J. Phys. Soc. Jpn. 81, 024101 (2012) [8 Pages]
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Search for Radiative Decays of Cosmic Background Neutrino using Cosmic Infrared Background Energy Spectrum

Shin-Hong Kim1, Ken-ichi Takemasa1, Yuji Takeuchi1, and Shuji Matsuura2
+ Affiliations
1Graduate School of Pure and Applied Sciences, University of Tsukuba, Tsukuba, Ibaraki 305-8571, Japan2Institute of Space and Astronautical Science, JAXA, Sagamihara 252-5210, Japan
Received September 8, 2011; Revised November 22, 2011; Accepted December 1, 2011; Published January 18, 2012

We propose to search for the neutrino radiative decay by fitting a photon energy spectrum of the cosmic infrared background to a sum of the photon energy spectrum from the neutrino radiative decay and a continuum. By comparing the present cosmic infrared background energy spectrum observed by AKARI and Spitzer to the photon energy spectrum expected from neutrino radiative decay with a maximum likelihood method, we obatined a lifetime lower limit of 3.1 ×10 12 to 3.8 ×10 12 years at 95% confidence level for the third generation neutrino ν 3 in the ν 3 mass range between 50 and 150 meV/ c 2 under the present constraints by the neutrino oscillation measurements. In the left–right symmetric model, the minimum lifetime of ν 3 is predicted to be 1.5 ×10 17 years for m 3 of 50 meV/ c 2 . We studied the feasibility of the observation of the neutrino radiative decay with a lifetime of 1.5 ×10 17 years, by measuring a continuous energy spectrum of the cosmic infrared background.

©2012 The Physical Society of Japan
https://doi.org/10.1143/JPSJ.81.024101
KEYWORDS: neutrino radiative decay, neutrino mass, cosmic background neutrino, cosmic infrared background, COBE, AKARI, Spitzer

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