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The measured energy density of a fixed tensor depends on the observer congruence
A flat-space kinematic counterexample in the framework's reading: the energy density assigned by the observer split of a fixed smooth symmetric tensor depends on the chosen observer congruence, shown for a static dust tensor measured by a static and by a boosted congruence. The statement refuted is the observer independence of the measured energy density in the smooth branch; no dynamics, no conservation, no measurement and no empirical claim is involved.
Statement refuted
Statement refuted: "Let be a nonempty open subset of a time-oriented smooth Lorentzian four-manifold and let be a smooth symmetric covariant -tensor field on . If and are smooth observer congruences on , then the measured energy densities of The observer split of a symmetric two-tensor: energy density, energy-momentum current, flux and stress agree, on ."
Facts & Assumptions
Given: The flat Lorentzian four-manifold with identity chart, and time orientation , with the metric-selected connection; the constant , read as rest energy density in with the SI rest-mass density; the dust model with and tensor (The dust matter model: rest density, four-velocity, stress-energy and dust system); the number , ; and the vector fields and .
and are smooth future-directed unit timelike vector fields on , hence observer congruences: , , and , (Observer congruences, their observer curves and adapted charts, Observers, rest spaces and the spatial projection at an event, Timelike, null, spacelike and causal vectors of a Lorentz vector space, Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).
The measured energy density is (The observer split of a symmetric two-tensor: energy density, energy-momentum current, flux and stress clause (b), Physical reading of the observer split: measured energy density, energy flux and momentum density, and measured stress clause (a)).
On the identity chart the metric equals its inverse, , and with (The inverse metric, musical isomorphisms and index raising, Smooth covariant 2-tensor fields on a smooth manifold).
Counterexample
(Two congruences.) By [L1], and are both smooth observer congruences on , and they are distinct because has the nonzero spatial component .
(The tensor.) is the tensor of the dust model ; it is a smooth symmetric type tensor field, equivalently after lowering both indices with [L3].
(Energy density for the static congruence.) For , [L3] gives , so by [L2].
(Energy density for the boosted congruence.) For , [L1] and [L3] give . Hence by [L2], and because implies .
(Conclusion.) The fixed smooth symmetric tensor assigns the energy density to the congruence and to the congruence , and these values differ since . The displayed statement is therefore refuted: in the framework's reading, measured energy density is observer dependent. This completes the counterexample.
Remarks
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What the counterexample does not say. It does not contradict the algebraic decomposition of The orthogonal observer decomposition of a symmetric two-tensor and its uniqueness, which holds for each congruence separately; it shows that the measured density is not a property of alone. In the framework's reading this is the kinematic fact that a moving medium has a boosted energy density.
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No empirical content. Both congruences are idealizations and no measurement is asserted; the comparison is between two exact model readings of one prescribed tensor.
Depends on
The observer split of a symmetric two-tensor: energy density, energy-momentum current, flux and stress
The orthogonal observer decomposition of a symmetric two-tensor and its uniqueness
Physical reading of the observer split: measured energy density, energy flux and momentum density, and measured stress
The dust matter model: rest density, four-velocity, stress-energy and dust system
Observer congruences, their observer curves and adapted charts
Observers, rest spaces and the spatial projection at an event
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Metric compatibility, torsion freedom and the metric-selected connection class
Smooth covariant 2-tensor fields on a smooth manifold
The inverse metric, musical isomorphisms and index raising
Timelike, null, spacelike and causal vectors of a Lorentz vector space
Dependency tree · 2 levels
Sources
- E. Gourgoulhon, 3+1 Formalism and Bases of Numerical Relativity, arXiv:gr-qc/0703035v1 (2007), section 4.1.2: the energy density E = T(n,n) is the density measured by the Eulerian observer, so it is tied to the chosen normal n, printed p. 52 (PDF p. 52)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 4.5.3: T_{mu nu}u^mu u^nu = rho is the energy density measured by an observer comoving with the fluid, printed p. 186 (PDF p. 193)