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Half-compactness constant-density Einstein star

Physical scope

The explicit constant-density family at u=1/2, with its adopted vacuum exterior; not an observed star, realistic EOS, or generic compactness result.

Example

Specialize the constant-density family of Verified constant-density static star and vacuum exterior to u=1/2. Then a=12,P(0)ε0=2−13−2∈(0,1),eϕ(0)=3/2−12>0. At the surface, b(R)=1/2 and eϕ(R)=1/2. The prescribed vacuum exterior has M=MR, b(r)=1−R/(2r) and eϕ(r)=b(r) for r≥R.

Facts & Assumptions

Given: The exact static star family and its equations from Verified constant-density static star and vacuum exterior, with the specialization u=1/2.

[F1]

Verified constant-density static star and vacuum exterior gives a=1−u, B(r)=1−ur2/R2, P(0)/ε0=(1−a)/(3a−1), eϕ(0)=(3a−1)/2, and the vacuum exterior b(r)=1−uR/r, eϕ=b.

Verification

1.1givenF1algebra

Substitution of u=1/2 gives a=1/2 and hence P(0)/ε0=(2−1)/(3−2). Both numerator and denominator are positive, and 2−1<3−2 because 2<2; thus the ratio lies strictly between zero and one. Also eϕ(0)=(3/2−1)/2>0, b(R)=a2=1/2, and eϕ(R)=a=1/2.

2.1F1step 1.1∎

With u=1/2, the exterior formula in [F1] becomes b(r)=1−R/(2r); it is positive for r≥R and has eϕ=b. The theorem supplies the matching and field-equation verification for this family, so this specialization is a finite, positive-pressure example within the adopted model.

Depends on

Dependency tree · 2 levels

Sources