By means of numerical simulations we study the radial-orbit instability in anisotropic self-gravitating N-body systems under the effect of noise. We find that the presence of additive or multiplicative noise has a different effect on the onset of the instability, depending on the initial value of the orbital anisotropy.

Noise, friction and the radial-orbit instability in anisotropic stellar systems: stochastic N-body simulations

Di Cintio;Pierfrancesco;
2022

Abstract

By means of numerical simulations we study the radial-orbit instability in anisotropic self-gravitating N-body systems under the effect of noise. We find that the presence of additive or multiplicative noise has a different effect on the onset of the instability, depending on the initial value of the orbital anisotropy.
2022
Stellar dynamics
Galaxies: kinematics and dynamics
Methods: n-body simulations
Diffusion
Astrophysics - Astrophysics of Galaxies
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/420287
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