For the process \(1+2 \rightarrow 3+4\), the Mandelstam variables \(s, t\) and \(u\) are defined as \(s=\left(p_{1}+p_{2}\right)^{2}\), \(t=\left(p_{1}-p_{3}\right)^{2}\) and \(u=\left(p_{1}-p_{4}\right)^{2}\). Show that $$ s+u+t=m_{1}^{2}+m_{2}^{2}+m_{3}^{2}+m_{4}^{2} $$

Short Answer

Expert verified
The sum of the Mandelstam variables is equal to the sum of the squares of the masses of all particles: \( s + t + u = m_1^2 + m_2^2 + m_3^2 + m_4^2 \).

Step by step solution

01

- Understand the Mandelstam Variables

Before diving into the calculation, understand what the Mandelstam variables represent. They are combinations of the four-momenta of particles involved in a scattering process: - The variable s represents the Mandelstam invariant mass squared of the initial state particles. - The variable t is the momentum transfer between initial particle 1 and final particle 3. - The variable u is the momentum transfer between initial particle 1 and final particle 4.
02

- Write the Definitions

Use the definitions provided in the problem statement for our process: - The variable s: \[ s = (p_1 + p_2)^2 \] - The variable t: \[ t = (p_1 - p_3)^2 \] - The variable u: \[ u = (p_1 - p_4)^2 \]
03

- Expand Each Definition

Expand each squared term using the inner product of four-vectors: - For s: \[ s = (p_1 + p_2)^2 = p_1^2 + p_2^2 + 2 p_1 \bullet p_2 \] - For t: \[ t = (p_1 - p_3)^2 = p_1^2 + p_3^2 - 2 p_1 \bullet p_3 \] - For u: \[ u = (p_1 - p_4)^2 = p_1^2 + p_4^2 - 2 p_1 \bullet p_4 \]
04

- Sum s, t, and u

Add s, t, and u together: \[ s + t + u = (p_1^2 + p_2^2 + 2 p_1 \bullet p_2) + (p_1^2 + p_3^2 - 2 p_1 \bullet p_3) + (p_1^2 + p_4^2 - 2 p_1 \bullet p_4) \]
05

- Simplify the Expression

Combine like terms in the sum: - Note the terms with \( p_1 \bullet p_2 \), \( p_1 \bullet p_3 \), and \( p_1 \bullet p_4 \) cancel out. This gives us: \[ s + t + u = p_1^2 + p_2^2 + p_3^2 + p_4^2 + p_1^2 + p_1^2 + p_1^2 \]
06

- Recognize the Masses Involved

Identify each four-momentum squared as the square of the mass of the respective particles: \[ p_1^2 = m_1^2 \] \[ p_2^2 = m_2^2 \] \[ p_3^2 = m_3^2 \] \[ p_4^2 = m_4^2 \]
07

- Conclude the Proof

Substitute back these mass relations into the equation: \[ s + t + u = m_1^2 + m_2^2 + m_3^2 + m_4^2 \]

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Key Concepts

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

Scattering Process
In particle physics, a scattering process describes an interaction where particles collide and scatter into new directions or transform into different particles. Understanding this concept is crucial for analyzing high-energy physics experiments. Typically, we represent a scattering process as \(1+2 \rightarrow 3+4\). Here:
  • Particle 1 and Particle 2 are the initial state particles that interact.
  • Particle 3 and Particle 4 are the final state particles resulting from the interaction.
The scattering process allows us to explore fundamental forces and particle interactions in experiments using particle colliders. Learning about the energy and momentum exchanged during these interactions helps us to understand the fundamental forces and the properties of particles. This is where the Mandelstam variables come in handy, as they encapsulate the essential information about the scattering event.
Four-Momentum
Four-momentum is a foundational concept in relativity and particle physics that combines energy and momentum into a single four-vector. It is denoted as \(p = (E/c, \mathbf{p})\) where:
  • \(E\) is the total energy of the particle.
  • \(\mathbf{p}\) is the three-momentum vector of the particle.
The four-momentum vector is crucial for relativistic physics because it remains consistent across all reference frames. This makes calculations more straightforward and ensures physical laws hold true in all scenarios. In a scattering process:
  • \(p_1\) and \(p_2\) represent the four-momenta of the initial-state particles.
  • \(p_3\) and \(p_4\) represent the four-momenta of the final-state particles.
Each magnitude of these four-momenta squares equals the mass squared of the respective particle, that is, \(p_i^2 = m_i^2\) where \(i\) can be 1, 2, 3, or 4. This property is utilized in the given exercise to derive the sum of Mandelstam variables.
Invariant Mass
Invariant mass is an essential property in high-energy physics, representing the mass of a system that remains unchanged regardless of the reference frame. It is a scalar quantity derived from four-momentum vectors. When considering two particles, their invariant mass is given by: \[ M^2 = (p_1 + p_2)^2 \] Usually, the sum of Mandelstam variables \(s, t, \) and \(u\) relates to the invariant masses of the particles involved. In the context of the scattering process \(1 + 2 \rightarrow 3 + 4\), the Mandelstam variables are:
  • \(s = (p_1 + p_2)^2\), which represents the invariant mass squared of the initial state particles.
  • \(t = (p_1 - p_3)^2\), indicating the momentum transfer between initial particle 1 and final particle 3.
  • \(u = (p_1 - p_4)^2\), indicating the momentum transfer between initial particle 1 and final particle 4.
By understanding and summing these variables, one can confirm that:\[ s + t + u = m_1^2 + m_2^2 + m_3^2 + m_4^2 \] where each \(m_i^2\) corresponds to the squared invariant mass of particle \(i\).

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Most popular questions from this chapter

In the laboratory frame, denoted \(\Sigma\), a particle travelling in the z-direction has momentum \(\mathbf{p}=p_{z} \hat{\mathbf{z}}\) and energy \(E\). (a) Use the Lorentz transformation to find expressions for the momentum \(p_{z}^{\prime}\) and energy \(E^{\prime}\) of the particle in a frame \(\Sigma^{\prime}\), which is moving in a velocity \(\mathbf{v}=+v \hat{z}\) relative to \(\Sigma\), and show that \(E^{2}-p_{2}^{2}=\left(E^{\prime}\right)^{2}-\left(p_{2}^{\prime}\right)^{2}\). (b) For a system of particles, prove that the total four-momentum squared, $$ p^{\mu} p_{\mu} \equiv\left(\sum_{i} E_{i}\right)^{2}-\left(\sum_{i} \mathbf{p}_{i}\right)^{2} $$ is invariant under Lorentz transformations.

Consider the Compton scattering of a photon of momentum \(\mathbf{k}\) and energy \(E=|\mathbf{k}|=\mathrm{k}\) from an electron \(a\) t rest. Writing the four-momenta of the scattered photon and electron respectively as \(k^{\prime}\) and \(p^{\prime}\), conservation of fourmomentum is expressed as \(k+p=k^{\prime}+p^{\prime}\). Use the relation \(p^{\prime 2}=m_{e}^{2}\) to show that the energy of the scattered photon is given by $$ E^{\prime}=\frac{E}{1+\left(E / m_{e}\right)(1-\cos \theta)} $$ where \(\theta\) is the angle through which the photon is scattered.

In a collider experiment, \(\Lambda\) baryons can be identified from the decay \(\Lambda \rightarrow \pi^{-} p\), which gives rise to a displaced vertex in a tracking detector. In a particular decay, the momenta of the \(\pi^{+}\)and \(p\) are measured to be \(0.75 \mathrm{GeV}\) and \(4.25 \mathrm{GeV}\) respectively, and the opening angle between the tracks is \(9^{\circ}\). The masses of the pion and proton are \(139.6 \mathrm{MeV}\) and \(938.3 \mathrm{MeV}\). (a) Calculate the mass of the \(\Lambda\) baryon. (b) On average, \(\Lambda\) baryons of this energy are observed to decay at a distance of \(0.35 \mathrm{~m}\) from the point of production. Calculate the lifetime of the \(\Lambda\).

At the HERA collider, \(27.5 \mathrm{GeV}\) electrons were collided head-on with \(820 \mathrm{GeV}\) protons. Calculate the centre-ofmass energy.

Show that the process \(\gamma \rightarrow \mathrm{e}^{+} \mathrm{e}^{-}\)can not occur in the vacuum.

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