Bh thermodynamics
v208_bh_thermodynamics.py · horizon
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black-hole thermodynamics from the seam: the modular Hawking temperature and the scalaron-corrected Wald entropy (archive integration of the dropped tfpt-42 stationary-horizons/compact-objects section, re-typed through the current Tomita–Takesaki seam work v198/v199). [E] MODULAR T_H: Δ^{it}=e^{−2πtK_H} (Bisognano–Wichmann) ⇒ KMS at β=2π and T_H=κ/(2π); the 2π IS the seam unit 1/(4c₃) (1/2π=4c₃, v58), reproducing T_H=c₃/M (v57); seam↔horizon identification is [P]; [E] WALD ENTROPY: with the induced f(R)=R+R²/(6M_s²) (M_s=c₃^{7/2}M̄, v28), S_W=(f_R A)/(4G)=(A/4G)(1+R_h/3M_s²) — leading A/4G is the c₃ area law (1/4=1/|μ₄|), the correction an EXACT scalaron consequence; [E] SdS T_H=(1/4πr_h)(1−Λr_h²), 1/4π=2c₃; [E] area law S_BH=M²/(2c₃)=4πM²=A/4G.
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