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Determining neutrino properties using future galaxy redshift surveys

Abstract:

Current measurements of the large-scale structure of galaxies are able to place an $\sim 0.5 ~ \rm eV$ upper limit on the absolute mass scale of neutrinos. An order-of-magnitude improvement in raw sensitivity, together with an insensitivity to systematic effects, is needed to reach the lowest value allowed by particle physics experiments. We consider the prospects of determining both the neutrino mass scale and the number of of massive neutrinos using future redshift surveys, specifically tho...

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Publication status:
Published

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Authors


Abdalla, FB More by this author
Rawlings, S More by this author
Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
381
Issue:
4
Pages:
1313-1328
Publication date:
2007-02-12
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:d1fc7378-fa74-408e-bfe0-fceac4ffb6cd
Source identifiers:
15699
Local pid:
pubs:15699
Keywords:

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