Can we observe the QCD phase transition-generated gravitational waves through pulsar timing arrays?

by A. Brandenburg et al., temporary link: main.pdf

Run directories:

  • Fig.2 uses pcomp512.pro and pcomp512hel.pro, with data from directories noh1, noh2, noh3, noh4, hel1, hel2, hel3, hel4.
  • Tables I+II uses data from the additional directories noh5, noh6, noh7, noh8, hel5, hel6, hel7, hel8.
  • Fig.3 uses pcomp512_oo.pro and pcomp512hel_oo.pro, with data from the same directories.
  • Fig.4 uses pres.pro and EEGW_vs_EEKM.pro, with data from directories paper_idl
  • Fig.5 uses pspecm.pro and pspecm_hel.pro, with data from the same directories.
  • Fig.6 uses pbspecm.pro with data from the same directories.
  • Fig.7 uses pspecm_other.pro with data from the directories magnetic, vortical, irrotational.

    Description: readme.txt.


    References:

    Brandenburg, A., Clarke, E., He, Y., & Kahniashvili, T.: 2021, “Can we observe the QCD phase transition-generated gravitational waves through pulsar timing arrays?,” Phys. Rev. D, to be submitted

    Brandenburg, A., Clarke, E., He, Y., & Kahniashvili, T.: 2021, Datasets for “Can we observe the QCD phase transition-generated gravitational waves through pulsar timing arrays?” v2021.02.24. Zenodo, DOI:10.5281/zenodo.4560423 (HTML, DOI)


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    Axel Brandenburg
    $Date: 2021/02/24 17:18:51 $, $Author: brandenb $, $Revision: 1.4 $