- Page 6 and 7: AcknowledgementsThese lecture notes
- Page 8 and 9: immediately if a distant proton (or
- Page 10 and 11: and, to agree with experiment, shou
- Page 12 and 13: to about the TeV . This is precisel
- Page 14 and 15: where the official name for L is th
- Page 16 and 17: The initial data required on a Cauc
- Page 18 and 19: The definition of a Lorentz invaria
- Page 20 and 21: where A is the area bounding V and
- Page 22 and 23: where Γ ρµν is some function of
- Page 24 and 25: 1.3.4 Internal SymmetriesThe above
- Page 26 and 27: An Example: A Real Scalar FieldFor
- Page 28 and 29: from all the others. Free field the
- Page 30 and 31: Claim: The commutation relations fo
- Page 32 and 33: We can deal with the infinity in (2
- Page 34 and 35: But there’s a problem. E is infin
- Page 36 and 37: We interpret the state |⃗p〉 as
- Page 38 and 39: But is this Lorentz invariant? It
- Page 40 and 41: Since the classical field ψ is not
- Page 42 and 43: = i 2∫d 3 y (∇ y [φ(y), π(x)]
- Page 44 and 45: 2.7 PropagatorsWe could ask a diffe
- Page 46 and 47: ∫=d 3 p(2π) 3 12E ⃗pe −ip·(
- Page 48 and 49: this is equivalent to saying that |
- Page 50 and 51: which, on one-particle states, give
- Page 52 and 53:
One can also consider interactions
- Page 54 and 55:
• [λ 4 ] = 0: this term is small
- Page 56 and 57:
The scalar Yukawa theory has a slig
- Page 58 and 59:
where U(t, t 0 ) is a unitary time
- Page 60 and 61:
the interaction picture and follow
- Page 62 and 63:
ψ † ∼ b † + c. To get non-ze
- Page 64 and 65:
A similar discussion holds for comp
- Page 66 and 67:
momentum conservation, |⃗p 1 | =
- Page 68 and 69:
3.5 Examples of Scattering Amplitud
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p 1/p 1/p 2p 2+p 2p 1p /p / 21Figur
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3.5.1 Mandelstam VariablesWe see th
- Page 74 and 75:
Now we understand the profile of th
- Page 76 and 77:
vertex rather than (−iλ/4!). To
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where ω = E m −E n . This gives
- Page 80 and 81:
that A = −g for a single meson de
- Page 82 and 83:
and 〈Ω| Ω〉 = 1. Note that thi
- Page 84 and 85:
to an exponential,〈0|S |0〉 = ex
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So what’s the point of all of thi
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Note that an antisymmetric 4 × 4 m
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One can construct many other repres
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and the spinor rotation matrix beco
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so thatS[Λ] † = exp ( 12 Ω ρσ
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4.3 The Dirac EquationThe equation
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where we have introduced some new n
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4.4.3 ParityThe spinors ψ ± are r
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We’re now armed with new terms in
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4.6 Symmetries and Conserved Curren
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Here the second transformation foll
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4.7.1 Some ExamplesConsider the pos
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We have analogous results for the n
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5. Quantizing the Dirac FieldWe wou
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which means that H = ∫ d 3 x H ag
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The calculation of the Hamiltonian
- Page 118 and 119:
an electron, the two can annihilate
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• At least away from singularitie
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where, as usual, all fields are in
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• Each internal line gets a facto
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p,s/p,s/p,s/p,s/+q,r / /q,rq,r / /q
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and v(⃗p). In the non-relativisti
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6. Quantum ElectrodynamicsIn this s
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So what are we to make of this? We
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6.2 The Quantization of the Electro
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We now write ⃗ A in the usual mod
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and we can make the usual expansion
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• We could try to impose the cond
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PropagatorsFinally, it’s a simple
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charge. For QED, the theory of ligh
- Page 146 and 147:
In Coulomb gauge ∇ · ⃗A = 0, t
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The D 00 piece of the propagator do
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6.5.1 Charged Scalars“Pauli asked
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scattering process was one of the c
- Page 154 and 155:
The overall + sign comes from treat