EinsteinFieldEquation · section of the QIQT-H book

QIQTH.EinsteinFieldEquation

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EinsteinFieldEquation · entries 83–93 of 1000

Definition 83 (div02).  source ↗

Raised divergence ∇^μ X_{μν} = g^{μρ} ∇_ρ X_{μν} of a (0,2) tensor field.

div02 n g gi X ν x  :=  ∑μ∑ρgμρ(x)⋅∇2 g gi X ρ μ ν x\mathrm{div02}\,n\,g\,\mathrm{gi}\,X\,\nu\,x \;:=\; \sum_{\mu} \sum_{\rho} g^{{\mu}{\rho}}({x}) \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-covderiv02}{\nabla^{2}}\,g\,\mathrm{gi}\,X\,\rho\,\mu\,\nu\,x

Used by div02_add, div02_scalar_metric, divRiemann_trace_eq, twice_contracted_bianchi, einstein_field_equation, einstein_field_equation_real, einstein_field_equation_real_global, jacobson_einstein_equation_of_state, and 10 more.

Lemma 84 (div02_add).  source ↗

The raised divergence is additive in the tensor field.

(∀(abρ:Fin n),PdiffAt (λy↦X y a b) ρ x)→(∀(abρ:Fin n),PdiffAt (λy↦Y y a b) ρ x)→∀(ν:Fin n),(∇ ⁣⋅λyab↦X y a b+Y y a b)ν(x)=(∇ ⁣⋅X)ν(x)+(∇ ⁣⋅Y)ν(x)(\forall (a b \rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,(\lambda y \mapsto X\,y\,a\,b)\,\rho\,x) \to (\forall (a b \rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,(\lambda y \mapsto Y\,y\,a\,b)\,\rho\,x) \to \forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a b \mapsto X\,y\,a\,b + Y\,y\,a\,b})_{{\nu}}({x})} = \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {X})_{{\nu}}({x})} + \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {Y})_{{\nu}}({x})}

Proof. By pd, pd_add, christoffel, covDeriv02. □\square

Used by einstein_field_equation, div02_kgStress_eq.

Lemma 85 (div02_scalar_metric).  source ↗

The divergence of f·g is ∂_ν f. Metric compatibility kills the connection terms; the inverse metric collapses the contraction. (This is what makes the cosmological-constant term Λ·g covariantly constant.)

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→∀(f:Mn→R)(x:Mn),(∀(ρ:Fin n),PdiffAt f ρ x)→(∀(abρ:Fin n),PdiffAt (λy↦gab(y)) ρ x)→∀(ν:Fin n),(∇ ⁣⋅λyab↦f y⋅gab(y))ν(x)=∂ν(f)(x)(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to \forall (f : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathbb{R}) (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), (\forall (\rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,f\,\rho\,x) \to (\forall (a b \rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,(\lambda y \mapsto g_{{a}{b}}({y}))\,\rho\,x) \to \forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a b \mapsto f\,y \cdot g_{{a}{b}}({y})})_{{\nu}}({x})} = \href{/browser/qiqth-curvature#d-qiqth-curvature-pd}{\partial_{{\nu}}({f})({x})}

Proof. By pd_mul, christoffel, covDeriv02, metric_compat. □\square

Used by einstein_field_equation, div02_kgStress_eq.

Lemma 86 (divRiemann_trace_eq).  source ↗

T3 of the twice-contracted Bianchi: ∑_ρ ∑_{σν} g^{σν} ∇_ρ R^ρ_{σνλ} = −∇^μ Ric_{μλ}. Sum gi_trace_covDerivRiem_ricci over ρ and match −div02(ricci) (raised Ricci divergence) term-by-term via sum_comm + metric symmetry.

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(abc:Fin n),(λy↦Γbca(y))∈C∞)→∀(λ:Fin n)(x:Mn),∑ρ∑σ∑νgσν(x)⋅∇Riem g gi ρ ρ σ ν λ x=−(∇ ⁣⋅λyab↦Rab(y))λ(x)(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g_{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g^{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b c : \mathrm{Fin}\,n), ({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-christoffel}{\Gamma^{{a}}_{{b}{c}}({y})}})\in C^{\infty}) \to \forall (\lambda : \mathrm{Fin}\,n) (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), \sum_{\rho} \sum_{\sigma} \sum_{\nu} g^{{\sigma}{\nu}}({x}) \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-covderivriem}{\nabla\mathrm{Riem}}\,g\,\mathrm{gi}\,\rho\,\rho\,\sigma\,\nu\,\lambda\,x = -(\nabla\!\cdot {\lambda y a b \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a}{b}}({y})}})_{{\lambda}}({x})

Proof. By pd, covDeriv02, gi_trace_covDerivRiem_ricci. □\square

Used by twice_contracted_bianchi.

Lemma 87 (twice_contracted_bianchi).  source ↗

The twice-contracted (second) Bianchi identity ∇^μ Ric_{μλ} = ½ ∂_λ R — the contracted Bianchi ∇^μ G_{μλ}=0 in trace form. Obtained by contracting second_bianchi_contracted with g^{σν}: the three traced terms are ∂_λR (gi_trace_covDeriv_ricci), div02(ricci) (the Ricci divergence), and −div02(ricci) (divRiemann_trace_eq), giving ∂_λR − div02 − div02 = 0. Machine-checked, axiom-free — this discharges the bianchi hypothesis of einstein_field_equation.

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(abc:Fin n),(λy↦Γbca(y))∈C∞)→∀(λ:Fin n)(x:Mn),(∇ ⁣⋅λyab↦Rab(y))λ(x)=1/2⋅∂λ(λy↦R(y))(x)(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g_{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g^{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b c : \mathrm{Fin}\,n), ({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-christoffel}{\Gamma^{{a}}_{{b}{c}}({y})}})\in C^{\infty}) \to \forall (\lambda : \mathrm{Fin}\,n) (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), (\nabla\!\cdot {\lambda y a b \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a}{b}}({y})}})_{{\lambda}}({x}) = 1/2 \cdot \partial_{{\lambda}}({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-scalarcurv}{R({y})}})({x})

Proof. By covDeriv02, covDerivRiem, second_bianchi_contracted, gi_trace_covDeriv_ricci, divRiemann_trace_eq. □\square

Used by einstein_field_equation_real.

Lemma 88 (metric_contraction_trace).  source ↗

The metric–inverse-metric trace is the dimension: g^{μν} g_{μν} = n. Contracting the metric with its inverse over both indices yields ∑_μ δ^μ_μ = n (the number of dimensions).

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→∀(x:Mn),∑μ∑νgμν(x)⋅gμν(x)=n(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to \forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), \sum_{\mu} \sum_{\nu} g^{{\mu}{\nu}}({x}) \cdot g_{{\mu}{\nu}}({x}) = n

Proof. Immediate from the definitions. □\square

Used by hreg_kg.

Lemma 89 (einstein_field_equation).  source ↗

The Einstein field equation as the thermodynamic equation of state (Jacobson, PRL 1995), completed: from the post-crux relation + conservation + contracted Bianchi + metric compatibility, a·T_{μν} = G_{μν} + Λ·g_{μν} with Λ := f + ½R covariantly constant. The cited physics (Clausius/Raychaudhuri → crux, conservation → conserv) and the geometry (contracted Bianchi → bianchi) are explicit labeled hypotheses; the closure is machine-checked, axiom-free. tr is the scalar curvature R.

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→∀(TRic:Mn→Fin n→Fin n→R)(ftr:Mn→R)(a:R)(x:Mn),(∀(ρ:Fin n),PdiffAt f ρ x)→(∀(ρ:Fin n),PdiffAt tr ρ x)→(∀(abρ:Fin n),PdiffAt (λy↦gab(y)) ρ x)→(∀(abρ:Fin n),PdiffAt (λy↦Ric y a b) ρ x)→(∀(y:Mn)(a′b:Fin n),a⋅Ta′b(y)=Ric y a′ b+f y⋅ga′b(y))→(∀(ν:Fin n),(∇ ⁣⋅λya′b↦a⋅Ta′b(y))ν(x)=0)→(∀(ν:Fin n),(∇ ⁣⋅Ric)ν(x)=1/2⋅∂ν(tr)(x))→(∀(μν:Fin n),a⋅Tμν(x)=Ric x μ ν−1/2⋅tr x⋅gμν(x)+(f x+1/2⋅tr x)⋅gμν(x))∧∀(ν:Fin n),∂ν(λy↦f y+1/2⋅tr y)(x)=0(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to \forall (T \mathrm{Ric} : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathrm{Fin}\,n \to \mathrm{Fin}\,n \to \mathbb{R}) (f \mathrm{tr} : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathbb{R}) (a : \mathbb{R}) (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), (\forall (\rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,f\,\rho\,x) \to (\forall (\rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,\mathrm{tr}\,\rho\,x) \to (\forall (a b \rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,(\lambda y \mapsto g_{{a}{b}}({y}))\,\rho\,x) \to (\forall (a b \rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,(\lambda y \mapsto \mathrm{Ric}\,y\,a\,b)\,\rho\,x) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a^{\prime} b : \mathrm{Fin}\,n), a \cdot T_{{a^{\prime}}{b}}({y}) = \mathrm{Ric}\,y\,a^{\prime}\,b + f\,y \cdot g_{{a^{\prime}}{b}}({y})) \to (\forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({y})})_{{\nu}}({x})} = 0) \to (\forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\mathrm{Ric}})_{{\nu}}({x})} = 1/2 \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-pd}{\partial_{{\nu}}({\mathrm{tr}})({x})}) \to (\forall (\mu \nu : \mathrm{Fin}\,n), a \cdot T_{{\mu}{\nu}}({x}) = \mathrm{Ric}\,x\,\mu\,\nu - 1/2 \cdot \mathrm{tr}\,x \cdot g_{{\mu}{\nu}}({x}) + (f\,x + 1/2 \cdot \mathrm{tr}\,x) \cdot g_{{\mu}{\nu}}({x})) \wedge \forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pd}{\partial_{{\nu}}({\lambda y \mapsto f\,y + 1/2 \cdot \mathrm{tr}\,y})({x})} = 0

Proof. By pd_add, pd_const_mul, mul, div02_add, div02_scalar_metric. □\square

Used by einstein_field_equation_real.

Lemma 90 (einstein_field_equation_real).  source ↗

The Einstein field equation from the thermodynamic equation of state — with the ACTUAL curvature. Instantiating einstein_field_equation at Ric = ricci g gi, R = scalarCurv g gi, and discharging the bianchi hypothesis with the machine-checked twice_contracted_bianchi (∇^μRic=½∂R). The conclusion now features the genuine Einstein tensor einsteinTensor = Ric − ½R·g: a·T_{μν} = G_{μν} + Λ·g_{μν}, Λ := f + ½R covariantly constant. The ONLY remaining hypotheses are the cited physics — the post-crux Clausius relation a·T = Ric + f·g (area law + Unruh + Raychaudhuri, supplied as crux) and local conservation ∇^μ(aT)=0 (conserv). Everything geometric is now proven; axiom-free.

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(abc:Fin n),(λy↦Γbca(y))∈C∞)→∀(T:Mn→Fin n→Fin n→R)(f:Mn→R)(a:R)(x:Mn),(∀(ρ:Fin n),PdiffAt f ρ x)→(∀(y:Mn)(a′b:Fin n),a⋅Ta′b(y)=Ra′b(y)+f y⋅ga′b(y))→(∀(ν:Fin n),(∇ ⁣⋅λya′b↦a⋅Ta′b(y))ν(x)=0)→(∀(μν:Fin n),a⋅Tμν(x)=Gμν(x)+(f x+1/2⋅R(x))⋅gμν(x))∧∀(ν:Fin n),∂ν(λy↦f y+1/2⋅R(y))(x)=0(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g_{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g^{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b c : \mathrm{Fin}\,n), ({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-christoffel}{\Gamma^{{a}}_{{b}{c}}({y})}})\in C^{\infty}) \to \forall (T : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathrm{Fin}\,n \to \mathrm{Fin}\,n \to \mathbb{R}) (f : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathbb{R}) (a : \mathbb{R}) (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}), (\forall (\rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,f\,\rho\,x) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a^{\prime} b : \mathrm{Fin}\,n), a \cdot T_{{a^{\prime}}{b}}({y}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({y})} + f\,y \cdot g_{{a^{\prime}}{b}}({y})) \to (\forall (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({y})})_{{\nu}}({x})} = 0) \to (\forall (\mu \nu : \mathrm{Fin}\,n), a \cdot T_{{\mu}{\nu}}({x}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-einsteintensor}{G_{{\mu}{\nu}}({x})} + (f\,x + 1/2 \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-scalarcurv}{R({x})}) \cdot g_{{\mu}{\nu}}({x})) \wedge \forall (\nu : \mathrm{Fin}\,n), \partial_{{\nu}}({\lambda y \mapsto f\,y + 1/2 \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-scalarcurv}{R({y})}})({x}) = 0

Proof. By PdiffAt_of_contDiff, mul, PdiffAt_sum, PdiffAt_ricci, twice_contracted_bianchi, einstein_field_equation. □\square

Used by einstein_field_equation_real_global.

Lemma 91 (einstein_field_equation_real_global).  source ↗

The Einstein field equation with a GENUINE cosmological constant. If the cited physics holds at every point (crux everywhere — it already is — and conserv everywhere), then Λ := f + ½R is a true constant (not just covariantly constant at a point), by const_of_pd_zero on the connected domain Point n. The Einstein field equation holds globally: a·T_{μν} = G_{μν} + Λ·g_{μν} for a single constant Λ. Axiom-free; the only hypotheses are the cited physics + smoothness of f + ½R.

(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),gab(y)=gba(y))→(∀(y:Mn)(ab:Fin n),∑σgaσ(y)⋅gσb(y)=δab)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(ab:Fin n),(λy↦gab(y))∈C∞)→(∀(abc:Fin n),(λy↦Γbca(y))∈C∞)→∀(T:Mn→Fin n→Fin n→R)(f:Mn→R)(a:R),(∀(x:Mn)(ρ:Fin n),PdiffAt f ρ x)→(Differentiable R λy↦f y+1/2⋅R(y))→(∀(y:Mn)(a′b:Fin n),a⋅Ta′b(y)=Ra′b(y)+f y⋅ga′b(y))→(∀(x:Mn)(ν:Fin n),(∇ ⁣⋅λya′b↦a⋅Ta′b(y))ν(x)=0)→∃Λ,∀(x:Mn)(μν:Fin n),a⋅Tμν(x)=Gμν(x)+Λ⋅gμν(x)(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a b : \mathrm{Fin}\,n), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g_{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b : \mathrm{Fin}\,n), ({\lambda y \mapsto g^{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b c : \mathrm{Fin}\,n), ({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-christoffel}{\Gamma^{{a}}_{{b}{c}}({y})}})\in C^{\infty}) \to \forall (T : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathrm{Fin}\,n \to \mathrm{Fin}\,n \to \mathbb{R}) (f : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}} \to \mathbb{R}) (a : \mathbb{R}), (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (\rho : \mathrm{Fin}\,n), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,f\,\rho\,x) \to (\mathrm{Differentiable}\,\mathbb{R}\,\lambda y \mapsto f\,y + 1/2 \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-scalarcurv}{R({y})}) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (a^{\prime} b : \mathrm{Fin}\,n), a \cdot T_{{a^{\prime}}{b}}({y}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({y})} + f\,y \cdot g_{{a^{\prime}}{b}}({y})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (\nu : \mathrm{Fin}\,n), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({y})})_{{\nu}}({x})} = 0) \to \exists \Lambda, \forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{n}}}) (\mu \nu : \mathrm{Fin}\,n), a \cdot T_{{\mu}{\nu}}({x}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-einsteintensor}{G_{{\mu}{\nu}}({x})} + \Lambda \cdot g_{{\mu}{\nu}}({x})

Proof. By pd, const_of_pd_zero, einstein_field_equation_real. □\square

Used by jacobson_einstein_equation_of_state.

Lemma 92 (crux_of_pernull).  source ↗

Phase 3 — wire the per-null Clausius relation to the tensor crux. This derives the crux hypothesis (a·T = R + f·g) used everywhere above, from the genuinely primitive per-null Clausius relation: at each point, the heat tensor a·T − R vanishes on the entire null cone of the metric g x. That per-null relation is exactly Jacobson’s premise (the Clausius relation δQ = TδS imposed on every local Rindler horizon, with horizon entropy ∝ area). The upgrade from per-null-direction to a tensor is the algebraic crux, here for the general (curved) Lorentzian metric via symmTensor_eq_smul_metric_of_null_general — the Lorentzian structure enters as the pointwise congruence to Minkowski g x = Pᵀ·η·P (Sylvester’s law). …

(∀(x:M4)(a′b:Fin 4),Ta′b(x)=Tba′(x))→(∀(x:M4)(a′b:Fin 4),Ra′b(x)=Rba′(x))→∀(PPinv:M4→Fin 4→Fin 4→R),(∀(x:M4)(ij:Fin 4),∑kPik(x)⋅(P−1)kj(x)=δij)→(∀(x:M4)(ij:Fin 4),∑k(P−1)ik(x)⋅Pkj(x)=δij)→(∀(x:M4)(ij:Fin 4),gij(x)=∑k∑lPki(x)⋅ηkl⋅Plj(x))→(∀(x:M4)(v:Fin 4→R),(g x)(v,v)=0→(λa′b↦a⋅Ta′b(x)−Ra′b(x))(v,v)=0)→∃f,∀(x:M4)(a′b:Fin 4),a⋅Ta′b(x)=Ra′b(x)+f x⋅ga′b(x)(\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), T_{{a^{\prime}}{b}}({x}) = T_{{b}{a^{\prime}}}({x})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({x})} = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{b}{a^{\prime}}}({x})}) \to \forall (P \mathrm{Pinv} : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}} \to \mathrm{Fin}\,4 \to \mathrm{Fin}\,4 \to \mathbb{R}), (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), \sum_{k} P_{{i}{k}}({x}) \cdot (P^{-1})_{{k}{j}}({x}) = \delta_{ij}) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), \sum_{k} (P^{-1})_{{i}{k}}({x}) \cdot P_{{k}{j}}({x}) = \delta_{ij}) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), g_{{i}{j}}({x}) = \sum_{k} \sum_{l} P_{{k}{i}}({x}) \cdot \href{/browser/qiqth-einsteinequationofstate#d-qiqth-einsteineos-gm}{\eta_{{k}{l}}} \cdot P_{{l}{j}}({x})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (v : \mathrm{Fin}\,4 \to \mathbb{R}), \href{/browser/qiqth-einsteinequationofstate#d-qiqth-einsteineos-bl}{({g\,x})({v},{v})} = 0 \to ({\lambda a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({x}) - \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({x})}})({v},{v}) = 0) \to \exists f, \forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), a \cdot T_{{a^{\prime}}{b}}({x}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({x})} + f\,x \cdot g_{{a^{\prime}}{b}}({x})

Proof. By symmTensor_eq_smul_metric_of_null_general. □\square

Used by jacobson_einstein_equation_of_state.

Lemma 93 (jacobson_einstein_equation_of_state).  source ↗

THE END-TO-END THEOREM — Jacobson’s Einstein equation of state, wired together

jacobson_einstein_equation_of_state is the single theorem assembling the whole derivation: from the per-null Clausius relation (Jacobson’s one physics premise) to the Einstein field equation with a genuine cosmological constant, a·T_{μν} = G_{μν} + Λ·g_{μν}. It composes the two halves — crux_of_pernull (front) and einstein_field_equation_real_global (back) — through the proportionality scalar f. …

(∀(y:M4)(ab:Fin 4),gab(y)=gba(y))→(∀(y:M4)(ab:Fin 4),gab(y)=gba(y))→(∀(y:M4)(ab:Fin 4),∑σgaσ(y)⋅gσb(y)=δab)→(∀(ab:Fin 4),(λy↦gab(y))∈C∞)→(∀(ab:Fin 4),(λy↦gab(y))∈C∞)→(∀(abc:Fin 4),(λy↦Γbca(y))∈C∞)→∀(T:M4→Fin 4→Fin 4→R)(a:R),(∀(x:M4)(a′b:Fin 4),Ta′b(x)=Tba′(x))→(∀(x:M4)(a′b:Fin 4),Ra′b(x)=Rba′(x))→∀(PPinv:M4→Fin 4→Fin 4→R),(∀(x:M4)(ij:Fin 4),∑kPik(x)⋅(P−1)kj(x)=δij)→(∀(x:M4)(ij:Fin 4),∑k(P−1)ik(x)⋅Pkj(x)=δij)→(∀(x:M4)(ij:Fin 4),gij(x)=∑k∑lPki(x)⋅ηkl⋅Plj(x))→(∀(x:M4)(v:Fin 4→R),(g x)(v,v)=0→(λa′b↦a⋅Ta′b(x)−Ra′b(x))(v,v)=0)→(∀(f:M4→R),(∀(y:M4)(a′b:Fin 4),a⋅Ta′b(y)=Ra′b(y)+f y⋅ga′b(y))→(∀(x:M4)(ρ:Fin 4),PdiffAt f ρ x)∧Differentiable R λy↦f y+1/2⋅R(y))→(∀(x:M4)(ν:Fin 4),(∇ ⁣⋅λya′b↦a⋅Ta′b(y))ν(x)=0)→∃Λ,∀(x:M4)(μν:Fin 4),a⋅Tμν(x)=Gμν(x)+Λ⋅gμν(x)(\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a b : \mathrm{Fin}\,4), g_{{a}{b}}({y}) = g_{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a b : \mathrm{Fin}\,4), g^{{a}{b}}({y}) = g^{{b}{a}}({y})) \to (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a b : \mathrm{Fin}\,4), \sum_{\sigma} g_{{a}{\sigma}}({y}) \cdot g^{{\sigma}{b}}({y}) = \delta_{ab}) \to (\forall (a b : \mathrm{Fin}\,4), ({\lambda y \mapsto g_{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b : \mathrm{Fin}\,4), ({\lambda y \mapsto g^{{a}{b}}({y})})\in C^{\infty}) \to (\forall (a b c : \mathrm{Fin}\,4), ({\lambda y \mapsto \href{/browser/qiqth-curvature#d-qiqth-curvature-christoffel}{\Gamma^{{a}}_{{b}{c}}({y})}})\in C^{\infty}) \to \forall (T : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}} \to \mathrm{Fin}\,4 \to \mathrm{Fin}\,4 \to \mathbb{R}) (a : \mathbb{R}), (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), T_{{a^{\prime}}{b}}({x}) = T_{{b}{a^{\prime}}}({x})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({x})} = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{b}{a^{\prime}}}({x})}) \to \forall (P \mathrm{Pinv} : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}} \to \mathrm{Fin}\,4 \to \mathrm{Fin}\,4 \to \mathbb{R}), (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), \sum_{k} P_{{i}{k}}({x}) \cdot (P^{-1})_{{k}{j}}({x}) = \delta_{ij}) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), \sum_{k} (P^{-1})_{{i}{k}}({x}) \cdot P_{{k}{j}}({x}) = \delta_{ij}) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (i j : \mathrm{Fin}\,4), g_{{i}{j}}({x}) = \sum_{k} \sum_{l} P_{{k}{i}}({x}) \cdot \href{/browser/qiqth-einsteinequationofstate#d-qiqth-einsteineos-gm}{\eta_{{k}{l}}} \cdot P_{{l}{j}}({x})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (v : \mathrm{Fin}\,4 \to \mathbb{R}), \href{/browser/qiqth-einsteinequationofstate#d-qiqth-einsteineos-bl}{({g\,x})({v},{v})} = 0 \to ({\lambda a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({x}) - \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({x})}})({v},{v}) = 0) \to (\forall (f : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}} \to \mathbb{R}), (\forall (y : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (a^{\prime} b : \mathrm{Fin}\,4), a \cdot T_{{a^{\prime}}{b}}({y}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-ricci}{R_{{a^{\prime}}{b}}({y})} + f\,y \cdot g_{{a^{\prime}}{b}}({y})) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (\rho : \mathrm{Fin}\,4), \href{/browser/qiqth-curvature#d-qiqth-curvature-pdiffat}{\mathrm{PdiffAt}}\,f\,\rho\,x) \wedge \mathrm{Differentiable}\,\mathbb{R}\,\lambda y \mapsto f\,y + 1/2 \cdot \href{/browser/qiqth-curvature#d-qiqth-curvature-scalarcurv}{R({y})}) \to (\forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (\nu : \mathrm{Fin}\,4), \href{/browser/qiqth-einsteinfieldequation#d-qiqth-curvature-div02}{(\nabla\!\cdot {\lambda y a^{\prime} b \mapsto a \cdot T_{{a^{\prime}}{b}}({y})})_{{\nu}}({x})} = 0) \to \exists \Lambda, \forall (x : \href{/browser/qiqth-curvature#d-qiqth-curvature-point}{M^{{4}}}) (\mu \nu : \mathrm{Fin}\,4), a \cdot T_{{\mu}{\nu}}({x}) = \href{/browser/qiqth-curvature#d-qiqth-curvature-einsteintensor}{G_{{\mu}{\nu}}({x})} + \Lambda \cdot g_{{\mu}{\nu}}({x})

Proof. By einstein_field_equation_real_global, crux_of_pernull. □\square

Used by qiqt_bekenstein_gives_gr.


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