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- W1623702012 abstract "Abstract The eigenmodes of the adiabatic oscillations of stars are usually calculated numerically by solving the system of the four linear first-order differential equations using either the relaxation method or the shooting method. Finding some shortcomings in these conventional methods, we adopt another method, namely the Riccati method, in which it is not the system of the linear differential equations but the nonlinear matrix Riccati equation that is solved numerically. After describing the method, we discuss its advantages and give some demonstrations." @default.
- W1623702012 created "2016-06-24" @default.
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- W1623702012 date "2004-01-01" @default.
- W1623702012 modified "2023-09-23" @default.
- W1623702012 title "Application of The Riccati Method to The Adiabatic Oscillations of Stars" @default.
- W1623702012 cites W1568666422 @default.
- W1623702012 cites W2012190853 @default.
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- W1623702012 doi "https://doi.org/10.1017/s0252921100011192" @default.
- W1623702012 hasPublicationYear "2004" @default.
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