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Hubble constant, lensing, and time delay in Te Ve S
Published online by Cambridge University Press: 26 February 2013
Abstract
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The Hubble constant can be determined from the time delay of gravitationally lensed systems. We adopt Te Ve S as the relativistic version of Modified Newtonian Dynamics to study gravitational lensing phenomena and evaluate the Hubble constant from the derived time-delay formula. We test our method on observed quasar lensing published in the literature. Three candidates are suitable for our study, HE 2149-2745, FBQ J0951+2635, and SBS 0909+532.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S289: Advancing the Physics of Cosmic Distances , August 2012 , pp. 344 - 347
- Copyright
- Copyright © International Astronomical Union 2013
References
Clowe, D., Bradač, M., Gonzalez, A. H., Markevitch, M., Randall, S. W., Jones, C., & Zaritsky, D. 2006, ApJ, 648, L109Google Scholar
Skordis, C., Mota, D. F., Ferreira, P. G., & Boehm, C. 2006, Phys. Rev. Lett., 96, 011301Google Scholar
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