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Started:04/01/2000
PI: Donald E. Winget
University of Texas Austin

A Parallel Genetic-Algorithm-based approach to White Dwarf Pulsation Models
White dwarf asteroseismology offers the opportunity to probe the structure and composition of stellar objects governed by relatively simple principles. The observational requirements of asteroseismology have been addressed by the development of the Whole Earth Telescope (WET) in conjunction with the HST, but the analytical procedures need to be refined before this technique can yield the complete physical insight that the data can provide. We propose to develop an optimization method utilizing a genetic algorithm (GA) for fitting white dwarf pulsation models to the observations. We will develop software to use this global optimization approach in two distinct ways: (1) to investigate the uniqueness and objectivity of the solutions by combining existing models with a GA-based fitting routine, and (2) to investigate the completeness and adequacy of our understanding of the principles governing white dwarf interiors by parameterizing the constitutive physics and using a GA to find the family of solutions that produce observationally indistinguishable behavior. We have configured a specialized computational instrument to develop this software---a parallel metacomputer consisting of a network of 64 minimal PCs running Linux. The structure of a GA is very conducive to parallelization, so this metacomputer will allow us to develop and run the code on a practical timescale.

Bibliography
12C(alpha, gamma)16O from WD Asteroseismology Metcalfe; Salaris; Winget; ApJ, (2002) 573 pp. 803

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Last Updated: 01/18/2005