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We present a new method to compute the deflection of light rays in a perturbed FLRW geometry.
1933
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1976
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P. Schneider, J. Ehlers and E. Falco, Gravitational Lenses (Springer Verlag, Berlin, 1992)
1992
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M. Sasaki, “Cosmological gravitational lens equation: Its validity and limitation,” Prog. Theor. Phys. 90
1993
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E. Bertschinger, Cosmological Dynamics in Cosmology and Large Scale Structure, proc. Les Houches Summer School, Session LX, ed. R. Schaeffer, J. Silk, M. Spiro and J. Zinn-Justin (Amsterdam:Elsevier Science), 273-347, 1996; L. Bombelli, W. E. Couch and R. J. Torrence, “Perfect fluid perturbations of cosmological spacetimes in Stewart’s variables,” Class. Quant. Grav. 11
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F. Bernardeau, S. Colombi, E. Gaztanaga and R. Scoccimarro, “Large scale structure of the universe and cosmological perturbation theory,” Phys. Rept. 367
2002
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T. Pyne and M. Birkinshaw, “The luminosity distance in perturbed flrw spacetimes,” Mon. Not. Roy. Astron. Soc. 348
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T.W.B. Kibble and R. Lieu, “Average magnification effect of clumping of matter, ” Astrophys.J. 632
2005
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A. Lewis and A. Challinor, “Weak gravitational lensing of the cmb,” Phys. Rept. 429
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2011
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G. Marozzi, “The cosmological backreaction: gauge (in)dependence, observers and scalars,” JCAP 1101
2011
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2012
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2012
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2012
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2014
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2014
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2014
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2014
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2012
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C. Bonvin, R. Durrer and M. A. Gasparini, “Fluctuations of the luminosity distance,” Phys. Rev. D 73
2012
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2013
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2013
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2013
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2013
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2013
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2014
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2014
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2014
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J. Frieman, Probing the accelerating universe
2014
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2015
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2015
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