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Search for Ultra-low Mass Dark Matter

Authors :
Pierre Brun
Laurent Chevalier
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Source :
PoS, 2nd World Summit on Exploring the Dark Side of the Universe, 2nd World Summit on Exploring the Dark Side of the Universe, Jun 2018, Point a Pitre, France. pp.020, ⟨10.22323/1.335.0020⟩
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

International audience; The absence of observation of dark matter candidates above the GeV scale, at the LHC and in dedicated WIMP search experiments, led physicists to explore other mass domains, in particular below the electron-volt. Beside, the so-called strong CP problem is still an issue in the standard model. It can be solved by adding a new scalar field called axion. This scalar field could be a dark matter candidate. Depending of its coupling and in the range of mass ≈ [10^{−22},1] eV, it may solve the two issues described above at once. After the description of the strong CP problem and its simplest solution, I briefly present some mass limits for axions and similar fields (Axion Like Particle, Hidden Photon) and some of the experiments from which these limits have been extracted. At the end of this document, new limits on Hidden Photon are presented with a new experiment: Shuket.

Details

Language :
English
Database :
OpenAIRE
Journal :
PoS, 2nd World Summit on Exploring the Dark Side of the Universe, 2nd World Summit on Exploring the Dark Side of the Universe, Jun 2018, Point a Pitre, France. pp.020, ⟨10.22323/1.335.0020⟩
Accession number :
edsair.doi.dedup.....140a04e6df17322ef5d07b7f6920ccf9