Testing Fundamental QED and BSM Physics Theories in Leptonic and Hadronic Processes

A special issue of Particles (ISSN 2571-712X).

Deadline for manuscript submissions: 25 December 2024 | Viewed by 1595

Special Issue Editors


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Guest Editor
Theoretical Physics Section, University of Ioannina, GR 451 10 Ioannina, Greece
Interests: nuclear physics; nuclear astrophysics; neutrino physics; nuclear structure; muon physics; cold dark matter physics; purely leptonic atoms; micro-quasar jet emissions
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Guest Editor
Research Center for Nuclear Physics, Osaka University, Osaka 567-0047, Japan
Interests: experimental nuclear physics; muon physics; double beta decay; astroparticle physics; beyond the standard model physics; neutrino physics; astro-neutrinos; dark matter physics

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Guest Editor
Department of Physics, School of Sciences, University of Ioannina, GR 451 10 Ioannina, Greece
Interests: nuclear physics; double beta decay; particle physics; dark matter physics; cosmology; beyond the standard model physics; mathematical physics; group theory; lepton and lepton flavor violation; neutrino oscillation

Special Issue Information

*This Special Issue is dedicated to Dr. Eliahu Comay*

Dear Colleagues,

The aim of this Special Issue is to collect research articles focused on the current and future directions of electro-Weak, strong, and beyond the standard model (SM) Processes. In particular, the recent advances in beta and double beta decay modes, related processes in neutrino-nucleus (neutral current and charged current) reactions, as well as dark matter physics are welcome. Also, we welcome the submission of works focused on precision physics in purely leptonic atoms combined with accurate predictions deriving from advanced solutions of relevant fundamental differential equations.

Today, thanks to accumulated experimental and theoretical experience, it is widely known that a great portion of leptonic and hadronic processes cannot be fully interpreted within the standard model of electro-weak and strong interactions. Experimental verifications point to the necessity of going beyond the SM and investigating BSM processes. Towards achieving this aim, several double beta Decay experiments have taken data with enriched isotopes as the detection medium. The designed experiments plan to use ton-scale detectors of several isotopes and employ various detection techniques. Such experiments require the prediction of nuclear matrix elements with appreciable reliability and accuracy.

We aim for this Special Issue to include the complementary scientific areas of rare electroweak decays, neutrino properties, coherent elastic neutrino-nucleus scattering (CEvNS), and dark matter detection. BSM physics is searched through the lepton flavor violation (LFV) and charged-LFV (cLFV) with powerful probes as μ- to e±, etc.

This Special Issue invites contributions which focus on precision measurements in purely leptonic atoms as, e.g., the 1S-2S energy interval in the leptonic atom Mu (μ+e-), and the decay of the Ps (e+e-) atom capable of testing discrete symmetries.

Finally, since the wealth of available data in the above physics topics necessitate accurate predictions from physical theories (QED, BSM, etc.) governed by fundamental partial differential equations (PDEs), Schrödinger, Dirac, etc., research works on advanced solutions of these equations (physics-informed neural networks, etc.) are welcome.

Prof. Dr. Theocharis Kosmas
Prof. Dr. Hiroyasu Ejiri
Prof. Dr. John Vergados
Guest Editors

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Keywords

  • standard model of electroweak and strong interactions
  • beyond the standard model physics theories
  • beta and double beta decay modes
  • spectroscopy of purely leptonic atoms
  • the positronium as a probe of discrete symmetries
  • the muonium bound spectrum (theory and experiments)
  • neutral current neutrino-nucleus scattering (coherent and incoherent channel)
  • charge changing neutrino nucleus reactions
  • direct detection of dark matter
  • Physics Informed Neural Networks (PINNs) in Particle Physics

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Published Papers (1 paper)

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Research

16 pages, 900 KiB  
Article
Black Hole’s Spin-Dependence of γ-Ray and Neutrino Emissions from MAXI J1820+070, XTE J1550-564, and XTE J1859+226
by Dimitrios Rarras, Odysseas Kosmas, Theodora Papavasileiou and Theocharis Kosmas
Particles 2024, 7(3), 818-833; https://doi.org/10.3390/particles7030049 - 12 Sep 2024
Cited by 1 | Viewed by 837
Abstract
A black hole’s spin effects on the jet emissions of high-energy neutrinos and γ-rays from black hole X-ray binary systems (BHXRBs) are investigated. The BHXRBs consist of a stellar black hole, a companion (donor) star, a BH accretion disk, a BH corona, [...] Read more.
A black hole’s spin effects on the jet emissions of high-energy neutrinos and γ-rays from black hole X-ray binary systems (BHXRBs) are investigated. The BHXRBs consist of a stellar black hole, a companion (donor) star, a BH accretion disk, a BH corona, and two jets emitted from the black hole perpendicular to the accretion disk. For their description, properties of the accretion disk, specifically the accretion disk’s inner radius Rin and the accretion disk’s temperature profile T(R), play key roles since they depend on the black hole’s dimensionless spin parameter α. In this work, we focus on the main reaction mechanisms taking place inside jets from which high-energy γ-rays and neutrinos are created. The intensities and integral fluxes of neutrinos and γ-rays are obtained by integrating the respective source functions. Lastly, the γ-ray absorption due to e-e+ pair production is considered, particularly absorption from the accretion disk. For concrete applications, we have chosen the BHXRB systems MAXI J1820+070, XTE J1550-564, and XTE J1859+226. Full article
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Planned Papers

The below list represents only planned manuscripts. Some of these manuscripts have not been received by the Editorial Office yet. Papers submitted to MDPI journals are subject to peer-review.

 
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