using DifferentialEquations, Interpolations include("bisection.jl") include("common.jl") include("system.jl") const M_n = 939.0 # MeV/c2 const M_p = 939.0 # MeV/c2 "The spherical Dirac equation that returns du=[dg, df] in-place where u=[g, f] are the reduced radial components evaluated at r, κ is the generalized angular momentum, p is true for proton and false for neutron, E in the energy in MeV, f1(r) = M-Φ0(r)-W0(r)-(p-0.5)*2B0(r)-p*A0(r) is a function of r in MeV (see optimized_dirac_potentials()), f2(r) = -M+Φ0(r)-W0(r)-(p-0.5)*2B0(r)-p*A0(r) is a function of r in MeV (see optimized_dirac_potentials()), r is the radius in fm. Reference: P. Giuliani, K. Godbey, E. Bonilla, F. Viens, and J. Piekarewicz, Frontiers in Physics 10, (2023)" function dirac!(du::Vector{Float64}, u::Vector{Float64}, (κ, E, f1, f2), r::Float64) # TODO: Static typing (g, f) = u @inbounds du[1] = -(κ/(r + r_reg)) * g + (E + f1(r)) * f / ħc @inbounds du[2] = (κ/(r + r_reg)) * f - (E + f2(r)) * g / ħc end "Get the potentials f1 and f2 that goes into the Dirac equation, defined as f1(r) = M-Φ0(r)-W0(r)-(p-0.5)*2B0(r)-p*A0(r), f2(r) = -M+Φ0(r)-W0(r)-(p-0.5)*2B0(r)-p*A0(r)." function optimized_dirac_potentials(p::Bool, s::system) M = p ? M_p : M_n f1s = zero_array(s) f2s = zero_array(s) @. f1s = M - s.Φ0 - s.W0 - (p - 0.5) * 2 * s.B0 - p * s.A0 @. f2s = -M + s.Φ0 - s.W0 - (p - 0.5) * 2 * s.B0 - p * s.A0 f1 = linear_interpolation(rs(s), f1s) f2 = linear_interpolation(rs(s), f2s) return (f1, f2) end "Solve the Dirac equation and return the wave function u(r)=[g(r), f(r)] where divs is the number of mesh divisions so solution would be returned as a 2×(1+divs) matrix, shooting method divides the interval into two partitions at r_max/2, ensuring convergence at both r=0 and r=r_max, the other parameters are the same from dirac!(...)." function solveNucleonWf(κ, p::Bool, E, s::system; shooting=true, normalize=true, algo=Tsit5()) (f1, f2) = optimized_dirac_potentials(p, s) if shooting @assert s.divs % 2 == 0 "divs must be an even number when shooting=true" prob = ODEProblem(dirac!, [0, 1], (s.r_max, s.r_max / 2)) sol = solve(prob, algo, p=(κ, E, f1, f2), saveat=Δr(s)) wf_right = reverse(hcat(sol.u...); dims=2) next_r_max = s.r_max / 2 # for the next step else next_r_max = s.r_max end prob = ODEProblem(dirac!, [0, 1], (0, next_r_max)) sol = solve(prob, algo, p=(κ, E, f1, f2), saveat=Δr(s)) wf = hcat(sol.u...) if shooting # join two segments rescale_factor_g = wf[1, end] / wf_right[1, 1] rescale_factor_f = wf[2, end] / wf_right[2, 1] @assert isfinite(rescale_factor_g) && isfinite(rescale_factor_f) "Cannot rescale the right partition" isapprox(rescale_factor_g, rescale_factor_f; rtol=0.03) || @warn "Discontinuity between two partitions" wf_right_rescaled = wf_right .* ((rescale_factor_g + rescale_factor_f) / 2) wf = hcat(wf[:, 1:(end - 1)], wf_right_rescaled) end if normalize norm = sum(wf .* wf) * Δr(s) # integration by Reimann sum wf = wf ./ sqrt(norm) end return wf end "Returns a function that solves the Dirac equation in two partitions and returns the determinant of [g_left(r) g_right(r); f_left(r) f_right(r)], where is r is in fm." function determinantFunc(κ, p::Bool, s::system, r::Float64=s.r_max/2, algo=Tsit5()) (f1, f2) = optimized_dirac_potentials(p, s) prob_left = ODEProblem(dirac!, [0.0, 1.0], (0, r)) prob_right = ODEProblem(dirac!, [0.0, 1.0], (s.r_max, r)) function func(E) u_left = solve(prob_left, algo, p=(κ, E, f1, f2), saveat=[r]) u_right = solve(prob_right, algo, p=(κ, E, f1, f2), saveat=[r]) return u_left[1, 1] * u_right[2, 1] - u_right[1, 1] * u_left[2, 1] end return func end "Find all bound energies between E_min (=850.0) and E_max (=938.0) where tol_digits determines the precision for root finding and the threshold for identifying duplicates, the other parameters are the same from dirac!(...)." function findEs(κ, p::Bool, s::system, E_min=850.0, E_max=938.0; tol_digits=8) func = determinantFunc(κ, p, s) Es = find_all_zeros(func, E_min, E_max; partitions=20, tol=1/10^tol_digits) return unique(E -> round(E; digits=tol_digits), Es) end "Find all orbitals and return two lists containing κ values and corresponding energies for a single species where the other parameters are defined above" function findAllOrbitals(p::Bool, s::system, E_min=850.0, E_max=938.0) κs = Int[] Es = Float64[] # start from κ=-1 and go both up and down for direction in [-1, 1] for κ in direction * (1:100) # cutoff is 100 new_Es = findEs(κ, p, s, E_min, E_max) if isempty(new_Es); break; end append!(Es, new_Es) append!(κs, fill(κ, length(new_Es))) end end return (κs, Es) end "For a given list of κ values with corresponding energies, attempt to fill Z_or_N lowest lying orbitals and return the spectrum" function fillNucleons(Z_or_N::Int, κs, Es)::spectrum sort_i = sortperm(Es) occ = zeros(Int, length(κs)) for i in sort_i if Z_or_N ≤ 0; break; end; max_occ = 2 * j_κ(κs[i]) + 1 occ[i] = min(max_occ, Z_or_N) Z_or_N -= occ[i] end @assert Z_or_N == 0 "All orbitals could not be filled" return spectrum(κs, Es, occ) end "Total angular momentum j for a given κ value" j_κ(κ::Int) = abs(κ) - 1/2 "Orbital angular momentum l for a given κ value" l_κ(κ::Int) = abs(κ) - (κ < 0) # since true = 1 and false = 0 "Calculate scalar and vector densities of a nucleon species on [0,r_max] divided into (divs+1) points and returns them as vectors (ρ_s, ρ_v) where the arrays κs, Es, occs tabulate the energies and occupation numbers corresponding to each κ, the other parameters are defined above" function calculateNucleonDensity(p::Bool, s::system)::Tuple{Vector{Float64}, Vector{Float64}} spectrum = p ? s.p_spectrum : s.n_spectrum (κs, Es, occs) = (spectrum.κ, spectrum.E, spectrum.occ) ρr2 = zeros(2, s.divs + 1) # ρ×r² values for (κ, E, occ) in zip(κs, Es, occs) wf = solveNucleonWf(κ, p, E, s; shooting=true, normalize=true) wf2 = wf .* wf ρr2 += (occ / (4 * pi)) * wf2 # 2j+1 factor is accounted in the occupancy number end r2s = rs(s).^2 ρ = ρr2 ./ transpose(r2s) ρ[:, 1] .= ρ[:, 2] # dirty fix for NaN at r=0 ρ_s = ρ[1, :] - ρ[2, :] # g^2 - f^2 ρ_v = ρ[1, :] + ρ[2, :] # g^2 + f^2 return (ρ_s, ρ_v) end "For a nucleon species, solve the Dirac equation and save the spectrum & densities in-place where the other parameters are defined above" function solveNucleonDensity!(p::Bool, s::system, E_min=850.0, E_max=938.0) κs, Es = findAllOrbitals(p, s, E_min, E_max) spec = fillNucleons(Z_or_N(s, p), κs, Es) if p s.p_spectrum = spec else s.n_spectrum = spec end (ρ_s, ρ_v) = calculateNucleonDensity(p, s) if p s.ρ_sp = ρ_s s.ρ_vp = ρ_v else s.ρ_sn = ρ_s s.ρ_vn = ρ_v end end "Total energy of filled nucleons in the system" nucleon_E(s::system) = sum(s.p_spectrum.occ .* (s.p_spectrum.E .- M_p)) + sum(s.n_spectrum.occ .* (s.n_spectrum.E .- M_n))