SMDPL (smdpl)

Description

The Small MultiDark Planck simulation belongs to the series of MultiDark simulations with Planck cosmology. Its simulation box has a side length of only 400 Mpc/h, less than half of the MDPL-size. With 38403 particles inside this small box it achieves a mass resolution of 108 Msun/h per dark matter particle. Some more details for this simulation are described in Klypin et al. 2014.

Details

Box size 400 Mpc/h side length of the cosmological cube
Number of particles 38403 total number of dark matter particles
Mass resolution 9.63*107 Msun/h mass of one dark matter particle
Force resolution 1.5 kpc/h physical force resolution
Initial redshift 120 redshift at which the simulation started
Cosmology
h 0.6777 Hubble parameter
ΩΛ 0.692885 density parameter for dark energy
Ωm 0.307115 density parameter for matter (dark matter+baryons)
Ωb 0.048206 density parameter for baryonic matter
n 0.96 normalization of the Power spectrum
σ8 0.8228 amplitude of mass density fluctuation in 8 Mpc/h sphere (at redshift z=0)
Other constants
G 6.67428 * 10-8 cm3 g-1 s-2 Gravitational constant (Rev. Mod. Phys. 80 (2008) 633-730)
1 Mpc 30.85677 * 1023 cm 1 Mpc in cm
Msun 1.98892 ± 0.00025 1033 g Solar mass (Physics Reports 281 (1997) 309)

Attribution

In order to properly acknowledge our efforts, we request the following paragraph to be included in the "Acknowledgements" section of any publication which makes use of the simulation data above via the CosmoSim or MultiDark database:

Acknowledgements – Database

The CosmoSim database used in this paper is a service by the Leibniz-Institute for Astrophysics Potsdam (AIP). The MultiDark database was developed in cooperation with the Spanish MultiDark Consolider Project CSD2009-00064.

Acknowledgements – Simulations

The authors gratefully acknowledge the Gauss Centre for Supercomputing e.V. (www.gauss-centre.eu) and the Partnership for Advanced Supercomputing in Europe (PRACE, www.prace-ri.eu) for funding the MultiDark simulation project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre (LRZ, www.lrz.de). The Bolshoi simulations have been performed within the Bolshoi project of the University of California High-Performance AstroComputing Center (UC-HiPACC) and were run at the NASA Ames Research Center.

More information can be found on the credit page.

Tables

Table Description
AvailHalos
smdpl.availhalos

Gives an overview on the snapshots, for which halo data are stored in the halo catalogues tables. In particular, it gives the number of halos/FOF groups for each snapshot.

BDMV
smdpl.bdmv

BDM halo catalogue for all available snapshots, using the standard overdensity criterion with 360*background density

BDMW
smdpl.bdmw

BDM halo catalogue for all available snapshots, using 200*critical density as overdensity criterion

Dens512_z0
smdpl.dens512_z0

Density field on a 512^3 grid, for redshift z=0

FOF
smdpl.fof

Friends-of-Friends halo catalogue, level 0 with relative linking length 0.2

FOF1
smdpl.fof1

Friends-of-Friends halo catalogue, level 1 with relative linking length 0.1

FOF2
smdpl.fof2

Friends-of-Friends halo catalogue, level 2 with relative linking length 0.05

FOF3
smdpl.fof3

Friends-of-Friends halo catalogue, level 3 with relative linking length 0.025

FOF4
smdpl.fof4

Friends-of-Friends halo catalogue, level 4 with relative linking length 0.0125

FOF5
smdpl.fof5

Friends-of-Friends halo catalogue, level 5 with relative linking length 0.00625

LinkLength
smdpl.linklength

Linking lengths for each FOF level

Redshifts
smdpl.redshifts

Redshifts for snapshot numbers

Rockstar
smdpl.rockstar

Rockstar halo catalogue with consistent merger trees