Перейти к основному содержанию
AkademIndex

Продукты

Для разработчиков

AkademBaseОткрытый API экосистемы
Статья

Bound orbits and gravitational theory

Naresh DadhichCentre for Theoretical Physics, Jamia Millia Islamia, New Delhi 110025, India and Inter-University Centre for Astronomy & Astrophysics, Post Bag 4, Pune 411 007, IndiaSushant G. GhoshCentre for Theoretical Physics, Jamia Millia Islamia, New Delhi 110025, India and Inter-University Centre for Astronomy & Astrophysics, Post Bag 4, Pune 411 007, IndiaSanjay JhinganCentre for Theoretical Physics, Jamia Millia Islamia, New Delhi 110025, India and Inter-University Centre for Astronomy & Astrophysics, Post Bag 4, Pune 411 007, India
2013en
ABI

Аннотация

It can be easily shown that bound orbits around a static source can only exist in four dimensions for any force driven by the Laplace equation. This is true not only for Maxwell's electromagnetism and Newton's gravity, but for Einstein's theory of gravitation as well. In contrast to Maxwell's electrodynamics and Newton's gravity, general relativity has a natural and remarkable generalization in higher dimensions in Lovelock gravity. However, it is not Laplace driven and hence admits bound orbits around a static black hole in all even $D=2N+2$ dimensions, where $N$ is the degree of the Lovelock polynomial action. This is as general a result as Bertrand's theorem of classical mechanics, in which the existence of closed orbits uniquely singles out the inverse square law for a long-range central force.

Перевод пока недоступен

Идентификаторы

Цитирования и источники

Цитирований: 5Использованных источников: 0