Setting up a softened star
Hydrodynamical simulations of giant stars are computationally demanding, due to the wide range of dynamical times between the core and the enveleope. Typically, this problem is alleviated by replacing the stellar core with a point particle that only interacts gravitationally with the rest of the star via a softened potential. The stellar profile inside some softening radius is modified to preserve hydrostatic equilibrium.
Here, we show how to use Phantom to set up a softened star from a MESA stellar profile. We name our work directory “star” and make phantomsetup inside:
$ mkdir star $ cd star $ $PHANTOM_DIR/scripts/writemake.sh star > Makefile $ make setup $ ls Makefile phantomsetup*
To set up a star called “mystar”, run phantomsetup,
and answer the prompts. We would like to create a softened star from a MESA
profile, and so we select
Case 5 MESA star from file
and choose the desired EoS when prompted. Currently, stars can only be softened
with (i) Adiabatic/polytropic EoS (ieos = 1), (ii) Ideal gas plus radiation EoS
(ieos = 12), and (iii) MESA EoS (ieos = 10). For (i), you will also be prompted
the adiabatic index,
You will also be prompted the path to your MESA profile:
Enter file name containing density profile (blank="blank",default="P12_Phantom_Profile.data"):
By default, Phantom looks for the MESA headers “mass_grams”, “rho”, “cell_specific_IE”, “radius_cm”, “pressure”, “temperature”, “x_mass_fraction_H”, and “y_mass_fraction_He”, in any order and reads the data, assumming they are unlogged and in cgs units. If the headers of your MESA profile are not in this form, you will have to change them.
After providing the path to your MESA profile, answer “yes” to soften the profile, and you will be presented with three options:
Soften the core density profile and add a sink particle core? (default=no): yes Options for core softening: 1. Specify radius of density softening 2. Specify mass of sink particle core (not recommended) 3. Specify both radius of density softening length and mass of sink particle core (if you do not know what you are doing, you will obtain a poorly softened profile) Select option above : ([1:3], default=1):
Phantom’s core softening procedure requires two parameters: the softening radius, h, and the core mass, mcore. The softening radius is the radius below which the stellar profile is replaced with the softened profile. Option 1 is the recommended option, which allows the user to specify the softening radius, and automatically solves for a value for the core mass that would give a “nice” softened profile.
The core softening procedure will write a data file containing the softened profile. Specify the name of the file in the prompt shown below:
Enter output file name of cored stellar profile: (blank="blank",default="mysoftenedstar.dat"):
If you would like to relax the star automatically, answer yes to the following prompt:
Relax star automatically during setup? (default=no):
At the end of the procedure, a temporary dump file,
mystar_00000.tmp is written.
In this dump, gas particles are mapped to the softened profile, and a sink particle
core with mass mcore and softening length hsoft = h/2 is also added. A setup file,
mystar.setup is also written, which saves the setup options and allows the entire
setup procedure to be performed by running
./phantomsetup mystar.setup without
going through interactive prompting.
Setting up a softened star using the .setup file
The relevant options in the setup file for core softening are
# core softening and sink stellar core options isoftcore = T ! Soften the core of an input MESA profile ieos = 2 ! 1=isothermal,2=adiabatic,10=MESA,12=idealplusrad gamma = 1.667 ! adiabatic index isofteningopt = 3 ! 1=supply hsoft, 2=supply mcore, 3=supply both unsoftened_profile = profile51.data ! Path to MESA profile for softening outputfilename = mysoftenedstar.dat ! Output path for softened MESA profile hdens = 15. ! Radius of core softening mcore = 3.150 ! Mass of sink particle stellar core hsoft = 7.500 ! Softening length of sink particle stellar core isinkcore = T ! Add a sink particle stellar core
In this example,
The adiabatic EoS has been chosen (ieos = 2), and so the adiabatic index has also been specified (gamma = 1.667).
Both the softening radius and core mass have been specified (isofteningopt = 3). The core mass is 3.15 Msun, while the softening radius is 15 Rsun.
phantomsetup will read the original mesa profile, “profile51.data”, and write a softened profile, “mysoftenedstar.dat”.