https://orcid.org/0000-0002-7664-8490
Calculate extended gamma-ray source halo using crbeam simulation
This workflow provides a calculaiton of the power spectrum of Stochastic Gravitational Wave Backgorund (SGWB) from a first-order cosmological phase transition based on the parameterisations of Roper Pol et al. (2023). The power spectrum includes two components: from the sound waves excited by collisions of bubbles of the new phase and from the turbulence that is induced by these collisions.
The cosmological epoch of the phase transition is described by the temperature, T_star and by the number(s) ...
The tool provides a calculation of the power spectrum of Stochastic Gravitational Wave Backgorund (SGWB) from a first-order cosmological phase transition based on the parameterisations of Roper Pol et al. (2023). The power spectrum includes two components: from the sound waves excited by collisions of bubbles of the new phase and from the turbulence that is induced by these collisions.
The cosmological epoch of the phase transition is described by the temperature, T_star and by the number(s) of ...
Type: Galaxy
Creators: Andrii Neronov, Théo Boyer, Denys Savchenko, Volodymyr Savchenko
Submitter: Denys Savchenko
Protype demonstrator of a workflow reducing HESS and INTEGRAL/SPI-ACS data to common Light Curve format and combining the lightcurves into a multi-wavelength observation.
Type: Galaxy
Creators: Volodymyr Savchenko, Denys Savchenko, Andrii Neronov
Submitter: Volodymyr Savchenko
