output
19972026
most citedDiscovery of a quantum limit Chern magnet TbMn6Sn6

533 citations

Showing astro-ph.HEShow all

36 papers · 1 filter

astro-ph.HE2026★ 1 cited

Equatorially Asymmetric Magnetic Fields and Their Impact on Black Hole Accretion Dynamics

Ishika Palit, Indu Kalpa Dihingia, Yosuke Mizuno +1

We investigate the impact of equatorial asymmetry in the magnetic field geometry on accretion dynamics around a spinning black hole using axisymmetric general relativistic magnetoh…

astro-ph.HE2025

Exploring the Role of Vector Potential and Plasma- in Jet Formation from Magnetized Accretion Flows

Ishika Palit, Miles Angelo Paloma Sodejana, Hsiang-Yi Karen Yang

In this work, we investigate how the choice of initial vector potential and plasma parameters influences the development of accretion columns and jet formation in magnetized accret…

astro-ph.HE2025★ 1 cited

Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae

Zewei Xiong, Meng-Ru Wu, Noshad Khosravi Largani +2

Core-collapse supernovae undergoing a first-order quantum chromodynamics (QCD) phase transition experience the collapse of the central proto-neutron star that leads to a second bou…

astro-ph.HE2025★ 9 cited

Flavor Equilibration of Supernova Neutrinos: Exploring the Dynamics of Slow Modes

Ian Padilla-Gay, Heng-Hao Chen, Sajad Abbar +2

Neutrinos experience collective flavor conversion in extreme astrophysical environments such as core-collapse supernovae (CCSNe). One manifestation of collective conversion is slow…

astro-ph.HE2025★ 37 cited

Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers

Lucas Johns, Sherwood Richers, Meng-Ru Wu

Accurate neutrino transport is crucial for reliably modeling explosive astrophysical events like core-collapse supernovae (CCSNe) and neutron star mergers (NSMs). However, in these…

astro-ph.HE2024★ 12 cited

Actinide signatures in low electron fraction kilonova ejecta

Quentin Pognan, Meng-Ru Wu, Gabriel Martínez-Pinedo +4

Neutron star (NS) mergers are known to produce heavy elements through rapid neutron capture (r-process) nucleosynthesis. Actinides are expected to be created solely by the r-proces…

astro-ph.HE2024★ 15 cited

Evolution and the quasistationary state of collective fast neutrino flavor conversion in three dimensions without axisymmetry

Manu George, Zewei Xiong, Meng-Ru Wu +1

We investigate in this work the evolution of the collective fast neutrino flavor conversion (FFC) in a three dimensional (3D) cubic box with periodic boundary condition for three d…

astro-ph.HE2024★ 33 cited

Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects

Zewei Xiong, Meng-Ru Wu, Manu George +4

Fast flavor conversions (FFCs) of neutrinos, which can occur in core-collapse supernovae (CCSNe), are multiangle effects. They depend on the angular distribution of the neutrino's…

astro-ph.HE2023★ 3 cited

Effects of Annihilation with Low-Energy Neutrinos on High-Energy Neutrinos from Binary Neutron Star Mergers and Rare Core-Collapse Supernovae

Gang Guo, Yong-Zhong Qian, Meng-Ru Wu

We explore the possibility that high-energy (HE) neutrinos produced from choked jets can be annihilated with low-energy (LE) neutrinos emitted from the accretion disk around a blac…

astro-ph.HE2023★ 50 cited

Neutrinos and nucleosynthesis of elements

Tobias Fischer, Gang Guo, Karlheinz Langanke +3

Neutrinos are known to play important roles in many astrophysical scenarios from the early period of the big bang to current stellar evolution being a unique messenger of the fusio…

astro-ph.HE2023★ 57 cited

Evaluating approximate asymptotic distributions for fast neutrino flavor conversions in a periodic 1D box

Zewei Xiong, Meng-Ru Wu, Sajad Abbar +3

The fast flavor conversions (FFCs) of neutrinos generally exist in core-collapse supernovae and binary neutron-star merger remnants, and can significantly change the flavor composi…

astro-ph.HE2023★ 42 cited

Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters

Martin A. Bourne, Hsiang-Yi Karen Yang

Radio jets and the lobes they inflate are common in cool-core clusters and are known to play a critical role in regulating the heating and cooling of the intracluster medium (ICM).…

astro-ph.HE2023★ 7 cited

R-process beta-decay neutrino flux from binary neutron star mergers and collapsars

Yu An, Meng-Ru Wu, Gang Guo +3

This study investigates the antineutrinos production by -decay of -process nuclei in two astrophysical sites that are capable of producing gamma-ray bursts (GRBs): binary neu…

astro-ph.HE2023★ 14 cited

Dark Stars and Gravitational Waves: Topical Review

Kilar Zhang, Ling-Wei Luo, Jie-Shiun Tsao +2

Motivated by recent observations of compact binary gravitational wave events reported by LIGO/Virgo/KAGRA, we review the basics of dark and hybrid stars and examine their probabili…

astro-ph.HE2023★ 8 cited

Evolution and feedback of AGN Jets of different Cosmic-ray Composition

Yen-Hsing Lin, H. -Y. Karen Yang, Ellis R. Owen

Jet feedback from active galactic nuclei (AGN) is one of the most promising mechanisms for suppressing cooling flows in cool-core clusters. However, the composition of AGN jets and…

astro-ph.HE2022★ 69 cited

Evolution of collisional neutrino flavor instabilities in spherically symmetric supernova models

Zewei Xiong, Meng-Ru Wu, Gabriel Martínez-Pinedo +4

We implement a multi-group and discrete-ordinate neutrino transport model in spherical symmetry which allows to simulate collective neutrino oscillations by including realistic col…

astro-ph.HE2022★ 69 cited

The Photon Ring in M87*

Avery E. Broderick, Dominic W. Pesce, Paul Tiede +48

We report measurements of the gravitationally lensed secondary image -- the first in an infinite series of so-called "photon rings" -- around the supermassive black hole M87* via s…

astro-ph.HE2022★ 12 cited

Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants

Shiau-Jie Rau, Kuo-Chuan Pan

Recent theoretical and numerical studies of Type Ia supernova explosion within the single-degenerate scenario suggest that the non-degenerate companions could survive during the su…

astro-ph.HE2022★ 69 cited

Fermi and eRosita bubbles as relics of the past activity of the Galactic black hole

H. -Y. Karen Yang, M. Ruszkowski, E. Zweibel

The newly launched X-ray satellite, eRosita, has recently revealed two gigantic bubbles extending to ~80 degrees above and below the Galactic center. The morphology of these "eRosi…

astro-ph.HE2022★ 12 cited

Production Efficiencies of Sound Waves in the Intracluster Medium Driven by AGN Jets

Shiang-Chih Wang, H. -Y. Karen Yang

Feedback from active galactic nuclei (AGN) is believed to be the most promising solution to the cooling flow problem in cool-core clusters, though how exactly the jet energy is tra…

astro-ph.HE2021★ 22 cited

Self-interacting Dark Scalar Spikes around Black Holes via Relativistic Bondi Accretion

Wei-Xiang Feng, Alessandro Parisi, Chian-Shu Chen +1

We consider the spike mass density profile in a dark halo by self-consistently solving the relativistic Bondi accretion of dark matter onto a non-spining black hole of mass . We…

astro-ph.HE2021★ 9 cited

Emission from hadronic and leptonic processes in galactic jet-driven bubbles

Ellis R. Owen, H. -Y. Karen Yang

We investigate the multiwavelength emission from hadronic and leptonic cosmic rays (CRs) in bubbles around galaxies, analogous to the Fermi bubbles of the Milky Way. The bubbles ar…

astro-ph.HE2021★ 1 cited

Multi-wavelength emission from leptonic processes in ageing galaxy bubbles

Ellis R. Owen, H. -Y. Karen Yang

The evolutionary behavior and multi-wavelength emission properties of bubbles around galaxies, such as the \textit{Fermi} bubbles of the Milky Way, is unsettled. We perform 3D magn…

astro-ph.HE2020★ 2 cited

An adaptive mesh, GPU-accelerated, and error minimized special relativistic hydrodynamics code

Po-Hsun Tseng, Hsi-Yu Schive, Tzihong Chiueh

We present a new special relativistic hydrodynamics (SRHD) code capable of handling coexisting ultra-relativistically hot and non-relativistically cold gases. We achieve this by de…