Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter σ8

Dai G. Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino, and Grant. J. Mathews
Phys. Rev. D 81, 103519 – Published 17 May 2010

Abstract

We have made an analysis of limits on the neutrino mass based upon the formation of large-scale structure in the presence of a primordial magnetic field. We find that a new upper bound on the neutrino mass is possible based upon fits to the cosmic microwave background and matter power spectrum when the existing independent constraints on the matter density fluctuation parameter σ8 and the primordial magnetic field are taken into account.

  • Figure
  • Figure
  • Received 17 December 2009

DOI:https://doi.org/10.1103/PhysRevD.81.103519

©2010 American Physical Society

Authors & Affiliations

Dai G. Yamazaki1,*, Kiyotomo Ichiki2, Toshitaka Kajino3,4, and Grant. J. Mathews5

  • 1Institute of Astronomy and Astrophysics, Academia Sinica, 11F of Astronomy-Mathematics Building, National Taiwan University, No.1, Roosevelt Rd, Sec. 4, Taipei 10617, Taiwan, Republic of China
  • 2Department of Physics and Astrophysics, Nagoya Univresity, Nagoya 464-8602, Japan
  • 3National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan
  • 4Department of Astronomy, Graduate School of Science, The University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
  • 5Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA

  • *yamazaki@asiaa.sinica.edu.tw

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 81, Iss. 10 — 15 May 2010

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×