High school algebra -> relativistic conservation of momentum and energy

In summary, the relativistic conservation of momentum and energy states that if a massless photon (momentum po and energy Eo) collides with a stationary free electron, p=po and E=Eo.
  • #1
forrealfyziks
13
0
"high school" algebra -> relativistic conservation of momentum and energy

Homework Statement


Consider a head-on, elastic collision between a massless photon (momentum po and energy Eo) and a stationary free electron. (a) Assuming that the photon bounces directly back with momentum p (in the direction of -po) and energy E, use conservation of energy and momentum to find p.


Homework Equations


E=[tex]\gamma[/tex]mc2
p=[tex]\gamma[/tex]mu
massless: E=pc
rest mass: E=mc2
E2=(pc)2+(mc2)2
v/c=pc/E
[tex]\gamma[/tex]=1/[tex]\sqrt{1+(v/c)^2}[/tex]

The Attempt at a Solution


Note:First of all I know that this is relativity, but it boils down to just plain algebra. I can't figure it out and help is hard to find, so if you can help I would really appreciate it.

I assume that p is the momentum of the electron. m=mass of the electron u=velocity of the electron c=speed of light

conserving energy: poc+mc2=pc+[tex]\gamma[/tex]mc2
po+mc=p+[tex]\gamma[/tex]mc
po=p+[tex]\gamma[/tex]mc-mc

conserving momentum: po=p-p=[tex]\gamma[/tex]mu-p

Plugging the result I got in conserving energy into the momentum equation:
p-p=p+[tex]\gamma[/tex]mc-mc
p=2p+mc([tex]\gamma[/tex]-1)
 
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  • #2


Generally, it's a good idea when solving these types of problems to avoid using [itex]\gamma[/itex] and velocities if you can avoid them. Work with energy, momentum, and mass instead. Doing so usually makes the algebra simpler.

I think your best approach is to solve for the electron's energy. Once you have that, you can calculate its momentum. You can rewrite your equations as follows:

[tex]p_0 c - p c = E_e - m c^2[/tex]
[tex]p_0 + p = p_e[/tex]

Multiply the second equation by c, square both equations, then subtract the second one from the first, and use the relation [itex]E^2 - (pc)^2 = (mc^2)^2[/itex] to simplify what you get. Figure out how to eliminate p from the equation and solve for [itex]E_e[/itex].
 
  • #3


Thank you for the hints it has really helped. I worked through the things vela posted, and found myself stuck again, though.

If I add the two equations, I end up with (po2c2+p2c2)=Ee2-Eemc2

If I subtract the second from the first
-2ppoc2=-Eemc2+(mc2)2

On the first one, it obviously has the momentums on the left, and on the second one I also have momentums on the left.

With the first one the left almost looks like one of the conservations, but not quite. I'm going to fiddle around with the information vela has already given me and see if I can't find another way.
 
  • #4


It wasn't clear in your original post what terms are allowed in the final answer. I assume you want to get rid of p, the photon's final momentum. You can do that by solving for it in one of the conservation equations in terms of the other variables.
 
  • #5


I think I'm supposed to find p numerically, because the second part of the question asks you to verify your answer in part a using Compton's formula where [tex]\Theta[/tex]=[tex]\pi[/tex].
 
  • #6


I found out from a peer that the momentum you are finding is actually the photon's second momentum, and that you should solve in terms of po. It became incredibly easy once I knew I wasn't looking for something numerical... Thank you so much for your help!
 
  • #7


Oh! When they asked you to find p, they were probably referring to the momentum of the recoiling photon, not the electron's. What you want to do is get rid of [itex]E_e[/itex] from your answer.
 
  • #8


yes it was supposed to be photon's new momentum. Guess I should have put that second part of the question in, but I didn't think it was necessary. Going back over the derivation of Compton's formula, I noticed it was almost the exact thing I was doing. heh, well thanks again.
 

Related to High school algebra -> relativistic conservation of momentum and energy

What is high school algebra?

High school algebra is a branch of mathematics that focuses on the manipulation of symbols and solving equations using basic operations such as addition, subtraction, multiplication, division, and exponentiation.

What is relativistic conservation of momentum and energy?

Relativistic conservation of momentum and energy is a principle in physics that states that the total momentum and energy of a system remains constant in a relativistic framework, where the speed of objects is close to the speed of light.

Why is it important to understand both high school algebra and relativistic conservation of momentum and energy?

High school algebra provides the foundation for understanding and solving complex equations, which is necessary for grasping the concepts of relativistic conservation of momentum and energy. Understanding these concepts is important for accurately predicting the behavior of objects in high-speed situations, such as particle collisions.

What are some real-world applications of high school algebra and relativistic conservation of momentum and energy?

High school algebra is used in a variety of fields, such as engineering, economics, and science, to solve equations and make predictions. Relativistic conservation of momentum and energy is essential in fields such as particle physics, astrophysics, and nuclear energy, where high speeds and energies are involved.

How can I improve my understanding of high school algebra and relativistic conservation of momentum and energy?

To improve your understanding of high school algebra, practice solving equations and seek help from teachers or tutors if needed. To understand relativistic conservation of momentum and energy, study the principles and equations involved, and apply them to real-world problems. Additionally, staying updated on new developments in the field can also enhance your understanding.

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