From 8b2083b53c5f897aed7292f005d35674a962594a Mon Sep 17 00:00:00 2001 From: Aaron LI Date: Sun, 22 Oct 2017 16:21:41 +0800 Subject: clusters/halo: Add "use_max_merger" option to allow use max merger events --- fg21sim/configs/20-extragalactic.conf.spec | 14 ++++++++++---- 1 file changed, 10 insertions(+), 4 deletions(-) (limited to 'fg21sim/configs') diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec index ea6479f..042a808 100644 --- a/fg21sim/configs/20-extragalactic.conf.spec +++ b/fg21sim/configs/20-extragalactic.conf.spec @@ -108,10 +108,6 @@ # Unit: [Msun] merger_mass_min = float(default=1e12, min=1e10, max=1e14) - # Mass ratio of the main and sub clusters, below which is regarded as - # a major merger event. - ratio_major = float(default=3.0, min=1.0, max=10.0) - # The merger timescale, which roughly describes the duration of the # merger-induced disturbance (~2-3 Gyr). This timescale is much longer # the merger crossing time (~1 Gyr), and is also longer than the lifetime @@ -119,6 +115,16 @@ # Unit: [Gyr] tau_merger = float(default=2.0, min=1.0, max=5.0) + # Mass ratio of the main and sub clusters, below which is regarded as + # a major merger event. + ratio_major = float(default=3.0, min=1.0, max=10.0) + + # Whether to use the maximum merger event (i.e., biggest mass of the + # sub cluster) within the above ``tau_merger`` timescale to simulate the + # subsequent radio halo simulation? Otherwise only the most recent major + # merger event will be used. + use_max_merger = boolean(default=False) + # The fraction of the magnetic field energy density w.r.t. the ICM # thermal energy density, which is used to determine the mean magnetic # field strength within the ICM and is also assumed to be uniform. -- cgit v1.2.2