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    Computational Astrophysics

    29 курсов
    A Kinetic-Hydrodynamic Coupling Method for Self-Interacting Dark Matter (SIDM)
    Fields Institute

    A Kinetic-Hydrodynamic Coupling Method for Self-Interacting Dark Matter (SIDM)

    Simulations and Detailed Astrophysical Tests of Dark Matter on Sub-Galactic Scales
    Fields Institute

    Simulations and Detailed Astrophysical Tests of Dark Matter on Sub-Galactic Scales

    Understanding Dwarf Galaxies to Understand Dark Matter
    Fields Institute

    Understanding Dwarf Galaxies to Understand Dark Matter

    First Magnetohydrodynamic Simulations of Jets and Radiative Feedback from a Massive Star
    CIMPA UCR

    First Magnetohydrodynamic Simulations of Jets and Radiative Feedback from a Massive Star

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 5
    International Centre for Theoretical Sciences

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 5

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 2
    International Centre for Theoretical Sciences

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 2

    Multi-Dimensional Modeling of Core-Collapse Supernovae - IPAM at UCLA
    Institute for Pure & Applied Mathematics (IPAM)

    Multi-Dimensional Modeling of Core-Collapse Supernovae - IPAM at UCLA

    Emulating InterStellar Medium Chemistry with Physics Informed Neural Networks
    Alan Turing Institute

    Emulating InterStellar Medium Chemistry with Physics Informed Neural Networks

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 4
    International Centre for Theoretical Sciences

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 4

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 3
    International Centre for Theoretical Sciences

    Introduction to Numerical Relativistic Hydrodynamics - Lecture 3

    Partial Tidal Disruptions of Spinning Eccentric White Dwarfs by Spinning Intermediate Mass Black Holes
    Kavli Institute for Theoretical Physics

    Partial Tidal Disruptions of Spinning Eccentric White Dwarfs by Spinning Intermediate Mass Black Holes

    Constraining the Nature of Dark Matter with Galactic Halos
    Kavli Institute for Theoretical Physics

    Constraining the Nature of Dark Matter with Galactic Halos

    Theoretical Modeling of the Reionization Process
    Kavli Institute for Theoretical Physics

    Theoretical Modeling of the Reionization Process

    Novel Approaches to Simulating the First Galaxy Populations
    Kavli Institute for Theoretical Physics

    Novel Approaches to Simulating the First Galaxy Populations

    Neutrinos in Neutron Star Mergers
    Galileo Galilei Institute

    Neutrinos in Neutron Star Mergers

    Boltzmann Neutrino Transport Simulation of Core-Collapse Supernovae and the Collective Neutrino Flavor Instability
    Galileo Galilei Institute

    Boltzmann Neutrino Transport Simulation of Core-Collapse Supernovae and the Collective Neutrino Flavor Instability

    Simulating Early Structure and Galaxy Formation - The THESAN Project
    MICDE University of Michigan

    Simulating Early Structure and Galaxy Formation - The THESAN Project

    HARM3D and NUC: Numerical Simulations in Relativistic Astrophysics
    Center For Computational Relativity and Gravitation

    HARM3D and NUC: Numerical Simulations in Relativistic Astrophysics

    Tutorial on Simulation Analysis
    Center For Computational Relativity and Gravitation

    Tutorial on Simulation Analysis

    Radiation Transport in Athena++ - 2023 North American Einstein Toolkit School
    Center For Computational Relativity and Gravitation

    Radiation Transport in Athena++ - 2023 North American Einstein Toolkit School

    Harm3D: Highly Accurate Relativistic MHD in 3D
    Center For Computational Relativity and Gravitation

    Harm3D: Highly Accurate Relativistic MHD in 3D