Cosmic Dark Energy Density from Classical Mechanics and Seemingly Redundant Riemannian Finitely Many Tensor Components of Einstein’s General Relativity

• 作者: Mohamed El Naschie
• 来源期刊: 力学国际期刊(英文)
• 学科: 数学
• 关键词: Semi Classical Quantum Systems Dark Energy Accelerated COSMIC Expansion RIEMANNIAN TENSOR Infinite Dimensional Topology NONLOCAL Elasticity
• 年，卷（期）: 2014,（6）
• 页码范围: 153-156
• 页数: 4页
• 分类号: O1

摘要

We determine the limit of the ratio formed by the independent components of the Riemann tensor to the non-zero component as space dimensionality tends to infinity and find it to be 12. Subsequently we use this result in conjunction with Newtonian classical mechanics to show that the ordinary measurable cosmic energy density is given by while the dark energy density is obviously the Legendre transformation dual energy E(D) = 1 -?E(O). The result is in complete agreement with the COBE, WMAP and type 1a supernova measurements.