Hybrid Algorithms for Solving the Algebraic Eigenvalue Problem with Sparse Matrices

2017 ◽  
Vol 53 (6) ◽  
pp. 937-949 ◽  
Author(s):  
A. N. Khimich ◽  
A. V. Popov ◽  
O. V. Chistyakov
1969 ◽  
Vol 3 (5) ◽  
pp. 711-722 ◽  
Author(s):  
A. Wallis ◽  
D. L. S. McElwain ◽  
H. O. Pritchard

1983 ◽  
Vol 66 ◽  
pp. 331-341
Author(s):  
M. Knölker ◽  
M. Stix

AbstractThe differential equations describing stellar oscillations are transformed into an algebraic eigenvalue problem. Frequencies of adiabatic oscillations are obtained as the eigenvalues of a banded real symmetric matrix. We employ the Cowling-approximation, i.e. neglect the Eulerian perturbation of the gravitational potential, and, in order to preserve selfadjointness, require that the Eulerian pressure perturbation vanishes at the outer boundary. For a solar model, comparison of first results with results obtained from a Henyey method shows that the matrix method is convenient, accurate, and fast.


1997 ◽  
Vol 119 (1) ◽  
pp. 110-119 ◽  
Author(s):  
L. Meirovitch

Closed-form solutions to differential eigenvalue problems associated with natural conservative systems, albeit self-adjoint, can be obtained in only a limited number of cases. Approximate solutions generally require spatial discretization, which amounts to approximating the differential eigenvalue problem by an algebraic eigenvalue problem. If the discretization process is carried out by the Rayleigh-Ritz method in conjunction with the variational approach, then the approximate eigenvalues can be characterized by means of the Courant and Fischer maximin theorem and the separation theorem. The latter theorem can be used to demonstrate the convergence of the approximate eigenvalues thus derived to the actual eigenvalues. This paper develops a maximin theorem and a separation theorem for discretized gyroscopic conservative systems, and provides a numerical illustration.


1966 ◽  
Vol 20 (96) ◽  
pp. 621
Author(s):  
E. I. ◽  
J. H. Wilkinson

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