| Commit message (Collapse) | Author | Age | Files | Lines |
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Adopt the same beta-model for the gas density profile to calculate the
gas/baryon mass within the turbulence region (<R_turb).
Meanwhile, change the '_velocity_turb()` method to a property without
depending on the time, to further simplify the model a bit.
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This function calculates the stripping radius of the sub-cluster when it
falling through the main cluster.
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The "merger_mass1", "merger_mass2", "merger_z", and "merger_age" may be NumPy
arrays, e.g., the catalog data are manually modified.
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* time_turbulence_avg
* mach_turbulence_avg
* tau_acceleration_avg
* time_acceleration_fraction
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Change "tau_acceleration" from a attribute to a method with the time
parameter, and then simplify "fp_diffusion()" method.
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The RadioHaloAM class is intended to account for all merger events, and there
are a lot of methods to be implemented.
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Add emission.HaloEmission class to calculate halo emissivity, power, flux,
brightness etc.
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