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White dwarfs are almost completely degenerate objects that cannot obtain energy from thermonuclear sources, so their evolution is just a gravothermal cooling process.
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A. H. Córsico, L.G. Althaus, A.D. Romero, M.H. Miller Bertolami, E. García–Berro, & J. Isern, “Constraining the axion mass through the asteroseismology of the ZZ Ceti star G117–B15A”, Proc. of “The 61st Fujuhara Seminar: Progress in solar/stellar physics with helio and asteroseismology”, in press (2011)
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2011
Later among the works it cites.