activity
20072018
most citedParametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies

354 citations · 478 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2018★ 3 cited

Nuclear -ray emission from very hot accretion flows

Ervin Kafexhiu, Felix Aharonian, Maxim Barkov

Optically thin accretion plasmas can reach ion temperatures K and thus trigger nuclear reactions. Using a large nuclear interactions network, we studied the…

astro-ph.HE2018★ 3 cited

Gamma-ray emission of hot astrophysical plasmas

Ervin Kafexhiu, Felix Aharonian, Maxim Barkov

Very hot plasmas with ion temperature exceeding K can be formed in certain astrophysical environments. The distinct radiation signature of such plasmas is the -ray emi…

astro-ph.HE2018★ 31 cited

On the shape of the gamma-ray spectrum around the "-bump"

Rui-zhi Yang, Ervin Kafexhiu, Felix Aharonian

The "pion-decay" bump is a distinct signature of the differential energy spectrum of -rays between 100 MeV and 1 GeV produced in hadronic interactions of accelerated particles (…

astro-ph.HE2018★ 13 cited

Energetic gamma-ray emission from solar flares

Ervin Kafexhiu, Carlo Romoli, Andrew M. Taylor +1

Recent advances in the -ray observations of solar flares by the \textit{Fermi} satellite, demand revisions in the hadronic -ray flux computation below 1 GeV. In this work we…

astro-ph.HE2016★ 12 cited

Parametrization of the nucleus-nucleus gamma-ray production cross sections below 100 GeV/nucleon: Subthreshold pions and Hard photons

Ervin Kafexhiu

"Subthreshold pions" and so-called "hard photons" are two important channels for producing less than 1 GeV -rays and pairs from nuclear collisions with energy per nucleo…

astro-ph.HE2014★ 44 cited

Detection of persistent gamma-ray emission toward SS433/W50

Pol Bordas, Ruizhi Yang, Ervin Kafexhiu +1

The microquasar SS433 features the most energetic jets known in our Galaxy. A large fraction of the jet kinetic power is delivered to the surrounding W50 nebula at the jet terminat…