Weakly interacting massive particle dark matter and radiative neutrino mass from Peccei-Quinn symmetry

Basudeb Dasgupta, Ernest Ma, Koji Tsumura

研究成果: Contribution to journalArticle

42 引用 (Scopus)

抜粋

The Peccei-Quinn anomalous global U(1)PQ symmetry is important for solving the strong CP problem with a cosmologically relevant axion. We add to this the simple (but hitherto unexplored) observation that it also has a residual Z2 symmetry which may be responsible for a second component of dark matter, i.e., an absolutely stable weakly interacting singlet scalar. This new insight provides a theoretical justification for this simplest of all possible dark-matter models. It also connects with the notion of generating radiative neutrino mass through dark matter. Two such specific realizations are proposed. In our general scenario, dark-matter detection is guaranteed at existing direct-detection experiments and/or axion searches. Observable signals at the Large Hadron Collider are discussed.

元の言語英語
記事番号041702
ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
89
発行部数4
DOI
出版物ステータス出版済み - 2 25 2014
外部発表Yes

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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