activity
20142025
most citedHigh-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints

71 citations · 135 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2025

Impact of neutrino decays on the Cosmic Neutrino Background anisotropies

Nicola Terzaghi, Guillermo Franco Abellán, Fabian Zimmer +1

The anisotropies of the Cosmic Neutrino Background (CB) offer an ideal tool to test non-standard neutrino interactions, since they directly trace the perturbations in the neutri…

astro-ph.CO2025

Numerical treatment of annual modulation of relic neutrinos

Fabian Zimmer, Shin'ichiro Ando

We present a numerical treatment of the annual modulation of relic neutrinos due to the Sun's gravitational influence. Extending our previously developed N-1-body simulation framew…

astro-ph.CO2024

Effects of primordial fluctuations on relic neutrino simulations

Fabian Zimmer, Guillermo Franco Abellán, Shin'ichiro Ando

After decoupling, relic neutrinos traverse the evolving gravitational imhomogeneities along their trajectories. Once they turn non-relativistic, this results in a significant ampli…

hep-ph2021★ 13 cited

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…

astro-ph.HE2015★ 51 cited

Tomographic Constraints on High-Energy Neutrinos of Hadronuclear Origin

Shin'ichiro Ando, Irene Tamborra, Fabio Zandanel

Mounting evidence suggests that the TeV-PeV neutrino flux detected by the IceCube telescope has mainly an extragalactic origin. If such neutrinos are primarily produced by a single…

astro-ph.HE2014★ 71 cited

High-energy gamma-ray and neutrino backgrounds from clusters of galaxies and radio constraints

Fabio Zandanel, Irene Tamborra, Stefano Gabici +1

Cosmic-ray protons accumulate for cosmological times in clusters of galaxies as their typical radiative and diffusive escape times are longer than the Hubble time. Their hadronic i…