Commit message (Collapse) | Author | Age | Files | Lines | |
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* | Bump version to 0.6.4v0.6.4 | Aaron LI | 2017-12-31 | 1 | -2/+2 |
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* | clusters/halo: Add back "mach_turbulence" attribute | Aaron LI | 2017-12-31 | 2 | -4/+15 |
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* | clusters/halo: Rework the turbulence acceleration timescale calculation | Aaron LI | 2017-12-31 | 2 | -49/+53 |
| | | | | | | | | The new method adopted to determine the turbulence acceleration timescale follows [miniati2015] and [pinzke2017], in which the merger-induced turbulence cascades into small scales (and thus accelerate electrons) through the TTD (transit-time damping) mechanism by scattering mainly with the relativistic particles (cosmic-ray protons and electrons). | ||||
* | clusters/halo: calc turbulence velocity dispersion based on merger | Aaron LI | 2017-12-31 | 2 | -9/+41 |
| | | | | | Also update the description of option "extragalactic/halos/eta_turb" and change its default value to 0.1 | ||||
* | clusters/halo/helper: Add fmass_nfw() to calc NFW mass profile | Aaron LI | 2017-12-31 | 1 | -0/+30 |
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* | Minor cleanups | Aaron LI | 2017-12-31 | 2 | -13/+24 |
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* | Minor cleanups | Aaron LI | 2017-12-30 | 2 | -6/+6 |
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* | clusters/halo: support to drop out the most powerful halos | Aaron LI | 2017-12-30 | 2 | -0/+29 |
| | | | | | The new option "extragalactic/clusters/halo_dropout" is added to specify how many halos to be dropped out. | ||||
* | clusters/halo: Add virial_speed() helper function | Aaron LI | 2017-12-30 | 1 | -2/+13 |
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* | clusters/halo: Estimate turbulence acceleration w.r.t. injection scale | Aaron LI | 2017-12-30 | 3 | -16/+39 |
| | | | | The turbulence injection scale ~ halo size | ||||
* | cluster/halo: Estimate halo radius ~ 0.33*R_vir (main cluster) | Aaron LI | 2017-12-30 | 3 | -10/+20 |
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* | clusters/halo: Tune the maximum acceleration timescale to 10 Gyr | Aaron LI | 2017-11-16 | 1 | -6/+17 |
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* | logging: report line numbers to help debug | Aaron LI | 2017-11-16 | 1 | -1/+1 |
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* | clusters/halo: improve advection calculation | Aaron LI | 2017-11-16 | 1 | -10/+10 |
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* | Deprecate np.int, np.float | Aaron LI | 2017-11-03 | 4 | -9/+9 |
| | | | | See: https://github.com/numpy/numpy/pull/6103 | ||||
* | fg21sim: Bump version to 0.6.3v0.6.3 | Aaron LI | 2017-10-30 | 2 | -6/+6 |
| | | | | | * Update the __init__ description a bit * Add the missing parameter change for ``f_acc`` | ||||
* | clusters/halo: Tune default parameters | Aaron LI | 2017-10-30 | 1 | -4/+4 |
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* | products.py: Add a note about updating against with sky.py | Aaron LI | 2017-10-29 | 1 | -1/+3 |
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* | Update logging messages | Aaron LI | 2017-10-29 | 2 | -3/+5 |
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* | clusters/configs: Update f_acc default to 1.0; also update descriptions | Aaron LI | 2017-10-26 | 2 | -2/+8 |
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* | utils/grid.py: Disable Numba JIT for make_ellipse() & make_grid_ellipse() | Aaron LI | 2017-10-26 | 1 | -8/+0 |
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* | clusters/halo: Calc turbulence injection scale w.r.t. sub-cluster radius | Aaron LI | 2017-10-26 | 1 | -6/+8 |
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* | configs: update option "gamma_min" default to 1 (old: 10) | Aaron LI | 2017-10-25 | 1 | -1/+3 |
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* | clusters/solver: Update buffer_np description and handling | Aaron LI | 2017-10-25 | 2 | -4/+11 |
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* | clusters/solver: Remove an empty method | Aaron LI | 2017-10-25 | 1 | -8/+0 |
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* | clusters/halo: Fix fp_advection() w.r.t. initial electron spectrum calc. | Aaron LI | 2017-10-25 | 1 | -2/+4 |
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* | clusters/halo: Adjust initial electron spectrum calculation | Aaron LI | 2017-10-25 | 2 | -5/+7 |
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* | configs: two small changes; set time_step default to 0.01 | Aaron LI | 2017-10-25 | 1 | -4/+5 |
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* | clusters/halo: Add method to derive the initial electron spectrum | Aaron LI | 2017-10-25 | 2 | -11/+56 |
| | | | | | Also add the option "time_init" to control how long a period is used to derive the initial electron spectrum. | ||||
* | clusters/halo: Fix passing the "configs" object | Aaron LI | 2017-10-25 | 2 | -4/+6 |
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* | clusters/halo: Always pass the using configs | Aaron LI | 2017-10-24 | 2 | -9/+12 |
| | | | | | The user-using `configs` object may be different to the global `CONFIGS`, which may be forgotten to load the up-to-date user configurations. | ||||
* | configs: Add parameter "reset" to "read_userconfig()" | Aaron LI | 2017-10-24 | 1 | -12/+20 |
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* | configs: add __getitem__() and __setitem__() methods | Aaron LI | 2017-10-24 | 1 | -1/+8 |
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* | clusters/halo: Change zbegin/zend to tstart/tsop (use cosmic time) | Aaron LI | 2017-10-24 | 1 | -19/+20 |
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* | clusters/halo: Add method "_magnetic_field()" | Aaron LI | 2017-10-24 | 1 | -2/+23 |
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* | clusters/halo: Rename property "magnetic_field" to "B_obs" | Aaron LI | 2017-10-24 | 2 | -4/+4 |
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* | clusters/halo: Allow specify magnetic field in calc_emissivity() | Aaron LI | 2017-10-24 | 1 | -9/+14 |
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* | clusters/halos: Fix halo radius calculation | Aaron LI | 2017-10-23 | 1 | -3/+5 |
| | | | | Also change the parameter "nr" default to 2.0 for draw_halo() function. | ||||
* | clusters/psformalism: Use functools.lru_cache() | Aaron LI | 2017-10-23 | 1 | -0/+3 |
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* | clusters/halo: merge halo_rprofile() & draw_halo(); Fix halo radius error | Aaron LI | 2017-10-23 | 2 | -40/+28 |
| | | | | | | | * Fix the error that misses to divide the halo radius by 3 for the e-folding radius, which causes the generated halo image has a 3x size! * Merge function "halo_rprofile()" into "draw_halo()" * Skip transform circular halo into elliptical one if "felong" is None | ||||
* | utils/transform/circle2ellipse: skip rotation if it's None | Aaron LI | 2017-10-23 | 1 | -4/+5 |
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* | clusters/halo: Use "lru_cache()", also improves some performance | Aaron LI | 2017-10-23 | 3 | -13/+26 |
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* | clusters/formation: Fix problem that no mergers occurred | Aaron LI | 2017-10-22 | 2 | -2/+9 |
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* | clusters/halo: Add "use_max_merger" option to allow use max merger events | Aaron LI | 2017-10-22 | 2 | -24/+40 |
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* | clusters/formation: Add method to found the maximum merger event | Aaron LI | 2017-10-22 | 1 | -1/+51 |
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* | clusters/halo: Add option "kT_out" to tune cluster temperature | Aaron LI | 2017-10-22 | 3 | -5/+16 |
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* | configs: Update option description | Aaron LI | 2017-10-21 | 1 | -4/+5 |
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* | clusters/halo: Rewrite turbulence acceleration & diffusion coefficient! | Aaron LI | 2017-10-21 | 3 | -60/+104 |
| | | | | | | | | | | | | The previous calculation of the turbulence acceleration efficiency has significant problems, which is too low, i.e., the acceleration timescale is too large (~10 Gyr). However, it is reported that turbulent acceleration has a timescale ~100 Myr (0.1 Gyr). I believe this problem is due to the over-simplification to the formula proposed by [cassano2005]. Rewrite the turbulence acceleration and diffusion coefficient calculations, adopting the method proposed by [brunetti2016]. To this end, two new options "f_lturb" and "f_acc" are introduced to tune the results. | ||||
* | clusters/halos: Add more cluster and halo properties | Aaron LI | 2017-10-21 | 2 | -12/+39 |
| | | | | | | * Rvir0, Rvir_main, Rvir_sub * kT_main, kT_sub (replace kT_merger) * radius -> Rhalo, angular_radius -> Rhalo_angular, B -> B0 | ||||
* | clusters: Fix a comment about "felong" | Aaron LI | 2017-10-21 | 1 | -2/+1 |
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