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Explicit isotropic-to-areal conversion and the second-order scalar-coefficient comparison of the Schwarzschild exterior
Example
Let be the Schwarzschild exterior datum with Schwarzschild radius , and (The Schwarzschild exterior model datum: domain, metric, mass parameter and time orientation, The Schwarzschild exterior datum is a smooth time-oriented Lorentzian four-manifold). Let
be the isotropic-to-areal radius map of The isotropic coordinate form of the Schwarzschild exterior metric and the isothermal radius shift and let be its inverse, so that the isotropic coefficient of the spatial metric is the function and the areal coefficient is . The two displayed functions are coefficients in different radial bases. The following scalar-function comparisons do not identify their tensor components after a change of basis; that transformation is included in clause 5.
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Exact form and positivity. and on ; the inverse is .
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Conversion and areal expansion. With , These are expansions as with fixed . The areal coefficient satisfies, exactly for , so its expansion is .
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Isotropic coefficient after argument substitution. With one has and Hence these scalar functions agree through first order and differ at second order by .
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Failure of the unconverted comparison. Evaluating the isotropic coefficient at instead of at gives which differs from the areal coefficient of clause 2 by at second order: the consistency of the leading Newtonian-type term is unaffected, but the comparison of coefficients in the unchanged chart is already wrong at relative order .
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Radial tensor transformation. Put . Differentiating gives . Consequently the radial coefficient in the areal basis is exactly Moreover , so this coefficient is : the apparent discrepancy of clause 3 disappears when the basis is transformed.
Facts & Assumptions
Given: The exterior datum with Schwarzschild radius , the functions , , the areal coefficient and the isotropic coefficient .
is a smooth bijection of onto with smooth inverse , , the exact algebraic identity , and the asymptotic expansion for fixed as (The isotropic coordinate form of the Schwarzschild exterior metric and the isothermal radius shift clauses (a) and (c), The derivative of at a point that is a limit point of , and differentiability on a set, Sums, scalar multiples, products and quotients: , , , and when , Rational powers of a positive base).
For , by multiplication by (Sums, scalar multiples, products and quotients: , , , and when , Rational powers of a positive base).
In the isotropic chart of the datum the spatial coefficient is and in a spherical-polar product chart (The isotropic coordinate form of the Schwarzschild exterior metric and the isothermal radius shift clause (b), The Schwarzschild exterior datum is a smooth time-oriented Lorentzian four-manifold clause (a), The Schwarzschild exterior model datum: domain, metric, mass parameter and time orientation clause (c)).
The identity holds for every real ; on one has so and , and the interval is nonempty (Sums, scalar multiples, products and quotients: , , , and when , Intervals of : the nine order-convex forms, nondegeneracy, and length, Rational powers of a positive base).
The chain rule for differentiable functions on open real intervals gives from (The chain rule, in one line from Carathéodory: if is differentiable at and is differentiable at , then is differentiable at with ); the radial term of the metric in [L3] is , so in the areal chart.
Proof
(Exact form and inverse.) By [L1], , so , which is positive exactly because , that is ; [L1] also gives the displayed inverse , and the identity holds on . This is clause 1.
(Expansion of the inverse.) By [L1], for fixed and , Write , where . For all sufficiently large , , and the exact identity gives All remainder estimates here are for fixed and . This proves the two expansions of clause 2.
(Areal expansion.) For the identity is exact by [L2]; since by [L4], the last term is positive and satisfies , so with remainder at most , which is on . This is the second display of clause 2.
(Isotropic coefficient after conversion.) By step 1.2, , so with , [L4] gives , hence . Combining with step 1.3, the two coefficients agree in their constant and terms and differ in their terms by ; this is clause 3.
(Unconverted comparison.) Evaluating at gives and by [L4] ; subtracting the areal expansion of step 1.3 termwise gives the mismatch at second order, while the constant and first-order terms continue to agree. This is clause 4 as a comparison of scalar coefficient functions, not a metric transformation.
(Transforming the radial basis.) By [L1] and [L5], with . Since for , the transformed radial coefficient is . Step 1.2 gives ; for , the exact remainder identity gives . Multiplication by the expansion of step 2.1 changes its second-order coefficient from to , exactly as in step 1.3. This proves clause 5.
Remarks
- What the example checks. The computation is exact finite algebra with remainder bounds as : after argument substitution alone, the second-order isotropic coefficient is , where comes from the coordinate shift in and from the fourth-power expansion. The areal coefficient has second-order coefficient , so their difference is ; the remainder of contributes only at third order. The radial tensor coefficient additionally includes the squared Jacobian of clause 5 and agrees exactly with the areal coefficient. No numerical value of , no observed system and no measurement occurs.
Depends on
The Schwarzschild exterior model datum: domain, metric, mass parameter and time orientation
The isotropic coordinate form of the Schwarzschild exterior metric and the isothermal radius shift
The Schwarzschild exterior datum is a smooth time-oriented Lorentzian four-manifold
The derivative of at a point that is a limit point of , and differentiability on a set
Sums, scalar multiples, products and quotients: , , , and when
Rational powers of a positive base
Continuity and derivatives of positive-base real powers
Intervals of : the nine order-convex forms, nondegeneracy, and length
The chain rule, in one line from Carathéodory: if is differentiable at and is differentiable at , then is differentiable at with
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 7: the Schwarzschild metric (7.29) and its reduction to conformally flat spatial form by r = rho(1+GM/2rho)^2, printed pp. 169-172 (PDF pp. 176-179)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 5.1.1: the warning that Newtonian-limit coefficients must be compared in one and the same coordinate system, printed p. 210 (PDF p. 217); section 6.1: the Schwarzschild metric (6.1) and its domain r > 2GM, printed pp. 232-233 (PDF pp. 239-240)
- P. K. Townsend, Black Holes, arXiv:gr-qc/9707012v1 (1997), section 2.3.3 (2.60): the isotropic form ds^2 = -[(1-M/2rho)/(1+M/2rho)]^2 dt^2 + (1+M/2rho)^4(drho^2 + rho^2 dOmega^2), printed p. 25