Introduction

Technically, an observer can only measure time using his own proper time by bringing a clock with him and read it out. This is beacuse without a proper synchronization scheme, there is no definition of simultaneity for clocks placed at different places. Let us say there is some arbitrary synchronziation scheme that the observer uses to define the time coordinate in the whole spacetime, denoted as tt, so that each spacetime location is (t,x)\p{t,x}, where the space coordinate xx lives on a (static) connected Riemannian manifold MM (so the spacetime is R×M\bR\times M). Denote x=ox=o to be a fixed point on MM where the observer stays, and tt gives the proper time for the observer on the worldline t↦(t,o)t\mapsto\p{t,o}. In principle, a function τ:R×M→R\tau:\bR\times M\to\bR such that τ ⁣(t,o)=t\fc\tau{t,o}=t and that (t,x)↦(τ ⁣(t,x),x)\p{t,x}\mapsto\p{\fc\tau{t,x},x} is bijective defines a gauge to produce a different time coordinate which is just as good as (t,x)↦t\p{t,x}\mapsto t. The speed of light is then gauge-dependent, so the naive interpretation of constant speed of light fails.

However, there is still something physically meaningful to measure: the average speed of light along a closed path on MM starting and ending at oo. Because the time coordinate of the event (t,o)\p{t,o} must be tt (physically the proper time of the observer) in any gauge, if the emission and the reception of a light signal are both at oo, then their time difference is gauge independent, so the average speed of this light signal can be physically measured. The natural question to ask is then whether a gauge where the speed of light is constant everywhere always exists as long as the roundtrip average speed of light is always constant.

Minguzzi and Macdonald (2003) addressed the same problem in a less general way.

Gauge transformation

As we stated before, a gauge transformation is given by a function τ:R×M→R\tau:\bR\times M\to\bR such that τ ⁣(t,o)=t\fc\tau{t,o}=t and that (t,x)↦(τ ⁣(t,x),x)\p{t,x}\mapsto\p{\fc\tau{t,x},x} is bijective. Equivalently, τ ⁣(⋅,x)\fc\tau{\cdot,x} is bijective for any x∈Mx\in M and is specially the identity function for x=ox=o. Abusing the notation, denote t ⁣(⋅,x)\fc t{\cdot,x} as the inverse function of τ ⁣(⋅,x)\fc\tau{\cdot,x}. Then we say t:R×M→Rt:\bR\times M\to\bR gives the inverse gauge transformation of τ:R×M→R\tau:\bR\times M\to\bR.

Now let us find the gauge transformation for the speed of light. Let us assume that the speed of light depends only on properties local to each point on the trajectory along which the light travels: the spacetime coordinates and the tangent direction of the trajectory at that point. In other words, the inverse speed of light c−1 ⁣(t,x,u)∈R\fc{c^{-1}}{t,x,u}\in\bR is a function of time t∈Rt\in\bR, spatial location x∈Mx\in M, and direction u∈UTxMu\in\mrm{UT}_xM (the unit sphere of TxM\mrm T_xM; I will denote the unit tangent bundle of MM as UTM\mrm{UT}M).

It is easy to write down the differential equation governing the propagation of light on a given trajectory. From now on, when I say a curve or path on MM, I mean a length-parametrized piecewise differentiable curve on MM. Let γ\gma be a curve on MM. Denote γ′ ⁣(s)\fc{\gma'}s to be the tangent vector at parameter value ss, which is a unit vector in Tγ ⁣(s)M\mrm T_{\fc\gma s}M. Then, the worldline of the light travelling along γ\gma parametrized by ss is s↦(t ⁣(s),γ ⁣(s))s\mapsto\p{\fc ts,\fc\gma s}, where tt satisfies the differential equation t′ ⁣(s)=c−1 ⁣(t ⁣(s),γ ⁣(s),γ′ ⁣(s)).\fc{t'}s=\fc{c^{-1}}{\fc ts,\fc\gma s,\fc{\gma'}s}. (1)(1) From Equation 1 and the chain rule, one can easily derive the gauge transformation of the inverse speed of light. For a different time coordiante τ ⁣(t,x)\fc\tau{t,x} that is differentiable, the new inverse speed of light c~−1 ⁣(τ,x,u)\fc{\tilde c^{-1}}{\tau,x,u} relates to c−1 ⁣(t,x,u)\fc{c^{-1}}{t,x,u} by c~−1 ⁣(τ ⁣(t,x),x,u)=c−1 ⁣(t,x,u)∂tτ ⁣(t,x)+u∇xτ ⁣(t,x).\fc{\tilde c^{-1}}{\fc\tau{t,x},x,u}=\fc{c^{-1}}{t,x,u}\fc{\partial_t\tau}{t,x}+u\fc{\nabla_x\tau}{t,x}.

Derivation

Along the worldline, we have dtds=c−1 ⁣(t,x,u),dxds=u.\fr{\d t}{\d s}=\fc{c^{-1}}{t,x,u},\quad\fr{\d x}{\d s}=u. In transformed coordinates (τ,x)\p{\tau,x}, Equation 1 reads c~−1 ⁣(τ,x,u)=dτds=dtds ∂tτ ⁣(t,x)+dxds ∇xτ ⁣(t,x).\fc{\tilde c^{-1}}{\tau,x,u}=\fr{\d\tau}{\d s} =\fr{\d t}{\d s}\,\fc{\partial_t\tau}{t,x}+\fr{\d x}{\d s}\,\fc{\nabla_x\tau}{t,x}. This recovers Equation ¿eq:transform?. Because γ\gma is arbitrary, it is true in general.

If the inverse gauge transformation t ⁣(τ,x)\fc t{\tau,x} is differentiable, we can also invert this relation: c−1 ⁣(t ⁣(τ,x),x,u)=c~−1 ⁣(τ,x,u)∂τt ⁣(τ,x)+u∇xt ⁣(τ,x).\fc{c^{-1}}{\fc t{\tau,x},x,u}=\fc{\tilde c^{-1}}{\tau,x,u}\fc{\partial_\tau t}{\tau,x}+u\fc{\nabla_xt}{\tau,x}. By this equation, if a gauge transformation makes the new speed of light be constant 11, then its inverse gauge transformation satisfies c−1 ⁣(t ⁣(τ,x),x,u)=∂τt ⁣(τ,x)+u∇xt ⁣(τ,x).\fc{c^{-1}}{\fc t{\tau,x},x,u}=\fc{\partial_\tau t}{\tau,x}+u\fc{\nabla_xt}{\tau,x}. (2)(2) As we will see, the inverse form is more useful because we will encounter a gauge transformation that is not differentiable in general but has differentiable inverse.

Main claim

I will now prove the following claim. There exists a gauge transformation τ ⁣(t,x)\fc\tau{t,x} such that its inverse t ⁣(τ,x)\fc t{\tau,x} is differentiable and satisfies Equation 2, given the following conditions:

  • c−1 ⁣(t,x,u)\fc{c^{-1}}{t,x,u} is continuous.
  • Unique propogation: The solution to Equation 1 uniquely exists for any length-parametrized piecewise differentiable curve γ\gma and any initial condition of the form t ⁣(s0)=t0\fc t{s_0}=t_0.
  • Constant roundtrip average speed: For any length-parametrized piecewise differentiable curve γ\gma such that γ ⁣(0)=γ ⁣(l)=o\fc\gma0=\fc\gma l=o, any solution to Equation 1 satisfies t ⁣(l)−t ⁣(0)=l\fc tl-\fc t0=l.

The new time coordinate τ ⁣(t,x)\fc\tau{t,x} is defined as follows. For any x∈Mx\in M, pick any length-parametrized curve γ\gma such that γ ⁣(0)=o\fc\gma0=o and γ ⁣(l)=x\fc\gma l=x. For any t∈Rt\in\bR, let t∗t^* be the solution to Equation 1 for γ\gma with the initial condition t∗ ⁣(l)=t\fc{t^*}l=t. Then, define τ ⁣(t,x)≔t∗ ⁣(0)+l\fc\tau{t,x}\ceq\fc{t^*}0+l. I will now show the following claims:

  • τ\tau is well defined: τ ⁣(t,x)\fc\tau{t,x} does not depend on the choice of γ\gma.
  • τ ⁣(⋅,x)\fc\tau{\cdot,x} is continuous and bijective (so the inverse gauge transformation exists and is continuous).
  • t ⁣(τ,x)\fc t{\tau,x} is continuously differentiable and satisfies Equation 2.
τ\tau is well defined

Consider two paths γ1,γ2\gma_1,\gma_2 with lengths l1,l2l_1,l_2 arriving at the same spacetime point (t,x)\p{t,x} with departure times t1,t2t_1,t_2. Append them with the same return path γ′\gma' with length l′l' from (t,x)\p{t,x} to (t′,o)\p{t',o}. Both loops end at t′t', so by the constant roundtrip average speed, we have t′=t1+l1+l′=t2+l2+l′.t'=t_1+l_1+l'=t_2+l_2+l'. We then have τ ⁣(t,x)=t1+l1=t2+l2\fc\tau{t,x}=t_1+l_1=t_2+l_2, so it is well-defined.

τ ⁣(⋅,x)\fc\tau{\cdot,x} is bijective

For any path γ\gma with finite length ll (parameter runs over [0,l]\b{0,l}), denote Tγ ⁣(t0)\fc{T_\gma}{t_0} to be t ⁣(l)\fc tl, where tt is the solution to Equation 1 with initial condition t ⁣(0)=t0\fc t0=t_0.

Consider a path γ\gma with length ll. Suppose that there exists t1<t2t_1<t_2 such that Tγ ⁣(t1)≥Tγ ⁣(t2)\fc{T_\gma}{t_1}\ge\fc{T_\gma}{t_2}. This means that there exists two solutions t1∗t_1^* and t2∗t_2^* to Equation 1 for γ\gma such that t1∗ ⁣(0)<t2∗ ⁣(0)\fc{t_1^*}0<\fc{t_2^*}0 and t1∗ ⁣(l)≥t2∗ ⁣(l)\fc{t_1^*}l\ge\fc{t_2^*}l. Because t1∗t_1^* and t2∗t_2^* must be continuous functions, there exists s0∈(0,l]s_0\in\left(0,l\right] such that t1∗ ⁣(s0)=t2∗ ⁣(s0)\fc{t_1^*}{s_0}=\fc{t_2^*}{s_0}. By the unique propogation, we must have t1∗=t2∗t_1^*=t_2^*, contradicting with t1∗ ⁣(0)<t2∗ ⁣(0)\fc{t_1^*}0<\fc{t_2^*}0. Therefore, TγT_\gma must be strictly monotonically increasing.

Consider a path γ\gma with length ll from oo to xx and a path γ′\gma' with length l′l' from xx to oo so that γ∪γ′\gma\cup\gma' forms a closed path. Therefore, Tγ′ ⁣(Tγ ⁣(t))=t+l+l′\fc{T_{\gma'}}{\fc{T_\gma}t}=t+l+l', so Tγ′∘TγT_{\gma'}\circ T_\gma is a surjection onto R\bR. Because both TγT_\gma and Tγ′T_{\gma'} are injective by monotinicity, they must both be surjective. Therefore, they are both bijective. Because they are monotonic, they are also continuous.

Now by definition we have τ ⁣(t,x)≔Tγ−1 ⁣(t)+l\fc\tau{t,x}\ceq\fc{T_\gma^{-1}}t+l, where Tγ−1T_\gma^{-1} is the inverse function of TγT_\gma, so τ ⁣(⋅,x)\fc\tau{\cdot,x} is continuous and bijective.

t ⁣(τ,x)\fc t{\tau,x} satisfies Equation 2

By construction, if light travels along a path of length ll from xx to yy, departing at t ⁣(τ,x)\fc t{\tau,x}, then it arrives at t ⁣(τ+l,y)\fc t{\tau+l,y}.

Let u∈UTxMu\in\mrm{UT}_xM and ε>0\veps>0. Define two paths γx,u,ε±\gma_{x,u,\veps}^\pm as γx,u,ε+ ⁣(s)≔exp⁡x ⁣(su),γx,u,ε− ⁣(s)≔exp⁡s ⁣((ε−s)u),s∈[0,ε].\fc{\gma_{x,u,\veps}^+}s\ceq\fc{\exp_x}{su},\quad \fc{\gma_{x,u,\veps}^-}s\ceq\fc{\exp_s}{\p{\veps-s}u},\quad s\in\b{0,\veps}. Then, for small ε\veps, by Equation 1 and the continuity of c−1c^{-1}, the time it takes to travel along γx,u,ε±\gma_{x,u,\veps}^\pm is εc−1 ⁣(t,x,±u)+o ⁣(ε)\veps\fc{c^{-1}}{t,x,\pm u}+\fc{\mrm o}\veps, where tt is the departure time.

Denote γx,u,ε\gma_{x,u,\veps} as the concatenation γx,u,ε+∪γx,u,ε−\gma_{x,u,\veps}^+\cup\gma_{x,u,\veps}^-, having length 2ε2\veps. The time it takes to travel along γx,u,ε\gma_{x,u,\veps}, with departure time t ⁣(τ,x)\fc t{\tau,x}, is then t ⁣(τ+2ε,x)−t ⁣(τ,x)=ε(c−1 ⁣(t ⁣(τ,x),x,u)+c−1 ⁣(t ⁣(τ+ε,x),x,−u))+o ⁣(ε).\fc t{\tau+2\veps,x}-\fc t{\tau,x} =\veps\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}+\fc{c^{-1}}{\fc t{\tau+\veps,x},x,-u}}+\fc{\mrm o}\veps. Divide both sides by 2ε2\veps and take limit at ε→0+\veps\to0^+, and we have (by the continuity of t ⁣(⋅,x)\fc t{\cdot,x}) ∂τ+t ⁣(τ,x)=12(c−1 ⁣(t ⁣(τ,x),x,u)+c−1 ⁣(t ⁣(τ,x),x,−u)).\partial_\tau^+\fc t{\tau,x}=\fr12\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}+\fc{c^{-1}}{\fc t{\tau,x},x,-u}}. Similarly, by considering the time it takes to travel along γexp⁡x ⁣(−εu),u,ε\gma_{\fc{\exp_x}{-\veps u},u,\veps} (where uu is understood as the parallel transport of uu from xx to exp⁡x ⁣(−εu)\fc{\exp_x}{-\veps u} along γx,−u,ε+\gma_{x,-u,\veps}^+), we get the same expression for the left derivative. Therefore, ∂τt ⁣(τ,x)=12(c−1 ⁣(t ⁣(τ,x),x,u)+c−1 ⁣(t ⁣(τ,x),x,−u)).\partial_\tau\fc t{\tau,x}=\fr12\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}+\fc{c^{-1}}{\fc t{\tau,x},x,-u}}. (3)(3) It is continuous.

Consider the time it takes to travel along γx,u,ε+\gma_{x,u,\veps}^+ to get t ⁣(τ+ε,exp⁡x ⁣(εu))−t ⁣(τ,x)=εc−1 ⁣(t ⁣(τ,x),x,u)+o ⁣(ε).\fc t{\tau+\veps,\fc{\exp_x}{\veps u}}-\fc t{\tau,x}=\veps\fc{c^{-1}}{\fc t{\tau,x},x,u}+\fc{\mrm o}\veps. Using the continuity of ∂τt ⁣(τ,x)\partial_\tau\fc t{\tau,x} to get t ⁣(τ+ε,exp⁡x ⁣(εu))−t ⁣(τ,exp⁡x ⁣(εu))=ε∂tt ⁣(τ,x)+o ⁣(ε).\fc t{\tau+\veps,\fc{\exp_x}{\veps u}}-\fc t{\tau,\fc{\exp_x}{\veps u}}=\veps\partial_t\fc t{\tau,x}+\fc{\mrm o}\veps. Subtract the two equations to get t ⁣(τ,exp⁡x ⁣(εu))−t ⁣(τ,x)=ε(c−1 ⁣(t ⁣(τ,x),x,u)−∂tt ⁣(τ,x))+o ⁣(ε).\fc t{\tau,\fc{\exp_x}{\veps u}}-\fc t{\tau,x} =\veps\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}-\partial_t\fc t{\tau,x}}+\fc{\mrm o}\veps. Divide by ε\veps and take the limit ε→0+\veps\to0^+ to get directional derivative of t ⁣(τ,x)\fc t{\tau,x} w.r.t. xx along uu to be c−1 ⁣(t ⁣(τ,x),x,u)−∂tt ⁣(τ,x)=12(c−1 ⁣(t ⁣(τ,x),x,u)−c−1 ⁣(t ⁣(τ,x),x,−u)).\fc{c^{-1}}{\fc t{\tau,x},x,u}-\partial_t\fc t{\tau,x} =\fr12\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}-\fc{c^{-1}}{\fc t{\tau,x},x,-u}}. Applying the argument to all u∈UTxMu\in\mrm{UT}_xM to establish that the coordinate partial derivatives exist for all coordinates. They are continuous because c−1c^{-1}, t ⁣(τ,x)\fc t{\tau,x}, and the metric are continuous. We then have the existence of the covariant derivative ∇xt ⁣(τ,x)\nabla_x\fc t{\tau,x} so that the directional derivatives are u∇xt ⁣(τ,x)=12(c−1 ⁣(t ⁣(τ,x),x,u)−c−1 ⁣(t ⁣(τ,x),x,−u)).u\nabla_x\fc t{\tau,x}=\fr12\p{\fc{c^{-1}}{\fc t{\tau,x},x,u}-\fc{c^{-1}}{\fc t{\tau,x},x,-u}}. (4)(4)

Add together Equation 3 and 4, and we recover Equation 2.

Reflections

Although t ⁣(τ,x)\fc t{\tau,x} is continuously differentiable, τ ⁣(t,x)\fc\tau{t,x} is not necessarily so because it is possible to have ∂τt ⁣(τ,x)=0\partial_\tau\fc t{\tau,x}=0 at some points. This suggests that the inverse gauge transformation (τ,x)↦(t,x)\p{\tau,x}\mapsto\p{t,x} is in fact a more natural object to work with instead of the gauge transformation (t,x)↦(τ,x)\p{t,x}\mapsto\p{\tau,x}. This suggests that, if we have constant roundtrip average speed of light, then it is natural to think of the ground truth of the universe is that the speed of light is actually constant, and an assumption of varying speed of light is an artifact of the gauge transformation t ⁣(τ,x)\fc t{\tau,x}, instead of the other way around (that the constant speed of light is an artifact of the gauge transformation τ ⁣(t,x)\fc\tau{t,x} that we constructed for convenience).

One may notice that the definition of τ\tau to get constant speed of light gives exactly the Einstein synchronization: if we place an observer at xx in MM and let his clock synchronize to the observer at oo using the Einstein synchronization, then the time on his clock will be τ ⁣(t,x)\fc\tau{t,x}.