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2022

Model marginalized constraints on neutrino properties from cosmology

di Valentino, Eleonora, Gariazzo, Stefano, Mena, Olga

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We present robust, model-marginalized limits on both the total neutrino mass ($\sum m_\nu$) and abundance ($N_{\rm eff}$) to minimize the role of parameterizations, priors and models when extracting neutrino properties from cosmology.

The cosmological observations we consider are CMB temperature fluctuation and polarization measurements, Supernovae Ia luminosity distances, BAO observations and determinations of the growth rate parameter from the Data Release 16 of the Sloan Digital Sky Survey IV.
The degenerate neutrino mass spectrum (which implies $\sum m_\nu>0$) is weakly (moderately) preferred over the normal and inverted hierarchy possibilities, which imply the priors $\sum m_\nu>0.06$ and $\sum m_\nu>0.1$ eV respectively.
Concerning the underlying cosmological model, the $\Lambda$CDM minimal scenario is almost always strongly preferred over the possible extensions explored here.

Model marginalized constraints on neutrino properties from cosmology · Around

Built on

I. M. Oldengott, G. Barenboim, S. Kahlen, J. Salvado, and D. J. Schwarz, JCAP 04
Original
1901
Earlier work this paper cites.
N. Aghanim et al. (Planck), Astron. Astrophys. 641
Original
1907
Earlier work this paper cites.
S. Roy Choudhury and S. Hannestad, JCAP 07
Original
1907
Earlier work this paper cites.
W. Handley, Phys. Rev. D 103
Original
1908
Earlier work this paper cites.
S. Gariazzo, Eur. Phys. J. C 80
Original
1910
Earlier work this paper cites.
N. Palanque-Delabrouille, C. Yèche, N. Schöneberg, J. Lesgourgues, M. Walther, S. Chabanier, and E. Armengaud, JCAP 04
Original
1911
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, and J. Silk, Nature Astron. 4
Original
1911
Earlier work this paper cites.
H. Jeffreys, Theory of Probability , The International series of monographs on physics (Clarendon Press, 1961)
1961
Earlier work this paper cites.
A. Gelman and D. B. Rubin, Statist. Sci. 7
1992
Earlier work this paper cites.
P. Astone and G. D’Agostini, Annals Phys. (1999), arXiv:hep-ex/9909047 [hep-ex]
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, Astrophys.J. 538
2000
Earlier work this paper cites.
G. D’Agostini, in Workshop on confidence limits, CERN, Geneva, Switzerland, 17-18 Jan 2000: Proceedings (2000) pp. 3–27, arXiv:hep-ex/0002055 [hep-ex]
2000
Earlier work this paper cites.
W. Yang, E. Di Valentino, O. Mena, S. Pan, and R. C. Nunes, Phys. Rev. D 101
Original
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys.Rev.D 66
2002
Earlier work this paper cites.
W. Yang, E. Di Valentino, O. Mena, and S. Pan, Phys. Rev. D 102
Original
2003
Earlier work this paper cites.
M. Archidiacono, S. Hannestad, and J. Lesgourgues, JCAP 09
Original
2003
Earlier work this paper cites.
G. D’Agostini, Bayesian Reasoning in Data Analysis (WORLD SCIENTIFIC, 2003)
2003
Earlier work this paper cites.
F. Capozzi, E. Di Valentino, E. Lisi, A. Marrone, A. Melchiorri, and A. Palazzo, Phys. Rev. D 95
Original
2003
Earlier work this paper cites.
S. Hannestad, New J. Phys. 6
2004
Earlier work this paper cites.
S. Hannestad, Phys. Rev. Lett. 95
2005
Earlier work this paper cites.
K. Akita and M. Yamaguchi, JCAP 08
Original
2005
Earlier work this paper cites.
P. F. de Salas, D. V. Forero, S. Gariazzo, P. Martínez-Miravé, O. Mena, C. A. Ternes, M. Tórtola, and J. W. F. Valle, JHEP 02
Original
2006
Earlier work this paper cites.
J. Lesgourgues and S. Pastor, Phys. Rept. 429
2006
Earlier work this paper cites.
A. Goobar, S. Hannestad, E. Mortsell, and H. Tu, JCAP 06
2006
Earlier work this paper cites.
J. E. Bautista et al. , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
H. Gil-Marin et al. , Mon. Not. Roy. Astron. Soc. 498
Original
2007
Earlier work this paper cites.
M. Escudero, J. Lopez-Pavon, N. Rius, and S. Sandner, JHEP 12
Original
2007
Earlier work this paper cites.

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