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The shape of the longitudinal development of the showers generated in the atmosphere by very high energy cosmic ray particles encodes information about the mass composition of the flux, and about the properties of hadronic interactions that…

High Energy Astrophysical Phenomena · Physics 2021-05-19 Paolo Lipari

We perform numerical simulations on the merger of multiple black holes (BHs) in primordial gas at early cosmic epochs. We consider two cases of BH mass: $M_{BH} = 30 M_{\odot}$ and $M_{BH} = 10^4 M_{\odot}$. Attention is concentrated on the…

Astrophysics of Galaxies · Physics 2015-05-14 Hiromichi Tagawa , Masayuki Umemura , Naoteru Gouda , Taihei Yano , Yuki Yamai

Air shower simulation programs are essential tools for the analysis of data from cosmic ray experiments and for planning the layout of new detectors. They are used to estimate the energy and mass of the primary particle. Unfortunately the…

Astrophysics · Physics 2009-11-07 J. Knapp , D. Heck , S. J. Sciutto , M. T. Dova , M. Risse

Large surface detectors might be sensitive not only with respect to extensive air showers induced by ultra high energy neutrinos but also to showers induced by hypothetical objects like microscopic black-holes. Microscopic black-holes might…

High Energy Astrophysical Phenomena · Physics 2009-06-17 D. Gora , M. Haag , M. Roth

Primordial Black Holes (PBHs) are hypothetical black holes predicted to have been formed from density fluctuations in the early Universe. PBHs with an initial mass around $10^{14}-10^{15}$g are expected to end their evaporation at present…

High Energy Astrophysical Phenomena · Physics 2023-05-10 H. E. S. S. collaboration , : , F. Aharonian , F. Ait Benkhali , J. Aschersleben , M. Boettcher , M. Backes , V. Barbosa Martins , R. Batzo , Y. Becherini , D. Berge , B. Bi , C. Boisson , J. Bolmont , M. de Bony de Lavergne , J. Borowska , F. Bradascio , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , S. Caro , S. Casanova , J. Celic , M. Cerruti , T. Chand , A. Chen , O. Chibueze , G. Cotter , J. Damascene Mbarubucyeye , A. Djannati-Atai , K. Egberts , C. van Eldik , J. -P. Ernenwein , M. Fussling , A. Fiasson , G. Fichet de Clairfontaine , G. Fontaine , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , G. Grolleron , M. -H. Grondin , L. Haerer , M. Haupt , J. A. Hinton , W. Hofmann , M. Holler , D. Horns , Zhiqiu Huang , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynski , B. Khelifi , S. Klepser , W. Kluzniak , Nu. Komin , K. Kosack , D. Kostunin , T. L. Holch , R. G. Lang , S. Le Stum , F. Leitl , A. Lemiere , J. -P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , V. Marandon , P. Marchegiani , P. Marinos , G. Marti-Devesa , R. Marx , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , J. Muller , K. Nakashima , M. de Naurois , J. Niemiec , P. O'Brien , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , G. Puehlhofer , S. Panny , M. Panter , R. D. Parsons , G. Peron , A. Priyana Noel , D. A. Prokhorov , H. Prokoph , M. Punch , A. Quirrenbach , P. Reichherzer , O. Reimer , F. Rieger , G. Rowell , B. Rudak , H. Rueda Ricarte , V. Sahakian , H. Salzmann , D. A. Sanchez , A. Santangelo , M. Sasaki , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , H. Sol , A. Specovius , S. Spencer , L. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , T. Tavernier , C. Thorpe-Morgan , N. Tsuji , Y. Uchiyama , M. Vecchi , J. Veh , C. Venter , J. Vink , S. J. Wagner , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , A. Zech , S. Zouari , N. Zywucka

Light primordial black holes (PBHs) may have originated in the early Universe, and could contribute to the dark matter in the Universe. Their Hawking evaporation into particles could eventually lead to the production of antinuclei, which…

High Energy Physics - Phenomenology · Physics 2025-09-04 Valentina De Romeri , Fiorenza Donato , David Maurin , Lorenzo Stefanuto , Agnese Tolino

High energy neutrinos play a very important role for the understanding of the origin and propagation of ultra high energy cosmic rays (UHECR). They can be produced as a consequence of the hadronic interactions suffered by the cosmic rays in…

Instrumentation and Methods for Astrophysics · Physics 2015-05-27 A. D. Supanitsky , G. Medina-Tanco

Any considerations on propagation of particles through the Universe must involve particle interactions: processes leading to production of particle cascades. While one expects existence of such cascades, the state of the art cosmic-ray…

The origin of ultrahigh-energy cosmic rays (UHECRs) is a half-century old enigma (Linsley 1963). The mystery has been deepened by an intriguing coincidence: over ten orders of magnitude in energy, the energy generation rates of UHECRs, PeV…

High Energy Astrophysical Phenomena · Physics 2018-10-16 Ke Fang , Kohta Murase

Cosmic rays are charged relativistic particles that reach the Earth with extremely high energies, providing striking evidence of the existence of effective accelerators in the Universe. Below an energy around $\sim 10^{17}$ eV cosmic rays…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Giovanni Morlino

We describe a method to analyse inclined air showers produced by ultra high energy cosmic rays using an analytical description of the muon densities. We report the results obtained using data from inclined events…

Astrophysics · Physics 2009-11-07 M. Ave , J. A. Hinton , R. A. Vazquez , A. A. Watson , E. Zas

Extensive air showers are complex objects, resulting of billions of particle reactions initiated by single cosmic ray at ultra-high-energy. Their characteristics are sensitive both to the mass of the primary cosmic ray and to the details of…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Lorenzo Cazon

The discovery of the Higgs boson marks a key ingredient to establish the electroweak structure of the Standard Model. Its non-abelian gauge structure gives rise to, yet unobserved, non-perturbative baryon and lepton number violating…

High Energy Physics - Phenomenology · Physics 2016-09-21 Gustaaf Brooijmans , Peter Schichtel , Michael Spannowsky

Various mechanisms have been suggested for the formation of Primordial Black Holes (PBHs), and this thesis focuses on the standard mechanism based on the critical collapse of cosmological fluctuations. The underlying idea is that during…

Cosmology and Nongalactic Astrophysics · Physics 2025-01-07 Antonio Junior Iovino

Cosmic Rays (CR) impinging on the terrestrial atmosphere provide a viable opportunity to study new physics in hadron-nucleus collisions at energies covering many orders of magnitude, including a regime well beyond LHC energies. The…

High Energy Physics - Phenomenology · Physics 2022-09-21 Oliver Fischer , Maximilian Reininghaus , Ralf Ulrich

Supermassive black hole (SMBH) growth plausibly occurs via runaway astrophysical black hole mergers in nuclear star clusters that form intermediate mass black hole seeds at high redshifts. Such a model yields an order-of-magnitude higher…

High Energy Astrophysical Phenomena · Physics 2026-03-18 Konstantinos Kritos , Joseph Silk

Supermassive black holes and intermediate mass black holes are believed to exist in the Universe. There is no established astrophysical explanation for their origin and considerations have been made in the literature that those massive…

Cosmology and Nongalactic Astrophysics · Physics 2014-10-17 Kazunori Kohri , Tomohiro Nakama , Teruaki Suyama

Many cosmological phenomena lead to the production of primordial black holes in the early Universe. These phenomena often create a population of black holes with extended mass and spin distributions. As these black holes evaporate via…

High Energy Physics - Phenomenology · Physics 2025-01-10 Andrew Cheek , Lucien Heurtier , Yuber F. Perez-Gonzalez , Jessica Turner

In these two lectures, we will address the topic of the creation of small black holes during particle collisions in a ground-based accelerator, such as LHC, in the context of a higher-dimensional theory. We will cover the main assumptions,…

High Energy Physics - Theory · Physics 2009-02-16 Panagiota Kanti

We investigate the physical mechanism of the GZ-effect that could explain the production of multiple primaries from an event initiated outside the Earth's atmosphere. In this case, there would correspondingly be multiple extensive air…

Astrophysics · Physics 2007-05-23 Giovanni Imponente , Gabriella Sartorelli
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