https://doi.org/10.1140/epjc/s10052-022-10518-3
Regular Article - Theoretical Physics
Weaker yet again: mass spectrum-consistent cosmological constraints on the neutrino lifetime
1
Sydney Consortium for Particle Physics and Cosmology, School of Physics, The University of New South Wales, 2052, Sydney, NSW, Australia
2
Centre for Cosmology, Particle Physics and Phenomenology, Université catholique de Louvain, Chemin du cyclotron, 2, 1348, Louvain-la-Neuve, Belgium
Received:
25
March
2022
Accepted:
11
June
2022
Published online:
25
July
2022
We consider invisible neutrino decay in the ultra-relativistic limit and compute the neutrino anisotropy loss rate relevant for the cosmic microwave background (CMB) anisotropies. Improving on our previous work which assumed massless
and
, we reinstate in this work the daughter neutrino mass
in a manner consistent with the experimentally determined neutrino mass splittings. We find that a nonzero
introduces a new phase space factor in the loss rate
proportional to
in the limit of a small squared mass gap between the parent and daughter neutrinos, i.e.,
, where
is the
rest-frame lifetime. Using a general form of this result, we update the limit on
using the Planck 2018 CMB data. We find that for a parent neutrino of mass
eV, the new phase space factor weakens the constraint on its lifetime by up to a factor of 50 if
corresponds to the atmospheric mass gap and up to
if the solar mass gap, in comparison with naïve estimates that assume
. The revised constraints are (i)
s and
s if only one neutrino decays to a daughter neutrino separated by, respectively, the atmospheric and the solar mass gap, and (ii)
s in the case of two decay channels with one near-common atmospheric mass gap. In contrast to previous, naïve limits which scale as
, these mass spectrum-consistent
constraints are remarkably independent of the parent mass and open up a swath of parameter space within the projected reach of IceCube and other neutrino telescopes in the next two decades.
© The Author(s) 2022
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