TY  - JOUR
AU  - Oldengott, I. M.
AU  - Barenboim, G.
AU  - Kahlen, S.
AU  - Salvado, J.
AU  - Schwarz, D. J.
PY  - 2019
DA  - 2019//
TI  - How to relax the cosmological neutrino mass bound
T2  - J. Cosmol. Astropart. Phys.
JO  - Journal of Cosmology and Astroparticle Physics
SP  - 049
EP  - 18pp
VL  - 04
IS  - 4
PB  - Iop Publishing Ltd
KW  - neutrino masses from cosmology
KW  - cosmological neutrinos
KW  - cosmological parameters from CMBR
KW  - cosmological parameters from LSS
AB  - We study the impact of non-standard momentum distributions of cosmic neutrinos on the anisotropy spectrum of the cosmic microwave background and the matter power spectrum of the large scale structure. We show that the neutrino distribution has almost no unique observable imprint, as it is almost entirely degenerate with the effective number of neutrino flavours, N-eff, and the neutrino mass, m(nu). Performing a Markov chain Monte Carlo analysis with current cosmological data, we demonstrate that the neutrino mass bound heavily depends on the assumed momentum distribution of relic neutrinos. The message of this work is simple and has to our knowledge not been pointed out clearly before: cosmology allows that neutrinos have larger masses if their average momentum is larger than that of a perfectly thermal distribution. Here we provide an example in which the mass limits are relaxed by a factor of two.
SN  - 1475-7516
UR  - https://arxiv.org/abs/1901.04352
UR  - https://doi.org/10.1088/1475-7516/2019/04/049
DO  - 10.1088/1475-7516/2019/04/049
LA  - English
N1  - WOS:000466578400003
ID  - Oldengott_etal2019
ER  -