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Physics 10 Online
OpenStudy (anonymous):

Determine the ratio of the relativistic to the non relativistic kinetic energy when V=1.5x10^-3 m/s and when V = 0.97 m/s. I have tried it three times and for some reason my answer is always zero

OpenStudy (anonymous):

\[KE _{rel}=mc ^{2}(\gamma-1)\] \[KE _{nonrel}=\frac{ 1 }{ 2 }mV ^{2}\]

OpenStudy (astrophysics):

Looks like fun, can you show your work please?

OpenStudy (astrophysics):

\[\gamma = \frac{ 1 }{ \sqrt{1-\left( \frac{ v }{ c } \right)}^2 }\] just to note the Lorentz factor

OpenStudy (anonymous):

Sure

OpenStudy (astrophysics):

It's probably best if you do the calculations separately

OpenStudy (astrophysics):

\[KE_{rel} = mc^2\left( \frac{ 1 }{ \sqrt{1-\left( \frac{ v }{ c } \right)^2} }-1 \right)\]

OpenStudy (astrophysics):

You should find what fraction of the speed of light the given velocities are and then you can find the ratio.

OpenStudy (astrophysics):

So \[1.5 \times 10^{-3} m/s = \frac{ 1 }{ 450,000 } c \]

OpenStudy (astrophysics):

\[\gamma = \frac{ 1 }{ \sqrt{1-\left( \frac{ (1/450,000)c)^2 }{ c^2 } \right)} }\]

OpenStudy (astrophysics):

The reason you're getting 0 is, when you subtract by 1 using a calculator it's approximating to 1 as the numbers are so small, we get something insane such as 0.9999999...

OpenStudy (michele_laino):

for small velocities (v<<c), we can write this (using Taylor expansion): \[\Large E = \gamma m{c^2} \cong m{c^2}\left( {1 + \frac{{{v^2}}}{{2{c^2}}}} \right) = m{c^2} + m\frac{{{v^2}}}{2}\] so we can write: \[\Large K{E_{rel}} = \gamma m{c^2} - m{c^2} \cong m\frac{{{v^2}}}{2} = K{E_{not\;rel}}\] so, in the case v << c, your ratio is equal to 1

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