Struct kidou::orbit::calc::models::m2::M2

pub struct M2 {}

This model uses the Plummer potential for bulge, the Miyamoto & Nagai potential for thin and thick disks, and the Navarro-Frenk-White potential for halo. The values of the parameters for the bulge, the thin disk and the thick disk are taken from Pouliasis et al. (2017, model I), values of the parameters for the halo are taken from Eilers (2018).

Trait Implementations

impl Model for M2

fn phi(&self, r: F, z: F) -> F

Calculate the value of the Galactic potential $ \Phi(R, Z) $ $[ 100 \, \text{km}^2 \, \text{s}^{-2} ]$

fn phi_dr(&self, r: F, z: F) -> F

Calculate the value of $ \partial \Phi(R, Z) / \partial R $ $[ 100 \, \text{km} \, \text{s}^{-2} ]$

fn phi_dz(&self, r: F, z: F) -> F

Calculate the value of $ \partial \Phi(R, Z) / \partial Z $ $[ 100 \, \text{km} \, \text{s}^{-2} ]$