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Draw a Feynman diagram for an electron-proton scattering, \(e^{-}+p \rightarrow e^{-}+p\), mediated by photon exchange.

Short Answer

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Question: Draw a Feynman diagram for an electron-proton scattering process, and briefly explain the structure of the diagram. Answer: In the electron-proton scattering process, an electron and a proton interact with each other through the exchange of a virtual photon. The Feynman diagram for this process can be represented as: ``` V1 V2 e^- →--------γ--------→ e^- / /\ \ / / \ \ / / \ \ p →--------γ--------→ p ``` In the diagram, the horizontal lines denote the electron (e^-) and proton (p) paths, with arrows indicating the direction of their movement. The wavy line connecting these particle paths represents the exchange of a virtual photon (γ), responsible for the interaction between the electron and the proton. The points V1 and V2 are labeled as vertices, signifying the points of interaction where the photon is absorbed or emitted by the particles.

Step by step solution

01

Identify the incoming and outgoing particles

First, identify the incoming and outgoing particles in the process. In this case, the incoming particles are an electron (\(e^{-}\)) and a proton (\(p\)), and the outgoing particles are also an electron (\(e^{-}\)) and a proton (\(p\)).
02

Draw the electron and proton lines

Draw two horizontal lines to represent the electron and proton. Since electron is a fermion, draw a solid line with an arrow for its path, and label it as \(e^{-}\). Similarly, draw another solid line with an arrow for the proton, and label it as \(p\). The arrow direction indicates the direction of the particle's movement. Place the initial particles on the left side of the diagram and the final particles on the right side.
03

Represent the photon exchange

Since the process is mediated by the exchange of a photon, draw a wavy line connecting the electron line to the proton line, representing the virtual photon exchanged between them. This photon is responsible for the interaction between the electron and the proton. Label the photon line with \(\gamma\) to indicate that it is a photon.
04

Label the vertices

Label the points where the photon line connects with the electron and proton lines as vertices \(V_{1}\) and \(V_{2}\). These vertices represent the points of interaction where the photon is absorbed or emitted by the particles.
05

Final Diagram

The final Feynman diagram for the electron-proton scattering can be represented as: ``` V1 V2 e^- →--------γ--------→ e^- / /\ \ / / \ \ / / \ \ p →--------γ--------→ p ``` The diagram shows the interaction between an electron and a proton through the exchange of a virtual photon, with the appropriate labeling of particles, vertices, and photon line.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Electron-Proton Scattering
When we talk about electron-proton scattering, we are examining a fundamental process in which an electron (\(e^{-}\)) and a proton (\(p\)) interact and then scatter off each other, but emerge as the same types of particles. This particular process is crucial for probing the structure of protons and understanding how electrons interact with the building blocks of matter. During the scattering, properties such as momentum and energy are exchanged between the electron and the proton, but their identities remain unchanged. It’s a bit like two ice skaters throwing a ball to each other; they push apart after the ball is thrown but remain skaters.

This phenomenon can be visualized using a Feynman diagram, a graphic representation that simplifies complex interactions into drawings that depict the movement and interaction of particles. From a physics standpoint, these diagrams provide a way to track the interaction at every stage, indicating the direction of particle motion and the points where interactions occur. The process of drawing such a diagram involves identifying the initial and final particles, drawing lines to represent them, and accounting for the mediating force, in this case, the photon exchange.
Photon Exchange
Photon exchange is the force-carrying action that occurs between charged particles in quantum electrodynamics (QED), the quantum field theory of electrodynamics. In the context of electron-proton scattering, the photon acts as the mediator of the electromagnetic force. Think of it as a temporary messenger that allows the electron and proton to 'communicate' with each other over a distance without actually touching.

In a Feynman diagram, the photon exchange is generally represented by a wavy line connecting the lines of charged particles. This depiction is symbolic; in reality, the photon isn't visible and doesn't travel in a wavy path, but the line helps us understand that an interaction took place. It's essential to note that the exchanged photon is often a virtual photon, meaning it can't be directly observed and exists only for a fleeting moment during the interaction between particles.
Virtual Photon
A virtual photon is an intermediate particle that facilitates the electromagnetic interaction between other charged particles, like electrons and protons. Unlike real photons, virtual photons are not directly observable; they are 'off-shell,' which means they do not have to adhere strictly to the mass-energy relation that real photons do. In essence, they can have various amounts of energy or mass that real photons couldn’t possess.

In Feynman diagrams, virtual photons are represented by internal lines, not ending on the edges of the diagram which are reserved for 'real' or detectable particles. Although they might sound mysterious, virtual photons are critical components in explaining the forces acting at the quantum level. They're akin to the temporary bridges that form between particles, allowing them to interact over short periods and distances without a physical photon being emitted or absorbed.
Particle Physics
Particle physics is the field that explores the smallest known building blocks of the universe and the forces that govern their interactions. Electron-proton scattering, as demonstrated in the given Feynman diagram, is a classic example of how particle physicists attempt to understand the nature of matter.

In particle physics, not only are particles like electrons and protons studied, but also the mediators of the fundamental forces—like the photons in electromagnetic interactions. Using the principles of quantum field theories, such as quantum electrodynamics (QED), particle physicists illustrate interactions using Feynman diagrams, calculate the probabilities of various outcomes, and conduct experiments to verify theoretical predictions. The understanding gained from particle physics not only satisfies our curiosity about the universe at the most fundamental level but also drives innovation in technology and medicine.

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Most popular questions from this chapter

The fundamental observation underlying the Big Bang theory of cosmology is Edwin Hubble's 1929 discovery that the arrangement of galaxies throughout space is expanding. Like the photons of the cosmic microwave background, the light from distant galaxies is stretched to longer wavelengths by the expansion of the universe. This is not a Doppler shift: Except for their local motions around each other, the galaxies are essentially at rest in space; it is the space itself that expands. The ratio of the wavelength of light \(\lambda_{\text {rec }}\) Earth receives from a galaxy to its wavelength \(\lambda_{\text {emit }}\) at emission is equal to the ratio of the scale factor (e.g., radius of curvature) \(a\) of the universe at reception to its value at emission. The redshift \(z\) of the light-which is what Hubble could measure - is defined by \(1+z=\lambda_{\text {rec }} / \lambda_{\text {emit }}=a_{\text {rec }} / a_{\text {emit }}\). a) Hubble's Law states that the redshift \(z\) of light from a galaxy is proportional to the galaxy's distance from us (for reasonably nearby galaxies): \(z \cong c^{-1} H \Delta s\), where \(c\) is the vacuum speed of light, \(H\) is the Hubble constant, and \(\Delta s\) is the distance of the galaxy. Derive this law from the first relationships stated in the problem, and determine the Hubble constant in terms of the scale-factor function \(a(t)\). b) If the present Hubble constant has the value \(H_{0}=72(\mathrm{~km} / \mathrm{s}) / \mathrm{Mpc},\) how far away is a galaxy, the light from which has redshift \(z=0.10\) ? (The megaparsec \((\mathrm{Mpc})\) is a unit of length equal to \(3.26 \cdot 10^{6}\) light-years. For comparison, the Great Nebula in Andromeda is approximately 0.60 Mpc from us.)

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