Quantum Field Theory Archives - Time Travel, Quantum Entanglement and Quantum Computing https://stationarystates.com/category/quantum-field-theory/ Not only is the Universe stranger than we think, it is stranger than we can think...Hiesenberg Tue, 19 May 2026 17:36:16 +0000 en-US hourly 1 https://wordpress.org/?v=6.9.4 Lorentz Invariance of Scalar Fields https://stationarystates.com/quantum-field-theory/lorentz-invariance-of-scalar-fields/?utm_source=rss&utm_medium=rss&utm_campaign=lorentz-invariance-of-scalar-fields https://stationarystates.com/quantum-field-theory/lorentz-invariance-of-scalar-fields/#respond Tue, 19 May 2026 17:36:14 +0000 https://stationarystates.com/?p=1132 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. […]

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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.

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Treating a bipartite Hamiltonian relativistically https://stationarystates.com/quantum-field-theory/treating-a-bipartite-hamiltonian-relativistically/?utm_source=rss&utm_medium=rss&utm_campaign=treating-a-bipartite-hamiltonian-relativistically https://stationarystates.com/quantum-field-theory/treating-a-bipartite-hamiltonian-relativistically/#respond Tue, 19 May 2026 16:48:25 +0000 https://stationarystates.com/?p=1130 For a relativistic bipartite system, you usually do not start with a simple Hamiltonian likeH=HA⊗IB+IA⊗HB+HintH = H_A \otimes I_B + I_A \otimes H_B + H_{\text{int}}H=HA​⊗IB​+IA​⊗HB​+Hint​ unless you are in a […]

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For a relativistic bipartite system, you usually do not start with a simple Hamiltonian likeH=HAIB+IAHB+HintH = H_A \otimes I_B + I_A \otimes H_B + H_{\text{int}}H=HA​⊗IB​+IA​⊗HB​+Hint​

unless you are in a special approximation. The relativistic treatment changes the framework.

The main issue is this:Relativity treats space and time together, but ordinary Hamiltonians single out time.\boxed{ \text{Relativity treats space and time together, but ordinary Hamiltonians single out time.} }Relativity treats space and time together, but ordinary Hamiltonians single out time.​

So the more natural object is the action or the field theory Lagrangian, not a nonrelativistic two-particle Hamiltonian.

For two relativistic particles/fields, one writes something likeS=d4xLA+d4xLB+d4xLintS = \int d^4x \, \mathcal L_A + \int d^4x \, \mathcal L_B + \int d^4x \, \mathcal L_{\text{int}}S=∫d4xLA​+∫d4xLB​+∫d4xLint​

or, schematically,L=LA+LB+Lint\mathcal L = \mathcal L_A + \mathcal L_B + \mathcal L_{\text{int}}L=LA​+LB​+Lint​

For two scalar fields,LA=12μϕAμϕA12mA2ϕA2\mathcal L_A = \frac12 \partial_\mu \phi_A \partial^\mu \phi_A – \frac12 m_A^2\phi_A^2LA​=21​∂μ​ϕA​∂μϕA​−21​mA2​ϕA2​ LB=12μϕBμϕB12mB2ϕB2\mathcal L_B = \frac12 \partial_\mu \phi_B \partial^\mu \phi_B – \frac12 m_B^2\phi_B^2LB​=21​∂μ​ϕB​∂μϕB​−21​mB2​ϕB2​

and an interaction might beLint=gϕA2ϕB2\mathcal L_{\text{int}} = -g \phi_A^2 \phi_B^2Lint​=−gϕA2​ϕB2​

Then the relativistic dynamics comes fromδS=0\delta S = 0δS=0

rather than from a simple two-body Schrödinger Hamiltonian.

For quantum theory, the state lives in a tensor product of field Hilbert spaces:H=HAHB\mathcal H = \mathcal H_A \otimes \mathcal H_BH=HA​⊗HB​

but the particles are excitations of fields, not little objects with fixed wavefunctions.

A bipartite relativistic state might look likeΨ=p,qC(p,q)aA(p)aB(q)0|\Psi\rangle = \sum_{p,q} C(p,q) \,a_A^\dagger(p) a_B^\dagger(q) |0\rangle∣Ψ⟩=p,q∑​C(p,q)aA†​(p)aB†​(q)∣0⟩

where aA(p)a_A^\dagger(p)aA†​(p) creates particle AAA with four-momentum ppp, and aB(q)a_B^\dagger(q)aB†​(q) creates particle BBB with four-momentum qqq.

The relativistic energy isEp=p2+m2E_{\mathbf p} = \sqrt{\mathbf p^2 + m^2}Ep​=p2+m2​

so the free Hamiltonian is roughlyH0=d3p(2π)3EpapapH_0 = \int \frac{d^3p}{(2\pi)^3} E_{\mathbf p} \,a^\dagger_{\mathbf p}a_{\mathbf p}H0​=∫(2π)3d3p​Ep​ap†​ap​

For two species,H0=d3p(2π)3EpAaA(p)aA(p)+d3q(2π)3EqBaB(q)aB(q)H_0 = \int \frac{d^3p}{(2\pi)^3} E^A_{\mathbf p} a_A^\dagger(\mathbf p)a_A(\mathbf p) + \int \frac{d^3q}{(2\pi)^3} E^B_{\mathbf q} a_B^\dagger(\mathbf q)a_B(\mathbf q)H0​=∫(2π)3d3p​EpA​aA†​(p)aA​(p)+∫(2π)3d3q​EqB​aB†​(q)aB​(q)

Then add an interaction Hamiltonian:H=HA+HB+HintH = H_A + H_B + H_{\text{int}}H=HA​+HB​+Hint​

But now HintH_{\text{int}}Hint​ comes from a Lorentz-invariant field interaction.

So the relativistic version of the bipartite Hamiltonian idea is:HAI+IHB+Hint\boxed{ H_A \otimes I + I \otimes H_B + H_{\text{int}} }HA​⊗I+I⊗HB​+Hint​​

but interpreted in QFT, where HAH_AHA​, HBH_BHB​, and HintH_{\text{int}}Hint​ act on field Fock spaces.

The clean hierarchy is:Nonrelativistic QM: two-particle Hamiltonian\boxed{ \text{Nonrelativistic QM: two-particle Hamiltonian} }Nonrelativistic QM: two-particle Hamiltonian​ Relativistic QM: constrained and delicate\boxed{ \text{Relativistic QM: constrained and delicate} }Relativistic QM: constrained and delicate​ Relativistic QFT: fields, Fock space, Lorentz-invariant action\boxed{ \text{Relativistic QFT: fields, Fock space, Lorentz-invariant action} }Relativistic QFT: fields, Fock space, Lorentz-invariant action​

So the safest answer is:Treat the bipartite system as two interacting quantum fields.\boxed{ \text{Treat the bipartite system as two interacting quantum fields.} }Treat the bipartite system as two interacting quantum fields.​

Not as two particles with an ordinary potential V(xAxB)V(\mathbf x_A-\mathbf x_B)V(xA​−xB​), because instantaneous potentials generally conflict with relativity.

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Why there are no macroscopic Spinor Fields? https://stationarystates.com/quantum-field-theory/why-there-are-no-macroscopic-spinor-fields/?utm_source=rss&utm_medium=rss&utm_campaign=why-there-are-no-macroscopic-spinor-fields https://stationarystates.com/quantum-field-theory/why-there-are-no-macroscopic-spinor-fields/#respond Mon, 18 May 2026 18:35:18 +0000 https://stationarystates.com/?p=1128 1. What Is a Spinor Field? A spinor field is a field describing spin-12\frac1221​ particles: The Dirac field is the standard example:ψ(x)\psi(x)ψ(x) Unlike scalar or vector fields, spinors transform differently […]

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1. What Is a Spinor Field?

A spinor field is a field describing spin-12\frac1221​ particles:

  • electrons
  • quarks
  • neutrinos

The Dirac field is the standard example:ψ(x)\psi(x)ψ(x)

Unlike scalar or vector fields, spinors transform differently under rotations and Lorentz transformations.


2. Classical Macroscopic Fields Exist for Bosons

Examples:

  • electromagnetic field Aμ(x)A_\mu(x)Aμ​(x)
  • classical light waves
  • laser beams
  • superfluids
  • Bose condensates

Why?

Because bosons can pile into the same quantum state.

The occupation number can become enormous:N1N \gg 1N≫1

This allows the quantum field operator to behave approximately like a classical field.

For example:A^μ(x)Aμclassical(x)\hat A_\mu(x) \rightarrow A_\mu^{\text{classical}}(x)A^μ​(x)→Aμclassical​(x)


3. Fermions Cannot Do This

Spinor fields describe fermions.

Fermions obey:Pauli exclusion principle\boxed{ \text{Pauli exclusion principle} }Pauli exclusion principle​

No two identical fermions can occupy the same quantum state.

Mathematically:{ap,aq}=δpq\{a_p,a_q^\dagger\}=\delta_{pq}{ap​,aq†​}=δpq​

instead of bosonic commutators:[ap,aq]=δpq[a_p,a_q^\dagger]=\delta_{pq}[ap​,aq†​]=δpq​

This changes everything.


4. Grassmann Nature of Fermionic Fields

In QFT, fermionic fields are not ordinary numbers.

They are Grassmann-valued:ψ1ψ2=ψ2ψ1\psi_1\psi_2=-\psi_2\psi_1ψ1​ψ2​=−ψ2​ψ1​

In particular:ψ2=0\boxed{ \psi^2=0 }ψ2=0​

This nilpotent property means you cannot build arbitrarily large coherent amplitudes from a fermion field.

That prevents a classical macroscopic field interpretation.


5. Why Electromagnetic Waves Exist but Electron Waves Do Not

For photons:

many photons can occupy one mode:N|N\rangle∣N⟩

with arbitrarily large NNN.

This produces classical EM waves.

But for electrons:

occupation is only:0 or 10 \text{ or } 10 or 1

per quantum state.

So there is no analog of a huge coherent classical electron field.


6. Macroscopic Matter Is NOT a Macroscopic Spinor Field

A metal contains enormous numbers of electrons.

But:the electron field itself is still quantum\boxed{ \text{the electron field itself is still quantum} }the electron field itself is still quantum​

The matter behaves macroscopically because:

  • enormous statistical averages emerge
  • collective variables become classical
  • densities and currents become classical observables

NOT because the spinor field becomes classical.


7. Contrast with Bose–Einstein Condensates

Bosonic field:ϕ(x)\phi(x)ϕ(x)

can acquire a macroscopic expectation value:ϕ(x)0\langle \phi(x)\rangle \neq 0⟨ϕ(x)⟩=0

This is a true classical order parameter.

For fermions:ψ(x)=0\langle \psi(x)\rangle =0⟨ψ(x)⟩=0

in ordinary macroscopic systems.

Instead, fermions form composite bosons:

Examples:

  • Cooper pairs
  • helium-4 atoms
  • mesons

Then THOSE bosonic composites can condense macroscopically.


8. Superconductivity Is the Key Example

Electrons themselves cannot form a classical spinor field.

But paired electrons:(ee)(e^- e^-)(e−e−)

form Cooper pairs with integer spin.

Those pairs behave bosonically.

Then you get a macroscopic condensate:ΨCooper pair0\langle \Psi_{\text{Cooper pair}}\rangle \neq 0⟨ΨCooper pair​⟩=0

leading to superconductivity.


9. Deep Geometric View

Bosonic classical fields correspond to smooth amplitudes over spacetime:ϕ(x)R or C\phi(x)\in \mathbb R \text{ or } \mathbb Cϕ(x)∈R or C

Fermionic fields instead live in Grassmann algebra.

Grassmann quantities do not have ordinary macroscopic classical limits.

So:fermionic fields are fundamentally quantum objects\boxed{ \text{fermionic fields are fundamentally quantum objects} }fermionic fields are fundamentally quantum objects​

while bosonic fields can emerge into classicality.


10. Important Caveat

People sometimes write “classical Dirac fields.”

This means:

  • using the Dirac equation classically
  • before quantization

But these are mathematical tools.

Physical macroscopic spinor fields are not observed in nature the way classical EM fields are.


The short version:Bosons stack. Fermions exclude.\boxed{ \text{Bosons stack. Fermions exclude.} }Bosons stack. Fermions exclude.​

and therefore:bosonic fields can become classical macroscopic fields,\boxed{ \text{bosonic fields can become classical macroscopic fields,} }bosonic fields can become classical macroscopic fields,​

whilefermionic spinor fields cannot.\boxed{ \text{fermionic spinor fields cannot.} }fermionic spinor fields cannot.​

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What is the difference between δ and ∂ in this derivation https://stationarystates.com/quantum-field-theory/what-is-the-difference-between-%ce%b4-and-%e2%88%82-in-this-derivation/?utm_source=rss&utm_medium=rss&utm_campaign=what-is-the-difference-between-%25ce%25b4-and-%25e2%2588%2582-in-this-derivation https://stationarystates.com/quantum-field-theory/what-is-the-difference-between-%ce%b4-and-%e2%88%82-in-this-derivation/#respond Mon, 18 May 2026 12:16:56 +0000 https://stationarystates.com/?p=1126 For the derivation of the Least Action Principle in classical field theory , what is the difference between δ and ∂? This is one of the most important conceptual distinctions […]

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For the derivation of the Least Action Principle in classical field theory , what is the difference between δ and ∂?

This is one of the most important conceptual distinctions in field theory.

The symbols \partial∂ and δ\deltaδ represent completely different operations.


1. The Partial Derivative \partial

\partial∂ means:

“How does a function change as spacetime coordinates change?”

For a fieldϕ(x)=ϕ(t,x)\phi(x) = \phi(t,\mathbf x)ϕ(x)=ϕ(t,x)

the derivativeμϕ\partial_\mu \phi∂μ​ϕ

describes how the field changes from point to point in spacetime.

Examples:0ϕ=ϕt\partial_0 \phi = \frac{\partial \phi}{\partial t}∂0​ϕ=∂t∂ϕ​

(time variation)

andiϕ=ϕxi\partial_i \phi = \frac{\partial \phi}{\partial x^i}∂i​ϕ=∂xi∂ϕ​

(spatial variation)

So:=ordinary spacetime derivative\boxed{ \partial = \text{ordinary spacetime derivative} }∂=ordinary spacetime derivative​

It acts inside spacetime.


2. The Variation δ\deltaδ

δ\deltaδ means:

“Suppose I slightly deform the entire field configuration.”

This is not motion through spacetime.

Instead:ϕ(x)ϕ(x)+δϕ(x)\phi(x) \rightarrow \phi(x)+\delta\phi(x)ϕ(x)→ϕ(x)+δϕ(x)

means:

  • keep spacetime point xxx fixed
  • slightly change the value of the field there

So δϕ\delta\phiδϕ is an infinitesimal “test deformation” of the whole function.


Visual Intuition

Think of the field as a rubber sheet over spacetime.

  • ϕ\partial\phi∂ϕ:
    measures the slope of the sheet from point to point
  • δϕ\delta\phiδϕ:
    slightly lifts or perturbs the sheet itself

Why Both Appear Together

The Lagrangian depends on:L(ϕ,μϕ)\mathcal L(\phi,\partial_\mu\phi)L(ϕ,∂μ​ϕ)

meaning:

  • the field value
  • and its spacetime gradients

When varying the action:δS=δd4xL\delta S = \delta \int d^4x\,\mathcal LδS=δ∫d4xL

you must vary BOTH:δϕ\delta\phiδϕ

andδ(μϕ)\delta(\partial_\mu\phi)δ(∂μ​ϕ)

Since differentiation and variation commute:δ(μϕ)=μ(δϕ)\boxed{ \delta(\partial_\mu\phi) = \partial_\mu(\delta\phi) }δ(∂μ​ϕ)=∂μ​(δϕ)​

This relation is central to the derivation.


Deep Geometric Interpretation

\partial∂ lives within spacetime.

δ\deltaδ lives in the infinite-dimensional space of all possible field configurations.

So:

SymbolMeaningActs On
μ\partial_\mu∂μ​spacetime derivativecoordinates
δ\deltaδvariation between nearby field configurationsfunction space

Analogy with Classical Mechanics

For a particle trajectory:x(t)x(t)x(t)

we distinguish:

Velocity:dxdt\frac{dx}{dt}dtdx​

vs variation of the path:x(t)x(t)+δx(t)x(t)\rightarrow x(t)+\delta x(t)x(t)→x(t)+δx(t)

The first measures motion along the path.

The second compares neighboring possible paths.

Field theory is exactly the same idea, but with fields instead of trajectories.


The Key Philosophical Idea

The action principle says:

Nature compares all nearby possible field configurations and selects the one whereδS=0\boxed{ \delta S=0 }δS=0​

That does NOT mean the action is zero.

It means:first-order change in action vanishes\text{first-order change in action vanishes}first-order change in action vanishes

which is analogous to:dfdx=0\frac{df}{dx}=0dxdf​=0

for extrema in ordinary calculus.


The field equation emerges because the true field configuration is a stationary point in the space of all possible field configurations.

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The principle of stationary action derivation https://stationarystates.com/quantum-field-theory/the-principle-of-stationary-action-derivation/?utm_source=rss&utm_medium=rss&utm_campaign=the-principle-of-stationary-action-derivation https://stationarystates.com/quantum-field-theory/the-principle-of-stationary-action-derivation/#respond Mon, 18 May 2026 12:13:59 +0000 https://stationarystates.com/?p=1124 Start with the actionS[ϕ]=∫d4x L(ϕ,∂μϕ)S[\phi]=\int d^4x \, \mathcal{L}(\phi,\partial_\mu \phi)S[ϕ]=∫d4xL(ϕ,∂μ​ϕ) The physical field configuration is the one for which a small variation of the field,ϕ(x)→ϕ(x)+δϕ(x)\phi(x)\rightarrow \phi(x)+\delta\phi(x)ϕ(x)→ϕ(x)+δϕ(x) does not change the action to […]

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Start with the actionS[ϕ]=d4xL(ϕ,μϕ)S[\phi]=\int d^4x \, \mathcal{L}(\phi,\partial_\mu \phi)S[ϕ]=∫d4xL(ϕ,∂μ​ϕ)

The physical field configuration is the one for which a small variation of the field,ϕ(x)ϕ(x)+δϕ(x)\phi(x)\rightarrow \phi(x)+\delta\phi(x)ϕ(x)→ϕ(x)+δϕ(x)

does not change the action to first order:δS=0\delta S=0δS=0

Now vary the action:δS=d4x[Lϕδϕ+L(μϕ)δ(μϕ)]\delta S = \int d^4x \left[ \frac{\partial \mathcal{L}}{\partial \phi}\delta\phi + \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \delta(\partial_\mu\phi) \right]δS=∫d4x[∂ϕ∂L​δϕ+∂(∂μ​ϕ)∂L​δ(∂μ​ϕ)]

Since variation and differentiation commute,δ(μϕ)=μ(δϕ)\delta(\partial_\mu\phi) = \partial_\mu(\delta\phi)δ(∂μ​ϕ)=∂μ​(δϕ)

soδS=d4x[Lϕδϕ+L(μϕ)μ(δϕ)]\delta S = \int d^4x \left[ \frac{\partial \mathcal{L}}{\partial \phi}\delta\phi + \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \partial_\mu(\delta\phi) \right]δS=∫d4x[∂ϕ∂L​δϕ+∂(∂μ​ϕ)∂L​∂μ​(δϕ)]

Now integrate the second term by parts:d4xL(μϕ)μ(δϕ)=d4xμ[L(μϕ)]δϕ\int d^4x\, \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \partial_\mu(\delta\phi) = – \int d^4x\, \partial_\mu \left[ \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \right] \delta\phi∫d4x∂(∂μ​ϕ)∂L​∂μ​(δϕ)=−∫d4x∂μ​[∂(∂μ​ϕ)∂L​]δϕ

The boundary term vanishes because we assumeδϕ=0\delta\phi=0δϕ=0

on the boundary of spacetime.

Therefore,δS=d4x[Lϕμ(L(μϕ))]δϕ\delta S = \int d^4x \left[ \frac{\partial \mathcal{L}}{\partial \phi} – \partial_\mu \left( \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \right) \right]\delta\phiδS=∫d4x[∂ϕ∂L​−∂μ​(∂(∂μ​ϕ)∂L​)]δϕ

For the action to be stationary for arbitrary δϕ\delta\phiδϕ, the bracket must vanish:Lϕμ(L(μϕ))=0\boxed{ \frac{\partial \mathcal{L}}{\partial \phi} – \partial_\mu \left( \frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} \right) =0 }∂ϕ∂L​−∂μ​(∂(∂μ​ϕ)∂L​)=0​

This is the Euler–Lagrange equation for a field.

For the scalar field,L=12μϕμϕ12m2ϕ2\mathcal{L} = \frac{1}{2}\partial_\mu\phi\,\partial^\mu\phi – \frac{1}{2}m^2\phi^2L=21​∂μ​ϕ∂μϕ−21​m2ϕ2

we getLϕ=m2ϕ\frac{\partial \mathcal{L}}{\partial \phi} = -m^2\phi∂ϕ∂L​=−m2ϕ

andL(μϕ)=μϕ\frac{\partial \mathcal{L}}{\partial(\partial_\mu\phi)} = \partial^\mu\phi∂(∂μ​ϕ)∂L​=∂μϕ

So the Euler–Lagrange equation becomesm2ϕμμϕ=0-m^2\phi-\partial_\mu\partial^\mu\phi=0−m2ϕ−∂μ​∂μϕ=0

or(μμ+m2)ϕ=0\boxed{ (\partial_\mu\partial^\mu+m^2)\phi=0 }(∂μ​∂μ+m2)ϕ=0​

That is the Klein–Gordon equation.

In plain English:δS=0field chooses stationary actionEuler–Lagrange equationKlein–Gordon equation\boxed{ \delta S=0 \quad\Rightarrow\quad \text{field chooses stationary action} \quad\Rightarrow\quad \text{Euler–Lagrange equation} \quad\Rightarrow\quad \text{Klein–Gordon equation} }δS=0⇒field chooses stationary action⇒Euler–Lagrange equation⇒Klein–Gordon equation

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Slow Moving vs Fast Moving Electrons – Photon Interaction https://stationarystates.com/basic-quantum-theory/slow-moving-vs-fast-moving-electrons-photon-interaction/?utm_source=rss&utm_medium=rss&utm_campaign=slow-moving-vs-fast-moving-electrons-photon-interaction Fri, 10 Oct 2025 20:26:28 +0000 https://stationarystates.com/?p=1032 Electron–Photon Interaction: Slow vs Fast Electrons Is There a Difference Between a Slow-Moving and a Fast-Moving Electron Interacting with a Photon? Yes — the interaction depends strongly on the electron’s […]

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Electron–Photon Interaction: Slow vs Fast Electrons



Is There a Difference Between a Slow-Moving and a Fast-Moving Electron Interacting with a Photon?

Yes — the interaction depends strongly on the electron’s speed (equivalently its kinetic energy and Lorentz factor). Below is a structured comparison.

1. Energy and Momentum Transfer

Slow (Nonrelativistic) Electron

  • Kinetic energy is small compared to typical photon energies in many scenarios.
  • Thomson scattering applies (elastic; negligible photon frequency change).

    \[       \frac{d\sigma}{d\Omega} \;=\; \frac{r_e^2}{2}\,\big(1+\cos^2\theta\big),     \]

where r_e is the classical electron radius.

Fast (Relativistic) Electron

  • Significant Doppler shifts and energy exchange with photons.
  • Compton scattering with electron recoil; frequency can change substantially.
  • In electron’s rest frame, incident photons are blue-shifted; after scattering, lab-frame photons can be strongly boosted (inverse Compton).

2. Reference Frame Effects

  • Slow electron: Electron frame \approx lab frame; photon field nearly unchanged under transformation.
  • Fast electron: Incident radiation is Lorentz-transformed; photons are aberrated into a forward cone and blue-shifted.

3. Cross-Section Regimes

Thomson (low energy/slow electron): total cross section approximately constant \sigma_T for \hbar\omega \ll m_e c^2.

Klein–Nishina (relativistic/high energy): energy-dependent, decreases as photon energy rises:

    \[       \frac{d\sigma}{d\Omega}       \;=\;       \frac{r_e^2}{2}       \left(\frac{\omega'}{\omega}\right)^{\!2}       \left(         \frac{\omega'}{\omega}         + \frac{\omega}{\omega'}         - \sin^2\theta       \right),     \]

with \omega and \omega' the incident and scattered photon angular frequencies (in the same frame).

4. Physical Outcomes

  • Slow electron + photon: Elastic scattering; photon energy nearly unchanged; angular pattern \propto 1+\cos^2\theta.
  • Fast electron + photon: Large frequency shifts (Compton redshift or inverse-Compton blueshift); forward-peaked scattering; potential production of high-energy photons.

5. Examples

  • Photoelectric/low-energy scattering in solids: Conduction electrons interacting with visible light \rightarrow Thomson limit for scattering.
  • Astrophysics: Relativistic electrons in jets upscatter CMB/starlight to X-rays or \gamma-rays (inverse Compton); synchrotron plus IC spectra.
  • Laboratory: High-energy electron beams colliding with lasers produce energetic backscattered photons due to strong Doppler boosting.

Summary Table

Feature Slow Electron Fast Electron (Relativistic)
Regime Thomson (classical) Compton / Klein–Nishina (relativistic)
Energy exchange Negligible (elastic) Significant (inelastic with recoil)
Photon frequency shift Minimal Doppler shift + recoil (large)
Angular distribution 1+\cos^2\theta Forward-peaked
Cross section \approx \sigma_T (constant for \hbar\omega \ll m_e c^2) Energy-dependent; decreases at high energies
Dominant processes Thomson scattering; (in media) photoelectric absorption Compton / inverse Compton; synchrotron + IC in astrophysics

Key takeaway:
For slow electrons, scattering is essentially elastic and classical (Thomson). For fast, relativistic electrons, kinematics and cross sections are altered by Lorentz effects and recoil, leading to substantial frequency shifts and high-energy radiation.


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Historical Context of the Coupling Constant https://stationarystates.com/quantum-field-theory/historical-context-of-the-coupling-constant/?utm_source=rss&utm_medium=rss&utm_campaign=historical-context-of-the-coupling-constant Mon, 29 Sep 2025 18:17:42 +0000 https://stationarystates.com/?p=984 Origin of the QED Coupling Constant The Coupling Constant in QED The QED coupling constant is one of the most famous “mystery numbers” in physics, better known as the fine-structure […]

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Origin of the QED Coupling Constant

The Coupling Constant in QED

The QED coupling constant is one of the most famous “mystery numbers” in physics, better known as the
fine-structure constant, usually denoted:

    \[\alpha = \frac{e^2}{4 \pi \epsilon_0 \hbar c} \approx \frac{1}{137.035999...}.\]

1. What is the coupling constant in QED?

  • In quantum electrodynamics (QED), the coupling constant is the strength with which charged particles
    (like electrons) interact with the electromagnetic field (photons).
  • Mathematically, the electron charge e enters the QED Lagrangian as the coefficient in the interaction term:

        \[\mathcal{L}_{\text{int}} = -e \, \bar{\psi}\gamma^\mu A_\mu \psi,\]

    where \psi is the electron field and A_\mu is the photon field.

  • In natural units (\hbar = c = 1), the dimensionless form of the coupling is exactly
    \alpha = \frac{e^2}{4\pi}.

So, the origin of the QED coupling constant is: it’s the coefficient that sets the interaction strength
between the fundamental electron field and the photon field in the theory.

2. Why is it ~1/137?

This is the deeper mystery:

  • Experimental input: QED does not predict the value of \alpha. Instead, it must be measured in experiments (atomic spectroscopy, electron g-2, quantum Hall effect).
  • Running with energy: \alpha is not really constant. It “runs” with energy scale due to vacuum polarization. At low energies, \alpha \approx 1/137. At the Z boson scale (\sim 90 \,\text{GeV}), it increases to about 1/128.
  • Attempts at explanation: Many physicists (Dirac, Eddington) wondered whether 1/137 has a deeper mathematical or cosmological origin. The Standard Model does not explain it; in GUT or string theory, coupling constants may emerge from vacuum expectation values of fields or geometry of extra dimensions.
  • Anthropic speculation: If \alpha were very different, chemistry and stable matter might not exist. Its value could be constrained by conditions necessary for life.

3. Why that number matters

  • \alpha controls atomic structure (fine splitting in hydrogen, hence the name).
  • It governs scattering probabilities in particle physics.
  • Its smallness explains why QED perturbation theory converges so well (each higher order suppressed by ~1/137).

4. Historical Attempts to Explain 1/137

The unusual appearance of the fine-structure constant sparked fascination and speculation among some of the
greatest physicists of the 20th century:

  • Arthur Eddington: Proposed a numerological approach, claiming that \alpha^{-1} was exactly 137.
    He sought a purely mathematical derivation of this number, linking it to cosmology and fundamental constants.
    His attempts, though elegant, are not considered physically correct.
  • Paul Dirac: Dirac was deeply intrigued by the number 137, suspecting it pointed to a deep connection
    between quantum mechanics and cosmology. He noted that certain large-number coincidences (ratios of cosmic
    to microscopic quantities) involved numbers near powers of 137. He hoped future theory would derive \alpha
    rather than taking it as input.
  • Richard Feynman: Famously described \alpha as “one of the greatest damn mysteries of physics: a magic number
    that comes to us with no understanding by man.” He emphasized that while QED uses \alpha to extraordinary precision,
    the theory itself does not explain why it has this value.
  • Modern Views: In grand unified theories (GUTs), \alpha is not fundamental but emerges from a common high-energy
    coupling that splits into the three Standard Model couplings as the universe cools. In string theory, coupling constants
    may arise from geometric features of extra dimensions or vacuum expectation values of scalar fields (“moduli”).
    Still, no unique derivation of 1/137 has been achieved.

Summary

The QED coupling constant originates from the coefficient of the electron–photon interaction in the QED Lagrangian.
Its numerical value (\alpha \approx 1/137) is not derived from deeper principles in the Standard Model;
it is a fundamental constant determined by experiment. Why it has this particular value is one of the biggest unsolved
questions in physics — possibly to be explained only by a deeper unification theory or anthropic reasoning.
The fascination with 137 reflects a century-long quest for a deeper understanding of nature’s most mysterious number.


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The Coupling Constant in QED https://stationarystates.com/quantum-field-theory/the-coupling-constant-in-qed/?utm_source=rss&utm_medium=rss&utm_campaign=the-coupling-constant-in-qed Mon, 29 Sep 2025 18:15:56 +0000 https://stationarystates.com/?p=982 The Coupling Constant in QED The QED coupling constant is one of the most famous “mystery numbers” in physics, better known as the fine-structure constant, usually denoted:     1. […]

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The Coupling Constant in QED

The QED coupling constant is one of the most famous “mystery numbers” in physics, better known as the
fine-structure constant, usually denoted:

    \[\alpha = \frac{e^2}{4 \pi \epsilon_0 \hbar c} \approx \frac{1}{137.035999...}.\]

1. What is the coupling constant in QED?

  • In quantum electrodynamics (QED), the coupling constant is the strength with which charged particles
    (like electrons) interact with the electromagnetic field (photons).
  • Mathematically, the electron charge e enters the QED Lagrangian as the coefficient in the interaction term:

        \[\mathcal{L}_{\text{int}} = -e \, \bar{\psi}\gamma^\mu A_\mu \psi,\]

    where \psi is the electron field and A_\mu is the photon field.

  • In natural units (\hbar = c = 1), the dimensionless form of the coupling is exactly
    \alpha = \frac{e^2}{4\pi}.

So, the origin of the QED coupling constant is: it’s the coefficient that sets the interaction strength
between the fundamental electron field and the photon field in the theory.

2. Why is it ~1/137?

This is the deeper mystery:

  • Experimental input: QED does not predict the value of \alpha. Instead, it must be measured in experiments (atomic spectroscopy, electron g-2, quantum Hall effect).
  • Running with energy: \alpha is not really constant. It “runs” with energy scale due to vacuum polarization. At low energies, \alpha \approx 1/137. At the Z boson scale (\sim 90 \,\text{GeV}), it increases to about 1/128.
  • Attempts at explanation: Many physicists (Dirac, Eddington) wondered whether 1/137 has a deeper mathematical or cosmological origin. The Standard Model does not explain it; in GUT or string theory, coupling constants may emerge from vacuum expectation values of fields or geometry of extra dimensions.
  • Anthropic speculation: If \alpha were very different, chemistry and stable matter might not exist. Its value could be constrained by conditions necessary for life.

3. Why that number matters

  • \alpha controls atomic structure (fine splitting in hydrogen, hence the name).
  • It governs scattering probabilities in particle physics.
  • Its smallness explains why QED perturbation theory converges so well (each higher order suppressed by ~1/137).

Summary

The QED coupling constant originates from the coefficient of the electron–photon interaction in the QED Lagrangian.
Its numerical value (\alpha \approx 1/137) is not derived from deeper principles in the Standard Model;
it is a fundamental constant determined by experiment. Why it has this particular value is one of the biggest unsolved
questions in physics — possibly to be explained only by a deeper unification theory or anthropic reasoning.

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Relativistic Particle in Complex Spacetime – A New Take on 4D Reality https://stationarystates.com/particle-physics/relativistic-particle-in-complex-spacetime-a-new-take-on-4d-reality/?utm_source=rss&utm_medium=rss&utm_campaign=relativistic-particle-in-complex-spacetime-a-new-take-on-4d-reality Wed, 07 May 2025 17:04:57 +0000 https://stationarystates.com/?p=909 From the August 2009 paper (Progress of Theoretical Physics) by Takayuki Hori Relativistic Particle in Complex Spacetime – A New Take on 4D Reality The 2009 paper “Relativistic Particle in […]

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From the August 2009 paper (Progress of Theoretical Physics) by Takayuki Hori

Relativistic Particle in Complex Spacetime – A New Take on 4D Reality

The 2009 paper “Relativistic Particle in Complex Spacetime” by Takayuki Hori proposes a novel particle model
where spacetime coordinates are complex-valued. The ultimate aim? To explain why the universe appears to have
exactly four spacetime dimensions.

? Core Idea

The particle’s position is written as a complex number:
zμ = xμ + i aμ. That is, it exists simultaneously in a real and imaginary
spacetime — a doubled universe of sorts. But gauge symmetries constrain the unphysical degrees of freedom.

? Why This Matters

The model’s structure is such that only in four dimensions do the quantum constraints allow physical momentum eigenstates.
Thus, the model gives a mathematical reason for why our universe might have 4D spacetime.

? Key Results

1. Lagrangian and Gauge Symmetry

The action for the particle includes complex terms:

∫ dτ (ẋ² / 2V + iλ ẋ·z + c.c.)

Here, V and λ are complex-valued gauge fields. The system shows SL(2, ℝ) symmetry and generates constraints through its dynamics.

2. Physical Equivalence and Dirac’s Conjecture

There are three first-class constraints, but only two gauge degrees of freedom — apparently violating Dirac’s conjecture.
Hori proposes a new criterion: states are physically equivalent if they have the same conserved charges, not just if they are
connected by gauge transformations.

3. Quantum Conditions Select 4D

Using BRST quantization, the model reveals that only in 4D does a consistent momentum eigenstate space exist.
This imposes a quantum-mechanical restriction on the dimension of spacetime.

4. Propagator and Scattering

Path integrals are computed to find a propagator and a toy scattering amplitude. Interestingly, the usual 1/k² behavior is
absent — suggesting new physics but also raising questions about how this model would connect to the Standard Model.

? Diagram: Complex Spacetime Particle Model

Complex Spacetime Model Diagram

? Significance

  • Reformulates particle physics in a complexified spacetime background.
  • Introduces a new way to think about gauge equivalence and constraints.
  • Provides a possible explanation for why we live in a 4D universe.

⚖ Strengths & Limitations

Pros:

  • Mathematically consistent and gauge-invariant.
  • Offers a dimensionality constraint from quantum principles.

Cons:

  • No spin, internal quantum numbers, or Standard Model coupling.
  • Propagator lacks a physical pole structure (no 1/k²).

? Summary

This paper offers a novel mathematical model where a particle lives in a complexified spacetime.
Quantization under constraints reveals that only four-dimensional spacetime yields viable physics — suggesting
our universe’s dimensionality may emerge from quantum geometry.

 

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Free Scalar Field Equation – Solved using matrix mechanics https://stationarystates.com/quantum-field-theory/free-scalar-field-equation-solved-using-matrix-mechanics/?utm_source=rss&utm_medium=rss&utm_campaign=free-scalar-field-equation-solved-using-matrix-mechanics Wed, 01 Jan 2025 03:17:48 +0000 https://stationarystates.com/?p=697 Free Scalar Field: Field Equation and Matrix Mechanics Solution Field Equation for a Free Scalar Field The action for a free scalar field φ(x) in four-dimensional spacetime is given by: […]

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Free Scalar Field: Field Equation and Matrix Mechanics Solution

Field Equation for a Free Scalar Field

The action for a free scalar field φ(x) in four-dimensional spacetime is given by:

S = ∫ d⁴x [ (1/2) ∂μφ ∂μφ – (1/2) m²φ² ],

where:

  • φ(x) is the scalar field.
  • m is the mass of the scalar field.
  • μ = ημνν, with the metric signature (+, -, -, -).

The Euler-Lagrange equation for this action yields the Klein-Gordon equation:

□φ + m²φ = 0,

where:

□ = ∂μμ = ∂²/∂t² – ∇²

is the d’Alembertian operator.

Matrix Mechanics Representation

1. Discretizing Spacetime

Spacetime is replaced by a finite lattice with points xi (e.g., i = 1, 2, …, N). The field φ(x) is represented as a vector:

φ(x) → ? = [ φ(x₁), φ(x₂), …, φ(xN) ]T.

2. Representing Derivatives with Matrices

The derivative operators μ and are approximated using finite difference methods:

  • The spatial Laplacian ∇² is represented by a matrix ?.
  • The time derivative ∂²/∂t² is represented by another matrix.

The d’Alembertian becomes:

□φ → ??,

where ? is the discretized representation of .

3. Equation in Matrix Form

The Klein-Gordon equation in matrix form is:

?? + m²? = 0.

4. Solution Using Eigenmodes

The solution can be found by diagonalizing the operator ? + m²?. Let ? be the matrix of eigenvectors and Λ the diagonal matrix of eigenvalues:

? = ?Λ?.

The solution to the matrix equation is then:

?(t) = ? e-i√Λt?,

where ? is determined by the initial conditions.

Physical Interpretation

  • Eigenmodes: Each eigenmode corresponds to a plane wave solution e-i(E t – k⋅x) with the dispersion relation E² = k² + m².
  • Superposition: The field evolution is a superposition of eigenmodes governed by the eigenvalues and eigenvectors of ?.

Applications

This matrix mechanics representation is commonly used in numerical simulations of quantum field theories and lattice field theory computations.

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