activity
20162021
most citedInterpreting IceCube 6-year HESE data as an evidence for hundred TeV decaying Dark Matter

56 citations · 161 across the 6 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2021

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…

hep-ph20212 cited

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…

astro-ph.HE202133 cited

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…

hep-ph2021

Robust Limits from Upcoming Neutrino Telescopes and Implications on Minimal Dark Matter Models

S. Basegmez du Pree, C. Arina, A. Cheek +3

Experimental developments in neutrino telescopes are drastically improving their ability to constrain the annihilation cross-section of dark matter. In this paper, we employ an ang…

hep-ph2021

Dark Matter in the Type Ib Seesaw Model

Marco Chianese, Bowen Fu, Stephen F. King

We consider a minimal type Ib seesaw model where the effective neutrino mass operator involves two different Higgs doublets, and the two right-handed neutrinos form a heavy Dirac m…

astro-ph.HE202053 cited

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…