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Secondary particles produced in spallation reactions of cosmic rays with the interstellar gas provide valuable information that allow us to investigate the injection and transport of charged particles in the Galaxy. A good understanding of…

High Energy Astrophysical Phenomena · Physics 2022-07-20 Pedro de la Torre Luque , Mario Nicola Mazziotta , Alfredo Ferrari , Francesco Loparco , Paola Sala , Davide Serini

Relativistic Runaway Electron Avalanches (RREA) are central to understanding a spectrum of high-energy atmospheric phenomena, including Terrestrial Gamma-ray Flashes (TGFs), Thunderstorm Ground Enhancements (TGEs), and gamma-ray glows.…

Atmospheric and Oceanic Physics · Physics 2025-06-24 A. Chilingarian

Calculation of secondary particles produced by the interaction of cosmic rays with the nuclei of Earth's atmosphere pose important requirements to particle production models. Here we summarize the important features of hadronic simulations,…

High Energy Physics - Phenomenology · Physics 2009-11-07 G. Battistoni , A. Ferrari , P. R. Sala

Various particle accelerators operate in the space plasmas, filling the Galaxy with high energy particles, primary cosmic rays. Reaching the atmosphere of the earth, these particles originate extensive air showers consisting of millions of…

High Energy Astrophysical Phenomena · Physics 2023-10-17 A. Chilingarian

Substantial fluxes of protons and leptons with energies below the geomagnetic cutoff have been measured by the AMS experiment at altitudes of 370-390 Km, in the latitude interval +/- 51.7 degrees. The production mechanisms of the observed…

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly relativistic jets emitted in core collapse supernova explosions (SNe). The result of the event, probably, is not just a compact object plus…

Astrophysics · Physics 2009-11-06 Arnon Dar

Relativistic flows resulting from sudden explosive events upscatter ambient interstellar photons of local radiation fields. For Lorentz factor $ > 100$ and dense optical - UV radiation fields the emergent signal is a typical gamma ray…

Astrophysics · Physics 2015-06-24 Amotz Shemi

High-energy gamma radiation in the Earth's atmosphere is associated with the bremsstrahlung of Relativistic Runaway Electron Avalanches (RREA) developing in thunderstorm electric fields. In this paper, RREA development is studied in the…

Atmospheric and Oceanic Physics · Physics 2023-01-03 Egor Stadnichuk , Daria Zemlianskaya , Ekaterina Svechnikova , Eduard Kim , Alexander Sedelnikov , Oraz Anuaruly

Star quakes and internal phase transitions within anomalous x-ray pulsars (AXPs) and soft $\gamma$-ray repeaters (SGRs) can produce mini contractions and pulsar glitches. Shocks break out from their surface following such contractions…

High Energy Astrophysical Phenomena · Physics 2020-10-21 Shlomo Dado , Arnon Dar

Extrasolar planets appear in a chemical diversity unseen in our own solar system. Despite their atmospheres being cold, continuous and transient plasma processes do affect these atmosphere where clouds form with great efficiency. Clouds can…

Solar and Stellar Astrophysics · Physics 2018-09-26 Ch. Helling , I. Vorgul

When a star undergoes core collapse, a vast amount of energy is released in a ~10 s long burst of neutrinos of all species. Inverse beta decay in the star's hydrogen envelope causes an electromagnetic cascade which ultimately results in a…

High Energy Astrophysical Phenomena · Physics 2024-08-06 Cecilia Lunardini , Joshua Loeffler , Mainak Mukhopadhyay , Matthew J. Hurley , Ebraheem Farag , F. X. Timmes

We study particle production in infrared-modified gravitational theories in the contemporary universe. It is shown that in astronomical systems with rising mass density, the curvature scalar may oscillate with very high frequency. These…

General Relativity and Quantum Cosmology · Physics 2015-06-16 E. V. Arbuzova , A. D. Dolgov , L. Reverberi

Clusters of galaxies and the large scale filaments that connect neighboring clusters are expected to be sites of acceleration of charged particles and sources of non-thermal radiation from radio frequencies to gamma rays. Gamma rays are…

Astrophysics · Physics 2009-11-13 Pasquale Blasi , Stefano Gabici , Gianfranco Brunetti

During solar flares fast electron beams generated in the solar corona are non-thermal radio sources in terms of type III bursts. Sometimes they can enter into the interplanetary space, where they can be observed by in-situ measurements as…

Solar and Stellar Astrophysics · Physics 2011-12-23 H. Önel , G. Mann , E. Sedlmayr

The measured fluxes of secondary particles produced by the interactions of Cosmic Rays (CRs) with the astronomical environment play a crucial role in understanding the physics of CR transport. In this work we present a comprehensive…

High Energy Astrophysical Phenomena · Physics 2017-03-06 M. N. Mazziotta , F. Cerutti , A. Ferrari , D. Gaggero , F. Loparco , P. R. Sala

This work presents a unified conceptual and observational framework that reinterprets these radiation bursts as manifestations of the same runaway processes happening at different atmospheric depths (Dual-stage model, DSM). We review recent…

Space Physics · Physics 2025-12-16 A. Chilingarian , L. Hovhannisyan , B. Sargsyan , M. Zazyan

The article is devoted to electromagnetic phenomena in the atmosphere. The set of experimental data on the thunderstorm activity is analyzed. It helps to identify a possible physical mechanism of lightning flashes. This mechanism can…

Plasma Physics · Physics 2024-02-07 S. N. Artekha , A. V. Belyan

We establish that the nonlinear dynamics of collisions between particles favors the charging of a insulating, friable, self-replicating granular material that undergoes nucleation, growth, and fission processes; we demonstrate with a…

The prompt emission of gamma-ray bursts (hereafter GRBs) probably comes from a highly relativistic wind which converts its kinetic energy into radiation via the formation of shocks within the wind itself. Such "internal shocks" can occur if…

Astrophysics · Physics 2007-05-23 Frederic Daigne , Robert Mochkovitch

Particle acceleration is expected to take place at shocks that form during the process of large scale structure formation. Electrons accelerated at such shocks can upscatter a small fraction of the photons in the cosmic microwave background…

Astrophysics · Physics 2007-05-23 Stefano Gabici