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Constructed regular-center local static TOV branch

Physical scope

Local branch around a regular center for a supplied smooth positive EOS and compact central-pressure range in the adopted classical static isotropic Lambda=0 model; no global surface, global horizon avoidance, realistic EOS, empirical claim, or dynamical stability.

Statement

Assume the adopted model Static spherical Einstein-fluid model with a supplied equation of state with its supplied C∞ positive EOS E:IP→(0,∞) on an open pressure interval IP⊂(0,∞). Let Pc⊂IP be a nonempty compact interval, let δ>0 be such that its closed δ-neighbourhood lies in IP, and choose a central pressure P0∈Pc and a dimensionless central lapse eϕc>0. Under the exact mathematical convention ZF+ACω of Regular-center TOV local existence and dependence, put K=4πG/c4. There is a common R0>0 and, for each P0∈Pc, smooth even profiles P,v on [−R0,R0] with P(r)∈IP for every ∣r∣≤R0 and satisfying v(r)=K∫01s2E(P(rs)) ds,P(r)=P0−∫0rt(E(P(t))+P(t))(v(t)+KP(t))1−2t2v(t) dt, with P(0)=P0, v(0)=KE(P0)/3, b(r):=1−2r2v(r)≥1/2, and P′(0)=v′(0)=0. Defining M(r)=c2Gr3v(r),ϕ(r)=ϕc+∫0rtv(t)+KP(t)1−2t2v(t) dt, gives a positive-lapse C2 metric center and a local solution of the adopted Einstein-fluid equations. On r>0 its equations are M′=4πr2E(P)c2,ϕ′=GM/c2+4πGr3P/c4r2b,P′=−G(E(P)+P)(M+4πr3P/c2)c2r2b. No conclusion is made that the branch reaches a finite zero-pressure surface, remains horizon-free globally, or is dynamically stable.

Facts & Assumptions

Given: The adopted static Einstein-fluid model, a smooth positive supplied EOS, a compact central-pressure range with the stated margin, ϕc∈R, and the exact ZF+ACω convention of the mathematical suppliers.

[F1]

Static spherical Einstein-fluid model with a supplied equation of state adopts the Λ=0 field equation on each open fluid interval J, where its pressure map is P∈C∞(J,IP), the restriction of the earlier pressure component p, and its energy density is E∘P; E is a supplied smooth positive function, not a derived EOS.

[F2]

Regular-center TOV local existence and dependence: for positive smooth E on IP, compact Pc with a closed pressure margin, and ϕc∈R, the even Volterra profiles displayed in the Statement exist smoothly on a common interval and obey ∣P(r)−P0∣≤δ, hence P(r)∈IP; they satisfy b≥1/2 and give a C2 Cartesian center and local continuity in P0. The theorem assumes ZF+ACω.

[F3]

Complete spherical Einstein and conservation reduction: on every smooth r>0 interval with b>0, the mass, lapse, and pressure equations are equivalent to all mixed Einstein equations under the stated (−,+,+,+) curvature convention.

[A1]

The field equation and EOS in [F1] are adopted model premises, not deductions about nature.

Proof

1.1givenA1F1F2

The supplied E, compact interval Pc, pressure margin δ, and central lapse meet [F2] exactly. Its Volterra construction gives the even smooth P,v, the lower bound b≥1/2, and the displayed integral formula for ϕ; in particular the center is regular in the stated C2 Cartesian sense.

2.1A1F1F2F3step 1.1algebra∎

The constructed profiles satisfy the mass, pressure, and lapse equations in [F3] on r>0, with ε(r)=E(P(r)) and b>0. The converse direction of [F3] therefore gives every mixed Einstein component of the adopted model on the punctured neighborhood. In Cartesian coordinates the static unit vector u=e−ϕ∂x0 and metric are continuous, and the isotropic stress has covariant form Tab=(ε+P)uaub+Pgab, so its components extend continuously to the center. A C2 metric has a continuous Einstein tensor; equality on the punctured neighborhood therefore extends to the center.

Depends on

Dependency tree · 2 levels

Sources