309 citations · 4.3k across the 87 of their papers we have counts for
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A Strong Test of the Dark Matter Origin of the 1.4 TeV DAMPE Signal Using IceCube Neutrinos
Yue Zhao, Ke Fang, Meng Su +1
A tentative excess in the electron spectrum at 1.4 TeV was recently reported by the DArk Matter Particle Explorer (DAMPE). A non-astrophysical scenario in which dark matter particl…
Ultra-High Energy Cosmic Rays and Neutrinos from Tidal Disruptions by Massive Black Holes
Claire Guépin, Kumiko Kotera, Enrico Barausse +2
Tidal disruptions are extremely powerful phenomena that have been designated as candidate sources of ultra-high-energy cosmic rays. The disruption of a star by a black hole can nat…
The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives
Ke Fang, Jaime Álvarez-Muñiz, Rafael Alves Batista +33
The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau lepton…
High-Energy Neutrinos from Millisecond Magnetars formed from the Merger of Binary Neutron Stars
Ke Fang, Brian D. Metzger
The merger of a neutron star (NS) binary may result in the formation of a long-lived, or indefinitely stable, millisecond magnetar remnant surrounded by a low-mass ejecta shell. A…
IceCube and HAWC constraints on very-high-energy emission from the Fermi bubbles
Ke Fang, Meng Su, Tim Linden +1
The nature of the -ray emission from the \emph{Fermi} bubbles is unknown. Both hadronic and leptonic models have been formulated to explain the peculiar -ray signal observed…
Linking High-Energy Cosmic Particles by Black-Hole Jets Embedded in Large-Scale Structures
Ke Fang, Kohta Murase
The origin of ultrahigh-energy cosmic rays (UHECRs) is a half-century old enigma (Linsley 1963). The mystery has been deepened by an intriguing coincidence: over ten orders of magn…
Using HAWC to Discover Invisible Pulsars
Tim Linden, Katie Auchettl, Joseph Bramante +5
Observations by HAWC and Milagro have detected bright and spatially extended TeV gamma-ray sources surrounding the Geminga and Monogem pulsars. We argue that these observations, al…
HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess
Dan Hooper, Ilias Cholis, Tim Linden +1
Recent measurements of the Geminga and B0656+14 pulsars by the gamma-ray telescope HAWC (along with earlier measurements by Milagro) indicate that these objects generate significan…
The Giant Radio Array for Neutrino Detection
Olivier Martineau-Huynh, Mauricio Bustamante, Washington Carvalho +19
The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ~200 000 radio antennas deployed over ~200 000 km2 in a mountainous site. It aims primarly at detecting h…