Simplifying KE/Momentum Relativistic Problem

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Homework Help Overview

The problem involves a D0 meson decaying into a K0 meson and a \pi0 meson, with the goal of determining the kinetic energy of the \pi0 meson. The context is within relativistic physics, specifically focusing on energy and momentum conservation in particle decay processes.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss various methods to approach the problem, including the use of energy and momentum conservation equations. Some express difficulty with the algebra involved in solving for velocities, while others suggest alternative methods that avoid direct velocity calculations.

Discussion Status

There is ongoing exploration of different approaches to the problem. Some participants have provided guidance on using energy and momentum conservation without needing to solve for velocities directly. One participant has made progress in calculating numerical values for momentum and velocity, indicating a productive direction in the discussion.

Contextual Notes

Participants mention the complexity of the algebra involved and the constraints of time in their attempts to solve the problem. There is also a reference to the potential utility of four-vectors in simplifying the calculations, which some participants had not previously considered in their approach.

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Homework Statement



A D0 meson (with a rest mass of 1.86 GeV/c2), initially at rest, decays into a K0 meson (with a rest mass of .51 GeV/c2) and a \pi0 meson (with a rest mass of .12 GeV/c2). What is the Kinetic Energy of the \pi0 meson?


Homework Equations



E=\gammam0c2

p=\gammam0v

The Attempt at a Solution



Subtracting final rest energy from intial energy its easy to see that the KE(K0+\pi0)=1.23 GeV

Also: \gammaK0mK0c2+\gamma\pi0m\pi0c2 = 1.86 GeV/c^2 (The total energy of the two Mesons must equal the first meson)
Without going through all the horrible steps me and my friend did, eventually we got a equation that solved: VK0=f(V\pi0) (I don't have the final equation we got on me)


When then plugged that back into: \gammaK0mK0c2+\gamma\pi0m\pi0c2 = 1.86 GeV/c^2


Now at this point we had a solvable equation, the only variable was V\pi0, but it was a hellish equation. After about 20 minutes working on trying to solve it we ran out of time and had to give up- the algebra was just to hard.
Had we had enough time, I'm completely confident we could have solved it, as it was simply a matter of foiling again and again (I think we needed to do it three levels down).
My question is: Is there a way of solving this problem without having to go in and solve for one of the variables in terms of the other, or doing that in a simpler equation?

Thank you, especially if you made it through this.
 
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If you don't need the velocities (i.e. you're not asked for them explicitly), don't take that route to find the energies of the outgoing particles. Instead, use

E^2 = (pc)^2 + (m_0 c^2)^2

which is true for each particle, together with conservation of energy and conservation of momentum. You never have to see a single "v".
 
Two suggestions:

1. Stick with energy (total, not kinetic) and momentum.
2. Take advantage of E^2 - (pc)^2 = (mc^2)^2.

If you learn how to use four-vectors, you can get the answer in about three or four lines of simple algebra. Read Griffith's chapter on special relativity in his Introduction to Particle Physics.
 
Thank you to both of you, while I haven't actually gotten the answer yet, I have gotten numerical values for both the momentum and velocity of one of the particles, I'll be able to get the answer with about 5 more minutes of work.

In addition, I know the momentum energy four vector, but I've never been given a problem requiring it so using it didn't occur to me, I am going to look at its usefulness more carefully.
 

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