Zobrazeno 1 - 10
of 156
pro vyhledávání: '"Mauro, Mattia"'
Autor:
Manconi, Silvia, Woo, Jooyun, Shang, Ruo-Yu, Krivonos, Roman, Tang, Claudia, Di Mauro, Mattia, Donato, Fiorenza, Mori, Kaya, Hailey, Charles J.
Geminga is the first pulsar around which a remarkable TeV gamma-ray halo extending over a few degrees was discovered by MILAGRO, HAWC and later by H.E.S.S., and by Fermi-LAT in the GeV band. More middle-aged pulsars have exhibited gamma-ray halos, an
Externí odkaz:
http://arxiv.org/abs/2403.10902
Autor:
Arina, Chiara, Di Mauro, Mattia, Fornengo, Nicolao, Heisig, Jan, Jueid, Adil, de Austri, Roberto Ruiz
The energy spectra of particles produced from dark matter (DM) annihilation or decay are one of the fundamental ingredients to calculate the predicted fluxes of cosmic rays and radiation searched for in indirect DM detection. We revisit the calculati
Externí odkaz:
http://arxiv.org/abs/2312.01153
We employ a data-driven approach to investigate the rigidity and spatial dependence of the diffusion of cosmic rays in the turbulent magnetic field of the Milky Way. Our analysis combines data sets from the experiments Voyager, AMS-02, CALET, and DAM
Externí odkaz:
http://arxiv.org/abs/2311.17150
Autor:
McDaniel, Alex, Ajello, Marco, Karwin, Christopher M., Di Mauro, Mattia, Drlica-Wagner, Alex, Sanchez-Conde, Miguel A.
The Milky Way (MW) dwarf spheroidal satellite galaxies (dSphs) are particularly intriguing targets to search for gamma rays from Weakly Interacting Massive Particle (WIMP) dark matter (DM) annihilation or decay. They are nearby, DM-dominated, and lac
Externí odkaz:
http://arxiv.org/abs/2311.04982
The singlet scalar Higgs portal model provides one of the simplest explanations of dark matter in our Universe. Its Higgs resonant region, $m_\text{DM}\approx m_h/2$, has gained particular attention, being able to reconcile the tension between the re
Externí odkaz:
http://arxiv.org/abs/2305.11937
Publikováno v:
Phys. Rev. D 108, 063024, 2023
The Galactic flux of cosmic-ray (CR) positrons in the GeV to TeV energy range is very likely due to different Galactic components. One of these is the inelastic scattering of CR nuclei with the atoms of the interstellar medium. The precise amount of
Externí odkaz:
http://arxiv.org/abs/2304.01261
Clusters of galaxies are the largest gravitationally-bound systems in the Universe. Their dynamics are dominated by dark matter (DM), which makes them among the best targets for indirect DM searches. We analyze 12 years of data collected by the Fermi
Externí odkaz:
http://arxiv.org/abs/2303.16930
Publikováno v:
Phys. Rev. D (2023) 107, 083031
The flux of $\gamma$ rays is measured with unprecedented accuracy by the $\textit{Fermi}$ Large Area Telescope from 100 MeV to almost 1 TeV. In the future, the Cherenkov Telescope Array will have the capability to measure photons up to 100 TeV. To ac
Externí odkaz:
http://arxiv.org/abs/2302.01943
Satellite galaxies of the Milky Way with high mass-to-light ratios and little baryon content, i.e. dwarf spheroidal galaxies (dSphs), are among the most promising targets to detect or constrain the nature of dark matter (DM) through its final annihil
Externí odkaz:
http://arxiv.org/abs/2212.06850
Publikováno v:
Phys.Rev.D 105 (2022) 12, 123021
The cosmic-ray fluxes of electrons and positrons ($e^{\pm}$) are measured with high precision by the space-borne particle spectrometer AMS-02. To infer a precise interpretation of the production processes for $e^{\pm}$ in our Galaxy, it is necessary
Externí odkaz:
http://arxiv.org/abs/2203.13143