Tides and angular momentum redistribution inside low-mass stars hosting planets: a first dynamical model

DOI10.1007/s10569-016-9714-zzbMath1407.70030arXiv1606.08623OpenAlexW3103271307MaRDI QIDQ333844

A. F. Lanza, S. Mathis

Publication date: 31 October 2016

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1606.08623

zbMATH Keywords

turbulencehydrodynamicsbinariesphysical modelplanet-star interactionsstars rotation

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Orbital mechanics (70M20)

Cites Work

• A hybrid method for computing the intersection and tangency points of plane curves
• Two simple proofs of the Kochen-Specker theorem
• Turbulent viscosity, magnetic diffusivity, and heat conductivity under the influence of rotation and magnetic field
• Inertial waves in a differentially rotating spherical shell
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