Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-30T04:40:13.506Z Has data issue: false hasContentIssue false

Effect of Spin-Gravity Interaction on the Cosmological Parameters

Published online by Cambridge University Press:  26 May 2016

M. I. Wanas*
Affiliation:
Astronomy Department, Faculty of Science, Cairo University, Egypt. email: [email protected]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Cosmological information is usually carried by, and extracted from massless spinning particles, “carriers of cosmological information”. The photon (spin 1-particle) is a good candidate representing one type of these carriers. Recently, the neutrino (spin 1/2-particle) entered the playground as another type. We expect, in the near future, that a third type of carriers, the graviton (spin 2-particle), to be used for extracting cosmological information. Two factors affect the properties of these carriers. The first is the source of the carrier. The second factor is the trajectory of the carrier, in the cosmic space, from its source to the receiver. The first factor implies the information carried, which reflect the properties of the source. The second factor represents the impact of the cosmic space-time on the properties of the carrier. So, information carried by these particles contain, a part connected to their sources, and another part related to the space-time through which these particles traveled.

Type
Part XII: Poster Papers
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Kermack, W. O. McCrea, W. H. & Whittaker, E. T. 1933, Proc. Roy.Soc.Edin., 53, 31.CrossRefGoogle Scholar
Robertson, H. P. 1932, Ann. Math. Princeton (2), 33, 496.CrossRefGoogle Scholar
Wanas, M. I, Melek, M. & Kahil, M. E. 1995, Astrophys.space Sci., 228, 273.Google Scholar
Wanas, M. I. 1998, Astrophys.space Sci., 258, 237.CrossRefGoogle Scholar
Wanas, M. I, Melek, M. & Kahil, M. E. 1998, gr-qc/9812085.Google Scholar
Wanas, M. I., Melek, M. & Kahil, M. E. 2000, Paper presented in MG9, (AT3a), held in Rome 2–8 Aug.Google Scholar