90 citations · 1.1k across the 52 of their papers we have counts for
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Exploring memory-burdened primordial black holes with ultra-high-energy cosmic-rays
Antonio Ambrosone, Marco Chianese, Carmelo Evoli
Quantum backreaction effects may quench Hawking evaporation through a ``memory burden'', allowing primordial black holes (PBHs) with formation masses well below $10^{15}~\mathrm{g}…
High-energy gamma-ray emission from memory-burdened primordial black holes
Marco Chianese
Theoretical studies on the memory-burden effect suggest that Primordial Black Holes (PBHs) with masses smaller than grams may be viable dark matter candidates and, conseq…
Light burden of memory: Constraining primordial black holes with high-energy neutrinos
Marco Chianese, Andrea Boccia, Fabio Iocco +2
Recent studies point out that quantum effects, referred to as "memory burden", may slow down the evaporation of black holes. As a result, a population of light primordial black hol…
Constraining the hadronic properties of star-forming galaxies above with 15-years Fermi-LAT data
Antonio Ambrosone, Marco Chianese, Antonio Marinelli
Star-forming and starburst galaxies (SFGs and SBGs) are powerful emitters of non-thermal -rays and neutrinos, due to their intense phases of star-formation activity, which shoul…
Constraints on heavy decaying dark matter from 570 days of LHAASO observations
The LHAASO Collaboration, Zhen Cao, F. Aharonian +276
The Kilometer Square Array~(KM2A) of the Large High Altitude Air Shower Observatory (LHAASO) aims at surveying the northern gamma-ray sky at energies above 10 TeV with unprecedente…
Starburst Nuclei as Light Dark Matter Laboratories
Antonio Ambrosone, Marco Chianese, Damiano F. G. Fiorillo +2
Starburst galaxies are well-motivated astrophysical emitters of high-energy gamma-rays. They are well-known cosmic-ray "reservoirs", thanks to their large magnetic fields which con…
Multi-messenger High-Energy Signatures of Decaying Dark Matter and the Effect of Background Light
Barbara Skrzypek, Marco Chianese, Carlos Argüelles Delgado
The IceCube Neutrino Observatory at the South Pole has measured astrophysical neutrinos using through-going and starting events in the TeV to PeV energy range. The origin of these…
Observable Signatures of Cosmic Rays Transport in Starburst Galaxies on Gamma-ray and Neutrino Observations
A. Ambrosone, M. Chianese, D. F. G. Fiorillo +2
The gamma-ray emission from Starburst and Starforming Galaxies (SBGs and SFGs) strongly suggest a correlation between star-forming activity and gamma-ray luminosity. However, the v…
EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade
R. Alves Batista, M. A. Amin, G. Barenboim +134
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the…
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…
Starburst galaxies strike back: a multi-messenger analysis with Fermi-LAT and IceCube data
Antonio Ambrosone, Marco Chianese, Damiano F. G. Fiorillo +3
Starburst galaxies, which are known as "reservoirs" of high-energy cosmic-rays, can represent an important high-energy neutrino "factory" contributing to the diffuse neutrino flux…