%0 Generic %1 sharma2022frequency %A Sharma, Ramkishor %A Brandenburg, Axel %D 2022 %K gw mhd turbulence %T Low frequency tail of gravitational wave spectra from hydromagnetic turbulence %U http://arxiv.org/abs/2206.00055 %X Hydrodynamic and magnetohydrodynamic (MHD) turbulence in the early Universe can drive gravitational waves (GWs) and imprint their spectrum onto that of GWs, which might still be observable today. We study the production of the GW background from freely decaying MHD turbulence for helical and nonhelical initial magnetic fields. To understand the produced GW spectra, we develop a simple model on the basis of the evolution of the magnetic stress tensor. We find that the GW spectra obtained in this model reproduce those obtained in numerical simulations if we consider the time evolution of the low frequency tail of the stress spectrum from numerical simulations. We also show that the shapes of the produced GW frequency spectra are different for helical and nonhelical cases for the same initial magnetic energy spectra. Such differences can help distinguish helical and nonhelical initial magnetic fields from a polarized background of GWs -- especially when the expected circular polarization cannot be detected directly.

@misc{sharma2022frequency, abstract = {Hydrodynamic and magnetohydrodynamic (MHD) turbulence in the early Universe can drive gravitational waves (GWs) and imprint their spectrum onto that of GWs, which might still be observable today. We study the production of the GW background from freely decaying MHD turbulence for helical and nonhelical initial magnetic fields. To understand the produced GW spectra, we develop a simple model on the basis of the evolution of the magnetic stress tensor. We find that the GW spectra obtained in this model reproduce those obtained in numerical simulations if we consider the time evolution of the low frequency tail of the stress spectrum from numerical simulations. We also show that the shapes of the produced GW frequency spectra are different for helical and nonhelical cases for the same initial magnetic energy spectra. Such differences can help distinguish helical and nonhelical initial magnetic fields from a polarized background of GWs -- especially when the expected circular polarization cannot be detected directly.}, added-at = {2022-06-06T05:50:31.000+0200}, author = {Sharma, Ramkishor and Brandenburg, Axel}, biburl = {https://www.bibsonomy.org/bibtex/2f12e99603910810da0791c7637d93cbe/ericblackman}, description = {Low frequency tail of gravitational wave spectra from hydromagnetic turbulence}, interhash = {8deb73f5c72b4c2eb2b2a3392e13fbb1}, intrahash = {f12e99603910810da0791c7637d93cbe}, keywords = {gw mhd turbulence}, note = {cite arxiv:2206.00055Comment: 12 pages, 12 figures, 2 tables}, timestamp = {2022-06-06T05:50:31.000+0200}, title = {Low frequency tail of gravitational wave spectra from hydromagnetic turbulence}, url = {http://arxiv.org/abs/2206.00055}, year = 2022 }