Energy spectrum of electromagnetic showers.

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SUMMARY

The discussion centers on the energy spectrum of secondary particles in electromagnetic showers, specifically demonstrating that the spectrum follows a power law of E^{-2} for energy ranges where E_0 >> E >> E_c. The model describes how an initial particle, such as an electron or photon, generates secondary particles through processes like bremsstrahlung or pair production after each radiation length. The confusion arises regarding the interpretation of the energy spectrum and the calculation of the number of particles with energy exceeding a certain threshold, leading to the conclusion that the number of particles with energy greater than E is proportional to E^{-2}.

PREREQUISITES
  • Understanding of electromagnetic showers and radiation lengths
  • Knowledge of bremsstrahlung and pair production processes
  • Familiarity with energy spectrum concepts in particle physics
  • Basic calculus for integration and differentiation
NEXT STEPS
  • Study the derivation of energy spectra in electromagnetic showers
  • Learn about the critical energy E_c and its significance in particle interactions
  • Explore the mathematical modeling of particle production in high-energy physics
  • Investigate the implications of energy loss mechanisms such as ionization in calorimetry
USEFUL FOR

Students and researchers in particle physics, particularly those focusing on electromagnetic interactions and calorimetry, as well as educators teaching concepts related to energy spectra and particle production.

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Homework Statement



Use the simple model for electromagnetic showers (explained below) to show that the energy spectrum of all secondary particles contained in an electromagnetic shower falls like E^{-2} for E_0 >> E >> E_c

The Attempt at a Solution



An electron or a photon with energy E_0 goes through an electromagnetic calorimeter and undergoes bremmstrahlung or pair production respectively after a radiation length. Hence after 1 radiation length there are 2 particles (considering photons as particles for ease), after 2 lengths there are 4 etc. So after t radiation lengths there are 2^t particles and each particle has a mean energy of \frac {E_0}{2^t}.

When the particle energy goes below the critical energy E_c the main source of energy loss is ionisation, the showering process then stops.

Now I'm confused by what the question actually wants and what is meant by "energy spectrum". Is it just asking for a given energy E, how many particles N will exist? Because that would just be \frac {E_0}{E}. It's not though, because the answer says;

The number of particles with energy exceeding E is

N(>E) = \int^{t(E)}_{0} N(t)dt

It then goes on to show N(>E) = \frac {E_0}{ln(2) E} and then says

"implying dN/dE \propto E^{-2}".

I'm entirely confused here. So what exactly was the quantity that was wanted? The rate of change (with E) of the amount of particles with energy greater than E?

But the way I see it the number of particles with energy greater than E is the same as the area under a graph of E versus N from E to E_0. i.e.

N(>E) = \int^{E_0}_{E} N(E)dE.

But N(E) = \frac {E_0}{E}

So the derivative of \int^{E_0}_{E} N(E)dE with respect to E is just N(E) = \frac {E_0}{E}

Why are there two different results for the same thing?
 
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Am I missing something here?EDIT:The simple model for electromagnetic showers is that each particle undergoes bremmstrahlung or pair production after a radiation length and each daughter particle has half the energy of its parent.
 

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