Index of /~aklypin/PM/TEST128x256
Name Last modified Size Description
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Parent Directory 03-Sep-2003 18:07 -
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Catalog.DAT.gz 09-Jun-2000 17:53 459k
Catshort.DAT.gz 09-Jun-2000 17:53 49k
PMcrd.DAT.gz 09-Jun-2000 17:53 1k
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Pkevolution.eps 09-Jun-2000 17:53 49k
Res128x256.DAT.gz 09-Jun-2000 17:53 6k
Sp128x256.052.DAT.gz 09-Jun-2000 17:53 4k
Sp128x256.072.DAT.gz 09-Jun-2000 17:53 4k
Sp128x256.092.DAT.gz 09-Jun-2000 17:53 4k
Sp128x256.192.DAT.gz 09-Jun-2000 17:53 4k
Sp128x256.a100.DAT.gz 09-Jun-2000 17:53 4k
Sp128x256.init.DAT.gz 09-Jun-2000 17:53 4k
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halos.sm 09-Jun-2000 17:53 3k
halosxy.ps 09-Jun-2000 17:53 28k
model.052.dat 09-Jun-2000 17:53 6k
model.072.dat 09-Jun-2000 17:53 6k
model.092.dat 09-Jun-2000 17:53 6k
model.192.dat 09-Jun-2000 17:53 6k
model.dat 09-Jun-2000 17:53 6k
points.ps.gz 09-Jun-2000 17:53 6.7M
points.sm 09-Jun-2000 17:53 3k
power.sm 09-Jun-2000 17:53 2k
slice.dat.gz 09-Jun-2000 17:53 2.8M
Test run of PM code with 128^3 particles,
------------------- 256^3 mesh, LCDM, Omega_0=0.3
h = 0.70
sigma_8 =1.0
n =1 (slope)
Box = 20h^-1Mpc
List of files in TEST128x256 directory:
-------------------------------------
Res128x256.DAT Protocol of running PM code.
Gives energies and error in
energy at different moments.
model.dat Output of running PMmodels:
description of the cosmological model
and approximations used to set initial
conditions. In this case a flat cosmological
model with cosmological constant was used.
Format: line1 -- Omegas, hubble
line2 -- parameters of approximation
for P(k) (Holtzman in this case)
line3-13 Age(in 10^9yrs), redshift,
expansion parameter, Hubble/100,
delta_rho, d(log delta)/d(log a)
line14 self-explanatory
line15 rms velocity of 50h-1Mpc sphere
line16-126 Power Spectrum at z=0 (a=1)
line127 self-explanatory
line128- Power Spectrum at z=30
model.052.dat The same as model.dat, but gives P(k) at a=0.052
model.072.dat a=0.072
model.092.dat a=0.092
model.192.dat a=0.192
Sp128x256.init.dat Density distribution and Power spectrum
in simulations at z=30.
Sp128x256.052.dat Density distribution and Power spectrum
in simulations at z=18.2 (a=0.052)
Sp128x256.a100.dat Density distribution and Power spectrum
in simulations at final moment z=0 (a=1)
Pkevolution.eps Comparison of the evolution of the power
spectrum in the simualtion with the linear
theory.
coordinates.ascii.a100 Coordinates and velocities of particles
in the simulation at z=0. This file was
produced by PM_to_ASCII. Coordinates are
in Mpcs (0-20). Peculiar velocities are
in km/s
points.ps Color Postscript file shows all 128^3 particles
at z=0. Colors code peculiar velocities of
particles.
PMcrd.DAT PM data files for z=0 (a=1.00)
PMcrs0.DAT
Catalog.DAT Halos identified in the simulation using PMhalos
Catshort.DAT List of halos