:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Simon, Emily, Caprioli, Damiano, Haggerty, Colby, Reville, Brian
Formato:	Preprint
Publicado:	2024
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	https://arxiv.org/abs/2402.01048
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

A "Faux-Shock" Method for Hybrid Simulations of Astrophysical Shocks
por: Simon, Emily R., et al.
Publicado: (2025)

Efficient Particle Acceleration in 2.5-Dimensional, Hybrid-Kinetic Simulations of Decaying, Supersonic, Plasma Turbulence
por: Gootkin, Keyan, et al.
Publicado: (2025)

Modeling the Saturation of the Bell Instability using Hybrid Simulations
por: Zacharegkas, Georgios, et al.
Publicado: (2022)

Acceleration of Heavy Ions at Non-Relativistic Collisionless Shocks
por: Caprioli, Damiano, et al.
Publicado: (2025)

Detecting Neutrino Emission from Supernova Remnants: A Theoretically Motivated Target Catalog
por: Simon, Emily, et al.
Publicado: (2025)

Ultrahigh-energy neutrinos as a probe of espresso-shear acceleration in jets of Centaurus A
por: Mbarek, Rostom, et al.
Publicado: (2024)

Hybrid Simulations of Supersonic Shear Flows: II) Cosmic Ray Viscosity
por: Liang, Naixin, et al.
Publicado: (2026)

Hybrid Simulations of Supersonic Shear Flows: I) Particle Acceleration
por: Liang, Naixin, et al.
Publicado: (2025)

Revisiting Propagation Delays of Ultra-High-Energy Cosmic Rays from Long-lived Sources
por: Mbarek, Rostom, et al.
Publicado: (2025)

How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations
por: Smirnova, P., et al.
Publicado: (2024)

Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
por: Desai, Dhvanil D., et al.
Publicado: (2025)

The Importance of Heat Flux in Quasi-Parallel Collisionless Shocks
por: Haggerty, Colby C., et al.
Publicado: (2023)

Investigating Nonlinear Landau Damping in Hybrid Simulations
por: Schroer, Benedikt, et al.
Publicado: (2025)

Shock Acceleration in the Intracluster Medium: Implications of Micromirror Confinement
por: Diesing, Rebecca, et al.
Publicado: (2025)

Microphysics of diffusive shock acceleration: impact on the spectrum of accelerated particles
por: Cristofari, Pierre, et al.
Publicado: (2022)

Understanding Streaming Instabilities in the Limit of High Cosmic Ray Current Density
por: Lichko, Emily, et al.
Publicado: (2024)

IXPE observations of supernova remnants
por: Ferrazzoli, Riccardo
Publicado: (2025)

3D MHD simulations of runaway pulsars in core collapse supernova remnants
por: Meyer, D. M. A., et al.
Publicado: (2025)

On the properties of turbulence in the remnant of Tycho supernova
por: Petruk, Oleh, et al.
Publicado: (2025)

Stellar-wind feedback and magnetic fields around young compact star clusters: 3D MHD simulations
por: Härer, Lucia, et al.
Publicado: (2025)

Electron Acceleration at Quasi-parallel Non-relativistic Shocks: A 1D Kinetic Survey
por: Gupta, Siddhartha, et al.
Publicado: (2024)

The role of non-linear Landau damping for cosmic-ray transport
por: Schroer, Benedikt, et al.
Publicado: (2024)

Speed-dependent Threshold for Electron Injection into Diffusive Shock Acceleration
por: Gupta, Siddhartha, et al.
Publicado: (2025)

Regions of suppressed diffusion around supernova remnants?
por: Bao, Yiwei, et al.
Publicado: (2024)

Particle acceleration at radiative supernova remnant shocks
por: Cristofari, Pierre
Publicado: (2025)

Is the low-energy tail of shock-accelerated protons responsible for over-ionized plasma in supernova remnants?
por: Sawada, Makoto, et al.
Publicado: (2024)

The population of Galactic supernova remnants in the TeV range
por: Batzofin, Rowan, et al.
Publicado: (2024)

Diffusive shock acceleration of dust grains at supernova remnants
por: Cristofari, P., et al.
Publicado: (2024)

Broadband radio study of the supernova remnant Kes 73
por: Loru, S., et al.
Publicado: (2025)

Deep Learning Analysis of Ions Accelerated at Shocks
por: Swierc, Paxson, et al.
Publicado: (2025)

Ultra-high-energy $γ$-ray imprints from PeV particles accelerated by supernova remnants
por: Cao, Zhen, et al.
Publicado: (2026)

Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443
por: Cao, Zhen, et al.
Publicado: (2025)

Evidence of gradients of density and magnetic field in the remnant of Tycho's supernova
por: Petruk, Oleh, et al.
Publicado: (2024)

The vela supernova remnant: The unique morphological features of jittering jets
por: Soker, Noam, et al.
Publicado: (2024)

Learning from core-collapse supernova remnants on the explosion mechanism
por: Soker, Noam
Publicado: (2024)

Initial state of the recombining plasma in supernova remnant W 28
por: Himono, Rui, et al.
Publicado: (2024)

On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants
por: Petruk, O., et al.
Publicado: (2025)

Broadband $γ$-ray spectrum of supernova remnant Cassiopeia A
por: Cao, Zhen, et al.
Publicado: (2025)

The precessing jet axis of the supernova remnant 3C 397
por: Klimov, Aleksei, et al.
Publicado: (2026)

On the progenitor of the type Ia supernova remnant 0509-67.5
por: Soker, Noam
Publicado: (2025)