Calculating Energy and Time for a Proton Crossing the Milky Way Galaxy

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SUMMARY

The discussion focuses on calculating the energy and time required for a proton to cross the Milky Way galaxy, which is approximately 100,000 light-years in diameter. The mass of the proton is given as 1.6726 x 10-27 kg, and the energy is calculated using the equation E = γmc2, where γ is the Lorentz factor. The time dilation effect is also considered, with the time taken in the galaxy's reference frame being T = γX 5 min. The estimated energy of the proton is on the order of 103 joules, equivalent to approximately 931 MeV.

PREREQUISITES
  • Understanding of special relativity concepts, particularly time dilation and Lorentz factor.
  • Familiarity with energy-momentum equations, specifically E = γmc2.
  • Basic knowledge of particle physics, including the mass-energy equivalence.
  • Ability to convert units, particularly between joules and electronvolts (eV).
NEXT STEPS
  • Study the derivation and application of the Lorentz factor (γ) in special relativity.
  • Learn how to apply the time dilation equation in various reference frames.
  • Explore the relationship between energy and momentum in relativistic physics.
  • Investigate the conversion of energy units from joules to electronvolts (eV) for particle physics applications.
USEFUL FOR

This discussion is beneficial for physics students, particularly those studying special relativity and particle physics, as well as educators seeking to explain the concepts of energy and time in relativistic contexts.

jk4

Homework Statement


In its own frame of reference, a proton takes 5 min to cross the Milky Way galaxy, which is about [tex]10^{5}[/tex] light-years in diameter.
(a) What is the approximate energy of the proton in electronvolts?
(b) About how long would the proton take to cross the galaxy as measured by an observer in the galaxy's reference frame?

mass of proton = [tex]1.6726 x 10^{-27} kg[/tex]
[tex]1eV = 1.602 x 10^{-19} J*s[/tex]

Homework Equations


It says the problem belongs to the "Energy and Momentum" section, so here are those equations:
[tex]E = \gamma mc^{2}[/tex]
[tex]p = \gamma mv[/tex]
[tex]E^{2} = (mc^{2})^{2} + p^{2}c^{2}[/tex]
[tex]E = pc[/tex] (Massless particle, probably doesn't apply to this problem)

The Attempt at a Solution


well, I'm pretty confused. I calculated that the distance of [tex]10^{5}[/tex] light-years corresponds to about [tex]9.45 x 10^{15} m[/tex]. But I can't figure out how to proceed from here.
I'm not necessarily looking for an answer but a little help.
 
Last edited by a moderator:
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I'm no expert so take this with a grain of salt.
Write down the time dilation equation. Then use
[tex]v={L\over \Delta t^'}[/tex] i.e. proper length divided time observed by a stationary observer in the Milky way.
Putting these together you can get the speed. The rest is gravy.
As a guide, I get the order of 10^3 in joules for the energy. That sucker is flyin.

Good luck.
 
Last edited:
The galaxies velocity in the proton's rest frame is
v/c=(L/5 min)/gamma (a dimensionless number).
Use this equation to find gamma. Be careful with the numbers
The proton's energy is E=\gamma mc^2. Use mc^2=931 MeV for a proton.
The time to cross the galaxy in its rest frame is T=gamma X 5 min.
 

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