activity
20092026
most citedThe First LHAASO Catalog of Gamma-Ray Sources

247 citations · 2.6k across the 118 of their papers we have counts for

collaborators
Showing 2019Show all

7 papers · 1 filter

astro-ph.HE2019

Core-collapse Supernovae as Cosmic Ray Sources

V. Dwarkadas, A. Marcowith, M. Renaud +2

Core-collapse supernovae produce fast shocks which expand into the dense circumstellar medium (CSM) of the stellar progenitor. Cosmic rays (CRs) accelerated at these shocks can ind…

astro-ph.HE2019★ 3 cited

Combined Dark Matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, HESS, MAGIC and VERITAS

Louise Oakes, Celine Armand, Eric Charles +13

The search for Dark Matter (DM) has great potential to reveal physics beyond the Standard Model. As such, searches for evidence of DM particles are being carried out using a wide r…

astro-ph.HE2019★ 1 cited

Electron Acceleration in the Crab Nebula

Gwenael Giacinti, John G. Kirk

We study electron and positron acceleration at the termination shock of a striped pulsar wind. Drift motion along the shock surface keeps either electrons or positrons -but not bot…

astro-ph.HE2019★ 12 cited

HAWC Contributions to the 36th International Cosmic Ray Conference (ICRC2019)

A. U. Abeysekara, A. Albert, R. Alfaro +127

List of proceedings from the HAWC Collaboration presented at the 36th International Cosmic Ray Conference, 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.HE2019★ 4 cited

Inductive acceleration of ions in Poynting-flux dominated outflows

John G. Kirk, Gwenael Giacinti

Two-fluid (electron-positron) plasma modelling has shown that inductive acceleration can convert Poynting flux directly into bulk kinetic energy in the relativistic flows driven by…

astro-ph.HE2019

Numerical Simulations of Cosmic-Ray Acceleration at Core-Collapse Supernovae

Gwenael Giacinti, Vikram Dwarkadas, Alexandre Marcowith +1

Core-collapse supernovae exploding in dense winds are favorable sites for cosmic-ray (CR) acceleration to very high energies. We present our CR-radiation-hydrodynamics simulations…