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
Unique-IP document downloads: 112 times
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.