Published August 2005 | Version v1
Journal article

Constraints on the Neutrino Mass from Cosmology and their impact on world neutrino data

  • 1. Dipartimento di Fisica and Sezione INFN, Universita degli Studi di Roma 'La Sapienza', P.le Aldo Moro 5, 00185, Rome (Italy)
  • 2. Dipartimento di Fisica and Sezione INFN di Bari, Via Amendola 173, 70126, Bari (Italy)
  • 3. Dipartimento di Fisica, Universita degli Studi di Roma 'La Sapienza', P.le Aldo Moro 5, 00185, Rome (Italy)
  • 4. Astrophysics, Denys Wilkinson Building, Keble Road, OX13RH, Oxford (United Kingdom)

Description

We derive upper limits on the sum of neutrino masses from an updated combination of data from Cosmic Microwave Background experiments and Galaxy Redshifts Surveys. The results are discussed in the context of three-flavor neutrino mixing and compared with neutrino oscillation data, with upper limits on the effective neutrino mass in Tritium beta decay from the Mainz and Troitsk experiments and with the claimed lower bound on the effective Majorana neutrino mass in neutrinoless double beta decay from the Heidelberg-Moscow experiment

Additional details

Identifiers

DOI
10.1016/j.nuclphysbps.2005.04.025;
arXiv
arXiv:astro-ph/0501531v1;
PII
S0920-5632(05)00522-0;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
145
Journal Page Range
p. 290-294
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
Neutrino oscillation workshop
Acronym
NOW 2004
Dates
11-17 Sep 2004
Place
Otranto (Italy)

Optional Information

Copyright
Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.