Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-28T06:50:18.880Z Has data issue: false hasContentIssue false

Vacuum Decaying Cosmological Models And Gravitational Lensing

Published online by Cambridge University Press:  25 May 2016

I. Waga
Affiliation:
NASA/Fermilab Astrophysics Center Fermi National Accelerator Laboratory, Batavia, IL 60510 Universidade Federal do Rio de Janeiro, Instituto de Física Rio de Janeiro - RJ - Brasil-21943
L. F. Bloomfield Torres
Affiliation:
Universidade Federal do Rio de Janeiro, Instituto de Física Rio de Janeiro - RJ - Brasil-21943

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.

We investigate the statistical properties of gravitational lenses for flat models in which a cosmological term decreases with time as ⁁ ∝ am, where a is the scale factor and m is a parameter (0 ≤ m < 3) (Bloomfield Torres and Waga 1995).

Type
Chapter 1: Classical Cosmology
Copyright
Copyright © Kluwer 1996 

References

Bloomfield Torres, L. F., & Waga, I., 1995, submitted to MNRAS Google Scholar
Fukugita, M., & Peebles, P. J. E., 1995, submitted to ApJL Google Scholar
Fukugita, M., & Turner, E.L., 1991, MNRAS, 253, 99 CrossRefGoogle Scholar
Kochanek, C. S., 1993, ApJ, 419, 12 Google Scholar
Maoz, D., et al., 1993, ApJ, 409, 28 Google Scholar
Wallington, S., & Narayan, R., 1993, ApJ, 403, 517 CrossRefGoogle Scholar