Linked from

The 19 pages that link to N-body simulation, each with the reason it gives.

• Cosmic webRelated: Simulations show how gravity shapes dark matter into filaments, nodes, and voids.

• Large-scale structure of the universeRelated: Simulations show how gravity builds web-like patterns from initial conditions.

• Tidal strippingRelated: Simulations predict how satellite material becomes streams under a host's tidal field.

• Density wave theoryRelated: Simulations test whether stellar disks develop and sustain spiral density patterns.

• Cold dark matterRelated: Simulations test how cold dark matter particles assemble into halos and cosmic structure.

• Stellar streamRelated: Simulations show how a progenitor’s orbit and mass shape its stream.

• Planet NineRelated: Simulations test whether a hypothesized planet can produce the observed orbital structure.

• Magellanic StreamRelated: Simulations test whether Cloud orbits can reproduce the Stream’s observed extent and shape.

• Nuclear star clusterRelated: Simulations test whether inward cluster migration can build a dense stellar nucleus.

• Rogue planetRelated: Simulations test how often system dynamics produce unbound planets.

• Andromeda–Milky Way collisionRelated: Simulations test how measurement uncertainties and nearby galaxies change the predicted encounter.

• Primordial fluctuationsRelated: Cosmological simulations test how specified primordial perturbations develop into matter structures.

• Astronomical system of unitsRelated: Astronomical units help scale simulations of planetary and stellar systems.

• Giant VoidRelated: Simulations trace how gravity sculpts voids from early density fluctuations.

• Planets beyond NeptuneRelated: Simulations test whether a proposed planet can produce observed orbital patterns.