Index of /~aklypin/PM/TEST32x128

      Name                    Last modified       Size  Description


[DIR] Parent Directory        03-Sep-2003 18:07      -  
[   ] InStart.dat             09-Jun-2000 17:53     1k  
[   ] PMcrd.DAT.32x128.a100   09-Jun-2000 17:53     1k  
[   ] PMcrd.DAT.init          09-Jun-2000 17:53     1k  
[   ] PMcrs0.DAT.32x128.a100  09-Jun-2000 17:53   768k  
[   ] PMcrs0.DAT.init         09-Jun-2000 17:53   768k  
[   ] Pkevolution32.eps       09-Jun-2000 17:53    29k  
[   ] RESNEW.DAT              09-Jun-2000 17:53     1k  
[   ] Res32x128.DAT           09-Jun-2000 17:53    40k  
[   ] Sp32x128.01225.dat      09-Jun-2000 17:53     7k  
[   ] Sp32x128.a100.dat       09-Jun-2000 17:53     7k  
[   ] Sp32x128.init.dat       09-Jun-2000 17:53     7k  
[   ] coordinates.ascii.a1..> 09-Jun-2000 17:53   685k  
[   ] model.dat               09-Jun-2000 17:53     6k  
[   ] model.dat.a0.1225       09-Jun-2000 17:53     4k  
[   ] points.ps.gz            09-Jun-2000 17:53   127k  
[   ] points.sm               09-Jun-2000 17:53     3k  
[   ] power.sm                09-Jun-2000 17:53     1k  

Test run of PM code with 32^3 particles,
-------------------      128^3 mesh, LCDM, Omega_0=0.3
                                           h = 0.70
                                           sigma_8 =1.0
                                           n  =1 (slope)
                                           Box = 20h^-1Mpc
List of files in TEST32x128 directory:
-------------------------------------
Res32x128.DAT			Protocol of running PM code.
                     Gives energies and error in
                     energy at different moments.

InStart.dat          Input file used to generate
							initial conditions: PMstartCDM <InStart.dat 

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=15 (a=0.0625)

model.dat.a0.1225		The same as model.dat, but gives P(k)
							at z=7.16326 (a=0.1225)

Sp32x128.init.dat    Density distribution and Power spectrum
                     in simulations at z=15. (a=0.0625)

Sp32x128.01225.dat	Density distribution and Power spectrum
                     in simulations at z=7.16326 (a=0.1225)  

Sp32x128.a100.dat	   Density distribution and Power spectrum
                     in simulations at final moment z=0  (a=1)  

Pkevolution32.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 32^3 particles
							at z=0. Colors code peculiar velocities of
							particles.

RESNEW.DAT				Output of PMstartCDM

PMcrd.DAT.32x128.a100	PM data files for z=0 (a=1.00)
PMcrs0.DAT.32x128.a100           

PMcrd.DAT.init         PM data files with initial conditions 
PMcrs0.DAT.init