# Higher-order gravitational lensing reconstruction using Feynman diagrams

@article{Jenkins2014HigherorderGL, title={Higher-order gravitational lensing reconstruction using Feynman diagrams}, author={Elizabeth Ellen Jenkins and Aneesh V. Manohar and Wouter J. Waalewijn and Amit P. S. Yadav}, journal={Journal of Cosmology and Astroparticle Physics}, year={2014}, volume={2014}, pages={024 - 024} }

We develop a method for calculating the correlation structure of the Cosmic Microwave Background (CMB) using Feynman diagrams, when the CMB has been modified by gravitational lensing, Faraday rotation, patchy reionization, or other distorting effects. This method is used to calculate the bias of the Hu-Okamoto quadratic estimator in reconstructing the lensing power spectrum up to πͺ (Ο4) in the lensing potential Ο. We consider both the diagonal noise TT TT, EB EB, etc. and, for the first timeβ¦Β

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