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Phys. Rev. D 69, 081301(R) (2004) [4 pages]

Note on the robustness of the neutrino mass bounds from cosmology

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Robert H. Brandenberger*
Department of Physics, Brown University, Providence, Rhode Island 02912, USA
Perimeter Institute for Theoretical Physics, Waterloo, Canada N2J 2W9

Anupam Mazumdar
Department of Physics, McGill University, Montréal, Québec, Canada H3A 2T8

Masahide Yamaguchi
Department of Physics, Brown University, Providence, Rhode Island 02912, USA

Received 29 January 2004; published 16 April 2004

The recent high precision maps of cosmic microwave anisotropies combined with measurements of the galaxy power spectrum from new large-scale redshift surveys have allowed stringent bounds on the sum of the neutrino masses to be placed. The past analyses, however, have implicitly assumed that the spectrum of primordial density fluctuations is adiabatic and coherent, as predicted in the simplest models of inflation. In this paper, we show that the limits hold even if the assumption on the primordial power spectrum is relaxed to allow for a contribution of nonadiabatic, incoherent fluctuations such as would be predicted by topological defects.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.69.081301
DOI:
10.1103/PhysRevD.69.081301
PACS:
98.80.Cq

*Email address: rhb@het.brown.edu

Email address: anupamm@hep.physics.mcgill.ca

Email address: gucci@het.brown.edu