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Initial and final state radiation

Initial and final state radiation is a physics topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Initial and final state radiation rather than just read about it. In short: In quantum field theory, initial and final state radiation refers to certain kinds of radiative emissions that are not due to particle annihilation. It is important in experimental and theoretical studies of interactions at particle colliders.

Initial and final state radiation — main illustration
Initial and final state radiation — illustration

Key takeaways

  • Initial and final state radiation belongs to physics; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Initial and final state radiation to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Initial and final state radiation from memory before moving on to harder problems.

Reference excerpt

In quantum field theory, initial and final state radiation refers to certain kinds of radiative emissions that are not due to particle annihilation. It is important in experimental and theoretical studies of interactions at particle colliders.

Description Particle accelerators and colliders produce collisions (interactions) of particles (like the electron or the proton). In the terminology of the quantum state, the colliding particles form the initial state. In the collision, particles can be annihilated or/and exchanged, producing possibly different sets of particles, the final states. The initial and final states of the interaction relate through the so-called scattering matrix (S-matrix). The probability amplitude for a transition of a quantum system from the initial state having state vector | i ⟩ {\displaystyle |i\rangle } to the final state vector | f ⟩ {\displaystyle |f\rangle } is given by the scattering matrix element

S f i = ⟨ f | S | i ⟩ , {\displaystyle S_{fi}=\langle f|S|i\rangle \;,}

where S {\displaystyle S} is the S-matrix.

Electron-positron annihilation example

The electron-positron annihilation interaction:

e + e − → 2 γ {\displaystyle e^{+}e^{-}\to 2\gamma }

has a contribution from the second order Feynman diagram shown adjacent: In the initial state (at the bottom; early time) there is one electron (e−) and one positron (e+) and in the final state (at the top; late time) there are two photons (γ). Other states are possible. For example, at LEP, e+ + e− → e+ + e−, or e+ + e− → μ+ + μ− are processes where the initial state is an electron and a positron colliding to produce an electron and a positron or two muons of opposite charge: the final states.

Phenomenology

In the case of initial-state radiation, one of the incoming particles emit radiation (such as a photon, wlog) before the interaction with the others, so reduces the beam energy prior to the momentum transfer; while for final-state radiation, the scattered particles emit radiation, and since the momentum transfer has already occurred, the resulting beam energy decreases. In analogy with bremsstrahlung, if the radiation is electromagnetic it is sometimes called beam-strahlung, and similarly can have gluon-strahlung (as shown in the Feynman figure with the gluon) as well in the case of QCD.

Computational issues In these simple cases, no automatic calculation software packages are needed and the cross-section analytical expression can be easily derived at least for the lowest approximation: the Born approximation also called the leading order or the tree level (as Feynman diagrams have only trunk and branches, no loops). Interactions at higher energies open a large spectrum of possible final states and consequently increase the number of processes to compute, however. The calculation of probability amplitudes in theoretical particle physics requires the use of rather large and complicated integrals over a large number of variables. These integrals do, however, have a regular structure, and may be represented graphically as Feynman diagrams. A Feynman diagram is a contribution of a particular class of particle paths, which join and split as described by the diagram. More precisely, and technically, a Feynman diagram is a graphical representation of a perturbative contribution to the transition amplitude or correlation function of a quantum mechanical or statistical field theory. Within the canonical formulation of quantum field theory, a Feynman diagram represents a term in the Wick's expansion of the perturbative S-matrix. Alternatively, the path integral formulation of quantum field theory represents the transition amplitude as a weighted sum of all possible histories of the system from the initial to the final state, in terms of either particles or fields. The transition amplitude is then given as the matrix element of the S-matrix between the initial and the final states of the quantum system.

References

External links Initial and final state radiation in Z production, A Quantum Diaries Survivor. Beam-Beam Interaction, D. Schulte ISR and Beamstrahlung

Illustrations

Initial and final state radiation: In this Feynman diagram, an electron and a positron annihilate, producing a
photon (represented by the blue sine wave) that becomes a quark-antiquark pair, after which one particle radiates a gluon (represented by the green spiral).
In this Feynman diagram, an electron and a positron annihilate, producing a photon (represented by the blue sine wave) that becomes a quark-antiquark pair, after which one particle radiates a gluon (represented by the green spiral).

Worked examples

Example 1 — a first encounter with Initial and final state radiation

Start with the simplest possible case. Write down what Initial and final state radiation claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Initial and final state radiation before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Initial and final state radiation ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Initial and final state radiation

In research
Initial and final state radiation appears in physics research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Initial and final state radiation in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Initial and final state radiation is common in secondary-school and first-year university syllabi. It links to neighbouring topics Quantum field theory, so understanding it makes those chapters shorter.
In everyday life
Look for Initial and final state radiation outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

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How to study Initial and final state radiation in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Initial and final state radiation means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Initial and final state radiation out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Initial and final state radiation in simple terms?

In quantum field theory, initial and final state radiation refers to certain kinds of radiative emissions that are not due to particle annihilation. It is important in experimental and theoretical studies of interactions at particle colliders.

Why does Initial and final state radiation matter?

Because it connects several physics ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Initial and final state radiation?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Initial and final state radiation.

Tags

  • Quantum field theory

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