Connecting neutrino physics with dark matter

Massimiliano Lattanzi (Dipartimento di Fisica e Scienza della Terra, Universitá di Ferrara and INFN sezione di Ferrara, Polo Scientifico e Tecnologico—Edificio C Via Saragat, 1, I-44122 Ferrara, Italy) ; Roberto A Lineros (Instituto de Física Corpuscular—CSIC/Universitad de Valencia, Parc Científic, calle Catedrático José Beltrán, 2, E-46980 Paterna, Spain) ; Marco Taoso (Institut de Physique Théorique, CNRS, URA 2306 CEA/Saclay, F-91191 Gif-sur-Yvette, France)

The origin of neutrino masses and the nature of dark matter are two in most pressing open questions in modern astro-particle physics. We consider here the possibility that these two problems are related, and review some theoretical scenarios which offer common solutions. A simple possibility is that the dark matter particle emerges in minimal realizations of the seesaw mechanism, as in the majoron and sterile neutrino scenarios. We present the theoretical motivation for both models and discuss their phenomenology, confronting the predictions of these scenarios with cosmological and astrophysical observations. Finally, we discuss the possibility that the stability of dark matter originates from a flavor symmetry of the leptonic sector. We review a proposal based on an A4 flavor symmetry.

{
  "_oai": {
    "updated": "2018-04-13T10:36:31Z", 
    "id": "oai:repo.scoap3.org:5265"
  }, 
  "authors": [
    {
      "raw_name": "Lattanzi, Massimiliano", 
      "affiliations": [
        {
          "country": "Italy", 
          "value": "Dipartimento di Fisica e Scienza della Terra, Universit\u00e1 di Ferrara and INFN sezione di Ferrara, Polo Scientifico e Tecnologico\u2014Edificio C Via Saragat, 1, I-44122 Ferrara, Italy"
        }
      ], 
      "surname": "Lattanzi", 
      "given_names": "Massimiliano", 
      "full_name": "Lattanzi, Massimiliano"
    }, 
    {
      "raw_name": "Lineros, Roberto A", 
      "affiliations": [
        {
          "country": "Spain", 
          "value": "Instituto de F\u00edsica Corpuscular\u2014CSIC/Universitad de Valencia, Parc Cient\u00edfic, calle Catedr\u00e1tico Jos\u00e9 Beltr\u00e1n, 2, E-46980 Paterna, Spain"
        }
      ], 
      "surname": "Lineros", 
      "given_names": "Roberto A", 
      "full_name": "Lineros, Roberto A"
    }, 
    {
      "raw_name": "Taoso, Marco", 
      "affiliations": [
        {
          "country": "France", 
          "value": "Institut de Physique Th\u00e9orique, CNRS, URA 2306 CEA/Saclay, F-91191 Gif-sur-Yvette, France"
        }
      ], 
      "surname": "Taoso", 
      "given_names": "Marco", 
      "full_name": "Taoso, Marco"
    }
  ], 
  "titles": [
    {
      "source": "Institute of Physics Publishing/Deutsche Physikalische Gesellschaft", 
      "title": "Connecting neutrino physics with dark matter"
    }
  ], 
  "dois": [
    {
      "value": "10.1088/1367-2630/16/12/125012"
    }
  ], 
  "publication_info": [
    {
      "journal_title": "New Journal of Physics", 
      "page_start": "125012", 
      "material": "article", 
      "journal_issue": "12", 
      "year": 2014
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2014-12-22T00:00:00", 
    "source": "Institute of Physics Publishing/Deutsche Physikalische Gesellschaft", 
    "method": "scoap3", 
    "submission_number": "75c1bb743f0611e881c402163e01809a"
  }, 
  "page_nr": [
    19
  ], 
  "license": [
    {
      "url": "http://creativecommons.org/licenses/by/3.0/", 
      "license": "CC-BY-3.0"
    }
  ], 
  "copyright": [
    {
      "statement": "\u00a9 2014 IOP Publishing Ltd and Deutsche Physikalische Gesellschaft", 
      "year": "2014"
    }
  ], 
  "control_number": "5265", 
  "record_creation_date": "2014-12-22T00:00:00", 
  "_files": [
    {
      "checksum": "md5:223b73b442e1de4226876b2d8ae61eaa", 
      "filetype": "pdf", 
      "bucket": "7af984e7-cf28-4a5c-97cf-551e0d724391", 
      "version_id": "abbecc39-0d7c-46c3-808e-217b29b45146", 
      "key": "10.1088/1367-2630/16/12/125012.pdf", 
      "size": 1314600
    }, 
    {
      "checksum": "md5:763c8bdab7214c333fc0f801ebf5f804", 
      "filetype": "xml", 
      "bucket": "7af984e7-cf28-4a5c-97cf-551e0d724391", 
      "version_id": "945fab51-70e5-4c16-8249-6dd539ee68fd", 
      "key": "10.1088/1367-2630/16/12/125012.xml", 
      "size": 225516
    }
  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-ph", 
        "astro-ph.CO"
      ], 
      "value": "1406.0004"
    }
  ], 
  "abstracts": [
    {
      "source": "Institute of Physics Publishing/Deutsche Physikalische Gesellschaft", 
      "value": "The origin of neutrino masses and the nature of dark matter are two in most pressing open questions in modern astro-particle physics. We consider here the possibility that these two problems are related, and review some theoretical scenarios which offer common solutions. A simple possibility is that the dark matter particle emerges in minimal realizations of the seesaw mechanism, as in the majoron and sterile neutrino scenarios. We present the theoretical motivation for both models and discuss their phenomenology, confronting the predictions of these scenarios with cosmological and astrophysical observations. Finally, we discuss the possibility that the stability of dark matter originates from a flavor symmetry of the leptonic sector. We review a proposal based on an A4 flavor symmetry."
    }
  ], 
  "imprints": [
    {
      "date": "2014-12-22", 
      "publisher": "Institute of Physics Publishing/Deutsche Physikalische Gesellschaft"
    }
  ]
}
Published on:
22 December 2014
Publisher:
Institute of Physics Publishing/Deutsche Physikalische Gesellschaft
Published in:
New Journal of Physics (2014)
Issue 12
DOI:
https://doi.org/10.1088/1367-2630/16/12/125012
arXiv:
1406.0004
Copyrights:
© 2014 IOP Publishing Ltd and Deutsche Physikalische Gesellschaft
Licence:
CC-BY-3.0

Fulltext files: