413(6):: Orbital Shrinkage Equation

The shrinkage is expressed most clearly through equations (11) and (12), in which r can be plotted against t, resulting in Eq. (12). The shrinking orbit is then Eq. (14), from which the half right latitude can be plotted as a function of t. The orbit is given correctly by both the lagrangian and hamiltonian methods, so all is self consistent. The dependence of r on time of a binary pulsar can be measured in astronomy and the ECE theory compared with the data.

a413thpapernotes6.pdf

### Like this:

Like Loading...

*Related*

This entry was posted on August 28, 2018 at 10:17 am and is filed under asott2. You can follow any responses to this entry through the RSS 2.0 feed.
Both comments and pings are currently closed.