Special Relativity collision problem

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SUMMARY

The discussion focuses on solving a collision problem in special relativity involving a photon of energy E_0 colliding with a stationary particle of mass m_0. The key equations utilized are the conservation of energy, E_0 = E_s + m_0c^2γ, and the conservation of momentum in both x and y directions. A more efficient approach is suggested, avoiding the introduction of γ, by using the equation E^2 = m^2c^4 + p^2c^2 for energy conservation. This method leads to three simultaneous equations that can be solved to find the scattering angle β of the particle.

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  • Understanding of special relativity concepts, particularly energy and momentum conservation.
  • Familiarity with the relationship between energy, momentum, and mass in relativistic physics.
  • Knowledge of trigonometric identities, specifically the tangent function.
  • Ability to solve simultaneous equations in physics problems.
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  • Study the derivation and application of the energy-momentum relation E^2 = m^2c^4 + p^2c^2.
  • Learn how to apply conservation laws in relativistic collisions.
  • Practice solving simultaneous equations in the context of physics problems.
  • Explore alternative methods for simplifying complex algebraic expressions in physics.
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Students and educators in physics, particularly those focusing on special relativity and particle collisions, as well as anyone looking to enhance their problem-solving techniques in advanced physics scenarios.

subsonicman
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Homework Statement


A photon of Energy E_0 collides with a free particle of mass m_0 at rest. If the scattered photon flies off at angle θ, what is the scattering angle of the particle, β?


Homework Equations


The relevant equations are conservation of momentum in x and y direction and conservation of energy.

Conservation of energy:
E_0=E_s+m_0c^2γ

Conservation of momentum:
x direction: E_0/c=E_s*cosθ/c+m_0vγ*cosβ
y direction: E_s*sinθ=m_0vγ*sinβ

The Attempt at a Solution


Of course I need to first get rid of E_s and v (which is also inside of γ) and then solve for β. So first I get rid of E_s by plugging in E_0-m_0c^2γ in the two momentum equations. Then I solve for v in the y direction momentum equation. When I plug it in I get this ridiculous quadratic equation that, while it can be solved, becomes even more ridiculous when I plug it into the x direction momentum equation. And I can't solve it.

I was wondering if possibly there is some nicer way to solve this problem, possibly with better substitutions at the start or some other technique I'm not seeing. Anyways, thanks in advance!
 
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subsonicman said:

Homework Statement


A photon of Energy E_0 collides with a free particle of mass m_0 at rest. If the scattered photon flies off at angle θ, what is the scattering angle of the particle, β?


Homework Equations


The relevant equations are conservation of momentum in x and y direction and conservation of energy.

Conservation of energy:
E_0=E_s+m_0c^2γ

Conservation of momentum:
x direction: E_0/c=E_s*cosθ/c+m_0vγ*cosβ
y direction: E_s*sinθ=m_0vγ*sinβ

The Attempt at a Solution


Of course I need to first get rid of E_s and v (which is also inside of γ) and then solve for β. So first I get rid of E_s by plugging in E_0-m_0c^2γ in the two momentum equations. Then I solve for v in the y direction momentum equation. When I plug it in I get this ridiculous quadratic equation that, while it can be solved, becomes even more ridiculous when I plug it into the x direction momentum equation. And I can't solve it.

I was wondering if possibly there is some nicer way to solve this problem, possibly with better substitutions at the start or some other technique I'm not seeing. Anyways, thanks in advance!

It's still a pretty ugly result (well, it's not pretty), but I don't get a quadratic. Here's how I did it:

I generally prefer not to introduce ##\gamma## into these problems because it complicates the algebra. Instead, I use ##E^2 = m^2c^4 + p^2c^2## for the energy conservation. Remember that this E represents the sum of the rest-mass energy plus the kinetic energy of a body. For a photon, it simply reduces to E = pc. Rewrite the photon momenta immediately in terms of energy.

You should get 3 simultaneous equations when you write down the conservation statements for energy, horiz. momentum and vert. momentum. There are three unknowns: ##E'##, the energy of the photon post-collision, ##p##, the momentum of the particle post-collision and ##\beta##, what you need to solve for. I first solved for ##E'## in terms of the givens using the energy conservation equation, then substituted that into the equations for momentum conservation. A simple division of one equation over another should now give you the answer, if you remember that ##\frac{\sin \beta}{\cos \beta} = \tan \beta##.
 

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