Calculating Minimum Energy for Relativistic Collision of Proton and Photon

Click For Summary
SUMMARY

The discussion focuses on calculating the minimum energy required for a proton (p+) to collide with a cosmic microwave-background (CMB) photon (γ) to produce a delta baryon (∆+). The photon energy is given as 2.3 × 10-4 eV, and the mass of the delta baryon is 1232 MeV/c2. The minimum energy of the proton must significantly exceed its rest energy of 938.3 MeV, particularly when considering the implications of the Greisen-Zatsepin-Kuzmin (GZK) limit, which is crucial for understanding the energy dynamics in this relativistic collision scenario.

PREREQUISITES
  • Understanding of relativistic energy-momentum equations (E2 - (pc)2 = (mc2)2)
  • Familiarity with the concept of rest mass energy (K = E - mc2)
  • Knowledge of the Greisen-Zatsepin-Kuzmin (GZK) limit and its implications
  • Basic understanding of head-on collision dynamics in particle physics
NEXT STEPS
  • Research the Greisen-Zatsepin-Kuzmin (GZK) limit and its relevance to cosmic ray physics
  • Learn about relativistic collision dynamics and center of momentum frame calculations
  • Explore the implications of Doppler shifting in high-energy photon interactions
  • Study the properties and decay channels of delta baryons (∆+) in particle physics
USEFUL FOR

Physicists, students studying particle physics, and anyone interested in high-energy astrophysics, particularly those exploring cosmic ray interactions and relativistic collisions.

joriarty
Messages
61
Reaction score
0

Homework Statement



Consider the following reaction that is possible when a proton (p+) collides with a photon (γ):
p+ + γ → ∆+.

Suppose that the photon is a cosmic microwave-background (CMB) photon of energy 2.3 × 10−4eV. Calculate the minimum energy that the proton must have for this reaction to take place. m = 1232eV/c2.

Hints:

• The minimum energy will be for a head-on collision. Be careful with the signs of the momenta when doing the calculation.

• The answer is a very large energy, so you will be able to make the approximation that the the proton energy is much bigger than it’s rest energy.

• You might find it interesting to look up Greisen-Zatsepin-Kuzmin limit. (is this relevant?)

Homework Equations



K = E − mc2
E2 −(pc)2 =(mc2)2

The Attempt at a Solution



(See attached table)

I am thinking that because I'm after the minimum energy of the proton for a head on collision, would this mean that the delta baryon is going to have zero kinetic energy and momentum thus a total energy 1232 MeV?

I can then say that the proton has momentum pc = -2.3*10-10MeV. But that just makes the energy of the proton also equal to 938.3 MeV within the precision of my calculator. That's not right, I should get Eproton>>mprotonc2.

Where to now? Does the change in mass of 293.7 MeV have anything to do with this?

Thanks!
 

Attachments

  • table.png
    table.png
    2.8 KB · Views: 521
Physics news on Phys.org
The GZK limit is very relevant, that's what this whole problem is about. The 10^(-4)ev CMB photon energy is it's energy in the 'lab' frame, one at rest with respect to the CMB background. If you consider the collision in the center of momentum frame of a highly energetic proton, the photon will be 'doppler shifted' up to a high enough energy to produce a delta. You want the energy of the proton in the 'lab' frame.
 

Similar threads

  • · Replies 54 ·
2
Replies
54
Views
11K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 8 ·
Replies
8
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 7 ·
Replies
7
Views
2K
Replies
3
Views
2K
Replies
2
Views
2K
Replies
9
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K