eff}$), where perhaps, \textbf{$\xi_{\nu}$} may take a non-null value up to 95 percent CL from future experiments such as CMB-S4.

Built on

Freese K., Kolb E.W., and Turner M.S., Phys. Rev. D, 27, 1689 (1983)
1983
Earlier work this paper cites.
Affleck I. and Dine M., Nucl. Phys. B 249, 361 (1985)
1985
Earlier work this paper cites.
Kang, H.-S., & Steigman, G. 1992, Nuclear Physics B, 372, 494
1992
Earlier work this paper cites.
Hu W., Scott D., Sugiyama N., White M., 1995, Phys. Rev. D, 52, 5498, astro-ph/9505043
1995
Earlier work this paper cites.
Sarkar, S. 1996, Reports on Progress in Physics, 59, 1493. arXiv:hep-ph/9602260
1996
Earlier work this paper cites.
Casas A., Cheng W.Y. and Gelmini G., 1999, Nucl. Phys. B, 538, 297. arXiv:hep-ph/9709289
1999
Earlier work this paper cites.
Kinney W.H., Riotto A., 1999, Phys. Rev. Lett., 83, 3366, hep-ph/9903459
1999
Earlier work this paper cites.
Lesgourgues J., Pastor S., 1999, Phys. Rev. D, 60, 103521, arXiv:hep-ph/9904411
1999
Earlier work this paper cites.
Abazajian K.N., Beacom J.F., Bell N.F., 2002, Phys. Rev. D, 66, 013008, astro-ph/0203442
2002
Earlier work this paper cites.
Dolgov A.D., 2002, Phys. Rept., 370, 333. arXiv:hep-ph/0202122
2002
Earlier work this paper cites.
Dolgov A. D., Hansen S. H., Pastor S., Petcov S. T., Raffelt G. G., Semikoz D. V., 2002, Nuclear Physics B, 632, 363. arXiv:hep-ph/0201287
2002
Earlier work this paper cites.
Wong Y.Y., 2002, Phys. Rev. D, 66, 025015, hep-ph/0203180
2002
Earlier work this paper cites.
Lattanzi M., Ruffni R., Vereshchagin G.V., 2005, Phys. Rev. D, 72, 063003, astro-ph/0509079
2005
Earlier work this paper cites.
Serpico P.D., Raffelt G.G., 2005, Phys. Rev. D, 71, 127301, astro-ph/0506162
2005
Earlier work this paper cites.
Lesgourgues J., Pastor S., Phys. Rept., 429, 307, arXiv:astro-ph/0603494
2006
Earlier work this paper cites.
Ichiki K., Yamaguchi M., Yokoyama J., 2007, Phys. Rev D, 75, 084017, hep-ph/0611121
2007
Earlier work this paper cites.
Popa L.A., Vasile A., 2008, Journal of Cosmology and Astro-Particle Physics, 06, 028, arXiv:0804.2971
Original
2008
Earlier work this paper cites.
Simha V., Steigman G., 2008, Journal of Cosmology and Astro-Particle Physics, 08, 011, arXiv:0806.0179
Original
2008
Earlier work this paper cites.
Pastor S., Pinto T. and Raffelt G. G., Phys. Rev. Lett., 102 (2009) 241302. arXiv:0808.3137
Original
2009
Earlier work this paper cites.
Schwarz, D. J., & Stuke, M. 2009, Journal of Cosmology and Astro-Particle Physics, 11, 025. arXiv:0906.3434
Original
2009
Earlier work this paper cites.
Semikoz, V. B., Sokoloff, D. D., & Valle, J. W. F. 2009, Phys. Rev. D, 80, 083510. arXiv:0905.3365
Original
2009
Earlier work this paper cites.