This is one of the foundational derivations in relativistic quantum field theory:

showing that the Klein–Gordon scalar field transforms consistently under Lorentz transformations and that the theory is Lorentz invariant.

The key idea is:Physics must look identical in all inertial frames.\boxed{ \text{Physics must look identical in all inertial frames.} }Physics must look identical in all inertial frames.​

For scalar fields, this turns out to be beautifully simple.


1. Start with the Klein–Gordon Equation

The scalar field satisfies:(μμ+m2)ϕ(x)=0(\partial_\mu\partial^\mu + m^2)\phi(x)=0(∂μ​∂μ+m2)ϕ(x)=0

or equivalently(+m2)ϕ(x)=0(\Box + m^2)\phi(x)=0(□+m2)ϕ(x)=0

whereμμ\Box \equiv \partial_\mu\partial^\mu□≡∂μ​∂μ

is the d’Alembertian operator.

Using metric signature (+,,,)(+,-,-,-)(+,−,−,−),=2t22\Box = \frac{\partial^2}{\partial t^2} – \nabla^2□=∂t2∂2​−∇2


2. Lorentz Transformations

A Lorentz transformation changes coordinates:xμxμx^\mu \rightarrow x’^\muxμ→x′μ

withxμ=Λ νμxνx’^\mu = \Lambda^\mu_{\ \nu}x^\nux′μ=Λ νμ​xν

The matrix Λ\LambdaΛ satisfiesΛTηΛ=η\Lambda^T \eta \Lambda = \etaΛTηΛ=η

which preserves the spacetime interval:xμxμ=xμxμx_\mu x^\mu = x’_\mu x’^\muxμ​xμ=xμ′​x′μ


3. What Is a Scalar Field?

A scalar field is defined by:ϕ(x)=ϕ(x)\boxed{ \phi'(x’)=\phi(x) }ϕ′(x′)=ϕ(x)​

This means:

  • the numerical value of the field is unchanged
  • only the coordinates labeling spacetime points change

This is the defining property of a Lorentz scalar.


4. Transforming Derivatives

Now derive how derivatives transform.

Using the chain rule:xμ=xνxμxν\frac{\partial}{\partial x’^\mu} = \frac{\partial x^\nu}{\partial x’^\mu} \frac{\partial}{\partial x^\nu}∂x′μ∂​=∂x′μ∂xν​∂xν∂​

Sincexμ=Λ νμxνx’^\mu = \Lambda^\mu_{\ \nu}x^\nux′μ=Λ νμ​xν

the inverse transformation isxν=(Λ1) μνxμx^\nu = (\Lambda^{-1})^\nu_{\ \mu}x’^\muxν=(Λ−1) μν​x′μ

Therefore:μ=(Λ1) μνν\partial’_\mu = (\Lambda^{-1})^\nu_{\ \mu}\partial_\nu∂μ′​=(Λ−1) μν​∂ν​

or equivalentlyμ=Λ νμν\partial’^\mu = \Lambda^\mu_{\ \nu}\partial^\nu∂′μ=Λ νμ​∂ν

So derivatives transform like four-vectors.


5. Transforming the d’Alembertian

Now examine=μμ\Box’ = \partial’_\mu\partial’^\mu□′=∂μ′​∂′μ

Substitute the transformed derivatives:=(Λ1) μννΛ ρμρ\Box’ = (\Lambda^{-1})^\nu_{\ \mu}\partial_\nu \Lambda^\mu_{\ \rho}\partial^\rho□′=(Λ−1) μν​∂ν​Λ ρμ​∂ρ

Using(Λ1) μνΛ ρμ=δρν(\Lambda^{-1})^\nu_{\ \mu}\Lambda^\mu_{\ \rho} = \delta^\nu_{\rho}(Λ−1) μν​Λ ρμ​=δρν​

we get=νν=\Box’ = \partial_\nu\partial^\nu = \Box□′=∂ν​∂ν=□

Thus: is Lorentz invariant\boxed{ \Box \text{ is Lorentz invariant} }□ is Lorentz invariant​

This is the central result.


6. Lorentz Invariance of the KG Equation

Now apply this to the field equation:(+m2)ϕ(x)=0(\Box + m^2)\phi(x)=0(□+m2)ϕ(x)=0

Under Lorentz transformation:(+m2)ϕ(x)=(+m2)ϕ(x)(\Box’ + m^2)\phi'(x’) = (\Box + m^2)\phi(x)(□′+m2)ϕ′(x′)=(□+m2)ϕ(x)

Since the RHS is zero,(+m2)ϕ(x)=0(\Box’ + m^2)\phi'(x’)=0(□′+m2)ϕ′(x′)=0

Therefore the Klein–Gordon equation has exactly the same form in every inertial frame.

So:The KG equation is Lorentz invariant\boxed{ \text{The KG equation is Lorentz invariant} }The KG equation is Lorentz invariant​


7. Lorentz Invariance of the Action

The action isS=d4xLS = \int d^4x\, \mathcal LS=∫d4xL

withL=12μϕμϕ12m2ϕ2\mathcal L = \frac12\partial_\mu\phi\partial^\mu\phi – \frac12m^2\phi^2L=21​∂μ​ϕ∂μϕ−21​m2ϕ2

Now check each term.


Kinetic Term

μϕμϕ\partial_\mu\phi\partial^\mu\phi∂μ​ϕ∂μϕ

is a Lorentz scalar because it contracts two four-vectors.

Like:AμAμA_\mu A^\muAμ​Aμ


Mass Term

ϕ2\phi^2ϕ2

is also scalar since ϕ\phiϕ itself is scalar.


Volume Element

Lorentz transformations preserve spacetime volume:d4x=d4xd^4x’ = d^4xd4x′=d4x

for proper Lorentz transformations.

Therefore:S=SS’ = SS′=S

Thus the action is Lorentz invariant.


8. Physical Interpretation

The scalar field has:

  • no direction in spacetime
  • no spin index
  • no vector structure

It behaves like temperature distributed through spacetime.

All observers agree on the field value at the same spacetime event.


9. Contrast with Spinors and Vectors

Scalar:ϕ(x)=ϕ(x)\phi'(x’)=\phi(x)ϕ′(x′)=ϕ(x)

Vector:Aμ(x)=Λ νμAν(x)A’^\mu(x’) = \Lambda^\mu_{\ \nu}A^\nu(x)A′μ(x′)=Λ νμ​Aν(x)

Spinor:ψ(x)=S(Λ)ψ(x)\psi'(x’) = S(\Lambda)\psi(x)ψ′(x′)=S(Λ)ψ(x)

where S(Λ)S(\Lambda)S(Λ) is the spinor representation of the Lorentz group.

Spinors transform much more subtly.


10. The Deep Idea

The entire structure of relativistic QFT comes from demanding:the action be Lorentz invariant\boxed{ \text{the action be Lorentz invariant} }the action be Lorentz invariant​

That requirement strongly constrains:

  • allowed fields
  • allowed interactions
  • allowed dynamics

For the Klein–Gordon field, Lorentz invariance emerges because:μμ\boxed{ \partial_\mu\partial^\mu }∂μ​∂μ​

is a spacetime scalar operator.