Fine structure of the Poynting-Robertson effect for a luminous spinning relativistic star

Details Fine structure of the Poynting-Robertson effect for a luminous spinning relativistic star Fine structure of the Poynting-Robertson effect for a luminous spinning relativistic star

2010-11-13

arxiv.org/abs/1011.3105v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

7 pages, 4 figures

Scientific paper

As a sequel to our recent works challenging toward the systematic inclusion of the effect of radiation on the trajectory of a test particle orbiting around a luminous spinning relativistic star eventually aiming at its application to the accretion flow. We explore in the present work the fine structure of the trajectory of test particle just entering the ``suspension orbit" under the purpose of a detailed investigation of test particle's trajectory in the vicinity of the ``suspension orbit". We end up with a rather puzzling behavior that, contrary to our expectation, the specific angular momentum of the test particle instantly rises instead of decreasing monotonically just before the test particle enters the ``suspension orbit".

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