Does the solar interior rotate rigidly?

Details Does the solar interior rotate rigidly? Does the solar interior rotate rigidly?

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...377..707g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 377, Aug. 20, 1991, p. 707-711.

Astronomy and Astrophysics

Astrophysics

Elementary Particle Interactions, Solar Interior, Solar Neutrinos, Solar Oscillations, Solar Rotation, Heat Transmission, Momentum Transfer, Weak Interactions (Field Theory)

Scientific paper

If heat transport by weakly interacting massive particles (WIMPs) is the solution to the solar neutrino problem, these WIMPs would also be extremely efficient at transporting momentum. They would cause the region of the sun interior to a critical radius to rotate in a distinctive fashion, usually rigidly. The critical radius may be as great as about 0.5 solar radius for the lightest WIMPs. The boundary between the affected and unaffected regions would be extremely sharp, less than about 0.2 solar radius. This characteristic rotation profile could be observed or ruled out given sufficient improvement in the measurement of the azimuthal splitting of solar p-modes.

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