80 citations · 1.2k across the 83 of their papers we have counts for
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Axions from Neutron Star Mergers
Damiano F. G. Fiorillo, Fabio Iocco
Axion-like particles (ALP) can in principle be produced in very hot and dense astrophysical environments, escape from the extreme object where such conditions are met, and then be…
Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events
O. Sergijenko, A. Brown, D. Fiorillo +6
We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA…
Constraints on heavy decaying dark matter with current gamma-ray measurements
Marco Chianese, Damiano F. G. Fiorillo, Rasmi Hajjar +2
Among the several strategies for indirect searches of dark matter, one very promising one is to look for the gamma-rays from decaying dark matter. Here we use the most up-to-date u…
Unified thermal model for photohadronic neutrino production in astrophysical sources
Damiano F. G. Fiorillo
Astrophysical neutrino fluxes are often modeled as power laws of the energy. This is reasonable in the case of hadronic sources, but it does not capture the behavior in photohadron…
IceCube constraints on Violation of Equivalence Principle
Damiano F. G. Fiorillo
Among the information provided by high energy neutrinos, a promising possibility is to analyze the effects of a Violation of Equivalence Principle (VEP) on neutrino oscillations. W…
Sensitivity of KM3NeT to Violation of Equivalence Principle
Marco Chianese, Damiano F. G. Fiorillo, Gianpiero Mangano +3
The symmetry of the theory of relativity under diffeomorphisms strongly depends on the equivalence principle. Violation of Equivalence Principle (VEP) can be tested by looking for…
Direct Detection of Light Dark Matter from Evaporating Primordial Black Holes
Roberta Calabrese, Marco Chianese, Damiano F. G. Fiorillo +1
The direct detection of sub-GeV dark matter interacting with nucleons is hampered by the low recoil energies induced by scatterings in the detectors. This experimental difficulty i…
Primordial Black Hole Dark Matter evaporating on the Neutrino Floor
Roberta Calabrese, Damiano F. G. Fiorillo, Gennaro Miele +2
Primordial black holes (PBHs) hypothetically generated in the first instants of life of the Universe are potential dark matter (DM) candidates. Focusing on PBHs masses in the range…
Could nearby star-forming galaxies light up the point-like neutrino sky?
Antonio Ambrosone, Marco Chianese, Damiano F. G. Fiorillo +2
Star-forming and starburst galaxies, which are well-known cosmic-rays reservoirs, are expected to emit gamma-rays and neutrinos predominantly via hadronic collisions. In this Lette…
Towards baryogenesis via absorption from Primordial Black Holes
Antonio Ambrosone, Roberta Calabrese, Damiano F. G. Fiorillo +2
Recently Dolgov and Pozdnyakov proposed a new baryogenesis mechanism in which baryon asymmetry is produced without violating baryon number at the Lagrangian level. In this scenario…
A test of the hadronic origin of -rays from blazars with up to month-later follow-up of IceCube Alerts with Imaging Air Cherenkov Telescopes
Damiano F. G. Fiorillo, Konstancja Satalecka, Ignacio Taboada +1
The sources of IceCube neutrinos are as yet unknown. The multi-messenger observation of their emission in -rays can be a guide to their identification, as exemplified by the cas…
The TopFlavor scheme in the context of searches at LHC
Roberta Calabrese, Agostino De Iorio, Damiano F. G. Fiorillo +3
Many extensions of the Standard Model predict the existence of new charged or neutral gauge bosons, with a wide variety of phenomenological implications depending on the model adop…
Unified thermal model for photohadronic neutrino production in astrophysical sources
Damiano F. G. Fiorillo, Arjen Van Vliet, Stefano Morisi +1
High-energy astrophysical neutrino fluxes are, for many applications, modeled as simple power laws as a function of energy. While this is reasonable in the case of neutrino product…
Heavy decaying dark matter at future neutrino radio telescopes
Marco Chianese, Damiano F. G. Fiorillo, Rasmi Hajjar +3
In the next decades, ultra-high-energy neutrinos in the EeV energy range will be potentially detected by next-generation neutrino telescopes. Although their primary goals are to ob…