Holographic Origin of High Cosmological Constant Related to Large Mass Defect in Semiclosed Friedman Universe
cosmology; general relativity, quantum theory; information theoy; holography
Abstract
An extremely high value of Einstein's cosmological constant Λ ~10 122 in quantum cosmology compared to astronomical observations, 0 ≤ Λ ≤ 1, is related to the extremely large general relativistic mass defect of massive semiclosed universe.
Downloads
- Article PDF
- TEI XML Kaleidoscope (download in zip)* (Beta by AI)
- Lens* NISO JATS XML (Beta by AI)
- HTML Kaleidoscope* (Beta by AI)
- DBK XML Kaleidoscope (download in zip)* (Beta by AI)
- LaTeX pdf Kaleidoscope* (Beta by AI)
- EPUB Kaleidoscope* (Beta by AI)
- MD Kaleidoscope* (Beta by AI)
- FO Kaleidoscope* (Beta by AI)
- BIB Kaleidoscope* (Beta by AI)
- LaTeX Kaleidoscope* (Beta by AI)
How to Cite
References
S. Hawking (1984) Physics Letters 134B, 403.
L. Baum, Paul Frampton (2007) PRL 98, .... 7130.
S. Weinberg (1972) Gravitaion and cosmology .......John-Wiley & Sons, Inc.
R. Tolman (1934) 20, 169.
E. Milne 150, 489.
Ya Zel'dovich (1962) J. Exptl. Theoret. 43.
I. Novikov (1963) Soviet Astron.-A. 7, 537.
N. Hokkyo (1972) Prog. Theor. 48, 561.
Published
2014-11-10
Issue
Section
License
Copyright (c) 2014 Authors and Global Journals Private Limited
This work is licensed under a Creative Commons Attribution 4.0 International License.