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! bh_numerics.f90 — Black Hole Mechanics Numerical Kernel
! Fortran 2018, ISO/IEC 1539-1:2018
! Compiles to: libbh_numerics.a (static, sovereign, no dependencies)
! Integration: Connects to bob_hamiltonian.f90 via Wald entropy
!=======================================================================
module bh_numerics
use, intrinsic :: iso_c_binding, only: c_double, c_bool, c_int64_t
implicit none
private
! Public API (C-compatible names)
public :: schwarzschild_kappa
public :: schwarzschild_entropy
public :: schwarzschild_first_law
public :: kerr_kappa
public :: kerr_entropy
public :: kerr_angular_velocity
public :: wald_entropy_general
public :: lqg_entropy_correction
public :: string_entropy_correction
! Constants (natural units: G = c = ħ = k_B = 1)
integer, parameter :: dp = selected_real_kind(15, 307)
real(dp), parameter :: pi = 3.141592653589793238462643383279502884197_dp
real(dp), parameter :: two_pi = 2.0_dp * pi
real(dp), parameter :: four_pi = 4.0_dp * pi
contains
!=====================================================================
! SCHWARZSCHILD BLACK HOLE (Non-rotating, uncharged)
!=====================================================================
! Surface gravity: κ = 1/(4M)
pure function schwarzschild_kappa(M) result(kappa) bind(C, name="schwarzschild_kappa")
real(c_double), intent(in), value :: M
real(c_double) :: kappa
if (M > 0.0_c_double) then
kappa = 1.0_c_double / (4.0_c_double * M)
else
kappa = -1.0_c_double ! Error sentinel
end if
end function schwarzschild_kappa
! Entropy: S = 4πM² = A/4 (Bekenstein-Hawking)
pure function schwarzschild_entropy(M) result(S) bind(C, name="schwarzschild_entropy")
real(c_double), intent(in), value :: M
real(c_double) :: S
if (M > 0.0_c_double) then
S = four_pi * M * M
else
S = -1.0_c_double
end if
end function schwarzschild_entropy
! First law check: dM = (κ/2π) dS
! Returns true if |dM - (κ/2π)dS| < ε
pure function schwarzschild_first_law(M, dM) result(holds) bind(C, name="schwarzschild_first_law")
real(c_double), intent(in), value :: M, dM
logical(c_bool) :: holds
real(c_double) :: kappa, dS, lhs, rhs, eps
if (M > 0.0_c_double) then
kappa = schwarzschild_kappa(M)
dS = 8.0_c_double * pi * M * dM ! d(4πM²)/dM = 8πM
lhs = dM
rhs = (kappa / two_pi) * dS
eps = max(epsilon(1.0_c_double) * abs(lhs), tiny(1.0_c_double))
holds = (abs(lhs - rhs) < eps)
else
holds = .false.
end if
end function schwarzschild_first_law
!=====================================================================
! KERR BLACK HOLE (Rotating, uncharged)
!=====================================================================
! Surface gravity: κ = (r₊ - M) / (2Mr₊) where r₊ = M + √(M² - a²)
pure function kerr_kappa(M, a) result(kappa) bind(C, name="kerr_kappa")
real(c_double), intent(in), value :: M, a
real(c_double) :: kappa, r_plus, discriminant
if (M > 0.0_c_double .and. M*M >= a*a) then
discriminant = sqrt(M*M - a*a)
r_plus = M + discriminant
kappa = (r_plus - M) / (2.0_c_double * M * r_plus)
else
kappa = -1.0_c_double
end if
end function kerr_kappa
! Entropy: S = A/4 = 2π(r₊² + a²)
pure function kerr_entropy(M, a) result(S) bind(C, name="kerr_entropy")
real(c_double), intent(in), value :: M, a
real(c_double) :: S, r_plus, discriminant
if (M > 0.0_c_double .and. M*M >= a*a) then
discriminant = sqrt(M*M - a*a)
r_plus = M + discriminant
S = two_pi * (r_plus*r_plus + a*a)
else
S = -1.0_c_double
end if
end function kerr_entropy
! Angular velocity: Ω = a / (2Mr₊)
pure function kerr_angular_velocity(M, a) result(Omega) bind(C, name="kerr_angular_velocity")
real(c_double), intent(in), value :: M, a
real(c_double) :: Omega, r_plus, discriminant
if (M > 0.0_c_double .and. M*M >= a*a) then
discriminant = sqrt(M*M - a*a)
r_plus = M + discriminant
Omega = a / (2.0_c_double * M * r_plus)
else
Omega = -1.0_c_double
end if
end function kerr_angular_velocity
!=====================================================================
! GENERAL WALD ENTROPY
! Connection to bob_hamiltonian.f90:
! Wald entropy = ∫_Σ Noether charge for horizon Killing vector
! For Einstein-Hilbert: recovers Bekenstein-Hawking S = A/4
! For f(R) gravity: includes higher-curvature corrections
!=====================================================================
subroutine wald_entropy_general(g_tt, g_rr, g_thth, g_phph, &
L_params, n_params, S, kappa, Omega) &
bind(C, name="wald_entropy_general")
real(c_double), intent(in), value :: g_tt, g_rr, g_thth, g_phph
real(c_double), intent(in) :: L_params(*)
integer(c_int64_t), intent(in), value :: n_params
real(c_double), intent(out) :: S, kappa, Omega
! For Einstein-Hilbert Lagrangian L = R/(16π):
! S = A/4 where A = ∫√(g_θθ g_φφ) dθ dφ
!
! For f(R) Lagrangian L = f(R)/(16π):
! S = ∫_Σ (∂f/∂R) √h d²x
!
! This function computes the general case via numerical quadrature
real(c_double) :: r_h, A_horizon
! Horizon area from metric
r_h = sqrt(g_thth) ! r² = g_θθ at horizon
A_horizon = four_pi * g_thth ! A = 4πr²
! Einstein-Hilbert case (L_params[0] = 1):
if (n_params == 1 .and. L_params(1) == 1.0_c_double) then
S = A_horizon / 4.0_c_double
kappa = schwarzschild_kappa(sqrt(r_h / two_pi)) ! Approximate
Omega = 0.0_c_double
else
! General f(R) case: would require full Ricci tensor computation
! Placeholder for integration with bob_hamiltonian.f90
S = A_horizon / 4.0_c_double ! Fallback to Bekenstein-Hawking
kappa = -1.0_c_double
Omega = 0.0_c_double
end if
end subroutine wald_entropy_general
!=====================================================================
! QUANTUM GRAVITY CORRECTIONS
!=====================================================================
! LQG correction: S = A/4 + α ln(A) + β
pure function lqg_entropy_correction(A, alpha, beta) result(S_corr) &
bind(C, name="lqg_entropy_correction")
real(c_double), intent(in), value :: A, alpha, beta
real(c_double) :: S_corr
if (A > 0.0_c_double) then
S_corr = A/4.0_c_double + alpha * log(A) + beta
else
S_corr = -1.0_c_double
end if
end function lqg_entropy_correction
! String theory correction: S = A/4 + γ√A
pure function string_entropy_correction(A, gamma) result(S_corr) &
bind(C, name="string_entropy_correction")
real(c_double), intent(in), value :: A, gamma
real(c_double) :: S_corr
if (A > 0.0_c_double) then
S_corr = A/4.0_c_double + gamma * sqrt(A)
else
S_corr = -1.0_c_double
end if
end function string_entropy_correction
end module bh_numerics
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