Improved output and config
This commit is contained in:
Yohai Meiron
parent
5cb4282be4
commit
62b0d7e491
6 changed files with 126 additions and 107 deletions
188
phigrape.conf
188
phigrape.conf
|
|
@ -8,8 +8,8 @@ eps = 1E-4
|
|||
# End time of the calculation
|
||||
t_end = 0.25
|
||||
|
||||
# Interval of snapshot files output (xxxxxx.dat)
|
||||
dt_disk = 1.0
|
||||
# Interval of snapshot files output
|
||||
dt_disk = 0.125
|
||||
|
||||
# Interval for the energy control output (contr.dat)
|
||||
dt_contr = 0.125
|
||||
|
|
@ -20,100 +20,132 @@ dt_bh = 0.125
|
|||
# Parameter for timestep determination
|
||||
eta = 0.01
|
||||
|
||||
# Name of the input file; use "data.con" in most cases
|
||||
# Name of the input file; use "data.con" in most cases [default: data.con]
|
||||
input_file_name = data.con
|
||||
|
||||
output_hdf5 = true
|
||||
|
||||
##### NOT IMPLEMENTED #######################
|
||||
dt_min_warning = false
|
||||
#############################################
|
||||
##########
|
||||
# OUTPUT #
|
||||
##########
|
||||
|
||||
# Whether to use HDF5 format for snapshot and restart; regular ASCII snapshorts are saved if false [default: false]
|
||||
#output_hdf5 = true
|
||||
|
||||
# If using HDF5 output, use double precision or not [default: true]
|
||||
# Consider setting to false to save disk space. Restart file is always saved in double precision.
|
||||
#output_hdf5_double_precision = true
|
||||
|
||||
# If using ASCII output, the number of digits after the decimal point [default: 10]
|
||||
# Restart file is saved with 16 digits after the decimal point.
|
||||
#output_ascii_precision = 6
|
||||
|
||||
# Extra output: optionally save potential, acceleration and jerk in snapshot files [default: 0]
|
||||
# This is a number between 0 and 7 that encodes the output options in the following way:
|
||||
# [value] = [save jerk]*4 + [save acceleration]*2 + [save potential]
|
||||
# Example: choose 5 if it is needed to save the jerk and the potential, but not the acceleration for some reason.
|
||||
# Currently implemented in HDF5 output only.
|
||||
#output_extra_mode = 7
|
||||
|
||||
# Whether to output a warning on the screen when the minimum time step is encountered. [default: false]
|
||||
#dt_min_warning = false
|
||||
|
||||
####################
|
||||
# EXTERNAL GRAVITY #
|
||||
####################
|
||||
|
||||
ext_units_physical = false
|
||||
#unit_mass = 1e5
|
||||
#unit_length = 10
|
||||
# TODO add the option to normalize using other units
|
||||
# Remember that external gravity models are applied at the same coordinate system as the particles. If the idea is to simulate a globular cluster orbiting in an external field, be sure to set the initial conditions appropriately (applying a shift to the coordinates and velocities).
|
||||
|
||||
# Notice that if physical units are used, the "a" and "b" parameters are in kiloparsec, not parsec!
|
||||
# Whether the parameters for the external gravitational field given below are in physical units or Hénon units. If true, the system used is {kiloparsec, solar mass, kilometre per second} [default: false]
|
||||
#ext_units_physical = true
|
||||
|
||||
ext_m_bulge = 0
|
||||
ext_b_bulge = 0
|
||||
ext_m_disk = 0
|
||||
ext_a_disk = 0
|
||||
ext_b_disk = 0
|
||||
ext_m_halo_plummer = 0
|
||||
ext_b_halo_plummer = 0
|
||||
ext_log_halo_v = 0
|
||||
# here the length scale for the logarithmic halo is in kpc, not pc like in the old phigrape.
|
||||
ext_log_halo_r = 0
|
||||
# If Physical units were selected, specify the simulation's unit mass (is solar masses) and unit lenght (in parsec; not kiloparsec)
|
||||
# TODO: add the option to normalize using other units.
|
||||
#unit_mass = 4E5 # MSun
|
||||
#unit_length = 15 # pc
|
||||
|
||||
|
||||
# The bulge is a Plummer potential with the following total mass and radius.
|
||||
#ext_m_bulge = 5E9 # MSun
|
||||
#ext_b_bulge = 1.9 # kpc
|
||||
|
||||
|
||||
# The disk is a Miyamoto-Nagai potential with the following total mass, scale length, and scale height
|
||||
#ext_m_disk = 6.8E10 # MSun
|
||||
#ext_a_disk = 3.00 # kpc
|
||||
#ext_b_disk = 0.28 # kpc
|
||||
|
||||
|
||||
# This halo option is yet another Plummer potential with the following total mass and radius.
|
||||
#ext_m_halo_plummer = 8E11 # MSun
|
||||
#ext_b_halo_plummer = 245 # kpc
|
||||
|
||||
|
||||
# This halo option is a logarithmic potential with the following velocity and radius parameters.
|
||||
#ext_log_halo_v = 240 # km/s
|
||||
#ext_log_halo_r = 1 # kpc
|
||||
|
||||
|
||||
|
||||
####################################
|
||||
## LIVE SUPERMASSIVE BLACK HOLE(S) #
|
||||
####################################
|
||||
#
|
||||
## There is special treatment for particles representing supermassive black holes (SMBHs): they are integrated at every time step, they can have custom softening in SMBH-SMBH interactions, and post Newtonian terms can be added to the gravity.
|
||||
#
|
||||
## The number of SMBH particles. Can be 0 (no SMBH), 1, or 2. [default: 0]
|
||||
#live_smbh_count = 0
|
||||
#
|
||||
## Custom softening length for SMBH-SMBH interactions (can also be zero). If non-negative, the custom softening is applied. [default: -1]
|
||||
###################################
|
||||
# LIVE SUPERMASSIVE BLACK HOLE(S) #
|
||||
###################################
|
||||
|
||||
# There is special treatment for particles representing supermassive black holes (SMBHs): they are integrated at every time step, they can have custom softening in SMBH-SMBH interactions, and post Newtonian terms can be added to the gravity.
|
||||
|
||||
# The number of SMBH particles. Can be 0 (no SMBH), 1, or 2. [default: 0]
|
||||
#live_smbh_count = 2
|
||||
|
||||
# Custom softening length for SMBH-SMBH interactions (can also be zero). If non-negative, the custom softening is applied. [default: -1]
|
||||
#live_smbh_custom_eps = 0
|
||||
#
|
||||
## Output additional diagnostics about live SMBHs. [default: false]
|
||||
##TODO# dt_bh
|
||||
|
||||
# Output additional diagnostics about live SMBHs. [default: false]
|
||||
#live_smbh_output = true
|
||||
#
|
||||
## Output additional diagnostics about the SMBH's (or SMBHs') nearest neighbours (number could be set as shown below). [default: false]
|
||||
|
||||
# Output additional diagnostics about the SMBH's (or SMBHs') nearest neighbours (number could be set as shown below). [default: false]
|
||||
#live_smbh_neighbor_output = true
|
||||
#
|
||||
## Number of nearest neighbours to the SMBH (or SMBHs) to include in output. [default: 10]
|
||||
|
||||
# Number of nearest neighbours to the SMBH (or SMBHs) to include in output. [default: 10]
|
||||
#live_smbh_neighbor_number = 10
|
||||
#
|
||||
###################################
|
||||
## BINARY SUPERMASSIVE BLACK HOLE #
|
||||
###################################
|
||||
#
|
||||
## The following parameters can be set when `live_smbh_count` is 2.
|
||||
#
|
||||
## Output additional diagnostics about the SMBH's sphere of influence (size could be set as shown below). [default: false]
|
||||
|
||||
##################################
|
||||
# BINARY SUPERMASSIVE BLACK HOLE #
|
||||
##################################
|
||||
|
||||
# The following parameters can be set when live_smbh_count is 2.
|
||||
|
||||
# Output additional diagnostics about the sphere of influence (size could be set as shown below). [default: false]
|
||||
#binary_smbh_influence_sphere_output = true
|
||||
#
|
||||
## The influence sphere is centred at the binary SMBH's centre of mass, and its radius is the semi-major axis of the binary times the factor below. [default: 10.0]
|
||||
#binary_smbh_influence_radius_factor = 3.162277660168379497918067e+03
|
||||
#
|
||||
## Add post Newtonian terms to SMBH-SMBH gravity. [default: false]
|
||||
|
||||
# The influence sphere is centred at the binary SMBH's centre of mass, and its radius is the semi-major axis of the binary times the factor below. [default: 10]
|
||||
#binary_smbh_influence_radius_factor = 10
|
||||
|
||||
# Add post Newtonian terms to SMBH-SMBH gravity. [default: false]
|
||||
#binary_smbh_pn = true
|
||||
#
|
||||
## A mask array (zeros and ones) determining whether or not to use specific post-Newtonian terms.
|
||||
## The elements represent {0, 1, 2, 2.5, 3, 3.5, spin}
|
||||
|
||||
# A mask array (zeros and ones) determining whether or not to use specific post-Newtonian terms.
|
||||
# The elements represent {0, 1, 2, 2.5, 3, 3.5, spin} [default: {1,1,1,1,1,1,1}]
|
||||
#pn_usage = {1, 1, 1, 1, 0, 0, 0}
|
||||
#
|
||||
## The speed of light in N-body units [default: 500]
|
||||
|
||||
# The speed of light in N-body units [default: 500]
|
||||
#pn_c = 477.12
|
||||
#
|
||||
#####################################
|
||||
## Negative powers of two #
|
||||
#####################################
|
||||
## -1 1/2 0.5 #
|
||||
## -2 1/4 0.25 #
|
||||
## -3 1/8 0.125 #
|
||||
## -4 1/16 0.0625 #
|
||||
## -5 1/32 0.03125 #
|
||||
## -6 1/64 0.015625 #
|
||||
## -7 1/128 0.0078125 #
|
||||
## -8 1/256 0.00390625 #
|
||||
## -9 1/512 0.001953125 #
|
||||
## -10 1/1024 0.0009765625 #
|
||||
## -11 1/2048 0.00048828125 #
|
||||
## -12 1/4096 0.000244140625 #
|
||||
## -13 1/8192 0.0001220703125 #
|
||||
## -14 1/16384 0.00006103515625 #
|
||||
## -15 1/32768 0.000030517578125 #
|
||||
## -16 1/65536 0.0000152587890625 #
|
||||
#####################################
|
||||
|
||||
####################################
|
||||
# Negative powers of two #
|
||||
####################################
|
||||
# -1 1/2 0.5 #
|
||||
# -2 1/4 0.25 #
|
||||
# -3 1/8 0.125 #
|
||||
# -4 1/16 0.0625 #
|
||||
# -5 1/32 0.03125 #
|
||||
# -6 1/64 0.015625 #
|
||||
# -7 1/128 0.0078125 #
|
||||
# -8 1/256 0.00390625 #
|
||||
# -9 1/512 0.001953125 #
|
||||
# -10 1/1024 0.0009765625 #
|
||||
# -11 1/2048 0.00048828125 #
|
||||
# -12 1/4096 0.000244140625 #
|
||||
# -13 1/8192 0.0001220703125 #
|
||||
# -14 1/16384 0.00006103515625 #
|
||||
# -15 1/32768 0.000030517578125 #
|
||||
# -16 1/65536 0.0000152587890625 #
|
||||
####################################
|
||||
|
|
|
|||
Loading…
Add table
Add a link
Reference in a new issue