phyzguy said:
The formula KE = p^2/(2m) and TE = p^2/(2m) + mc^2 are non-relativistic approximations, and are only valid when pc << mc^2. They come about from taking the full relativistic equation and expanding the square root, keeping only the leading term, as follows:
[tex]mc^2 \sqrt{1+\frac{p^2 c^2}{m^2 c^4}}[/tex]
[tex]E \approx mc^2 (1+\frac{p^2 c^2}{2m^2 c^4})[/tex]
How does this make any sense at all? ignoring the square root and adding a 2 to the denominator?
When I expand the square root of (1+ε) in a Taylor series and keep only the first order term, I get:
[tex]\sqrt{1+\epsilon} \approx 1+\frac{\epsilon}{2}[/tex]
For example: [tex]\sqrt{1.01} = 1.004987 \ldots \approx 1.005[/tex]
One more comment. You need to have some of these more common approximations at your fingertips in order to do physics. Some of the most important are:
[tex]\sqrt{1+\epsilon} \approx 1+\frac{\epsilon}{2}[/tex]
[tex]\frac{1}{1+\epsilon} \approx 1-\epsilon[/tex]
[tex]sin(\epsilon) \approx \epsilon[/tex]
[tex]tan(\epsilon) \approx \epsilon[/tex]
[tex]cos(\epsilon) \approx 1+\frac{\epsilon^2}{2}[/tex]
[tex]ln(1+\epsilon) \approx \epsilon[/tex]