Pith. sign in
lemma

gMetric_offdiag

proved
show as:
module
IndisputableMonolith.Relativity.Cosmology.FRWComponentsProbe
domain
Relativity
line
56 · github
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plain-language theorem explainer

Off-diagonal components of the flat FRW metric vanish identically as functions of cosmic time. Anyone simplifying Christoffel symbols or Ricci terms in the Fin-4 FRW encoding cites this. The proof is a one-line unfold of the metric definition under the index inequality, discharged by simp after funext.

Claim. Let $a:\mathbb{R}\to\mathbb{R}$ be a scale factor and let $\mu,\nu\in\{0,1,2,3\}$ with $\mu\neq\nu$. Then the metric component $g_{\mu\nu}(a)$ is the zero function of cosmic time: $g_{\mu\nu}(a)(t)=0$ for all $t$.

background

The module is a standalone tractability probe for flat FRW geometry before locking a full two-layer Friedmann skeleton. Encoding: homogeneous flat FRW with $k=0$ and $c=1$; every field depends only on cosmic time $t$, so spatial partials vanish and $\partial_0$ is ordinary differentiation.

The metric is a componentwise map on $\mathrm{Fin},4\times\mathrm{Fin},4$ sending a scale factor $a$ to functions of $t$. Diagonal entries carry the usual $-1$ and $a(t)^2$ structure; off-diagonal slots are defined to be zero. Time is identified with $\mathbb{R}$ in RS-native units.

Probe targets named by the cosmo-chain panel are $\Gamma^0_{ii}=a\dot a$ and $\Gamma^i_{0i}=\dot a/a$. Vanishing off-diagonals are the first algebraic fact those Christoffel computations need.

proof idea

Term-style one-liner: extensionality on the cosmic-time argument, then simp unfolds the metric definition and uses the hypothesis $\mu\neq\nu$ to hit the zero branch. No external lemmas beyond the definition of the metric and the inequality on indices.

why it matters

This is the basic diagonal-support fact for the FRW component probe. Downstream, christoffel_symm in the Friedmann module uses it twice (once for each order of indices) to show $g_{mn}=g_{nm}$ when $m\neq n$, which makes the Christoffel bracket symmetric in the lower indices by definition. The sibling time-derivative lemma for $a^2$ is written in the lambda form that metric simp lemmas produce, so the off-diagonal rule participates in the same simp set.

If the probe closes ($\Gamma^0_{ii}=a\dot a$, $\Gamma^i_{0i}=\dot a/a$), the full skeleton (Ricci, Einstein tensor, Friedmann I/II from a named Einstein-equations proposition) locks as loop targets. The lemma is pure differential algebra on the Fin-4 encoding; it does not itself invoke the Recognition forcing chain, but it is the gate that must open before cosmological Einstein equations can be stated in this codebase.

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