OutputDir /u/sciteam/tenneti/scratch/Lowres_BTnew/IC-400MPC-dm/ % Directory for output FileBase IC % Base-filename of output files Nmesh 1760 % This is the size of the FFT grid used to % compute the displacement field. One % should have Nmesh >= Nsample. Nsample 1760 % sets the maximum k that the code uses, % i.e. this effectively determines the % Nyquist frequency that the code assumes, % k_Nyquist = 2*PI/Box * Nsample/2 % Normally, one chooses Nsample such that % Ntot = Nsample^3, where Ntot is the % total number of particles Ngrid 1760 BoxSize 400000.0 % Periodic box size of simulation Omega0 0.2814 % Total matter density (at z=0) OmegaLambda 0.7186 % Cosmological constant (at z=0) OmegaBaryon 0.0464 % Baryon density (at z=0) OmegaDM_2ndSpecies 0 % Omega for a second dark matter species (at z=0) HubbleParam 0.697 % Hubble paramater (may be used for power spec parameterization) Redshift 99 % Starting redshift Sigma8 0.820 % power spectrum normalization ProduceGas 0 SphereMode 1 % if "1" only modes with |k| < k_Nyquist are % used (i.e. a sphere in k-space), otherwise modes with % |k_x|,|k_y|,|k_z| < k_Nyquist are used % (i.e. a cube in k-space) WhichSpectrum 2 % "1" selects Eisenstein & Hu spectrum, % "2" selects a tabulated power spectrum in % the file 'FileWithInputSpectrum' % otherwise, Efstathiou parametrization is used FileWithInputSpectrum /u/sciteam/tenneti/BWSimIC/powerspectrum-wmap9.txt % filename of tabulated input % spectrum (if used) InputSpectrum_UnitLength_in_cm 3.085678e24 % defines length unit of tabulated % input spectrum in cm/h. % Note: This can be chosen different from UnitLength_in_cm ShapeGamma 0.201 % only needed for Efstathiou power spectrum PrimordialIndex 0.971 % may be used to tilt the primordial index Seed 181170 % seed for IC-generator UnitLength_in_cm 3.085678e21 % defines length unit of output (in cm/h) UnitMass_in_g 1.989e43 % defines mass unit of output (in g/cm) UnitVelocity_in_cm_per_s 1e5 % defines velocity unit of output (in cm/sec) WDM_On 0 % Putting a '1' here will enable a WDM small-scale % smoothing of the power spectrum WDM_Vtherm_On 0 % If set to '1', the (warm) dark matter particles will % receive an additional random thermal velocity % corresponding to their particle mass WDM_PartMass_in_kev 10.0 % This is the particle mass in keV of the WDM particle