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Sensitivity of neutrino mass experiments to the cosmic neutrino background

2010/06/09 by A. Kaboth, J. A. Formaggio, B. Monreal · 2 citations
Physics and Astronomy · #Astrophysics #COSMIC cancer database #Cosmic neutrino background #Dark Matter and Cosmic Phenomena #Electron neutrino #KATRIN #Neutrino #Neutrino Physics Research #Neutrino detector #Neutrino oscillation #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Sensitivity (control systems) #Solar neutrino #astro-ph.CO #hep-ex

paper · pdf · doi:10.1103/physrevd.82.062001

published as Phys.Rev.D82:062001,2010

arxiv created 2010/06/09 · openalex publication_date 2010/09/13 · arxiv updated 2014/11/21 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The KATRIN neutrino experiment is a next-generation tritium beta decay experiment aimed at measuring the mass of the electron neutrino to better than 200 meV at 90% C.L. Because of its intense tritium source, KATRIN can also serve as a possible target for the process of neutrino capture, \ensuremathνe+3H\ensuremath→3He++e^\ensuremath-. The latter process, possessing no energy threshold, is sensitive to the cosmic neutrino background (C\ensuremathνB). In this paper, we explore the potential sensitivity of the KATRIN experiment to the relic neutrino density. The KATRIN experiment is sensitive to a C\ensuremathνB overdensity ratio of 2.0\ifmmode×\else\texttimes\fi109 over standard concordance model predictions (at 90% C.L.), addressing the validity of certain speculative cosmological models.

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