Tag: problem set

  • Simple problems on relativistic energy and momentum

    Simple problems on relativistic energy and momentum


    We will focus on a few simple problems where we will manipulate the equations for relativistic energy and momentum.

    This could be seen as a second-year university-level post.


    Einstein had shown that the Lorentz transformations were the correct way to switch between the coordinate systems of different frames of reference [1]. He also taught us that Newton’s laws weren’t at all proper relativistic laws. For instance, Newtonian momentum $ \mathbf{p} = m \mathbf{v} $, and energy $ E = mv^2 / 2 $ were not at all accurate at speeds approaching that of light.

    Instead, we have all come to learn that the relativistic momentum is written as

    \begin{equation} \label{eq:relativistic momentum} \mathbf{p} = \frac{m \mathbf{v}}{\sqrt{1 – \dfrac{v^2}{c^2}}}. \end{equation}

    And that the correct relativistic expression for total energy is

    \begin{equation} \label{eq:relativistic energy} E_{\text{tot}} = \frac{mc^2}{\sqrt{1 – \dfrac{v^2}{c^2}}}. \end{equation}

    We will solve the following problem set:

    1. Prove, for a particle travelling at $ c $, that the magnitude of the relativistic energy is given by $ E = pc $.
    2. Show that the energy-momentum relation for a particle with any mass $ m $ travelling at any speed $ v $ is correct and do mind it is not the famous $ E = mc^2 $ we are referring to. Use the correct one, if you please.
    3. Given that the mass of a proton is $ m_p $, calculate its exact speed when its relativistic  translational kinetic energy (which is the relativistic total energy minus its relativistic mass energy) is four times its relativistic mass energy.

    Problem I

    Since $ E $ is expressed in terms of $ p $, we need to rewrite Eq. $ \eqref{eq:relativistic momentum} $ by solving for $ m $:

    \[ m = \frac{p \sqrt{1 – \dfrac{v^2}{c^2}}}{v}. \]

    Note, we do not use the vector quantities, just the magnitudes. We can now proceed to substitute this into Eq. $ \eqref{eq:relativistic energy} $:

    \[ E_{\text{tot}} = \frac{\left(\dfrac{p \sqrt{1 – \dfrac{v^2}{c^2}}}{v}\right)c^2}{\sqrt{1-\dfrac{v^2}{c^2}}}. \]

    This reduces to

    \begin{align}
    E_{\text{tot}} &= \frac{pc^2 \sqrt{1 – \dfrac{v^2}{c^2}}}{v \sqrt{1 – \dfrac{v^2}{c^2}}}, \\
    \therefore E_{\text{tot}} &= \frac{pc^2}{v}. \label{eq:E=pc^2/v}
    \end{align}

    As we are dealing with a particle travelling at speed $ c $, we know $ v = c $, rendering Eq. $ \eqref{eq:E=pc^2/v} $ to

    \begin{align}
    E_{\text{tot}} &= \frac{pc^2}{c}, \\
    \therefore E_{\text{tot}} &= pc.
    \end{align}

    Problem II

    The energy-momentum relation is

    \[ E^2_{\text{tot}} = p^2c^2 + m^2c^4. \]

    Substituting Eqs. $ \eqref{eq:relativistic momentum} $ and $ \eqref{eq:relativistic energy} $, yields

    \[ \left(\frac{mc^2}{\sqrt{1 – \dfrac{v^2}{c^2}}}\right)^2 = \left(\frac{m \mathbf{v}}{\sqrt{1 – \dfrac{v^2}{c^2}}}\right)^2c^2 + m^2c^4, \]

    which we can continue to work out as follows:

    \begin{align*}\left(\frac{mc^2}{\sqrt{1 – \dfrac{v^2}{c^2}}}\right)^2 – \left(\frac{m \mathbf{v}}{\sqrt{1 – \dfrac{v^2}{c^2}}}\right)^2c^2 – m^2c^4 &= 0, \\
    \frac{m^2c^4}{1 – \dfrac{v^2}{c^2}} – \frac{m^2v^2c^2}{1 – \dfrac{v^2}{c^2}} – m^2c^4 &= 0, \\
    \left(1-\dfrac{v^2}{c^2}\right)\left(\frac{m^2c^4}{1-\dfrac{v^2}{c^2}}\right) \qquad &\qquad \\ – \left(1-\dfrac{v^2}{c^2}\right)\left(\frac{m^2v^2c^2}{1-\dfrac{v^2}{c^2}}\right) &\qquad \\ – \left(1-\dfrac{v^2}{c^2}\right)m^2c^4 &= 0, \\
    m^2c^4 – m^2v^2c^2 – m^2c^4 + \frac{m^2v^2c^4}{c^2} &= 0, \\
    m^2c^4 – m^2c^4 – m^2v^2c^2 + m^2v^2c^2 &= 0, \\
    0 – 0 &= 0.
    \end{align*}

    Hence, for every value of $ m $, $ p $, and thus $ v $, the relation holds.

    Problem III

    Hydrogen bubble chamber Fermilab

    The relativistic (total) energy is

    \[ E_{\text{tot}} = E_{\text{trans}} + E_{\text{mass}}. \]

    If the relativistic translational kinetic energy is four times the relativistic mass energy, then we can write

    \[ E_{\text{trans}} = 4E_{\text{mass}}. \]

    In our case, this then yields for the relativistic (total) energy:

    \[ E_{\text{tot}} = 4E_{\text{mass}} + E_{\text{mass}} = 5E_{text{mass}}. \]

    To calculate the proton’s speed, we then write

    \begin{align*}
    \frac{m_pc^2}{\sqrt{1 – \dfrac{v^2}{c^2}}} &= 5E_{\text{mass}} = 5m_pc^2, \\
    \frac{1}{\sqrt{1 – \dfrac{v^2}{c^2}}} &= 5, \\
    \sqrt{1-v^2/c^2} &= \frac{1}{5}, \\
    1-\frac{v^2}{c^2} &= \frac{1}{25}, \\
    \frac{v^2}{c^2} &= \frac{24}{25}, \\
    v^2 &= \frac{24c^2}{25}, \\
    \therefore v &= \sqrt{\frac{24c}{25}} = \frac{2\sqrt{6}c}{5},
    \end{align*}

    which is about $ 0.98c $ rounded to two decimals, which means that the proton zips at about 98% of the speed of light through the fabric of the cosmos.

    Image Hydrogen bubble chamber Fermilab: Proton with 300 GeV energy producing 26 charged particles in the 30 inch hydrogen bubble chamber at Fermilab. Source: Wikimedia Commons

    [1] Einstein, A. (1905) ‘Zur Elektrodynamik bewegter Körper’, Annalen der Physik, 322(10), pp. 891–921. doi: 10.1002/andp.19053221004.


    This is a repost. Slight errors in the parsing of LaTeX in the original article of 24 December 2018 have been corrected.