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The weak energy condition does not imply conservation of a prescribed stress-energy tensor

Physical scope

Pointwise algebraic statement about a prescribed smooth symmetric stress-energy tensor field on an open region of the flat classical spacetime model: the weak energy condition is a pointwise positivity condition on the tensor and carries no conservation content. No dynamical model, no solution of the field equation, no measurement and no claim about nature is asserted; the example shows only that the named condition is not by itself the conservation identity.

Statement refuted

Statement refuted: "Let M=R4 carry the flat metric g=diag⁡(−1,1,1,1) and the identity chart, and let U be an open subset. Let T be a smooth symmetric covariant 2-tensor field on U which satisfies the weak energy condition of The pointwise energy conditions WEC, NEC, DEC and SEC: Tp(v,v)≥0 for every timelike v∈TpM and every p∈U (Timelike, null, spacelike and causal vectors of a Lorentz vector space). Then T is conserved, ∇aTab=0 on U."

Facts & Assumptions

Given: The flat Lorentzian four-manifold (R4,g) with identity chart, g=diag⁡(−1,1,1,1), time orientation N=∂0, metric-selected connection ∇; length coordinates xa in metres (x0=ct), fixed constants L>0 in m and E∗>0 in J m−3, the open set U:={x∈R4:∣x1∣<L}; and the smooth symmetric covariant 2-tensor field T on U with components T00=3E∗,T01=T10=E∗x1/L,Tij=0 otherwise.

[L1]

On the identity chart Γ≡0, so ∇ is the coordinate connection and ∇aTab=gac∂cTab=ηac∂cTab with η=diag⁡(−1,1,1,1) (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields, The inverse metric, musical isomorphisms and index raising).

[L2]

The weak energy condition at p is Tp(v,v)≥0 for every timelike v∈TpM; a vector v=(v0,v1,v2,v3) is timelike exactly when −(v0)2+(v1)2+(v2)2+(v3)2<0, which implies ∣v1∣<∣v0∣ (The pointwise energy conditions WEC, NEC, DEC and SEC, Timelike, null, spacelike and causal vectors of a Lorentz vector space).

[L3]

U is an open subset of the smooth manifold R4, hence carries a restricted smooth structure and the field with the displayed components is a smooth symmetric covariant 2-tensor field on U (An open subset of a smooth manifold has a canonical restricted smooth structure, Smooth covariant 2-tensor fields on a smooth manifold, Cr and smooth maps between smooth manifolds).

Counterexample

1.1L2L3algebra

(Weak energy condition.) Let p∈U and let v=(v0,v1,v2,v3) be timelike. By [L2], ∣v1∣<∣v0∣, so in particular v≠0 and v0≠0. By the components of T, Tp(v,v)=E∗[3(v0)2+2(x1/L)v0v1]≥E∗[3(v0)2−2(∣x1∣/L)∣v0∣∣v1∣]≥E∗(3−2∣x1∣/L)(v0)2>E∗(v0)2>0, using ∣v1∣<∣v0∣ and ∣x1∣/L<1 on U, with E∗>0. Thus the weak energy condition of [L2] holds at every point of U.

1.2L1algebra

(Nonconservation.) By [L1] and the components of T (which are independent of x0), ∇aTa0=η00∂0T00+η11∂1T10=(−1)⋅0+1⋅(E∗/L)=E∗/L≠0. Hence T is not conserved on U.

2.1step 1.1step 1.2algebra∎

(Conclusion.) The tensor field T of the Facts satisfies the weak energy condition on U by step 1.1 and is not conserved by step 1.2, so the displayed statement is refuted: the weak energy condition is a pointwise positivity condition and does not imply the conservation identity.

Remarks

  • Source scope. Carroll (4.72) and Tong section 4.5.7 supply the weak-energy-condition definition. The prescribed tensor and its nonconservation are established by the local calculation above; no source passage is cited as asserting this counterexample or the nonimplication.

  • No field-equation claim. The counterexample does not assert that T solves the Einstein equation with the flat metric; a model whose field law holds must additionally satisfy the conservation derived in Consistency conditions of the adopted field law: conservation, trace, parameter variation and the energy conditions of a perfect fluid, which this T fails. The point is exactly that the energy condition alone does not supply that consistency.

  • Sign conventions. The condition T(v,v)≥0 is evaluated with the metric convention g=diag⁡(−1,1,1,1); the inequality ∣v1∣<∣v0∣ used in the proof is the timelike condition of Timelike, null, spacelike and causal vectors of a Lorentz vector space for this convention.

  • No empirical content. No measurement or material realization is asserted. The constants E∗ and L set the units of the prescribed test field: every displayed tensor entry has energy-density units, and its nonzero divergence has units J m−4. No numerical measured values are assigned (SI unit and coordinate conventions of the classical gravitational framework).

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