ProofComplete

Proof of the First and Second Variation Formulas

The variation formulas compute how the energy of a curve changes under deformation, establishing geodesics as critical points and providing the tools for analyzing their stability.


Setup

Definition8.9Variation of a curve

A variation of a curve γ:[a,b]→M\gamma: [a,b] \to M is a smooth map Γ:[a,b]×(−ϵ,ϵ)→M\Gamma: [a,b] \times (-\epsilon, \epsilon) \to M with Γ(t,0)=γ(t)\Gamma(t, 0) = \gamma(t). The variation vector field is V(t)=∂Γ∂s(t,0)V(t) = \frac{\partial \Gamma}{\partial s}(t, 0). The variation is proper (fixed-endpoint) if Γ(a,s)=γ(a)\Gamma(a, s) = \gamma(a) and Γ(b,s)=γ(b)\Gamma(b, s) = \gamma(b) for all ss.


First Variation Formula

Theorem8.8First variation of energy

Let γ:[a,b]→M\gamma: [a,b] \to M be a smooth curve and Γ\Gamma a proper variation with variation vector field VV. Then

dEds∣s=0=−∫abg(∇γ′γ′,V) dt.\frac{dE}{ds}\Big|_{s=0} = -\int_a^b g(\nabla_{\gamma'}\gamma', V) \, dt.
Proof

Write T=∂Γ∂tT = \frac{\partial \Gamma}{\partial t} and V=∂Γ∂sV = \frac{\partial \Gamma}{\partial s}. Then:

dEds=12dds∫abg(T,T) dt=∫abg(∇VT,T) dt.\frac{dE}{ds} = \frac{1}{2}\frac{d}{ds}\int_a^b g(T, T) \, dt = \int_a^b g(\nabla_V T, T) \, dt.

By the symmetry lemma: ∇VT=∇TV\nabla_V T = \nabla_T V (since [T,V]=[∂t,∂s]=0[T, V] = [\partial_t, \partial_s] = 0). So:

dEds=∫abg(∇TV,T) dt=∫ab(ddtg(V,T)−g(V,∇TT))dt.\frac{dE}{ds} = \int_a^b g(\nabla_T V, T) \, dt = \int_a^b \left(\frac{d}{dt}g(V, T) - g(V, \nabla_T T)\right) dt.

The first term integrates to g(V,T)∣ab=0g(V, T)\Big|_a^b = 0 (proper variation: V(a)=V(b)=0V(a) = V(b) = 0). Thus:

dEds∣s=0=−∫abg(V,∇γ′γ′) dt.■\frac{dE}{ds}\Big|_{s=0} = -\int_a^b g(V, \nabla_{\gamma'}\gamma') \, dt. \quad \blacksquare
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RemarkGeodesics as critical points

The first variation vanishes for all proper variations if and only if ∇γ′γ′=0\nabla_{\gamma'}\gamma' = 0, i.e., γ\gamma is a geodesic. This is the Euler-Lagrange equation for the energy functional.


Second Variation Formula

Theorem8.9Second variation of energy

Let γ:[a,b]→M\gamma: [a,b] \to M be a geodesic and Γ\Gamma a proper variation with variation vector field VV. Then

d2Eds2∣s=0=∫ab(g(∇γ′V,∇γ′V)−g(R(V,γ′)γ′,V))dt=∫ab(∣V′∣2−K(V,γ′)∣V∧γ′∣2)dt,\frac{d^2 E}{ds^2}\Big|_{s=0} = \int_a^b \left(g(\nabla_{\gamma'} V, \nabla_{\gamma'} V) - g(R(V, \gamma')\gamma', V)\right) dt = \int_a^b \left(|V'|^2 - K(V, \gamma')|V \wedge \gamma'|^2\right) dt,

where V′=∇γ′VV' = \nabla_{\gamma'} V and KK is the sectional curvature.

Proof

Differentiating dEds=∫g(∇TV,T) dt\frac{dE}{ds} = \int g(\nabla_T V, T) \, dt once more:

d2Eds2=∫ab(g(∇V∇TV,T)+g(∇TV,∇VT))dt.\frac{d^2E}{ds^2} = \int_a^b \left(g(\nabla_V \nabla_T V, T) + g(\nabla_T V, \nabla_V T)\right) dt.

For the first term, use ∇V∇TV=∇T∇VV+R(V,T)V\nabla_V \nabla_T V = \nabla_T \nabla_V V + R(V, T)V (definition of curvature and [T,V]=0[T,V] = 0). At s=0s = 0, ∇TT=0\nabla_T T = 0 (geodesic), so integrating by parts:

∫g(∇T∇VV,T) dt=g(∇VV,T)∣ab−∫g(∇VV,∇TT) dt=0.\int g(\nabla_T \nabla_V V, T) \, dt = g(\nabla_V V, T)\Big|_a^b - \int g(\nabla_V V, \nabla_T T) \, dt = 0.

The curvature term gives ∫g(R(V,T)V,T) dt=−∫g(R(V,T)T,V) dt\int g(R(V, T)V, T) \, dt = -\int g(R(V, T)T, V) \, dt. The second term in the original sum is ∫∣∇TV∣2 dt\int |\nabla_T V|^2 \, dt. Combining at s=0s = 0:

d2Eds2∣s=0=∫ab(∣∇γ′V∣2−g(R(V,γ′)γ′,V))dt.■\frac{d^2E}{ds^2}\Big|_{s=0} = \int_a^b \left(|\nabla_{\gamma'} V|^2 - g(R(V, \gamma')\gamma', V)\right) dt. \quad \blacksquare
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The Index Form

Definition8.10Index form

The index form along a geodesic γ\gamma is the bilinear form on vector fields along γ\gamma vanishing at endpoints:

I(V,W)=∫ab(g(∇γ′V,∇γ′W)−g(R(V,γ′)γ′,W))dt.I(V, W) = \int_a^b \left(g(\nabla_{\gamma'} V, \nabla_{\gamma'} W) - g(R(V, \gamma')\gamma', W)\right) dt.

The second variation equals I(V,V)I(V, V). The geodesic is a local minimum if and only if II is positive definite, which holds precisely when there are no conjugate points in (a,b)(a, b).