466 citations · 7.4k across the 130 of their papers we have counts for
9 papers · 1 filter
Radio detection prospects for a bulge population of millisecond pulsars as suggested by Fermi LAT observations of the inner Galaxy
Francesca Calore, Mattia Di Mauro, Fiorenza Donato +2
Analogously to globular clusters, the dense stellar environment of the Galactic center has been proposed to host a large population of as-yet undetected millisecond pulsars (MSPs).…
Combined analysis of effective Higgs portal dark matter models
Ankit Beniwal, Filip Rajec, Christopher Savage +4
We combine and extend the analyses of effective scalar, vector, Majorana and Dirac fermion Higgs portal models of dark matter (DM), in which DM couples to the Standard Model (SM) H…
Global analysis of the pMSSM in light of the Fermi GeV excess: prospects for the LHC Run-II and astroparticle experiments
Gianfranco Bertone, Francesca Calore, Sascha Caron +4
We present a new global fit of the 19-dimensional phenomenological Minimal Supersymmetric Standard Model (pMSSM-19) that comply with all the latest experimental results from dark m…
The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts
Ilias Cholis, Carmelo Evoli, Francesca Calore +3
It has been proposed that a recent outburst of cosmic-ray electrons could account for the excess of GeV-scale gamma rays observed from the region surrounding the Galactic Center. A…
Strong support for the millisecond pulsar origin of the Galactic center GeV excess
Richard Bartels, Suraj Krishnamurthy, Christoph Weniger
Using gamma-ray data from the Fermi Large Area Telescope, various groups have identified a clear excess emission in the Inner Galaxy, at energies around a few GeV. This excess rese…
The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter
Fabio Zandanel, Christoph Weniger, Shin'ichiro Ando
We investigate for the first time the potential of angular auto- and cross-correlation power spectra in identifying sterile neutrino dark matter in the cosmic X-ray background. We…