Loop integrals and observable corrections

Perform representative perturbative field-theory calculations with explicit regularization, analytic continuation, divergence identification, and unitarity checks.

10 published lessons1 module300 min of guided study
  1. 01
    Loop integrals and observable correctionsresearch · 10 lessons

Follow the path or begin with a question. Every lesson is open.

Your notebook0 of 10 lessons completed

Your place, at your pace. Progress is optional and saved only in this browser when available.

Inside this module

Each lesson includes an interactive lab

Loop integrals and observable corrections

Perform representative perturbative field-theory calculations with explicit regularization, analytic continuation, divergence identification, and unitarity checks.

  1. 01

    Wick contractions and diagram symmetry factors

    Derive scalar diagram coefficients from explicitly labeled contractions and distinguish combinatorics from coupling powers.

    30 min
  2. 02

    One-loop scalar self-energy

    Evaluate a massive scalar tadpole with an explicit Euclidean cutoff and connect subtraction conditions to propagator poles.

    30 min
  3. 03

    Feynman parameter combination of denominators

    Combine propagators, complete the loop-momentum square, and preserve analytic prescriptions and regulator assumptions.

    30 min
  4. 04

    Dimensional loop integration

    Derive a Euclidean master integral and expand its ultraviolet pole with an explicit scale and subtraction convention.

    30 min
  5. 05

    Tensor integral reduction

    Use rotational identities and external momenta to reduce tensor numerators without discarding dimension-dependent finite terms.

    30 min
  6. 06

    One-loop four-point amplitudes

    Assemble the scalar s, t, and u bubbles, subtract their ultraviolet pole, and check renormalization-scale dependence.

    30 min
  7. 07

    Branch cuts and threshold discontinuities

    Locate the scalar two-particle threshold from parameter space and compute its imaginary part with a fixed causal branch.

    30 min
  8. 08

    Cutkosky cuts and perturbative unitarity

    Match a scalar bubble’s absorptive part to on-shell phase space with explicit state normalization and identical-particle factors.

    30 min
  9. 09

    Infrared divergences and inclusive observables

    Identify soft and collinear limits and state the measurement conditions needed for physical infrared cancellation.

    30 min
  10. 10

    Real–virtual cancellation in simple processes

    Combine regulated endpoint terms into a plus distribution and distinguish universal singular structure from supplied hard matching constants.

    30 min
All physics modules