activity
19992026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 23.4k across the 141 of their papers we have counts for

collaborators

145 papers

hep-ph2026

The neutrino magnetic moment and supernovae with strong magnetic fields

Clément Ehrhardt, Maria Cristina Volpe, Miguel Ángel Aloy +1

Despite several decades of searches, the neutrino magnetic moment remains unknown. If it is large, the neutrino evolution can be affected by its coupling to strong magnetic fields…

astro-ph.HE2026

EP260119a: A High-Redshift Gamma-Ray Quiet Fast X-ray Transient Probing a Potentially Hidden Population of Relativistic Explosions

Camila Angulo-Valdez, Asuka Kuwata, Edilberto Aguilar-Ruiz +41

Gamma-ray quiet fast X-ray transients (FXTs) provide a new approach for studying relativistic explosions that evade traditional gamma-ray triggers. In this work, we present multi-w…

astro-ph.SR2026

Fast-spinning massive black holes from slowly rotating low-metallicity stars: Implications for GW231123

N. H. Ismail, N. Yusof, R. Hirschi +4

The origin of massive black holes in the early universe remains uncertain and still unexplored. Pop III stars are among the first stellar sources capable of producing such remnants…

astro-ph.HE2026

Failed jet breakout in the metal-poor broad-lined type Ic supernova 2026gzf

Antonio Martin-Carrillo, Christina C. Thöne, James K. Leung +103

A long-standing question in the death of massive stars is the role of relativistic jets. While many gamma-ray bursts and some fast X-ray transients seem to be associated with broad…

astro-ph.HE2026

Impact of the equation of state on core collapse supernovae I: the low- instability

Marco Cusinato, Martin Obergaulinger, Miguel Ángel Aloy

Rapidly rotating core-collapse supernovae are promising sources of multimessenger emission, as non-axisymmetric dynamics in the newly formed proto-neutron star can leave characteri…

astro-ph.SR2026

The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology

Adam Griffiths, Miguel-Ángel Aloy, Martin Obergaulinger

The most energetic core-collapse supernovae are thought to arise from rapidly rotating, magnetised progenitors. However, the three-dimensional pre-collapse structure of their angul…