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¹Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Am Mühlenberg 1, D-14476 Potsdam-Golm, Germany
²Center for Gravitational Physics and Quantum Information, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, 606-8502, Japan
³Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai 980-8578, Japan
⁴Astronomical Institute, Tohoku University, Aoba, Sendai 980-8578, Japan
⁵Department of Physics, Toho University, Funabashi, Chiba 274-8510, Japan

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Articles Citing

Self-consistent scenario for jet and stellar explosions in collapsar: General relativistic magnetohydrodynamics simulation with a dynamo

Long-Lived Intermittent Accretion Disks in the Jittering Jets Explosion Mechanism (JJEM) of Core- Collapse Supernovae

Implications of a weakening N=126 shell closure away from stability for r-process astrophysical conditions

Numerical simulations of jet launching and breakout from collapsars

Jittering Jets Promote Dust Formation in Core-Collapse Supernovae

The r-process: history, required conditions, astrophysical sites, and observations

Jets from Scratch: Dynamo-generated Poloidal Magnetic Fields in Three-dimensional Collapsar Simulations

Fast X-Ray Transients Produced by Off-axis Jet Cocoons from Long Gamma-Ray Bursts

Accretion Regimes of Neutrino-cooled Flows onto Black Holes

The R-process Alliance: Actinide Abundances, Variation, and Evolution in Metal-poor Stars

Distinct First- to Second-Peak Yield Ratios and Timescales Reveal a Subdominant Prompt r-process Channel

Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae

The Actinide-boost Star LAMOST J122216.85–063345.2: A Detailed r-process Abundance Study with Gemini-S/GHOST

Rare Earth Element Nucleosynthesis in Collapsars: Sensitivity to (n, γ) Reaction Rates of Unstable Isotopes during Secondary i- and s-processes

Three-dimensional general relativistic MHD simulations of jet formation and propagation in self-gravitating collapsing stars

The Morphology of Supernova Remnant G0.9+0.1 Implies Explosion by Jittering-jets

Neutrino pair annihilation driven jets from black-hole torus systems

Collapsar disk outflows: Detectable neutrino and gravitational wave signatures

Attributing the Supernova Remnant RCW 89 to the Jittering Jets Explosion Mechanism

Learning from core-collapse supernova remnants on the explosion mechanism

EP 250108a/SN 2025kg: a magnetar-powered gamma-ray burst supernova originating from a close helium-star binary via isolated binary evolution

Multiple Shells in Supernova 2023ixf Support the Jittering Jets Explosion Mechanism

Spinning into the Gap: Direct-horizon Collapse as the Origin of GW231123 from End-to-end General-relativistic Magnetohydrodynamic Simulations

The Landscape of Collapsar Outflows: Structure, Signatures, and Origins of Einstein Probe Relativistic Supernova Transients

A Black Hole Is Born: 3D General-relativistic Magnetohydrodynamic Simulation of Black Hole Formation from Core Collapse

Gamma Rays as a Signature of r-process Producing Supernovae: Remnants and Future Galactic Explosions

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