Modified propagation of gravitational waves from the early radiation era

by Yutong He, Alberto Roper Pol, & Axel Brandenburg: temporary link: main.pdf

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Table 1 GR solutions: GR(RD,MD), GR(LD),

Table 1 series T0 (k1=1e-3): T0A, T0B, T0C, T0D,

Table 1 series M0 (k1=1e-3): M0A, M0A(LD), M0B, M0B(LD), M0C, M0C(LD), M0D, M0D(LD), M0E, M0E(LD), M0F, M0F(LD),

Table 1 series M0 (k1=1e-7): M0A, M0A(LD), M0B, M0B(LD), M0C, M0C(LD), M0D, M0D(LD), M0E, M0E(LD), M0F, M0F(LD),

Table 1 series M1 (k1=1e-3): M1A, M1A(LD), M1B, M1B(LD), M1C, M1C(LD), M1D, M1D(LD), M1E, M1E(LD),

Table 1 series M2 (k1=1e-3): M2A, M2A(LD), M2B, M2B(LD), M2C, M2C(LD), M2D, M2D(LD), M2E, M2E(LD),

Table 1 series M3 (k1=1e-3): M3A, M3A(LD), M3B, M3B(LD), M3C, M3C(LD), M3D, M3D(LD), M3E, M3E(LD), M3F, M3F(LD),

Table 1 series M3 (k1=1e-7): M3A, M3A(LD), M3B, M3B(LD), M3C, M3C(LD), M3D, M3D(LD), M3E, M3E(LD), M3F, M3F(LD),

Appendix: accuracy in time intervals (reference runs) M0AA,

Appendix: accuracy in time intervals (RD) M0A(dt_incr=0.2), M0A(dt_incr=0.1), M0A(dt_incr=0.05), M0A(dt_incr=0.02), M0A(dt_incr=0.01), M0D(dt_incr=0.2), M0D(dt_incr=0.1), M0D(dt_incr=0.05), M0D(dt_incr=0.02), M0D(dt_incr=0.01),

Appendix: accuracy in time intervals (MD) M0A(dt_incr=0.2), M0A(dt_incr=0.1), M0A(dt_incr=0.05), M0A(dt_incr=0.02), M0A(dt_incr=0.01), M0D(dt_incr=0.2), M0D(dt_incr=0.1), M0D(dt_incr=0.05), M0D(dt_incr=0.02), M0D(dt_incr=0.01),

Appendix: accuracy in time intervals (LD) M0A(dt=9e10), M0A(dt=2e10), M0A(dt=9e9), M0A(dt=5e9), M0D(dt=9e10), M0D(dt=2e10), M0D(dt=9e9), M0D(dt=5e9),

Description: readme.txt.

References:

He, Y., Roper Pol, A., & Brandenburg, A.: 2022, ``Modified propagation of gravitational waves from the early radiation era,'' J. Cosmol. Astropart. Phys., submitted (HTML)

He, Y., Roper Pol, A., & Brandenburg, A.: 2022, Datasets of ``Modified propagation of gravitational waves from the early radiation era'' v2022.11.16. Zenodo, DOI:10.5281/zenodo.7327770 (HTML , DOI)

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$Date: 2022/12/06 19:32:53 $, $Author: yutong $, $Revision: 1.12 $