http://arxiv.org/abs/1908.10075
We investigate how stable circular orbits around a main compact object appear depending on the presence of a second one by using the Majumudar-Papapetrou dihole spacetime with different masses. While the parameter range of the separation of the two objects is divided due to the appearance of stable circular orbits, this division depends on its mass ratio. We show that the mass ratio range separates into four parts, and find three critical values as the boundaries.
K. Nakashi and T. Igata
Wed, 28 Aug 19
6/60
Comments: 11 pages, 7 figures