Physics
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989amjph..57..159c&link_type=abstract
American Journal of Physics, Volume 57, Issue 2, pp. 159-166 (1989).
Physics
3
Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages
Scientific paper
Acton and Squire's [Solving Equations with Physical Understanding (Hilger, Bristol, 1985)] ``trial function'' method of handling boundary value problems is used to find approximate solutions to the equations of stellar structure; the calculations involved are as simple to carry out as the usual order-of-magnitude estimates, but are correct to a few tens of a percent. The method is also used to investigate why an order-of-magnitude estimate of solar luminosity can be wrong by up to three orders of magnitude, while a similar estimate of the central temperature can be closer to acceptable values.
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