Circular polarization of gravitational waves from early-universe helical turbulence

by T. Kahniashvili, A. Brandenburg, G. Gogoberidze, S. Mandal, & A. Roper Pol

Run directories:

  • Fig 1: pe_comp.pro using τ=0.1, 0.2, 0.5, 1, 2.
  • Fig 2: pcomp_M512k2_both_fixed.pro for ΩK with red, blue, and black lines, and for ΩM with red, blue, and black lines.
  • Fig 3: pgrah_comp.pro for panel (a) with red, orange, green, blue, and black lines, and for ΩM with red, orange, green, blue, and black lines.

    Description: readme.txt.



    References:

    Kahniashvili, T., Brandenburg, A., Gogoberidze, G., Mandal, S., & Roper Pol, A.: 2020, ``Circular polarization of gravitational waves from early-universe helical turbulence,'' Phys. Rev. Lett., to be submitted (HTML)

    Roper Pol, A., Mandal, S., Brandenburg, A., Kahniashvili, T., & Kosowsky, A.: 2020, ``Numerical Simulations of Gravitational Waves from Early-Universe Turbulence,'' Phys. Rev. D 102, 083512 (arXiv:1903.08585, ADS, DOI, HTML, PDF)

    Roper Pol, A., Brandenburg, A., Kahniashvili, T., Kosowsky, A., & Mandal, S.: 2020, ``The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence,'' Geophys. Astrophys. Fluid Dyn. 114, 130-161 (arXiv:1807.05479, ADS, HTML, DOI, PDF)

    Kahniashvili, T., Brandenburg, A., Gogoberidze, G., Mandal, S., & Roper Pol, A., Datasets for ``Circular polarization of gravitational waves from early-universe helical turbulence'' (v2020.11.07), https://doi.org/10.5281/zenodo.4256906. (HTML)



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    Axel Brandenburg
    $Date: 2020/11/08 06:20:36 $, $Author: brandenb $, $Revision: 1.5 $