2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/35543We present here an application of a new quantization scheme. We quantize the Taub cosmology by quantizing only the anisotropy parameter $β$ and imposing the super-Hamiltonian constraint as an expectation-value equation to recover the relationship between the scale factor $Ω$ and the time $t$. This approach appears to avoid the problem of time. (Paper to appear in the Seventh Marcel Grossmann Conference Proceedings.)7 pages (compressed and uuencoded postscript file), LAUR-94-3328General Relativity and Quantum Cosmologytext