Commit message (Collapse) | Author | Age | Files | Lines | |
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* | clusters: Move units.py and cosmology.py to utils | Aaron LI | 2017-06-01 | 1 | -2/+4 |
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* | clusters/halo.py: Add zbegin & zend parameters | Aaron LI | 2017-06-01 | 1 | -3/+37 |
| | | | | | * Add "zbegin" and "zend" parameters to "calculate_electron_spectrum()" * Add more detail docstrings | ||||
* | halo.py: Rewrite "_coef_acceleration()" method | Aaron LI | 2017-06-01 | 1 | -15/+44 |
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* | Bind ClusterFormation to HaloSingle | Aaron LI | 2017-06-01 | 1 | -1/+4 |
| | | | | Also add logging messages to simulate_mergertree() | ||||
* | Update to use custom units.py instead of astropy's | Aaron LI | 2017-06-01 | 1 | -40/+26 |
| | | | | Also fix a parameter error in "formation.py" | ||||
* | halo.py: Update to match MergerTree structures | Aaron LI | 2017-06-01 | 1 | -8/+8 |
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* | halo.py: Force a minimal value on acceleration coefficient | Aaron LI | 2017-06-01 | 1 | -1/+25 |
| | | | | | | | To avoid the too small (or zero) values for the diffusion coefficient of the Fokker-Planck equation. Also change config "extragalactic/halo/pmax" from 1e4 to 1e5 | ||||
* | clusters/halo: Add missing config "buffer_np" | Aaron LI | 2017-06-01 | 1 | -0/+2 |
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* | Add clusters/halo.py: simulate single halo for cluster | Aaron LI | 2017-06-01 | 1 | -0/+698 |
Simulate (giant) radio halos following the "statistical magneto-turbulent model" proposed by Cassano & Brunetti (2005). |