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      The Phenomenology of Right Handed Neutrinos

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          Abstract

          Neutrinos are the only particles in the Standard Model of particle physics that have only been observed with left handed chirality to date. If right handed neutrinos exist, they could be responsible for several phenomena that have no explanation within the Standard Model, including neutrino oscillations, the baryon asymmetry of the universe, dark matter and dark radiation. After a pedagogical introduction, we review recent progress in the phenomenology of right handed neutrinos. We in particular discuss the mass ranges suggested by hints for neutrino oscillation anomalies and dark radiation (eV), sterile neutrino dark matter scenarios (keV) and experimentally testable theories of baryogenesis (GeV to TeV). We summarize constraints from theoretical considerations, laboratory experiments, astrophysics and cosmology for each of these.

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                Author and article information

                Journal
                27 March 2013
                2013-09-18
                Article
                10.1142/S0218301313300191
                1303.6912
                30bd2afb-3916-409a-9cd5-71e22e7c2c72

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                TUM-HEP-881/13
                Int. J. Mod. Phys. E, 22, 1330019 (2013)
                Invited review for the International Journal of Modern Physics E. This preprint is identical to the published article up to a few rephrasings and a number of additional references that appeared after the article had been accepted for publication
                hep-ph astro-ph.CO hep-ex

                Cosmology & Extragalactic astrophysics,High energy & Particle physics
                Cosmology & Extragalactic astrophysics, High energy & Particle physics

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