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Solutions to the Equation of Motion

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Relativistic Dynamics of a Charged Sphere

Part of the book series: Lecture Notes in Physics Monographs ((LNPMGR,volume 11))

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Abstract

As a preliminary to solving the equation of motion (7.1) for the uniformly charged sphere of radius a and total charge e, write the magnitude of the four acceleration in (7.1) as

$$ \frac{{du_j }} {{ds}}\frac{{du^j }} {{ds}} = \frac{{(w \cdot w')^2 }} {{\gamma ^2 c^6 }} - \frac{{w'^2 }} {{c^4 }} $$
(8.1a)

where w is defined in terms of the velocity of the center of the shell by

$$ w = \gamma u, \gamma = (1 - u^2 /c^2 )^{ - 1/2} = (1 + w^2 /c^2 )^{1/2} $$
(8.1b)

and the primes denote derivatives with respect to the proper time

$$ d\tau = dt/\gamma . $$
(8.1c)

Insertion of (8.1) into (7.1) yields the three-vector equation for w

$$ \gamma F_{ext} = \frac{{e^2 }} {{8\pi \varepsilon _0 c^2 }}\left[ {\frac{{w'}} {a} - \frac{4} {{3a}}w'' + \frac{4} {{3c^3 }}\left( {w'^2 - \frac{{(w \cdot w')^2 }} {{c^2 \gamma ^2 }}} \right)w} \right] + O(a). $$
(8.2)

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© 1992 Springer-Verlag Berlin Heidelberg

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(1992). Solutions to the Equation of Motion. In: Relativistic Dynamics of a Charged Sphere. Lecture Notes in Physics Monographs, vol 11. Springer, New York, NY. https://doi.org/10.1007/978-0-387-73967-0_8

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  • DOI: https://doi.org/10.1007/978-0-387-73967-0_8

  • Publisher Name: Springer, New York, NY

  • Print ISBN: 978-0-387-97887-1

  • Online ISBN: 978-0-387-73967-0

  • eBook Packages: Springer Book Archive

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