YoVDO

Modeling the Kelvin-Helmholtz Instability in BNS Mergers

Offered By: Center For Computational Relativity and Gravitation via YouTube

Tags

Astrophysics Courses Fluid Dynamics Courses Gravitational Waves Courses Numerical Modeling Courses Computational Relativity Courses

Course Description

Overview

Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only!
Explore the complexities of modeling the Kelvin-Helmholtz instability in binary neutron star (BNS) mergers in this 37-minute conference talk delivered at the 2023 North American Einstein Toolkit School and Workshop. Gain insights into advanced computational techniques and theoretical frameworks used to simulate these astrophysical phenomena, as presented by an expert from the Center For Computational Relativity and Gravitation. Delve into the challenges and methodologies involved in accurately representing fluid dynamics and gravitational interactions during neutron star coalescence.

Syllabus

Michail Chabonov -- Modeling the Kelvin-Helmholtz instability in BNS mergers


Taught by

Center For Computational Relativity and Gravitation

Related Courses

Inflationary Cosmology
Massachusetts Institute of Technology via World Science U
Gravity! The Big Bang, Black Holes and Gravitational Waves
Paris Diderot University via FutureLearn
Gravité! Du Big Bang aux Trous Noirs
Paris Diderot University via France Université Numerique
Einstein's Astrophysical Messengers
Louisiana State University via World Science U
Introduction into General Theory of Relativity
Higher School of Economics via Coursera