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* configs/spec: Tweak gamma_max and gamma_npAaron LI2019-01-271-3/+3
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* clusters/halo: Tweak radius_turb() calculationAaron LI2019-01-271-4/+3
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* clusters/main: Calculate acceleration factorAaron LI2019-01-271-0/+2
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* clusters/halo: Rewrite is_genuine() to be calc_acc_factor()Aaron LI2019-01-272-23/+10
| | | | | | | Calculate the bolometric emissivity instead of the emissivity at a certain frequency. This should capture the acceleration effect more effectively. In addition, remove the now obsolete config options "fiducial_freq" and "fiducial_factor".
* clusters/emission: Add calc_emissivity_bolo()Aaron LI2019-01-271-6/+33
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* clusters/halo: Delete the RadioHalo wrapper classAaron LI2019-01-271-92/+0
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* clusters/halo: Implement calc_electron_spectrum() for multiple mergersAaron LI2019-01-271-0/+118
| | | | | | | For a cluster with multiple mergers, each merger has a different turbulence radius, so the accelerated spectrum needs appropriate adjustment to take the (may be significant) variation of turbulence radius into account.
* clusters/helper: Add simple density_number_electron()Aaron LI2019-01-271-0/+8
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* clusters/halo: Implement radius_turb_eff() methodAaron LI2019-01-271-0/+27
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* clusters/halo: Add 'radius_turb_max' propertyAaron LI2019-01-271-2/+10
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* clusters/halo: Tweak {duration,velocity}_turb()Aaron LI2019-01-261-8/+7
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* clusters/main: Adjust against halo radiusAaron LI2019-01-261-4/+3
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* clusters/halo: Reimplement the 'radius' propertyAaron LI2019-01-261-6/+11
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* clusters/halo: Reorder radius_{strip,turb}()Aaron LI2019-01-261-35/+35
| | | | | Rename radius_stripping() to radius_strip() and radius_turbulence() to radius_turb().
* clusters/halo: Clean up mass_main() methodAaron LI2019-01-261-12/+3
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* clusters/halo: Rewrite _merger_time() to get the effective mergerAaron LI2019-01-261-8/+24
| | | | | If the acceleration durations of multiple mergers overlap, the one with the largest efficiency (i.e., smallest tau_acc) is chosen.
* clusters/halo: Replace "age" with "t" (time)Aaron LI2019-01-261-31/+31
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* clusters/main: Replace "age" with "t" (time)Aaron LI2019-01-261-6/+6
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* clusters/halo: Fold _merger_idx() into _merger_event()Aaron LI2019-01-261-18/+11
| | | | Update _merger_time() accordingly.
* clusters/halo: Move and rename _velocity_turb() to _velocity_turb()Aaron LI2019-01-261-57/+57
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* clusters/halo: Rename _merger() to _merger_event()Aaron LI2019-01-261-4/+4
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* clusters/halo: Remove *_avg and *_fraction methodsAaron LI2019-01-262-54/+0
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* clusters/halo: Use t_merger for duration_turb() and mach_turb()Aaron LI2019-01-261-4/+6
| | | | Rename mach_turbulence() to mach_turb().
* clusters/halo: Simplify tau_acceleration() methodAaron LI2019-01-261-45/+14
| | | | Move the turbulence activity check into the fp_diffusion() method.
* clusters/halo: Some cleanupsAaron LI2019-01-261-28/+15
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* clusters/halo: Use t_merger to be more explicitAaron LI2019-01-261-13/+25
| | | | | Add _validate_t_merger() method to validate the given time to be an merger time.
* clusters/halo: Rename time_turbulence() to duration_turb()Aaron LI2019-01-262-11/+10
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* configs/spec: Various minor tweaksAaron LI2019-01-251-31/+32
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* clusters/halo: Fold _rho_gas_f() into _velocity_turb()Aaron LI2019-01-251-20/+8
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* clusters/halo: Account for mass scaling in tau_acceleration()Aaron LI2019-01-252-0/+22
| | | | Add configuration option "mass_index" to specify the scaling index.
* clusters/halo: Fold parameter "zeta_ins" into "f_acc"Aaron LI2019-01-252-10/+5
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* clusters/halo: Clean up tau_acceleration() methodAaron LI2019-01-251-14/+13
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* clusters: Assume equipartition between B field and CRAaron LI2019-01-253-16/+18
| | | | | | Equipartition between the magnetic fields and cosmic rays is assumed, i.e., eta_b == x_cr. Therefore remove "extragalactic/clusters/eta_b" configuration option.
* clusters/helper: Add plasma_beta() functionAaron LI2019-01-231-0/+26
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* clusters/helper: Do not pass the whole configs to functionsAaron LI2019-01-232-14/+40
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* clusters/helper: Fix a variable error in density_gas()Aaron LI2019-01-221-1/+1
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* clusters/helper: Add radius_overdensity() functionAaron LI2019-01-211-4/+29
| | | | e.g., to calculate R200, R500.
* clusters/helper: Improve density_energy_electron() calculationAaron LI2019-01-211-4/+4
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* clusters/helper: Add density_gas() functionAaron LI2019-01-211-0/+8
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* Update copyright yearAaron LI2019-01-191-1/+1
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* Purge obsolete pointsourcesAaron LI2019-01-199-1840/+0
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* clusters/halo: Minor cleanupAaron LI2019-01-191-4/+1
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* clusters/halo: Update turbulence velocity dispersion calcuationAaron LI2019-01-181-7/+6
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* clusters/halo: Update time_turbulence() calculationAaron LI2019-01-181-8/+9
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* clusters/helper: Pass beta to helper.radius_stripping()Aaron LI2019-01-182-7/+9
| | | | | * Add 'beta' parameter to radius_stripping() * Pass 'f_rc' and 'beta' to calc_gas_density_profile()
* Minor tweaksAaron LI2019-01-183-7/+8
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* cosmology: Update virial overdensity calculationAaron LI2019-01-171-10/+16
| | | | | | References: * https://en.wikipedia.org/wiki/Virial_mass * http://adsabs.harvard.edu/abs/1998ApJ...495...80B
* clusters/halo: Update the estimation of radius_turbulence()Aaron LI2019-01-171-4/+8
| | | | | The radius_turbulence is estimated as the stripping radius (r_s) if r_s is larger than the core radius (r_c) of the main cluster, otherwise, r_c.
* clusters/main: Account for baryon fraction in _simulate_mergers()Aaron LI2019-01-171-3/+4
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* clusters/main: Account for baryon fraction in _simulate_catalog()Aaron LI2019-01-172-6/+11
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