We derive quantization relations in the case when torsion effects are added in a De-Sitter spacetime metric with or without a black hole at the Planck mass and Planck length limit. To this end we use Zeldovich's definition of the cosmological constant.
Comments: 8 pages, Romanian Astronomical Journal, vol. 10, no. 1, 2009 and and SAO/NASA Astrophysics Data System.
[v1] 14 Feb 2010
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