Symmetry in Dark Matter and Cosmology
A special issue of Symmetry (ISSN 2073-8994). This special issue belongs to the section "Physics".
Deadline for manuscript submissions: closed (30 November 2023) | Viewed by 1754
Special Issue Editor
Interests: high-energy physics theory; beyond the standard model; baryon synthesis mechanism; dark matter
Special Issues, Collections and Topics in MDPI journals
Special Issue Information
Dear Colleagues,
Strong astrophysical and cosmological evidence on many scales indicates the existence of non-baryonic dark matter content in our Universe, which constitutes approximately 85 percent of the Universe’s matter density and 26 percent of its total energy density. Dark matter is generally believed to be new particles in new physics beyond the Standard Model, and these must be stable or have a much longer lifetime than the age of the Universe. Many theoretically well-motivated dark matter candidates have been proposed to explain the dark matter related astrophysical evidence, which possibly span an incredible mass range from 10−21 eV to above the Planck scale 1027 eV. Weakly interacting massive particles (WIMPs) between 1 GeV and 100 TeV that interact with the SM particles are the most promising dark matter candidates, for example, the lightest neutralino in supersymmetric (SUSY) models. Understanding the nature of dark matter and the search for dark matter signals are the most important tasks for particle physics and cosmology today.
In this Special Issue, we will focus on both the theoretical and experimental aspects of dark matter, including new proposals/candidates to explain the dark matter puzzle, the general theory and analysis of dark matter, the direct and indirect detections of dark matter particles, the constraints of DM from colliders, the connection of the DM to baryon asymmetry, dark matter related phenomenology, etc.
Prof. Dr. Fei Wang
Guest Editor
Manuscript Submission Information
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Keywords
- dark matter
- DM
- cosmology
- collider
- baryon asymmetry
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