using DifferentialEquations const ħc = 197.33 # MeVfm # Values defined in C. J. Horowitz and J. Piekarewicz, Phys. Rev. Lett. 86, 5647 (2001) # Values taken from Hartree.f (FSUGarnet) const m_s = 496.939473213388 # MeV/c2 const m_ω = 782.5 # MeV/c2 const m_ρ = 763.0 # MeV/c2 const m_γ = 0.000001000 # MeV/c2 # should be 0? const g2_s = 110.349189097820 # dimensionless const g2_v = 187.694676506801 # dimensionless const g2_ρ = 192.927428365698 # dimensionless const g2_γ = 0.091701236 # dimensionless # equal to 4πα const κ = 3.260178893447 # MeV const λ = -0.003551486718 # dimensionless # LambdaSS const ζ = 0.023499504053 # dimensionless # LambdaVV const Λv = 0.043376933644 # dimensionless # LambdaVR const r_reg = 1E-8 # fm # regulator for Green's functions "Green's function for Klein-Gordon equation in natural units" greensFunctionKG(m, r, rp) = -1 / (m * (r + r_reg) * (rp + r_reg)) * sinh(m * min(r, rp)) * exp(-m * max(r, rp)) "Green's function for Poisson's equation in natural units" greensFunctionP(r, rp) = -1 / (max(r, rp) + r_reg) "Solve the Klein-Gordon equation (or Poisson's equation when m=0) and return an array in MeV for a source array given in fm⁻³ where m is the mass of the meson in MeV/c2, r_max is the r-cutoff in fm." function solveKG(m, source, r_max) Δr = r_max / (length(source) - 1) rs = range(0, r_max; length=length(source)) int_measure = ħc .* Δr .* rs .^ 2 greensFunction = m == 0 ? greensFunctionP : (r, rp) -> greensFunctionKG(m / ħc, r, rp) greenMat = greensFunction.(rs, transpose(rs)) return greenMat * (int_measure .* source) end "Iteratively solve meson equations and return the wave functions u(r)=[Φ0(r), W0(r), B0(r), A0(r)] where divs is the number of mesh divisions so the arrays are of length (1+divs), ρ_sp, ρ_vp are the scalar and vector proton densities as arrays, ρ_sn, ρ_vn are the scalar and vector neutron densities as arrays, Φ0, W0, B0, A0 are the mean-field potentials (couplings included) in MeV as as arrays, r is the radius in fm, An initial guess initial_sol=(Φ0, W0, B0, A0) can be provided to speed up convergence (permuting!). Reference: P. Giuliani, K. Godbey, E. Bonilla, F. Viens, and J. Piekarewicz, Frontiers in Physics 10, (2023)" function solveMesonWfs(ρ_sp, ρ_vp, ρ_sn, ρ_vn, r_max, divs, iterations=10; initial_sol=(zeros(1 + divs) for _ in 1:4)) (Φ0, W0, B0, A0) = initial_sol (src_Φ0, src_W0, src_B0, src_A0) = (zeros(1 + divs) for _ in 1:4) # A0 doesn't need iterations @. src_A0 = -g2_γ * ρ_vp A0 .= solveKG(m_γ, src_A0, r_max) for _ in 1:iterations @. src_Φ0 = g2_s * ((κ/ħc)/2 * (Φ0/ħc)^2 + (λ/6) * (Φ0/ħc)^3) - g2_s * (ρ_sp + ρ_sn) @. src_W0 = g2_v * ((ζ/6) * (W0/ħc)^3 + 2Λv * (2B0/ħc)^2 * (W0/ħc)) - g2_v * (ρ_vp + ρ_vn) @. src_B0 = (2Λv * g2_ρ * (W0/ħc)^2 * (2B0/ħc) - g2_ρ/2 * (ρ_vp - ρ_vn)) / 2 Φ0 .= solveKG(m_s, src_Φ0, r_max) W0 .= (solveKG(m_ω, src_W0, r_max) .+ W0) ./ 2 # to supress oscillation B0 .= (solveKG(m_ρ, src_B0, r_max) .+ B0) ./ 2 # to supress oscillation end return (Φ0, W0, B0, A0) end