Literatura académica sobre el tema "Cosmic-ray phenomenology"
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Artículos de revistas sobre el tema "Cosmic-ray phenomenology"
Uchaikin, V. V. "Fractional phenomenology of cosmic ray anomalous diffusion". Physics-Uspekhi 56, n.º 11 (30 de noviembre de 2013): 1074–119. http://dx.doi.org/10.3367/ufne.0183.201311b.1175.
Texto completoUchaikin, Vladimir V. "Fractional phenomenology of cosmic ray anomalous diffusion". Uspekhi Fizicheskih Nauk 183, n.º 11 (2013): 1175–223. http://dx.doi.org/10.3367/ufnr.0183.201311b.1175.
Texto completoRecchia, Sarah. "Cosmic ray driven galactic winds". International Journal of Modern Physics D 29, n.º 07 (mayo de 2020): 2030006. http://dx.doi.org/10.1142/s0218271820300062.
Texto completoStenkin, Yu V. "EAS Phenomenology and Cosmic Ray Spectrum Ground Based Measurements". Physics of Atomic Nuclei 82, n.º 6 (noviembre de 2019): 808–11. http://dx.doi.org/10.1134/s1063778819660475.
Texto completoMorlino, Giovanni. "Supernova Remnant-Cosmic Ray connection: a modern view". Proceedings of the International Astronomical Union 12, S331 (febrero de 2017): 230–41. http://dx.doi.org/10.1017/s1743921317004793.
Texto completoJaupart, Étienne, Étienne Parizot y Denis Allard. "Contribution of the Galactic centre to the local cosmic-ray flux". Astronomy & Astrophysics 619 (noviembre de 2018): A12. http://dx.doi.org/10.1051/0004-6361/201833683.
Texto completoBahia, Carlos A. S., Mateus Broilo y Emerson G. S. Luna. "Regge Phenomenology at LHC Energies". International Journal of Modern Physics: Conference Series 45 (enero de 2017): 1760064. http://dx.doi.org/10.1142/s2010194517600643.
Texto completoBARBIERI, JAMES, GEORGE CHAPLINE y DAVID I. SANTIAGO. "QUANTUM CRITICALITY, EVENT HORIZONS AND COSMIC GAMMA RAY BURSTS". Modern Physics Letters A 18, n.º 39 (21 de diciembre de 2003): 2767–73. http://dx.doi.org/10.1142/s0217732303012489.
Texto completoAnchordoqui, Luis, María Teresa Dova, Analisa Mariazzi, Thomas McCauley, Thomas Paul, Stephen Reucroft y John Swain. "High energy physics in the atmosphere: phenomenology of cosmic ray air showers". Annals of Physics 314, n.º 1 (noviembre de 2004): 145–207. http://dx.doi.org/10.1016/j.aop.2004.07.003.
Texto completoDiesing, Rebecca y Damiano Caprioli. "Steep Cosmic-Ray Spectra with Revised Diffusive Shock Acceleration". Astrophysical Journal 922, n.º 1 (1 de noviembre de 2021): 1. http://dx.doi.org/10.3847/1538-4357/ac22fe.
Texto completoTesis sobre el tema "Cosmic-ray phenomenology"
Fornieri, Ottavio. "Cosmic-ray transport in the Milky Way and related phenomenology". Doctoral thesis, Università di Siena, 2021. http://hdl.handle.net/11365/1143115.
Texto completoGiesen, Gaelle. "Dark Matter Indirect Detection with charged cosmic rays". Thesis, Paris 11, 2015. http://www.theses.fr/2015PA112160/document.
Texto completoOverwhelming evidence for the existence of Dark Matter (DM), in the form of an unknownparticle filling the galactic halos, originates from many observations in astrophysics and cosmology: its gravitational effects are apparent on galactic rotations, in galaxy clusters and in shaping the large scale structure of the Universe. On the other hand, a non-gravitational manifestation of its presence is yet to be unveiled. One of the most promising techniques is the one of indirect detection, aimed at identifying excesses in cosmic ray fluxes which could possibly be produced by DM annihilations or decays in the Milky Way halo. The current experimental efforts mainly focus in the GeV to TeV energy range, which is also where signals from WIMPs (Weakly Interacting Massive Particles) are expected. Focussing on charged cosmic rays, in particular antiprotons, electrons and positrons, as well as their secondary emissions, an analysis of current and forseen cosmic ray measurements and improvements on astrophysical models are presented. Antiproton data from PAMELA imposes contraints on annihilating and decaying DM which are similar to (or even slightly stronger than) the most stringent bounds from gamma ray experiments, even when kinetic energies below 10 GeV are discarded. However, choosing different sets of astrophysical parameters, in the form of propagation models and halo profiles, allows the contraints to span over one or two orders of magnitude. In order to exploit fully the power of antiprotons to constrain or discover DM, effects which were previously perceived as subleading turn out to be relevant especially for the analysis of the newly released AMS-02 data. In fact, including energy losses, diffusive reaccelleration and solar modulation can somewhat modify the current bounds, even at large DM masses. A wrong interpretation of the data may arise if they are not taken into account. Finally, using the updated proton and helium fluxes just released by the AMS-02 experiment, the astrophysical antiproton to proton ratio and its uncertainties are reevaluated and compared to the preliminarly reported AMS-02 measurements. No unambiguous evidence for a significant excess with respect to expectations is found. Yet, some preference for thicker halos and a flatter energy dependence of the diffusion coefficient starts to emerge. New stringed constraints on DM annihilation and decay are derived. Secondary emissions from electrons and positrons can also be used to constrain DM annihilation or decay in the galactic halo. The radio signal due to synchrotron radiation of electrons and positrons on the galactic magnetic field, gamma rays from bremsstrahlung processes on the galactic gas densities and from Inverse Compton scattering processes on the interstellar radiation field are considered. With several magnetic field configurations, propagation scenarios and improved gas density maps and interstellar radiation field, state-of-art tools allowing the computaion of synchrotron and bremssttrahlung radiation for any WIMP DM model are provided. All numerical results for DM are incorporated in the release of the Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID). Finally, the possible GeV gamma-ray excess identified in the Fermi-LAT data from the Galactic Center in terms of DM annihilation, either in hadronic or leptonic channels is studied. In order to test this tantalizing interprestation, a multi-messenger approach is used: first, the computation of secondary emisison from DM with respect to previous works confirms it to be relevant for determining the DM spectrum in leptonic channels. Second, limits from antiprotons severely constrain the DM interpretation of the excess in the hadronic channel, for standard assumptions on the Galactic propagation parameters and solar modulation. However, they considerably relax if more conservative choices are adopted
Actas de conferencias sobre el tema "Cosmic-ray phenomenology"
DOVA, MARIA TERESA. "PHENOMENOLOGY OF COSMIC RAY AIR SHOWERS". En Proceedings of the Fifth International Workshop. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812774439_0005.
Texto completoCheek, Andrew, Suzan Basegmez du Pree, Chiara Arina, Marco Chianese, Ariane Dekker y Shin’ichiro Ando. "Dark Matter Phenomenology from Upcoming Neutrino Telescopes:". En 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0550.
Texto completoFornieri, Ottavio, Daniele Gaggero, Silvio Sergio Cerri, Pedro De La Torre Luque y Stefano Gabici. "Phenomenology of CR-scattering on pre-existing MHD modes". En 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0426.
Texto completoCummings, Austin, Roberto Aloisio, Mario E. Bertaina, Francesca Bisconti, Francesco Fenu y Francesco Salamida. "A More Complete Phenomenology of Tau Lepton Induced Air Showers". En 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0862.
Texto completoWiklich Sobrinho, Rafaela y Marcelo Augusto Leigui de Oliveira. "Study of the phenomenology of the hadronic interactions in the reconstruction of extensive air showers". En 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0467.
Texto completoMészáros, P. "GAMMA-RAY BURST PHENOMENOLOGY IN THE SWIFT ERA". En Proceedings of the 15th Course of the International School of Cosmic Ray Astrophysics. WORLD SCIENTIFIC, 2007. http://dx.doi.org/10.1142/9789812790156_0002.
Texto completoHasegawa, S. y M. Tamada. "Cosmic-ray family phenomenology of visible energy greater than 500 TeV observed in high mountain emulsion chambers". En The seventh international symposium on very high energy cosmic-ray interactions. AIP, 1993. http://dx.doi.org/10.1063/1.43877.
Texto completoMAURIN, D. "USINE: a new public cosmic ray propagation code Basic phenomenology, sample results, and a bit of USINE". En Proceedings of the 12th ICATPP Conference. WORLD SCIENTIFIC, 2011. http://dx.doi.org/10.1142/9789814329033_0053.
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