Abstract
Motivated by recent interest in the possibility of a long range gravitation-like force we have considered the effects a deviation from the Newtonian force law would have on the solar normal mode spectrum. Observations of low order and degree modes provide the most interesting limits to possible new physics. The constraint from solar oscillation observations is distinct from other planetary data in that it provides an integral bound on force law deviations on spatial scales between roughly 2×104 km and planetary scales. This limit is -0.02 ≤ δG/G ≤ 0.3 and is presently limited by systematic differences between the low-l observations and uncertainty in the solar model.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 International Astronomical Union
About this paper
Cite this paper
Kuhn, J.R. (1988). Non-Newtonian Forces and the Observed Solar Oscillation Spectrum. In: Christensen-Dalsgaard, J., Frandsen, S. (eds) Advances in Helio- and Asteroseismology. International Astronomical Union / Union Astronomique Internationale, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4009-3_26
Download citation
DOI: https://doi.org/10.1007/978-94-009-4009-3_26
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2615-5
Online ISBN: 978-94-009-4009-3
eBook Packages: Springer Book Archive