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This repository is a supplement to arXiv:1907.13109 (Non-linear contributions to angular power spectra) and contains the Mathematica notebooks used to compute 1-loop corrections in cosmological standard perturbation theory. The uploaded files are as follows: 1- P13.nb is a Mathematica notebook for computing P13 coefficients as explained in Appendix(A) of the paper. 2- P22.nb is a Mathematica notebook for computing P22 coefficients as explained in Appendix(A) of the paper. 3- pk_linear_CAMB_planck18_z0.0_neutrinomass0.dat is the linear power spectrum computed using CAMB with the parameters given in the paper. 4- P13_and_P22_coeffs.zip contains P13 and P22 coefficients computed with the given Mathematica notebooks. For questions and comments, please contact us: Basundhara.Ghosh@unige.ch Mona.Jalilvand@unige.ch
Standard perturbation theory, Non-linear power spectrum, Cosmology
Standard perturbation theory, Non-linear power spectrum, Cosmology
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