High-energy astrophysics
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- Can we constrain the binary neutron star merger time from kilonova light curves?
- A new view of the cosmic-ray knee after LHAASO
- The renormalization-group running of neutrino mixing is undetectable
- A Hybrid Neural Network Emulator for M1 Neutrino Reaction Rates in Binary Neutron Star Merger Simulations
- Prior volume effect inflates the gravitational-wave background in pulsar timing arrays
- The (missing) gamma-ray counterparts to EP events
- Exploring the origin of slow-rotating pulsars: Emission from STARS simulated white dwarfs
- Chana: A GPU-Accelerated Adaptive-Mesh Code for General Relativistic Magnetohydrodynamics with Multigroup M1 Neutrino Transport
- Dyonic black holes supporting nearly-black self-gravitating thin shells
- Constraints on Millimeter-wave Extragalactic Transient Populations from 4 Years of SPT-3G data
- Dynamical stability of Magnetic Supramassive Neutron Stars
- Identifying a jet-shaped point-symmetric morphology in the supernova remnant HB9
- Hybrid Stars with Different Amount of Quark Matter
- Hidden engines in tidal disruption events: multimessenger signatures in a lepto-hadronic framework
- On the Stability of Tolman Oppenheimer Volkoff Fireholes
- Pulsar J1909+0749 and Supernova Remnant G42.1-0.2: A case of a pulsar that has exited the shell of its associated supernova remnant
- Constraints on Dark Matter Annihilation from Starlight-Induced Inverse Compton Emission in Omega Centauri
- On the superbursts as photodisintegrators of ashes from the rp-process -- Numerical simulations of superbursts with MESA II
- Rapid Variability of Radiative Signatures from Driven Relativistic Reconnection
- Direct Urca process facilitated by non-Fermi-liquid quantum criticality
- The environments of type Ibn supernovae: evidence for a strong Wolf-Rayet star component
- A bright X-ray flaring event from the intermediate supergiant fast X-ray transient IGR J00370+6122 observed with NuSTAR
- What Shapes the Ultraviolet Spectra of Type Ia Supernovae?
- An improved self-gravity treatment in general relativistic smoothed particle hydrodynamics
- Short-timescale X-ray variability of the blazar 1ES 1959+650 observed with AstroSat/SXT