Light dark matter candidate in B–L gauged radiative inverse seesaw

2012/10/31 by Yuji Kajiyama, Hiroshi Okada, Takashi Toma · 1 citation
Mathematics · Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Geometry #Inverse #Mathematics #Neutrino #Particle physics #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Radiative transfer #Seesaw molecular geometry #hep-ph

paper · pdf · doi:10.1140/epjc/s10052-013-2381-2

10 pages, 1 table, 3 figures; version accepted for publication in European Physical Journal C

openalex publication_date 2013/03/01 · arxiv created 2013/03/19 · arxiv updated 2015/06/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We study a radiative inverse seesaw model with local B-L symmetry, in which we extend the neutrino mass structure that is generated through a kind of inverse seesaw framework to the more generic one than our previous work. We focus on a real part of bosonic particle as a dark matter and investigate the features in O(1-80) GeV mass range, reported by the experiments such as CoGeNT and XENON (2012).

Citations

• Dark matter maps reveal cosmic scaffolding
• Remarks on the Unified Model of Elementary Particles
• Verifiable radiative seesaw mechanism of neutrino mass and dark matter
• Effects of new leptons in electroweak precision data
• FIVE-YEARWILKINSON MICROWAVE ANISOTROPY PROBEOBSERVATIONS: COSMOLOGICAL INTERPRETATION
• Review of Particle Physics

Cited by

• A radiative seesaw model with higher order terms under an alternative U(1)−