Skip to content

Lecture 2

Chasse_neige

Why Massless Spin-2?

Classical Field Theory

First, consider a massless spin-1 particle

L=14FμνFμνeJμAμμFμν=eJνAμ=eJμ

for a static point source

{J0=qαδ3(xxα)J=0

So we can get the form of the vector potential

A0=eqα4π|xxα|

And the total energy

E=dxeJbμAμ=dxe(qbδ3(xxb))(eqα4π|xxα|)=αqaqb|xαxb|

Then consider a massive spin-0 (scalar field)

L=12(μϕ)212m2ϕ2+gϕja scalar source

and we can get

(m2)ϕ=gjjα=qαδ3(xxα)

the form of ϕ is

ϕ=dk(2π)3gqαk2+m2eik(xxα)=gqα4πem|xxα||xxα|

The total energy

E=gdxϕjb=g2qaqb4πem|xxα||xxα|

Lesson

  1. Inverse square law -> massless mediator
  2. Spin-0 mediates attractive force and Spin-1 mediates repulsive force

Gravity could be mediated by a massless spin-0 particle, but under this circumstance light won’t bend.

Field Theory for Spin-2

We guess

L12λhμνλhμνκhμνTμν

This will lead to

hμν=κTμν

where a static point particle is defined as

Ta00=maδ3(xxa)h00=κma4π|xxa|

and the total energy

E=κdxh00Tb00=κ24πmamb|xxa|

Massless Spinning Particles are peculiar!

Polarizations of the photon

for k=(0,0,k), we describe the polarization using the vector

ex=(1,0,0)ey=(0,1,0)

or using the circular polarization

e±=12(ex±iey)

for arbitrary momentum p

e±(p)Rz(ϕ)Ry(θ)e±(k)

is a SO(3) vector. But it is impossible to imbed e± into a Lorentz vector. (see the deduction from Feynman Lectures on Physics (3))

Guess

e±μ(k)=12(0,1,±i,0)T

and we’ll get

Ry1(θ)Lx(η2)Lz(η1)e±μ(k)=e±μ(k)+tanθ2k0kμ

So e±μ is a L-vec only up to an additive term kμ.

3 types of L-trans will leave kμ inv.

  1. Rotation around k: Rz(θ)
  2. R × L-type L-trans: Ry1LxLz
  3. R × L-type L-trans with xyyx: Rx1LyLz

we call them LGT (little group transformation, ISO(2)). The generators of the LGT’s commutations are

[Rz,Tx]=iTy[Rz,Ty]=iTx[Tx,Ty]=0

Polarization is a representation of not LGT, but SO(2).

The charge of SO(2) is called helicity: Rz(θ)X=eihθX, so the nonlinear term is price we have to pay for embedding h=±1 into “e±μ”.

The transformation ee+αk is traditionally called a gauge transformation. Gauge inv, is enforced by L-symmetry.

Graviton: Spin-2

Assume the momentum k=(k,0,0,k), and the polarization tensor is defined

eμν±(k)=eμ±(k)eν±(k)=12(000001±i00±i100000)

for transformations within LGT, the polarization tensor will act as

e±μν(k)e±μν(k)+tanθ2k0[e±μ(k)+tanθ2k0kμ]kν+μνe±μν(k)e±μν(k)+ξμkν+ξνkμ

Spin-3 Particles

The polarization tensor e±μνλ under LGT will be

e±μνλ(k)e±μνλ(k)+ξμνkλ+

Summary

Polarization tensors are up to LGT L-transf.

Built with VitePress