Should we use relativistic corrections for particles?

In summary, relativistic corrections are used to calculate the final velocity of an electron accelerating out of an electron gun. The equation for conservation of energy is modified to account for the relativistic mass of the particle, and the final velocity is found to be slightly higher than without the relativistic correction.
  • #1
pattiecake
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Does anyone know if we should use relativistic corrections for particles? Say an electron accelerating out of an electron gun at 2000V. How would you calculate the final velocity?
 
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  • #2
Does anyone know if we should use relativistic corrections for particles? Say an electron accelerating out of an electron gun at 2000V. How would you calculate the final velocity?

Classically the change in kinetic energy [tex]m_ev^2 [/tex] will equal the change in potential energy [tex]q_e V [/tex]. This yields [tex] v=\sqrt{\frac{q_e V}{m_e}[/tex]. With V=2000V, v=0,06256c. If you're only interested in a rough estimate you're done, but a refinement can be made treating the problem relativistically.

Relativistically conservation of energy involves the potential energy [tex]q_e V [/tex] and total relativistic energy: [tex] \frac{m_e c^2}{\sqrt{1-v^2/c^2}} [/tex]. Letting the sum of these energies be the same before and after the acceleration of the electron yields:

[tex]q_e V+m_e c^2=0+\frac{m_e c^2}{\sqrt{1-v^2/c^2}} [/tex]
[tex]\frac{q_eV}{m_e c^2}=1-\frac{1}{\sqrt{1-v^2/c^}} [/tex]

Which you can solve for [tex]v[/tex]. Often it is easier to use the relationship between relativistic momentum [tex]p=\frac{mv}{\sqrt{1-v^2/c^2}}[/tex] and energy:

[tex]E^2=c^2p^2 + m^2c^4[/tex]

With [tex]E=q_e V+m_e c^2[/tex] this makes:

[tex] \sqrt{\frac{(q_e V+m_e c^2)^2}{c^2} -(m_e)^2 c^2} = p = \frac{m_e v}{\sqrt{1-v^2/c^2}}[/tex]

Filling in numbers you get a final velocity of v=0,088216c
 
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  • #3
neat! Thanks! :smile:
 
  • #4
da willem,
did you get a HIGHER velocity with the relativistic correction?
 
  • #5
ehm, yes. This can't be right... I'll check it later...
 
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  • #6
pattiecake said:
Does anyone know if we should use relativistic corrections for particles?

As da_willem said, yes. In the present case conservation of energy is given by

Kinetic energy + potential energy = K + V = constant

When this equation is derived it is assumed that the proper mass (aka "rest mass") of the particle is constant. Let me be the proper mass of the electron (which obviously doesn't change). This gives, upon substitution of [tex]K = (\gamma - 1)m_ec^2[/tex]

[tex]K + V = (\gamma - 1)m_ec^2 + V = constant[/tex]

where V is the potential energy (I use "V" to mean something different than da_willem).

This can be written as

[tex] \gamma_{1} m_ec^2 - m_ec^2 + V(\mathbf{r}_1) = \gamma_{2} m_ec^2 - m_ec^2 + V(\mathbf{r}_2)[/tex]

Canceling the common factor gives

[tex] \gamma_{1} m_ec^2 + V(\mathbf{r}_1) = \gamma_{2} m_ec^2 + V(\mathbf{r}_2) = constant[/tex]

The potential energy V is related to the Coulomb potential [tex]\Phi[/tex] as

[tex]V = q_e\Phi[/tex]

Thus

[tex] \gamma_{1} m_ec^2 + q_e\Phi(\mathbf{r}_1) = \gamma_{2} m_ec^2 + q_e\Phi(\mathbf{r}_2)[/tex]

Another way to simplify is to define the quantity E = K + E0. Then

[tex] E = K + E_0 = (\gamma - 1)m_ec^2 + m_ec^2 = \gamma m_ec^2 = mc^2[/tex]

where [tex] m = \gamma m_ec^2[/tex] is the (relativistic) mass of the electron. This gives

[tex] E + V = mc^2 + V = mc^2 + q\Phi = \gamma m_ec^2 + q_e\Phi = constant[/tex]

as given above. The Lagrangian formulation may also be used to obtain a constant of motion known as Jacobi's integral since its an "integral of motion", aka a constant of motion. For the derivation see

http://www.geocities.com/physics_world/sr/relativistic_energy.htm

What value you get for Jacobi's integral depends on an arbitrary constant that you add to the Lagrangian.

See also -- http://www.geocities.com/physics_world/sr/work_energy.htm
 
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What are relativistic corrections?

Relativistic corrections are adjustments made to classical theories, such as Newtonian mechanics, to account for the effects of high speeds or strong gravitational fields predicted by Einstein's theory of relativity. These corrections are necessary to accurately describe and predict the behavior of objects moving at close to the speed of light.

Why are relativistic corrections important?

Relativistic corrections are important because they allow us to accurately describe the behavior of objects moving at high speeds or in strong gravitational fields. Without these corrections, our predictions would be significantly off and our understanding of the universe would be incomplete.

What is the difference between special and general relativistic corrections?

Special relativistic corrections apply to objects moving at constant speeds in the absence of gravitational forces, while general relativistic corrections apply to objects moving in the presence of strong gravitational fields. Special relativity deals with the effects of relative motion, while general relativity deals with the effects of gravity on spacetime.

How do relativistic corrections affect our understanding of time and space?

Relativistic corrections have shown us that time and space are not absolute, but are relative to the observer's frame of reference. This means that the passage of time and the measurement of distances can vary depending on the speed and gravitational field of the observer. It also leads to concepts such as time dilation and length contraction.

What are some practical applications of relativistic corrections?

Relativistic corrections have many practical applications, such as in GPS technology, particle accelerators, and space travel. Without these corrections, these technologies would not function properly. Relativistic corrections also play a crucial role in nuclear physics and cosmology, helping us understand the behavior of particles and the evolution of the universe.

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