This is my homepage. And there will update some papers I being reading recently.

==================2024/3/21==================

======astro-physics======

• From Cavitation to Astrophysics: Explicit Solution of the Spherical Collapse Equation
• Rayleigh Taylor Instability in Multiple Finite-Thickness Fluid Layers

==================2024/3/18==================

======astro-physics======

• Large Eddy Simulations of Magnetized Mergers of Black Holes and Neutron Stars

==================2024/3/14==================

======astro-physics======

• Nonlocal stability analysis of the MHD Kelvin-Helmholtz instability in a compressible plasma

==================2024/3/3==================

======astro-physics======

• Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers

==================2024/1/3==================

======astro-physics======

• Temperature-reducing shocks in optically-thin radiative MHD -- analytical and numerical results

==================2023/12/28==================

======astro-physics======

• Tearing-mediated reconnection in magnetohydrodynamic poorly ionized plasmas. I. Onset and linear evolution: ionization two fluid plasma

==================2023/12/20==================

======astro-physics======

• Planet-Driven Scatterings of Planetesimals Into a Star: Probability, Timescale and Applications：planetery fate
• GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods： GIZMO code

=====plasmas physics=====

• Rayleigh-Taylor instability in magnetohydrodynamics with finite resistivity in a horizontal magnetic field
• Unified treatment of mean-field dynamo and angular-momentum transport in magnetorotational instability-driven turbulence: MRI
• Magnetogenesis in a Collisionless Plasma: From Weibel Instability to Turbulent Dynamo: Zhou muni

==================2023/11/23==================

======astro-physics======

• Planetary Engulfment Prognosis within the ρ CrB System:planetery engulfment
• Inferring the Magnetic Field from the Rayleigh–Taylor Instability: MHD RTI

=====plasmas physics=====

• The Biermann catastrophe of numerical MHD: Biermann catastroph

==================2023/11/15==================

======astro-physics======

• Accreting Neutron Stars in 3D GRMHD Simulations: Jets, Magnetic Polarity, and the Interchange Slingshot: Parfrey, Tchekhovkoy
• Producing Ultrastrong Magnetic Fields in Neutron Star Mergers: KH induced magnetic fields: Not converged
• Impact of a mean field dynamo on neutron star mergers leading to magnetar remnants: introductin about some KHI dynamo
• Bondi-Hoyle-Lyttleton accretion in supergiant X-ray binaries: stability and disc formation
• A review of Bondi-Hoyle-Lyttleton accretion

=====plasmas physics=====

• Anisotropic evolutions of the magnetohydrodynamic Richtmyer-Meshkov instability induced by a converging shock: Jianhua Qin, Guodan Dong
• Improved ion heating in fast ignition by pulse shaping
• Hydrodynamic cumulation mechanism caused by quantum shell effects
• Rankine–Hugoniot Relations and Magnetic Field Enhancement in Turbulent Shocks: collisionless shock
• Generation, measurement, and modeling of strong magnetic felds generated by laser‑driven micro coils: review
• Modeling hydrodynamics, magnetic fields, and synthetic radiographs for high-energy-density plasma flows in shock-shear targets: shocktube KHI