Dark Matter and Cosmic Rays
A special issue of J (ISSN 2571-8800). This special issue belongs to the section "Physical Sciences".
Deadline for manuscript submissions: closed (15 November 2022) | Viewed by 6658
Special Issue Editors
2. INFN Laboratori Nazionali di Frascati, Rome, Italy
Interests: nuclear physics; dark matter; self-gravitating systems; experimental and phenomenological quantum physics
Interests: astroparticle physics; dark matter; particle detectors
Special Issues, Collections and Topics in MDPI journals
Special Issue Information
Dear Colleagues,
Dark Matter presently represents one of the main challenges in several sectors of theoretical and experimental physics. Despite decades of efforts, the nature and origin of the Dark Matter component of the universe is still unknown. The lack of a direct hint about the physics of Dark Matter introduces a spread for the plausible masses and cross sections of the Dark Matter candidates, extending over many orders of magnitude. The demand for an intertwined multidisciplinary effort is evident, to deepen, on one side, the investigation of the vast scenario of possible candidates—presently ranging from WIMPSs to axions, from the broad zoology of Stable Massive Particles to objects arising as topological field configurations—and to improve, on the other side, the sensitivity of the experimental searches, which range from underground and accelerator tests, to the development of detector systems to be operated in space. Cosmic rays provide a plethora of information, a big effort being presently invested to unveil, in the cosmic ray flux, indirect signatures of Dark Matter physics, e.g., the annihilation or decay of dark matter particles. The analysis of the self-gravitational equilibrium of galactic halos, and the study of the collective relaxation mechanisms, can provide further constraints on the accessible mass ranges and the Dark Matter distribution.
This Special Issue aims at promoting original and high-quality papers on topics related to Dark Matter searches in particular relation with the physics of Cosmic Rays. The Guest Editors aim to stimulate an interdisciplinary debate, seeking papers on theoretical and experimental investigation of Dark Matter particle candidates, development of innovative detector systems and data analysis models, application of avant-garde Machine Learning techniques to the interpretation of the observational surveys, development of long-range interaction statistical models for studying the stability of self-gravitating systems as well as the short and large scale Dark Matter distribution.
We cordially invite you to submit a high-quality original research paper or review to this Special Issue, “Dark Matter and Cosmic Rays”.
Dr. Kristian Piscicchia
Dr. Francesco Nozzoli
Guest Editors
Manuscript Submission Information
Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All papers will be peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.
Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. J is an international peer-reviewed open access quarterly journal published by MDPI.
Please visit the Instructions for Authors page before submitting a manuscript. Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.
Keywords
- dark matter
- cosmic rays
- antimatter in cosmic rays
- galactic halos
- astroparticle physics
- large-scale structure of the universe
- supersymmetry
- complexity
Benefits of Publishing in a Special Issue
- Ease of navigation: Grouping papers by topic helps scholars navigate broad scope journals more efficiently.
- Greater discoverability: Special Issues support the reach and impact of scientific research. Articles in Special Issues are more discoverable and cited more frequently.
- Expansion of research network: Special Issues facilitate connections among authors, fostering scientific collaborations.
- External promotion: Articles in Special Issues are often promoted through the journal's social media, increasing their visibility.
- Reprint: MDPI Books provides the opportunity to republish successful Special Issues in book format, both online and in print.
Further information on MDPI's Special Issue policies can be found here.