Stellar Evolution with Rotation and Magnetic Fields IV: The Solar Rotation Profile

Abstract

We examine the generation of a magnetic field in a solar-like star and its effects on the internal distribution of the angular velocity. We suggest that the evolution of a rotating star with magnetic fields leads to an equilibrium value of the differential rotation. This equilibrium is determined by the magnetic coupling, which favours a constant rotation profile, and meridional circulation which tends to build differential rotation. The global equilibrium stage is close to solid body rotation between about 0.7 and 0.2 R_sun, in good agreement with helioseismic measurements.

4 pages, 4 figures, accepted for publication in A&A Letters

References in corpus (8)

• Dynamo action by differential rotation in a stably stratified stellar interior
• Stellar evolution with rotation XI: Wolf-Rayet star populations at different metallicities
• A fossil origin for the magnetic fields of A-stars and white dwarfs
• Stellar Models with Microscopic Diffusion and Rotational Mixing I: Application to the Sun
• Angular momentum extraction by gravity waves in the Sun
• Stellar evolution with rotation and magnetic fields II: General equations for the transport by Tayler--Spruit dynamo
• The Rotation Of The Deep Solar Layers
• Stellar evolution with rotation and magnetic fields:I. The relative importance of rotational and magnetic effects

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