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Introduction to Numerical Relativistic Hydrodynamics - Lecture 5

Offered By: International Centre for Theoretical Sciences via YouTube

Tags

General Relativity Courses Black Holes Courses Partial Differential Equations Courses Neutron Stars Courses Gravitational Waves Courses Supercomputers Courses Numerical Relativity Courses Computational Astrophysics Courses Relativistic Hydrodynamics Courses

Course Description

Overview

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Delve into the fifth lecture of the "Introduction to Numerical Relativistic Hydrodynamics" series, presented by Kenta Kiuchi from the Albert Einstein Institute. Explore advanced concepts in numerical relativity and hydrodynamics as part of the Summer School on Gravitational-Wave Astronomy. Gain insights into solving field equations of General Relativity in conjunction with magnetohydrodynamics equations using supercomputers. Understand the crucial role of numerical simulations in accurately modeling mergers of black holes or neutron stars, massive star collapses, and accreting black holes. Learn about the significance of these simulations in interpreting gravitational-wave signals and multi-messenger observations. Discover how this field contributes to our understanding of high-energy astrophysical phenomena targeted by upcoming gravitational-wave, electromagnetic, and neutrino observatories.

Syllabus

Introduction to Numerical Relativistic Hydrodynamics (Lecture 5) by Kenta Kiuchi


Taught by

International Centre for Theoretical Sciences

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