"Common" relativistic variables.

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SUMMARY

The discussion focuses on calculating the common total energy, momentum, and total rest mass of a 3.0 MeV photon and an electron moving at 0.995c in opposite directions. The term "common" refers to the combined properties of the two particles rather than their individual characteristics. Participants emphasize the importance of applying fundamental relativistic equations to solve the problem effectively.

PREREQUISITES
  • Understanding of special relativity concepts, including relativistic energy and momentum.
  • Familiarity with fundamental relativistic equations, such as E=mc² and p=mv.
  • Knowledge of photon properties, including energy-momentum relationships.
  • Basic understanding of particle physics, particularly electron behavior at relativistic speeds.
NEXT STEPS
  • Study the derivation and application of the relativistic energy-momentum relation.
  • Learn how to calculate relativistic momentum for particles moving at high velocities.
  • Explore the implications of relativistic effects on particle interactions.
  • Investigate the concept of invariant mass in relativistic systems.
USEFUL FOR

Students and educators in physics, particularly those focusing on special relativity, particle physics, and energy-momentum calculations.

GravitonDiet
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So the thing I have issues with in this problem is that it's about 2 particles traveling relative to each other. Been going though the basics of relativity, relativistic lengths, times, kinetic energy, work and force. But this problem states two particles and I'm not sure how to approach it. The word "common" is where I get confused.

1. Homework Statement

A 3.0 MeV photon is moving in positive x-direction and an electron in the opposite direction at a velocity of 0.995c. Calculate their common total energy, momentum and total rest mass.

Homework Equations


Fundamental relativistic equations.
 
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I suspect the word "common" is added only to separate from "individual", i.e., you are asked to find the sum of the particle energies.
 

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