User:Tohline/2DStructure/ToroidalCoordinateIntegrationLimits
Toroidal-Coordinate Integration Limits
In support of our accompanying discussion of the gravitational potential of a uniform-density circular torus, here we explain in detail what limits of integration must be specified in order to accurately determine the volume — and, hence also the total mass — of such a torus using toroidal coordinates.
| Tiled Menu | Tables of Content | Banner Video | Tohline Home Page | |
Preamble
Referencing the illustration displayed in the left-hand panel of the following figure, our goal is to determine the gravitational potential at any cylindrical-coordinate location <math>~(R_0, Z_0)</math> due to a uniform-density circular torus whose major radius is <math>~\varpi_t</math> and whose cross-sectional radius is <math>~r_t</math>. Here we explain how a toroidal coordinate system — as defined, for example, by MF53 (see the schematic illustration in the right-hand panel of the following figure) — can be used to reduce the geometric complexity of this problem. In particular, we show how the three-dimensional integral over the mass distribution can be reduced to the sum of a small number (1 - 4) of one-dimensional integrals over the <math>~\xi_1</math> "radial" coordinate in toroidal coordinates.
Figure 1: Meridional slice through … | ||
---|---|---|
(Pink) Circular Torus | Toroidal Coordinate System (schematic) (see also Wikipedia's Apollonian Circles) | |
Quantitative Illustration of Employed Toroidal Coordinate System | ||
|
Schematic Zones | ||
---|---|---|
Zone I <math>~Z_0 > r_t</math>for any <math>~a</math> | Zone II <math>~r_t > Z_0 > 0</math>and<math>~a < \varpi_t - \sqrt{r_t^2 - Z_0^2}</math> | Zone III <math>~r_t > Z_0 > 0</math>and<math>~\varpi_t - \sqrt{r_t^2 - Z_0^2} < a < \varpi_t + \sqrt{r_t^2 - Z_0^2}</math> |
|
|
See Also
© 2014 - 2021 by Joel E. Tohline |