Abstract
We consider the dumbbell charge system, consisting of two like charges q e /2 rotating about a fixed center, in such a way that its axis always lies perpendicular to a radial line from the center of rotation passing through its midpoint, as shown in Fig. 9.1. As in the last chapter, both A and B have constant speeds. Although the velocities of A and B are not always exactly parallel to the axis joining them, we do not have to worry about changing FitzGerald contractions during the motion, as we did in Chap. 7 (where the whole system was changing length all the time), because each of A and B always has the same speed. So we can assume a fixed length for the system, but there is a question about what the fixed length should be, because we expect it to be contracted in some way as compared with its length when stationary relative to some inertial frame. We shall nevertheless denote the length by d for the moment, and return to the question of its value at the end of the calculation.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2010 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Lyle, S.N. (2010). Self-Force for Longitudinal Rotational Motion. In: Self-Force and Inertia. Lecture Notes in Physics, vol 796. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-04785-5_9
Download citation
DOI: https://doi.org/10.1007/978-3-642-04785-5_9
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-04784-8
Online ISBN: 978-3-642-04785-5
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)