3 papers
astro-ph.HE2026
Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
Zhao-Feng Wu, SofÃa Guevara-Montoya, Paz Beniamini +3
Particle acceleration in relativistic collisionless shocks remains an open problem in high-energy astrophysics. Particle-in-cell (PIC) simulations predict that electron acceleratio…
astro-ph.SR2026
Type-III solar radio bursts with spike-like toppings
Shuwang Chang, Chuanyang, Bing Wang +5
Spike-type III burst pairs represent a distinct class of solar radio emissions in which clusters of spike-like bursts appear atop the highfrequency onset of type III bursts. Using…
astro-ph.HE2025
Maximal Jet Energy of Gamma-Ray Bursts through the Blandford-Znajek Mechanism
Zhao-Feng Wu, Michail Damoulakis, Paz Beniamini +1
Gamma-ray bursts (GRBs) are among the most energetic events in the universe, driven by relativistic jets launched from black holes (BHs) formed during the collapse of massive stars…