darkmatter 0.0.2

Dark matter simulation engine — gravitational fields, particle dynamics, halo stability, and cosmological constants
Documentation 
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use crate::constants::physical::G;
use std::f64::consts::PI;

pub fn velocity_dependent_cross_section(
    v_km_s: f64,
    sigma_0_cm2_g: f64,
    v_ref_km_s: f64,
    power_index: f64,
) -> f64 {
    sigma_0_cm2_g * (v_km_s / v_ref_km_s).powf(power_index)
}

pub fn yukawa_cross_section(alpha_chi: f64, m_chi_gev: f64, m_phi_gev: f64, v_km_s: f64) -> f64 {
    let v_si = v_km_s * 1e3;
    let c = 3e8;
    let beta = v_si / c;
    let m_chi_kg = m_chi_gev * 1.782_661_92e-27;
    let mu = m_chi_kg / 2.0;
    let hbar = 1.054_571_817e-34;
    let a = m_phi_gev / (2.0 * alpha_chi * m_chi_gev);
    let b = m_chi_gev * beta / (2.0 * m_phi_gev);
    if b < 0.1 {
        let born_factor = a * a / (1.0 + a * a);
        let sigma = 8.0 * PI * alpha_chi * alpha_chi
            / (m_phi_gev * m_phi_gev * 1.782_661_92e-27 * 1.782_661_92e-27)
            * born_factor
            * hbar
            * hbar
            / (v_si * v_si * mu * mu + 1e-100);
        return sigma * 1e4;
    }
    let ln_term = (1.0 + b * b).ln();
    4.0 * PI * alpha_chi * alpha_chi
        / (m_chi_gev * m_chi_gev * 1.782_661_92e-27 * 1.782_661_92e-27 * beta.powi(4) * c.powi(4))
        * (ln_term - b * b / (1.0 + b * b))
        * hbar
        * hbar
        * 1e4
}

pub fn gravothermal_collapse_timescale(
    rho_core_kg_m3: f64,
    sigma_v_km_s: f64,
    r_core_kpc: f64,
    sigma_over_m_cm2_g: f64,
) -> f64 {
    let sigma_v = sigma_v_km_s * 1e3;
    let r_core = r_core_kpc * 3.0857e19;
    let kappa = sigma_over_m_cm2_g * 1e-1 * rho_core_kg_m3 * sigma_v;
    if kappa < 1e-50 {
        return f64::INFINITY;
    }
    150.0 * sigma_v / (G * rho_core_kg_m3 * r_core * kappa)
}

pub fn core_radius_sidm(
    rho_s_kg_m3: f64,
    r_s_kpc: f64,
    sigma_over_m_cm2_g: f64,
    age_gyr: f64,
) -> f64 {
    let t = age_gyr * 3.156e16;
    let sigma_v = (4.0 * PI * G * rho_s_kg_m3 * (r_s_kpc * 3.0857e19).powi(2) / 3.0).sqrt();
    let rate = sigma_over_m_cm2_g * 1e-1 * rho_s_kg_m3 * sigma_v;
    let n_scatter = rate * t;
    r_s_kpc * n_scatter.min(10.0).sqrt() * 0.5
}

pub fn isothermal_core_density(sigma_v_km_s: f64, r_core_kpc: f64) -> f64 {
    let sigma_v = sigma_v_km_s * 1e3;
    let r_core = r_core_kpc * 3.0857e19;
    9.0 * sigma_v * sigma_v / (4.0 * PI * G * r_core * r_core)
}

pub fn sidm_heat_conductivity(
    sigma_over_m_cm2_g: f64,
    rho_kg_m3: f64,
    sigma_v_km_s: f64,
    mean_free_path_kpc: f64,
) -> f64 {
    let sigma_v = sigma_v_km_s * 1e3;
    let mfp = mean_free_path_kpc * 3.0857e19;
    let l_eff = mfp.min(1.0 / (sigma_over_m_cm2_g * 1e-1 * rho_kg_m3 + 1e-100));
    rho_kg_m3 * sigma_v * l_eff * sigma_v * sigma_v / 3.0
}

pub fn mean_free_path_kpc(sigma_over_m_cm2_g: f64, rho_kg_m3: f64) -> f64 {
    let sigma_si = sigma_over_m_cm2_g * 1e-1;
    1.0 / (sigma_si * rho_kg_m3 + 1e-100) / 3.0857e19
}

pub fn scattering_rate_per_gyr(sigma_over_m_cm2_g: f64, rho_kg_m3: f64, sigma_v_km_s: f64) -> f64 {
    let sigma_si = sigma_over_m_cm2_g * 1e-1;
    let sigma_v = sigma_v_km_s * 1e3;
    sigma_si * rho_kg_m3 * sigma_v * 3.156e16
}

pub fn core_collapse_criterion(
    sigma_over_m_cm2_g: f64,
    rho_core_kg_m3: f64,
    sigma_v_km_s: f64,
    t_age_gyr: f64,
) -> bool {
    let rate = scattering_rate_per_gyr(sigma_over_m_cm2_g, rho_core_kg_m3, sigma_v_km_s);
    rate * t_age_gyr > 300.0
}

pub fn evaporation_rate(
    sigma_over_m_cm2_g: f64,
    m_sub_solar: f64,
    rho_host_kg_m3: f64,
    v_rel_km_s: f64,
    r_sub_kpc: f64,
) -> f64 {
    let sigma_si = sigma_over_m_cm2_g * 1e-1;
    let v_rel = v_rel_km_s * 1e3;
    let r_sub = r_sub_kpc * 3.0857e19;
    let m_sub = m_sub_solar * 1.989e30;
    let v_esc = (2.0 * G * m_sub / r_sub).sqrt();
    let frac = (-v_esc * v_esc / (2.0 * v_rel * v_rel)).exp();
    sigma_si * rho_host_kg_m3 * v_rel * PI * r_sub * r_sub * frac
}

pub fn bullet_cluster_offset_kpc(
    sigma_over_m_cm2_g: f64,
    sigma_dm_kg_m2: f64,
    v_collision_km_s: f64,
) -> f64 {
    let tau = sigma_over_m_cm2_g * 1e-1 * sigma_dm_kg_m2 / 1.989e30;
    let v = v_collision_km_s * 1e3;
    tau * v / 3.0857e19 * 1e-6
}

pub fn drag_deceleration(sigma_over_m_cm2_g: f64, rho_target_kg_m3: f64, v_rel_km_s: f64) -> f64 {
    let sigma_si = sigma_over_m_cm2_g * 1e-1;
    sigma_si * rho_target_kg_m3 * (v_rel_km_s * 1e3).powi(2)
}