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* clusters/halo: Support to calculate the fiducial electron spectrumAaron LI2018-10-311-7/+20
| | | | | | | The fiducial electron spectrum is the one that is derived with the turbulent acceleration turned off. It can be used to determine whether the acceleration is indeed effective for one cluster and then further determine whether the radio halo is formed/observable.
* clusters/halo: Simplify calc_electron_spectrum()Aaron LI2018-10-311-49/+6
| | | | | | | | Get rid of the 'electron_spec' property and the set_electron_spectrum() function. Simplify the calc_electron_spectrum() by removing the step adjustment. Other minor cleanups.
* clusters/halo: Rework the way to disable turbulent accelerationAaron LI2018-10-311-16/+13
| | | | | | Introduce a new property '_acceleration_disabled' to control whether the turbulent acceleration is disabled. With this new property, improve the code to derive the initial electron spectrum.
* clusters/halo: Use _is_turb_active() in fp_advection()Aaron LI2018-10-311-14/+6
| | | | Some other minor cleanups.
* clusters/halo: Add time argument to radius_turbulence()Aaron LI2018-10-311-10/+8
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* clusters/halo: Add time argument to _velocity_turb()Aaron LI2018-10-311-10/+10
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* clusters/halo: Add time argument to _gas_density_profile_t()Aaron LI2018-10-311-4/+6
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* clusters/halo: Rename 'injection_radius' to 'radius_turbulence'Aaron LI2018-10-301-16/+16
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* clusters/halo: Update time_turbulence() calculationAaron LI2018-10-302-28/+10
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* clusters/helper: Remove the obsolete fmass_nfw()Aaron LI2018-10-301-26/+0
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* clusters/halo: Update turbulence velocity calculationAaron LI2018-10-301-26/+40
| | | | | | | | 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.
* clusters/halo: Update calculations of injection and halo radiusAaron LI2018-10-302-36/+13
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* Deprecate the pointsource component (2)Aaron LI2018-10-301-2/+1
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* clusters/help: Add radius_stripping()Aaron LI2018-10-261-6/+73
| | | | | This function calculates the stripping radius of the sub-cluster when it falling through the main cluster.
* clusters/halo: Improve descriptions and commentsAaron LI2018-10-252-20/+16
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* clusters/halo: Change _merger() to accept time to simplify its usageAaron LI2018-10-251-12/+12
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* clusters/halo: Simplify the code a bitAaron LI2018-10-251-18/+8
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* clusters/halo: Fix a wrong variable in a logging messageAaron LI2018-10-251-6/+4
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* clusters/main: Minor improvementsAaron LI2018-10-241-13/+11
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* clusters: Add parameter felong_minAaron LI2018-05-221-3/+3
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* clusters: Fix cluster distribution calculation about massAaron LI2018-05-121-14/+8
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* cluster/formation: Fix merger tree simulation about cluster massAaron LI2018-05-111-24/+22
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* cluster/formation: update zmax default valueAaron LI2018-03-081-2/+2
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* cluster/formation: merger tree simulation should use dark matter massesAaron LI2018-03-031-41/+34
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* clusters: Fix dropout handlingAaron LI2018-02-031-8/+7
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* clusters: improve dropout handlingAaron LI2018-01-281-10/+26
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* clusters: calculate/save cosmic (~cluster) age to catalog & halos dataAaron LI2018-01-221-1/+6
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* clusters: coerce to plain list for concatenationAaron LI2018-01-221-4/+8
| | | | | The "merger_mass1", "merger_mass2", "merger_z", and "merger_age" may be NumPy arrays, e.g., the catalog data are manually modified.
* clusters/halo: most consistent turbulent acceleration and time calculationsAaron LI2018-01-212-3/+3
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* clusters/halo: simplify energy loss calculationsAaron LI2018-01-211-27/+14
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* clusters/emission: improve description symbols :-)Aaron LI2018-01-211-4/+4
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* clusters: minor updatesAaron LI2018-01-161-5/+4
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* clusters/main: minor cleanupsAaron LI2018-01-111-10/+8
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* clusters/halo: fix _is_turb_active() bool conditionAaron LI2018-01-061-2/+2
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* clusters: fix string formatting in _simulate_halos()Aaron LI2018-01-051-1/+1
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* clusters: small cleanupsAaron LI2018-01-052-12/+18
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* clusters/halo: fix self.time_step errorAaron LI2018-01-051-4/+4
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* clusters/halo: fix _merger_time() error when t < age_beginAaron LI2018-01-051-2/+7
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* clusters: update _simulate_halos() with new halo propertiesAaron LI2018-01-051-11/+9
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* clusters/halo: calculate several time-averaged propertiesAaron LI2018-01-051-0/+54
| | | | | | | * time_turbulence_avg * mach_turbulence_avg * tau_acceleration_avg * time_acceleration_fraction
* clusters/halo: move tau_max and time dependence to tau_acceleration()Aaron LI2018-01-051-27/+27
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* clusters/halo: add _is_turb_active(), update _velocity_turb() etc.Aaron LI2018-01-051-12/+29
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* clusters/halo: update turbulence acceleration calc. with _merger_time()Aaron LI2018-01-051-28/+20
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* clusters/halo: add _merger_time() and mass_sub() methodsAaron LI2018-01-051-0/+31
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* clusters/halo: refactor tau_acceleration() to help RadioHaloAMAaron LI2018-01-042-25/+39
| | | | | Change "tau_acceleration" from a attribute to a method with the time parameter, and then simplify "fp_diffusion()" method.
* clusters/halo: Add preliminary RadioHaloAM based on RadioHaloAaron LI2018-01-042-12/+115
| | | | | The RadioHaloAM class is intended to account for all merger events, and there are a lot of methods to be implemented.
* clusters/halo: small updates and some cleanupsAaron LI2018-01-042-60/+45
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* clusters/halo: minor cleanupsAaron LI2018-01-031-14/+15
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* clusters/halo: change "age_merger" to "age_begin"Aaron LI2018-01-031-23/+26
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* clusters/halo: update radius_halo() calculationAaron LI2018-01-032-15/+7
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