Relativistic Momentum: Deriving Why p=mγv

In summary, according to special relativity, relativistic momentum is defined as ##p=\gamma mv##. This is because after collision, coordinate system and observer in its origin move with ##u=v## from left to right at all times. This is why after collision, observer in ##xy## would say that balls don't move in ##x## direction, while observer in ##x'y'## would state, that they both move in opposite direction.
  • #1
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I have been trying to derive why relativistic momentum is defined as ##p=\gamma mv##.

I set up a collision between 2 same balls (##m_1 = m_2 = m##). Before the collision these two balls travel one towards another in ##x## direction with velocities ##{v_1}_x = (-{v_2}_x) = v##. After the collision these two balls travel away from each other with velocity ##{v_1}_y = (-{v_2}_y) = v##. Coordinate system travels from left to right with velocity ##u=v## at all times (after and before collision).

Please see the pictures below where picture (a) shows situation before collision and picture (b) after collision.

http://shrani.si/f/2A/m3/4kDXDQo1/momentum.png

Below is a proof that Newtonian momentum ##mv## is not preserved in coordinate system ##x'y'##. I used ##[\, | \,]## to split ##x## and ##y## components. ##p_z'## is momentum before collision where ##p_k'## is momentum after collision.

[itex]
\scriptsize
\begin{split}
p_z' &= \left[ m_1 {v_1}_x' + m_2 {v_2}_x'\, \biggl| \, 0 \right] = \left[ m_1 0 + m_2 \left( \frac{{v_2}_x - u}{1-{v_2}_x\frac{u}{c^2}} \right)\, \biggl| \, 0 \right]= \left[ m \left( \frac{-v - v}{1+ v \frac{v}{c^2}} \right) \, \biggl| \, 0 \right] \\
p_z' &= \left[ - 2mv \left( \frac{1}{1+ \frac{v^2}{c^2}}\right) \, \biggl| \, 0 \right]
\end{split}
[/itex]

[itex]
\scriptsize
\begin{split}
p_k' &= \left[-2mv \, \biggl| \,m_1 {v_1}_y' + m_2 {v_2}_y'\right]=\left[ -2mv \, \biggl| \, m_1 \left( \frac{{v_1}_y}{\gamma \left(1 - {v_1}_y \frac{u}{c^2}\right)} \right) + m_2 \left( \frac{{v_2}_y}{\gamma \left(1 - {v_2}_y \frac{u}{c^2}\right)} \right) \right]\\
p_k' &= \left[ -2mv \, \biggl| \, m \left( \frac{v}{\gamma \left(1 - v \frac{v}{c^2}\right)} \right) - m \left( \frac{v}{\gamma \left(1 - v \frac{v}{c^2}\right)} \right)\right]\\
p_k' &= \left[ -2mv \, \biggl| \, 0 \right]
\end{split}
[/itex]

It is clear that ##x## components differ by factor ##1/\left(1+\frac{v^2}{c^2}\right)##.

QUESTION: I want to know why do we multiply Newtonian momentum ##p=mv## by factor ##\gamma = 1/ \sqrt{1 - \frac{v^2}{c^2}}## and where is the connection between ##\gamma## and factor ##1/\left(1+\frac{v^2}{c^2}\right)## which i got?

FURTHER EXPLAINATION:
In the proof above I used velocity transformations derived below (derivation is taken from here):

[itex]
v_x' = \frac{dx'}{dt'}=\frac{\gamma (d x - u d t)}{\gamma \left(d t - d x \frac{u}{c^2} \right)} = \frac{d x - u d t}{d t - d x \frac{u}{c^2}} = \frac{\frac{d x}{d t} - u \frac{d t}{d t}}{\frac{d t}{d t} - \frac{d x}{d t} \frac{u}{c^2}} \Longrightarrow \boxed{v_x' = \frac{v_x - u}{1- v_x \frac{u}{c^2}}}
[/itex]


[itex]
v_y' = \frac{dy'}{dt'}=\frac{d y}{\gamma \left(d t - d x \frac{u}{c^2} \right)} = \frac{\frac{dy}{dt}}{\gamma \left(\frac{dt}{dt} - \frac{dx}{dt} \frac{u}{c^2} \right)} \Longrightarrow \boxed{v_y' = \frac{v_y}{\gamma \left(1 - v_x \frac{u}{c^2} \right)}}
[/itex]
 
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  • #2
Look carefully at the x component of the momentum in the first expression in the first line of your derivation of [itex]p_k^{'}[/itex]
 
  • #3
Nugatory said:
Look carefully at the x component of the momentum in the first expression in the first line of your derivation of [itex]p_k^{'}[/itex]

You mean this expression?

[itex]
p_k' = \left[ -2mv\, \biggl| \, m_1 {v_1}_y + m_2 {v_2}_y \right]
[/itex]

Coordinate system and observer in its origin move with ##u=v## from left to right at all times. This is why after collision observer in ##xy## would say that balls don't move in ##x## direction, while observer in ##x'y'## would state, that they both move in opposite direction. This is where i got my ##x## component ##m_1 {v_1}_x' + m_2 {v_2}_x' = m (-v) + m(-v) = -2mv##.
 
Last edited:

Related to Relativistic Momentum: Deriving Why p=mγv

1. What is Relativistic Momentum?

Relativistic momentum is a concept in physics that describes the momentum of an object moving at a high speed, close to the speed of light. It takes into account the effects of special relativity, which states that the laws of physics are the same for all observers in uniform motion.

2. How is Relativistic Momentum calculated?

The formula for relativistic momentum is p = mγv, where p is momentum, m is mass, γ is the Lorentz factor, and v is velocity. The Lorentz factor takes into account the effects of time dilation and length contraction at high speeds. It is calculated as γ = 1/√(1-(v/c)^2), where c is the speed of light.

3. What is the significance of Relativistic Momentum?

Relativistic momentum is significant because it allows us to accurately describe the behavior of objects moving at high speeds. The classical formula for momentum, p = mv, does not take into account the effects of special relativity. As an object approaches the speed of light, its relativistic momentum becomes increasingly important.

4. How does Relativistic Momentum differ from Classical Momentum?

Classical momentum is based on the laws of classical mechanics, which do not take into account the effects of special relativity. As a result, the classical formula for momentum, p = mv, is only accurate for objects moving at low speeds. Relativistic momentum, on the other hand, takes into account the effects of special relativity and is accurate for objects moving at any speed, including speeds close to the speed of light.

5. What are some real-world applications of Relativistic Momentum?

Relativistic momentum has many practical applications, including in particle accelerators, nuclear reactors, and space travel. It is also used in the development of high-speed transportation systems, such as maglev trains. Relativistic momentum is essential for accurately predicting the behavior of objects at high speeds and is crucial for advancing our understanding of the universe.

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