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What is derivation of the equation of total energy?

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Start with [math]E = {\gamma}mc^2[/math]

 

expand gamma, equating it to the right-hand side of the equation. Multiply through by the denominator

 

[math]{\gamma}m^2c^4-{\gamma}m^2v^2c^2 = m^2c^4[/math]

 

 

move the negative term to the other side and note that

 

[math]{\gamma}^2m^2v^2 = p^2[/math]

 

Left-hand side is E2 and the right-hand side is m2c4+p2c2

Edited by swansont
fix typo

  • Author

Start with [math]E = {\gamma}mc^2[/math]

 

expand gamma, equating it to the right-hand side of the equation. Multiply through by the denominator

 

[math]{\gamma}m^2c^4-{\gamma}m^2v^2c^2 = m^2c^4[/math]

 

 

move the negative term to the other side and note that

 

[math]{\gamma}m^2v^2 = p^2[/math]

 

Left-hand side is E2 and the right-hand side is m2c4+p2c2

I have understood only the start.

I think [math]{\gamma}^2m^2v^2 = p^2[/math]

I had a bad latex day recently so I have sketched the derivation out longhand.

You should have enough to fill in the arithmetic, ask if there are any steps you don't follow.

 

post-74263-0-97080600-1411135751_thumb.jpg

The question must now be where does [math]E = \gamma m c^{2}[/math] come from?

 

Another way to get at the equation you seek is to consider the world line action of a free relativistic particle. Depending on how you formulate this, there are several ways, you see that [math]E^{2}-p^{2}= m^{2}[/math] comes out as an equation of motion.

 

That is all classical physical particles must obey this relation, including massless particles. That why we can talk about on-shell and off-shell in quantum field theory. This means if the classical equations of motion are imposed or not. For example, people will talk about virtual particle being off-shell for exactly this reason; they are not constrained to obey the classical equations of motion.

Edited by ajb

The easiest way would be to use four-vectors. The four-momentum is:

 

[math]p^\mu = (E/c, \vec{p})[/math]

 

This can be found easily by simply defining four-momentum as mass times four-velocity, where four-velocity is the derivative of position [math]x^\mu =(ct,\vec{x})[/math] with respect to proper time. We know that the magnitude of the four-momentum must be constant for every observer:

 

[math]p_\mu p^\mu = const.[/math]

 

If we consider the frame where a particle is at rest, its momentum becomes:

 

[math]p^\mu = (E/c,0)[/math]

 

But when a particle is at rest its energy is just its rest energy, which is equal to its mass:

 

[math]p^\mu = (mc,0)[/math]

 

Its magnitude squared is:

 

[math]p_\mu p^\mu = m^2 c^2[/math]

 

In some other general reference frame we have:

 

[math]p_\mu p^\mu = E^2/c^2 - |\vec{p}|^2[/math]

 

But as I said these must be equal, so:

 

[math]E^2/c^2 - |\vec{p}|^2= m^2 c^2[/math]

 

You can do a little rearranging to get it into the more familiar form:

 

[math]E^2 = m^2 c^4 + |\vec{p}|^2 c^2[/math]

Edited by elfmotat

  • Author

you see that [math]E^{2}-p^{2}= m^{2}[/math] comes out as an equation of motion.

 

I see different units, how can they work in the equation?

kg2m4/s4 - kg2m2/s2 = kg2

I see different units, how can they work in the equation?

kg2m4/s4 - kg2m2/s2 = kg2

Try again , with this:

 

[math]E^2-(pc)^2=(mc^2)^2[/math]

 

It is standard practice to set c=1.

Indeed, for notational simplicity I set c = 1. It is very common to do this, but it can be confusing especially if you want to view c as a parameter that sets some scales in the theory.

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