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<title>fg21sim.git/fg21sim/extragalactic/clusters, branch v0.6.4</title>
<subtitle>Simulate foreground for 21cm EoR signal detection
</subtitle>
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<entry>
<title>clusters/halo: Add back "mach_turbulence" attribute</title>
<updated>2017-12-31T09:13:49+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-31T09:13:49+00:00</published>
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</entry>
<entry>
<title>clusters/halo: Rework the turbulence acceleration timescale calculation</title>
<updated>2017-12-31T08:36:56+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-31T08:36:56+00:00</published>
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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).
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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).
</pre>
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</content>
</entry>
<entry>
<title>clusters/halo: calc turbulence velocity dispersion based on merger</title>
<updated>2017-12-31T08:34:55+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-31T08:34:55+00:00</published>
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Also update the description of option "extragalactic/halos/eta_turb"
and change its default value to 0.1
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Also update the description of option "extragalactic/halos/eta_turb"
and change its default value to 0.1
</pre>
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</content>
</entry>
<entry>
<title>clusters/halo/helper: Add fmass_nfw() to calc NFW mass profile</title>
<updated>2017-12-31T08:29:51+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-31T08:29:51+00:00</published>
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</entry>
<entry>
<title>Minor cleanups</title>
<updated>2017-12-31T08:29:28+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T16:06:05+00:00</published>
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<entry>
<title>Minor cleanups</title>
<updated>2017-12-30T12:52:30+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T12:52:30+00:00</published>
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</entry>
<entry>
<title>clusters/halo: support to drop out the most powerful halos</title>
<updated>2017-12-30T12:52:17+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T12:23:52+00:00</published>
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The new option "extragalactic/clusters/halo_dropout" is added to specify how
many halos to be dropped out.
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The new option "extragalactic/clusters/halo_dropout" is added to specify how
many halos to be dropped out.
</pre>
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</entry>
<entry>
<title>clusters/halo: Add virial_speed() helper function</title>
<updated>2017-12-30T12:23:02+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T12:23:02+00:00</published>
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</entry>
<entry>
<title>clusters/halo: Estimate turbulence acceleration w.r.t. injection scale</title>
<updated>2017-12-30T12:21:48+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T12:21:48+00:00</published>
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<content type='text'>
The turbulence injection scale ~ halo size
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The turbulence injection scale ~ halo size
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</entry>
<entry>
<title>cluster/halo: Estimate halo radius ~ 0.33*R_vir (main cluster)</title>
<updated>2017-12-30T12:18:50+00:00</updated>
<author>
<name>Aaron LI</name>
<email>aly@aaronly.me</email>
</author>
<published>2017-12-30T12:18:50+00:00</published>
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