The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence

DOI10.1080/03091929.2019.1653460zbMath1482.83034arXiv1807.05479OpenAlexW3099501834WikidataQ114640050 ScholiaQ114640050MaRDI QIDQ5065699

Sayan Mandal, Alberto Roper Pol, Tina Kahniashvili, Arthur Kosowsky, Axel Brandenburg

Publication date: 22 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1807.05479

zbMATH Keywords

turbulencegravitational wavesearly universeaeroacoustics

Mathematics Subject Classification ID

Turbulence (76F99) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Gravitational waves (83C35)

Related Items (6)

Polarization of gravitational waves from helical MHD turbulent sources ⋮ Model-dependent analysis method for energy budget of the cosmological first-order phase transition ⋮ The scalar, vector, and tensor modes in gravitational wave turbulence simulations ⋮ Introduction ⋮ Electroweak bubble wall expansion: gravitational waves and baryogenesis in standard model-like thermal plasma ⋮ Tensor spectrum of turbulence-sourced gravitational waves as a constraint on graviton mass

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Low-storage Runge-Kutta schemes
• Cosmological backgrounds of gravitational waves
• Energy dissipation rate and energy spectrum in high resolution direct numerical simulations of turbulence in a periodic box
• Strong MHD helical turbulence and the nonlinear dynamo effect
• Bottleneck phenomenon in developed turbulence
• The generation of noise by isotropic turbulence
• On sound generated aerodynamically I. General theory
• On sound generated aerodynamically II. Turbulence as a source of sound

This page was built for publication: The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence