Frontiers in Astroparticle Physics and Particle Cosmology

A special issue of Universe (ISSN 2218-1997).

Deadline for manuscript submissions: closed (30 September 2021) | Viewed by 2390

Special Issue Editors


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Guest Editor
1. Department of Physical Sciences, Earth and Environment, University of Siena, 53100 Siena, Italy
2. Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, 56127 Pisa, Italy
Interests: astroparticle physics; cosmic rays; development of detectors and instrumentation; experimental high-energy particle physics; data analysis; medical applications of radiation detectors

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Guest Editor
Max Planck Institute for Nuclear Physics, Heidelberg, Germany
Interests: CP violation; flavor physics; neutrino interactions; physics beyond the standard model; particle cosmology; strong CP problem; symmetries and outer automorphisms

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Guest Editor
Theoretical Physics Department, CERN, 1211 Geneva, Switzerland
Interests: Beyond Standard Model physics; cosmology and astroparticle physics; gravitational wave particle physics

Special Issue Information

Dear Colleagues,

The cosmos provides us with a continuous influx of cosmic rays ranging from the tiniest quanta of energy, such as the yet undetected cosmic background neutrinos, up to the most energetic single-particle events ever observed by humanity. In this rising age of gravitational wave observatories, neutrino telescopes, and exquisitely precise photon detectors, it is essential that we exploit this information through a truly interdisciplinary approach to multi-messenger astronomy. This entails an enormous spectrum of new opportunities across all frontiers, ranging from the exploration and characterization of cosmic sources, charting the decomposition, origin, and evolution of the universe all the way to the exploration of elementary particle properties themselves.

Important lessons are to be learned, for example, about our cosmic neighborhood, the spectrum of binary black holes, as well as the possibility of primordial black holes as well motivated candidates for astrophysical dark matter. At the same time, particle dark matter searches are running with unprecedented sensitivities and will soon reach the neutrino floor, allowing for detection of coherent elastic neutrino-nucleus scattering. Furthermore, a new stage of cosmic microwave background experiments will afford probes of cosmic inflation, primordial gravitational waves, and novel dark sectors which have the ability to provide crucial insights into scenarios of grand unification, string theory, and extra dimensions.

All of which live at scales out of the reach of any future Earth-based collider.

Altogether, the unique laboratory of particle cosmology offers extraordinary possibilities for particle physics at all scales, allowing us to address the most profound questions we have about nature, such as the origin of matter and dark matter, the cosmological Hubble tension, the large separation of electroweak and Planck scales, as well as the origin and size of neutrino masses.

This Special Issue is open to contributions on all frontiers of particle cosmology in and beyond the standard models of both particle physics and cosmology. We are especially welcoming of new and groundbreaking ideas, formal and phenomenological considerations, as well as contributions aiding efforts in ongoing observations and experiments.

Dr. Paolo Maestro
Dr. Andreas Trautner
Dr. Toby Opferkuch
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 submissions that pass pre-check are 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. Universe is an international peer-reviewed open access monthly 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

  • gravitational waves
  • black holes
  • dark matter
  • beyond the standard model
  • cosmic neutrinos

Published Papers (1 paper)

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Research

18 pages, 1306 KiB  
Article
Perspective of Direct Search for Dark Components in the Universe with Multi-Wavelengths Stimulated Resonant Photon-Photon Colliders
by Kensuke Homma, Yuri Kirita and Fumiya Ishibashi
Universe 2021, 7(12), 479; https://0-doi-org.brum.beds.ac.uk/10.3390/universe7120479 - 06 Dec 2021
Cited by 3 | Viewed by 1862
Abstract
We explore a possibility to detect dark components in the Universe via stimulated photon–photon collisions by focusing two-frequency coherent electromagnetic fields in a vacuum. Those fields are assumed to be pulsed reaching Fourier transform limits in near-infrared, THz, and GHz frequency bands, respectively. [...] Read more.
We explore a possibility to detect dark components in the Universe via stimulated photon–photon collisions by focusing two-frequency coherent electromagnetic fields in a vacuum. Those fields are assumed to be pulsed reaching Fourier transform limits in near-infrared, THz, and GHz frequency bands, respectively. The numbers of signal photons as a result of exchange of a pseudoscalar-type pseudo Nambu–Goldstone boson have been evaluated in the individual frequency bands. Within presently available beam intensities, we found that the QCD axion scenarios are thoroughly testable in the mass range 106100 eV based on the common method. Furthermore, we show a possibility to reach the weak coupling domain even beyond the gravitationally weak coupling strength if pulse compression in the GHz band is realized in the near future development. Full article
(This article belongs to the Special Issue Frontiers in Astroparticle Physics and Particle Cosmology)
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