Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Oliva Alberto"'
Autor:
Palma, Francesco, Martucci, Matteo, Neubüser, Coralie, Sotgiu, Alessandro, Follega, Francesco Maria, Ubertini, Pietro, Bazzano, Angela, Rodi, James, Ammendola, Roberto, Badoni, Davide, Bartocci, Simona, Battiston, Roberto, Beolè, Stefania, Bertello, Igor, Burger, William Jerome, Campana, Donatella, Cicone, Antonio, Cipollone, Piero, Coli, Silvia, Conti, Livio, Contin, Andrea, Cristoforetti, Marco, D'Angelo, Giulia, De Angelis, Fabrizio, De Donato, Cinzia, De Santis, Cristian, Diego, Piero, Di Luca, Andrea, Fiorenza, Emiliano, Gebbia, Giuseppe, Iuppa, Roberto, Lega, Alessandro, Lolli, Mauro, Martino, Bruno, Masciantonio, Giuseppe, Mergè, Matteo, Mese, Marco, Morbidini, Alfredo, Nozzoli, Francesco, Nuccilli, Fabrizio, Oliva, Alberto, Osteria, Giuseppe, Palmonari, Federico, Panico, Beatrice, Papini, Emanuele, Parmentier, Alexandra, Perciballi, Stefania, Perfetto, Francesco, Perinelli, Alessio, Picozza, Piergiorgio, Piersanti, Mirko, Pozzato, Michele, Rebustini, Gianmaria, Recchiuti, Dario, Ricci, Ester, Ricci, Marco, Ricciarini, Sergio Bruno, Russi, Andrea, Sahnoun, Zouleikha, Savino, Umberto, Scotti, Valentina, Shen, Xuhui, Sparvoli, Roberta, Tofani, Silvia, Vertolli, Nello, Vilona, Veronica, Vitale, Vincenzo, Zannoni, Ugo, Zeren, Zhima, Zoffoli, Simona, Zuccon, Paolo
In this paper we report the detection of five strong Gamma-Ray Bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satellite (CSES-01), operational since 2018 on a Sun-synchronous polar orbit
Externí odkaz:
http://arxiv.org/abs/2310.16670
Autor:
Oliva Alberto
Publikováno v:
EPJ Web of Conferences, Vol 208, p 13002 (2019)
The Alpha Magnetic Spectrometer (AMS-02) is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and operating continuously since then. With a collection rate of approximately 1.7 × 1010 events/ye
Externí odkaz:
https://doaj.org/article/94c7ee9beaba4445ad0eff782674fbbc
Autor:
Bonifazi, Gianluca, Lista, Luca, Menasce, Dario, Mezzetto, Mauro, Oliva, Alberto, Pedrini, Daniele, Spighi, Roberto, Zoccoli, Antonio
We analyze the data about casualties in Italy in the period 01/01/2015 to 30/09/2020 released by the Italian National Institute of Statistics (ISTAT). The data exhibit a clear sinusoidal behavior, whose fit allows for a robust subtraction of the base
Externí odkaz:
http://arxiv.org/abs/2102.01629
Autor:
Raïch-Regué, Dalia, Tenorio, Raquel, Fernández de Castro, Isabel, Tarrés-Freixas, Ferran, Sachse, Martin, Perez-Zsolt, Daniel, Muñoz-Basagoiti, Jordana, Fernández-Sánchez, Sara Y., Gallemí, Marçal, Ortega-González, Paula, Fernández-Oliva, Alberto, Gabaldón, José A., Nuñez-Delicado, Estrella, Casas, Josefina, Roca, Núria, Cantero, Guillermo, Pérez, Mónica, Usai, Carla, Lorca-Oró, Cristina, Alert, Júlia-Vergara, Segalés, Joaquim, Carrillo, Jorge, Blanco, Julià, Clotet Sala, Bonaventura, Cerón-Carrasco, José P., Izquierdo-Useros, Nuria, Risco, Cristina
Publikováno v:
In Biomedicine & Pharmacotherapy August 2023 164
Publikováno v:
Res. Notes AAS 1 (2017) 35
The Alpha Magnetic Spectrometer (AMS) experiment has released new measurements of primary and secondary nuclei in cosmic rays at the TeV energy scale. Using these data, we present new results based on a global Bayesian analysis of our two halo model
Externí odkaz:
http://arxiv.org/abs/1712.03176
Autor:
Tomassetti, Nicola, Oliva, Alberto
Antimatter nuclei in cosmic rays (CR) represent a promising discovery channel for the indirect search of dark matter. We present astrophysical background calculations of CR antideuteron ($\overline{d}$) and antihelium ($\overline{He}$). These particl
Externí odkaz:
http://arxiv.org/abs/1712.03177
Antimatter nuclei in cosmic rays (CRs) are a promising tool for the indirect detection of dark-matter annihilation signatures. However, the search of new-physics signals in CRs relies on our knowledge of the astrophysical antimatter background which,
Externí odkaz:
http://arxiv.org/abs/1707.06918
Autor:
Tomassetti, Nicola, Oliva, Alberto
We compute the spectra of cosmic-ray (CR) nuclei and antinuclei under a scenario where hadronic interaction processes inside supernova remnants (SNRs) can produce a diffusively-shock-accelerated "source component" of secondary particles. This scenari
Externí odkaz:
http://arxiv.org/abs/1707.06919
Autor:
Tomassetti, Nicola, Oliva, Alberto
Publikováno v:
Astrophysical Journal Letters 844 (2017) L26
We compute the energy spectra of antideuterons and antihelium in cosmic rays (CRs) in a scenario where hadronic interactions inside supernova remnants (SNRs) can produce a diffusively-shock-accelerated "source component" of secondary antinuclei. The
Externí odkaz:
http://arxiv.org/abs/1707.06915
The antiparticle energy spectra of Galactic cosmic rays (CRs) have several exciting features such as the unexpected positron excess at $E\sim$10-200\,GeV and the remarkably hard antiproton flux at $E\sim$\,60--450\,GeV recently measured by the \AMS{}
Externí odkaz:
http://arxiv.org/abs/1612.08520