High energy seesaw models, GUTs and leptogenesis
High energy seesaw models, GUTs and leptogenesis
I review high energy (type I) seesaw models and in particular how they can be nicely embedded within grand-unified models and reproduce the observed matter-antimatter asymmetry with leptogenesis. I also discuss how high energy (type I) seesaw models can provide a candidate for very heavy cold dark matter, within the TeV-EeV range, whose decays might explain part of the IceCube high energy neutrino events in addition to an astrophysical component.
Di Bari, Pasquale
3fe21e59-0eff-41bc-8faa-fdd817146418
20 September 2017
Di Bari, Pasquale
3fe21e59-0eff-41bc-8faa-fdd817146418
Abstract
I review high energy (type I) seesaw models and in particular how they can be nicely embedded within grand-unified models and reproduce the observed matter-antimatter asymmetry with leptogenesis. I also discuss how high energy (type I) seesaw models can provide a candidate for very heavy cold dark matter, within the TeV-EeV range, whose decays might explain part of the IceCube high energy neutrino events in addition to an astrophysical component.
Text
Di_Bari_2017_J._Phys.-_Conf._Ser._888_012028
- Version of Record
More information
e-pub ahead of print date: 20 September 2017
Published date: 20 September 2017
Identifiers
Local EPrints ID: 416638
URI: http://eprints.soton.ac.uk/id/eprint/416638
ISSN: 1742-6588
PURE UUID: 5b9d50fd-d153-415c-8725-f1df92003efe
Catalogue record
Date deposited: 03 Jan 2018 17:31
Last modified: 15 Mar 2024 16:52
Export record
Altmetrics
Download statistics
Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.
View more statistics