|
gptkbp:instanceOf
|
computational method
|
|
gptkbp:application
|
gptkb:cosmology
galaxy formation
planetary system dynamics
dark matter distribution
star cluster evolution
|
|
gptkbp:canBe
|
gptkb:fast_multipole_method
collisionless
collisional
direct summation
particle-mesh method
tree code
|
|
gptkbp:hasModel
|
many-body systems
gravitational interactions
electrostatic interactions
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
N-body simulations
|
|
gptkbp:introducedIn
|
1940s
|
|
gptkbp:limitation
|
computational cost
approximation errors
finite resolution
|
|
gptkbp:mayInclude
|
black hole physics
hydrodynamics
star formation
chemical evolution
feedback processes
|
|
gptkbp:notableFor
|
gptkb:AMUSE
gptkb:GADGET
gptkb:NBODY6
gptkb:PKDGRAV
gptkb:RAMSES
|
|
gptkbp:notableSimulation
|
gptkb:Via_Lactea
gptkb:Aquarius_Project
gptkb:Bolshoi_Simulation
gptkb:Illustris
gptkb:Millennium_Simulation
|
|
gptkbp:output
|
positions
trajectories
energies
velocities
|
|
gptkbp:relatedTo
|
gptkb:Monte_Carlo_simulations
gptkb:Fokker-Planck_equation
smoothed particle hydrodynamics
|
|
gptkbp:requires
|
numerical integration
initial conditions
|
|
gptkbp:solvedBy
|
equations of motion
|
|
gptkbp:usedIn
|
gptkb:cosmology
astrophysics
plasma physics
molecular dynamics
|
|
gptkbp:bfsParent
|
gptkb:Schwarzschild_method
gptkb:Zel'dovich_approximation
gptkb:Zeldovich_approximation
|
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gptkbp:bfsLayer
|
6
|