For an extremely relativistic particle of rest energy e=mc² ,show that the momentum (P) is given by;
P=E[1-½(E/E)²]
Relativistic momentum p is classical momentum multiplied by the relativistic factor "\u03b3."
"p=\u03b3mu,"
where m is the rest mass of the object, "u" is its velocity relative to an observer, and the relativistic factor.
"\u03b3= \\large\\frac{1}{\\sqrt{1-\\large\\frac{u^2}{c^2}}}" "p=\\large\\frac{mu}{\\sqrt{1-\\large\\frac{u^2}{c^2}}}" "E = mc^2 \\to m = \\large\\frac{E}{c^2}"
is the three dimensional relativistic momentum of the object in the lab frame with magnitude |p| = p. The relativistic energy E and momentum p include the Lorentz factor defined by:
"{\\displaystyle \\gamma _{(\\mathbf {u} )}={\\frac {1}{\\sqrt {1-{\\frac {\\mathbf {u} \\cdot \\mathbf {u} }{c^{2}}}}}}={\\frac {1}{\\sqrt {1-\\left({\\frac {u}{c}}\\right)^{2}}}}}"
Some authors use relativistic mass defined by:
"{\\displaystyle m=\\gamma _{(\\mathbf {u} )}m_{0}}"
although rest mass m0 has a more fundamental significance and will be used primarily over relativistic mass m in this article.
Squaring the 3-momentum gives:
"{\\displaystyle p^{2}=\\mathbf {p} \\cdot \\mathbf {p} ={\\frac {m_{0}^{2}\\mathbf {u} \\cdot \\mathbf {u} }{1-{\\frac {\\mathbf {u} \\cdot \\mathbf {u} }{c^{2}}}}}={\\frac {m_{0}^{2}u^{2}}{1-\\left({\\frac {u}{c}}\\right)^{2}}}}"
then solving for u2 and substituting into the Lorentz factor obtains its alternative form in terms of 3-momentum and mass, rather than 3-velocity:
"\\gamma = \\sqrt{1 + \\left(\\frac{p}{m_0 c}\\right)^2}"
Inserting this form of the Lorentz factor into the energy equation:
"E = m_0c^2\\sqrt{1 + \\left(\\frac{p}{m_0 c}\\right)^2}" "\\large(\\frac{E}{E_o})^2" "=1+\\large\\frac{p^2}{E_o^2} \\to" "p^2 = E_o^2 (E^2-E_o^2) \\to p = E_o\\sqrt{E^2-E_o^2}"
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