Invariant mass and energy balance

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SUMMARY

The discussion focuses on calculating the invariant mass of a two-particle system involving a proton and a photon from the Cosmic Microwave Background (CMB). The invariant mass is expressed in terms of the energies and momenta of the particles, specifically using the equation $$ M_{inv}^2 c^4 = m_p^2 c^4 + 2k_B T_{CMB} (E + cp) $$. The participants derive the energy of the CMB photon and explore the relationship between the proton's energy and the invariant mass, ultimately leading to the expression $$ E= \frac {m_∆^2 c^4−m_p^2 c^4} {4k_BT_{CMB}}+δE $$, where δE is determined through algebraic manipulation. The discussion highlights the importance of Lorentz transformations and conservation laws in special relativity.

PREREQUISITES
  • Understanding of invariant mass in special relativity
  • Familiarity with Lorentz transformations
  • Knowledge of conservation of energy and momentum
  • Basic proficiency in algebraic manipulation of equations
NEXT STEPS
  • Study the derivation of invariant mass in particle collisions
  • Learn about the implications of Lorentz transformations in high-energy physics
  • Explore the role of the Cosmic Microwave Background in astrophysics
  • Investigate advanced topics in particle physics related to energy-momentum relations
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Students and professionals in physics, particularly those studying special relativity, particle physics, and astrophysics, will benefit from this discussion.

R3ap3r42
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Homework Statement
This is a question from a Special Relativity course. Uses invariant mass, Laurentz Transformation
Relevant Equations
Invariant mass, Lorentz Transformation, Conservation of Energy, Conservation of Momentum
a) Two particles have energies E1 and E2, and momenta p1 and p2. Write down an expression for the invariant mass of this two-particle system. Leave your answer in terms of E1 and E2, and p1 and p2.

b) A typical photon (γ) in the Cosmic Microwave Background (CMB) has an energy of kBTCMB, where TCMB = 2.73 K and kB is the Boltzmann constant. Such a photon can collide with a high-energy proton via the reaction p + γ → ∆+, where the ∆+ particle has a mass of 1.23 GeV/c2 .

i) Calculate the energy of the CMB photon in eV. [2 marks]

ii) If the proton and photon collide head-on, show that their invariant mass, $$ M_{inv} $$, satisfies

$$ M_{inv}^2 c^4 = m_p^2 c^4 + 2k_B T_{CMB} (E + cp) $$

where E, p and mp are the proton’s energy, momentum and mass. [4 marks] Hence show that the proton energy can be written

$$ E= \frac {m_∆^2 c^4−m_p^2 c^4} {4k_BT_{CMB}}+δE $$ and determine δE in terms of the particle masses and the photon energy.

iii) Compute the numerical values of δE and E in eV. [2 marks] iv) How would your expression for the proton energy change if the photon and proton collided at right angles?I got all the way to b) ii but I could not get to the given expression for E.
Can anyone point give me any clues? I am pretty sure it's just algebraic work that I can seem to simplify.

I manage to get to this:

$$ E= \frac {m_∆^2 c^4−m_p^2 c^4} {2k_BT_{CMB}} - cp $$

This seems close but I can't get rid of the cp (also note that mine is divided by 2 not 4 as expected).

Thanks a lot.
 
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R3ap3r42 said:
Homework Statement:: This is a question from a Special Relativity course. Uses invariant mass, Laurentz Transformation
Relevant Equations:: Invariant mass, Lorentz Transformation, Conservation of Energy, Conservation of Momentum

I got all the way to b) ii but I could not get to the given expression for E.
Show your work please.
 
1642958354075.png


Hope it is clear enough.
 
R3ap3r42 said:
I manage to get to this:

$$ E= \frac {m_∆^2 c^4−m_p^2 c^4} {2k_BT_{CMB}} - cp $$

This seems close but I can't get rid of the cp (also note that mine is divided by 2 not 4 as expected).

Thanks a lot.
You're missing the same trick I showed you yesterday. You have:
$$E + pc = X \ \ (1)$$where$$X = \frac {m_∆^2 c^4−m_p^2 c^4} {2k_BT_{CMB}}$$Now$$m_p^2c^4 = E^2 - p^2c^2 = (E-pc)(E+pc) = (E-pc)X$$$$\Rightarrow \ E - pc = \frac{m_p^2c^4}{X} \ \ (2)$$Now, add equations (1) and (2).
 
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Wow! This is unbelievable. I was blind and now I see. :)
I guess a need to do 100 more of these.

Thanks a lot!
 

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