| Commit message (Collapse) | Author | Age | Files | Lines |
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Calculate the synchrotron power (a.k.a. specific luminosity) and flux
density from the emissivity for the halo.
Signed-off-by: Aaron LI <aly@aaronly.me>
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This method invokes ``SynchrotronEmission`` to calculate the synchrotron
emissivity at specified frequencies for the derived electron spectrum.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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NOTE:
Since we just substitute ``p`` (electron momentum) for
``γ`` (electron Lorentz factor), i.e.,
N = int_p n(p) dp = int_γ n(γ) dγ ,
therefore the coefficient ``sqrt(3) e^3 B / (m c^2)`` does NOT need
modification (e.g., multiply an extra ``m c``)!
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Use 2D grid of (discrete) samples to optimize integration speed,
avoiding the more complicated integration w.r.t. functions.
WARNING:
Current calculation results seems wrong!
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Use interpolation to optimize the speed as well as to vectorize the
function to ease calling.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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This configuration option "beta_turb" has different meaning as
"eta_turb" in [Cassano & Brunetti 2005], though they can both be an
indicator for the turbulence acceleration efficiency.
Rename this configuration option to make the difference more clear.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Zero or negative diffusion coefficient leads to unstable or wrong
results due to numerical algorithm/scheme adopted to solve the
Fokker-Planck equation.
Also add a NOTE to the FokkerPlanckSolver class.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Update to use the global CONFIGS and COSMO
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Import the global "configs" in helper.py to make parameters lean.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Still WIP...
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Several methods/functions have been migrated into "helper.py", while
other methods/functions are obsolete.
Signed-off-by: Aaron LI <aly@aaronly.me>
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TODO:
adaptively determine the proper time step instead of using a
constant one.
Signed-off-by: Aaron LI <aly@aaronly.me>
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The "clusters.py" is deprecated and will be deleted later.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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And update the config specification accordingly with some cleanups.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Also update the configurations
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Simulate the formation history of each cluster and identify the
last/recent major merger event.
Also add new configuration option "tau_merger" and tweak several
configurations options.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Since the ``ClusterFormation`` is repeatedly invoked in
``GalaxyClusters``, so make the verbose information printed only at
DEBUG level.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Also calculate and add the mass ratio to the event dictionary.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Do not modify the root node of the merger tree, and return this root
node after tracing the formation history.
Also print some more information for debug.
Signed-off-by: Aaron LI <aly@aaronly.me>
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This function traces the main cluster and print its formation history to
the screen, for easier illustration and examination.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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A new parameter "ratio_major" added to distinguish between major and
minor merger events.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Also update "simulate_megertree()" default to trace only the main cluster.
Signed-off-by: Aaron LI <aly@aaronly.me>
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Signed-off-by: Aaron LI <aly@aaronly.me>
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