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Fokker-Planck equation

(shows likelihood of velocity over time of a disturbed particle)

The Fokker-Planck equation gives the density of the probability of possible velocities for a particle both experiencing drag and random disturbances, e.g., as per Brownian motion. The equation has uses in fluid dynamics, and in astrophysics it has also been used to model the effect stars have on other passing stars, such as within stellar clusters or entire galaxies.


(equation,statistical mechanics)
Further reading:
https://en.wikipedia.org/wiki/Fokker-Planck_equation
https://www.cfm.brown.edu/people/dobrush/am34/Mathematica/ch6/fp.html
http://www.phys.ufl.edu/~avinash/Notes/Fokker_Planck/Fokker_Planck.pdf
https://chem.libretexts.org/Bookshelves/Physical_and_Theoretical_Chemistry_Textbook_Maps/Non-Equilibrium_Statistical_Mechanics_(Cao)/01%3A_Stochastic_Processes_and_Brownian_Motion/1.03%3A_Fokker-Planck_Equations

Referenced by page:
stellar dynamics

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