Higher Modes of Non-Radial Oscillations of Stars by Variational Methods
Keyword(s):
The Ritz method is applied to a variational principle of Chandrasekhar to determine the normal modes of non-radial oscillation of a massive star. Although good results are obtained for the f-mode and the p-modes, it is shown that the method may fail to detect the g-modes. The effect of the choice of coordinate functions is considered.
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1960 ◽
Vol 64
(599)
◽
pp. 697-699
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2020 ◽
Vol 18
(06)
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pp. 2050030
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2005 ◽
Vol 05
(03)
◽
pp. 387-408
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