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@ARTICLE{Domcke:455482,
author = {Domcke, Valerie and Drewes, Marco and Hufnagel, Marco and
Lucente, Michele},
title = {{M}e{V}-scale {S}eesaw and {L}eptogenesis},
journal = {Journal of high energy physics},
volume = {01},
number = {1},
issn = {1029-8479},
address = {[Trieste]},
publisher = {SISSA},
reportid = {PUBDB-2021-01107, arXiv:2009.11678. CERN-TH-2020-158.
DESY-20-159},
pages = {200},
year = {2021},
abstract = {We study the type-I seesaw model with three right-handed
neutrinos and Majorana masses below the pion mass. In this
mass range, the model parameter space is not only strongly
constrained by the requirement to explain the light neutrino
masses, but also by experimental searches and cosmological
considerations. In the existing literature, three disjoint
regions of potentially viable parameter space have been
identified. In one of them, all heavy neutrinos decay
shortly before big bang nucleosynthesis. In the other two
regions, one of the heavy neutrinos either decays between
BBN and the CMB decoupling or is quasi-stable. We show that
previously unaccounted constraints from photodisintegration
of nuclei practically rule out all relevant decays that
happen between BBN and the CMB decoupling. Quite remarkably,
if all heavy neutrinos decay before BBN, the baryon
asymmetry of the universe can be quite generically explained
by low-scale leptogenesis, i.e. without further tuning in
addition to what is needed to avoid experimental and
cosmological constraints. This motivates searches for heavy
neutrinos in pion decay experiments.},
keywords = {* Automatic Keywords * (INSPIRE) / nucleosynthesis: big
bang (INSPIRE) / neutrino: heavy: decay (INSPIRE) / cosmic
background radiation: decoupling (INSPIRE) / neutrino: heavy
(INSPIRE) / neutrino: decay (INSPIRE) / neutrino: mass
(INSPIRE) / neutrino: heavy: search for (INSPIRE) /
neutrino: right-handed (INSPIRE) / pi: decay (INSPIRE) / pi:
mass (INSPIRE) / mass: Majorana (INSPIRE) / baryon:
asymmetry (INSPIRE) / leptogenesis (INSPIRE) / seesaw model
(INSPIRE) / nucleus (INSPIRE) / Beyond Standard Model
(autogen) / Cosmology of Theories beyond the SM (autogen) /
Neutrino Physics (autogen)},
cin = {T},
ddc = {530},
cid = {I:(DE-H253)T-20120731},
pnm = {611 - Fundamental Particles and Forces (POF4-611) / EXC
2121 - Das Quantisierte Universum (390833306) / NewAve - New
avenues towards solving the dark matter puzzle (638528)},
pid = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306 /
G:(EU-Grant)638528},
experiment = {EXP:(DE-MLZ)NOSPEC-20140101},
typ = {PUB:(DE-HGF)16},
eprint = {2009.11678},
howpublished = {arXiv:2009.11678},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2009.11678;\%\%$},
UT = {WOS:000616731700001},
doi = {10.1007/JHEP01(2021)200},
url = {https://bib-pubdb1.desy.de/record/455482},
}