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 5026

Special Issue Editors


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Guest Editor
1. Centro Ricerche Enrico Fermi—Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Roma, Italy
2. INFN Laboratori Nazionali di Frascati, Rome, Italy
Interests: nuclear physics; dark matter; self-gravitating systems; experimental and phenomenological quantum physics

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Guest Editor
INFN-TIFPA, I-38123 Trento, Italy
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 

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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.

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Keywords

  • dark matter
  • cosmic rays
  • antimatter in cosmic rays
  • galactic halos
  • astroparticle physics
  • large-scale structure of the universe
  • supersymmetry
  • complexity

Published Papers (2 papers)

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Research

16 pages, 407 KiB  
Article
Pulsar Wind Nebulae and Unidentified Galactic Very High Energy Sources
by Omar Tibolla, Sarah Kaufmann and Paula Chadwick
J 2022, 5(3), 318-333; https://0-doi-org.brum.beds.ac.uk/10.3390/j5030022 - 19 Jul 2022
Viewed by 1834
Abstract
The riddle of the origin of Cosmic Rays (CR) has been an open question for over a century. Gamma ray observations above 100 MeV reveal the sites of cosmic ray acceleration to energies where they are unaffected by solar modulation; recent evidence supports [...] Read more.
The riddle of the origin of Cosmic Rays (CR) has been an open question for over a century. Gamma ray observations above 100 MeV reveal the sites of cosmic ray acceleration to energies where they are unaffected by solar modulation; recent evidence supports the existence of hadronic acceleration in Supernova Remnants (SNR), as expected in the standard model of cosmic ray acceleration. Nevertheless, the results raise new questions, and no final answer has been provided thus far. Among the suggested possible alternative accelerators in the Very High Energy (VHE) gamma ray sky, pulsar wind nebulae (PWNe, which together with dark matter are the main candidates to explain the local positron excess as well) are the dominant population among known Galactic sources. However, the most numerous population in absolute terms is represented by unidentified sources (~50% of VHE gamma ray sources). The relationship between PWNe and unidentified sources seems very close; in fact, in a PWN, the lifetime of inverse Compton (IC) emitting electrons not only exceeds the lifetime of its progenitor pulsar, but also exceeds the age of the electrons that emit via synchrotron radiation. Therefore, during its evolution, a PWN can remain bright in IC such that its GeV-TeV gamma ray flux remains high for timescales much larger than the lifetimes of the pulsar and the X-ray PWN. In addition, the shell-type remnant of the supernova explosion in which the pulsar was formed has a much shorter lifetime than the electrons responsible for IC emission. Hence, understanding PWNe and VHE unidentified sources is a crucial piece of the solution to the riddle of the origin of cosmic rays. Both theoretical aspects (with particular emphasis on the ancient pulsar wind nebulae scenario) and their observational proofs are discussed in this paper. Specifically, the scientific cases of HESS J1616-508 and HESS J1813-126 are examined in detail. Full article
(This article belongs to the Special Issue Dark Matter and Cosmic Rays)
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11 pages, 1509 KiB  
Article
Search for Multi-Coincidence Cosmic Ray Events over Large Distances with the EEE MRPC Telescopes
by Marcello Abbrescia, Carlo Avanzini, Luca Baldini, Rinaldo Baldini Ferroli, Giovanni Batignani, Marco Battaglieri, Stefano Boi, Edoardo Bossini, Francesca Carnesecchi, Corrado Cicalò, Luisa Cifarelli, Fabrizio Coccetti, Eugenio Coccia, Alessandro Corvaglia, Daniele De Gruttola, Salvatore De Pasquale, Franco Fabbri, Lorenzo Galante, Marco Garbini, Gianluca Gemme, Ivan Gnesi, Stefano Grazzi, Despina Hatzifotiadou, Paola La Rocca, Zhang Liu, Giuseppe Mandaglio, Gaetano Maron, Mario Nicola Mazziotta, Alice Mulliri, Rosario Nania, Francesco Noferini, Francesco Nozzoli, Federico Palmonari, Marco Panareo, Maria Paola Panetta, Riccardo Paoletti, Carmelo Pellegrino, Ombretta Pinazza, Chiara Pinto, Silvia Pisano, Francesco Riggi, Giancarlo Righini, Cristina Ripoli, Matteo Rizzi, Gabriella Sartorelli, Eugenio Scapparone, Marco Schioppa, Angelo Scribano, Marco Selvi, Gabriella Serri, Sandro Squarcia, Marco Taiuti, Giuseppe Terreni, Antonio Trifirò, Marina Trimarchi, Cristina Vistoli, Lucia Votano, Crispin Williams, Antonino Zichichi and Roman Zuyeuskiadd Show full author list remove Hide full author list
J 2021, 4(4), 838-848; https://0-doi-org.brum.beds.ac.uk/10.3390/j4040057 - 01 Dec 2021
Cited by 1 | Viewed by 2439
Abstract
The existence of independent, yet time correlated, Extensive Air Showers (EAS) has been discussed over the past years, with emphasis on possible physical mechanisms that could justify their observation. The detector network of the Extreme Energy Events (EEE) Collaboration, with its approximately 60 [...] Read more.
The existence of independent, yet time correlated, Extensive Air Showers (EAS) has been discussed over the past years, with emphasis on possible physical mechanisms that could justify their observation. The detector network of the Extreme Energy Events (EEE) Collaboration, with its approximately 60 cosmic ray telescopes deployed over the Italian territory, has the potential to search for such events, employing different analysis strategies. In this paper, we have analyzed a set of EEE data, corresponding to an approximately five month observation period, searching for multi-coincidence events among several far telescopes, within a time window of 1 ms. Events with up to 12 coincident telescopes have been observed. Results were compared to expectations from a random distribution of events and discussed with reference to the relativistic dust grain hypothesis. Full article
(This article belongs to the Special Issue Dark Matter and Cosmic Rays)
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