Finite size effects on the Poynting-Robertson effect: a fully general relativistic treatment

@article{Oh2011FiniteSE,
  title={Finite size effects on the Poynting-Robertson effect: a fully general relativistic treatment},
  author={Jae Sok Oh and Hongsu Kim and Hyung-Mok Lee},
  journal={New Astronomy},
  year={2011},
  volume={16},
  pages={183-186}
}
Abstract Even since the first discovery of Poynting and Robertson, the radiation source has been treated as merely a point. Even in a very few studies where the size of the source has been taken into account, the treatment of the problem remained largely non-relativistic. In the present work, we address the issue of the finite size effects on the Poynting–Robertson effect in a fully relativistic manner for the first time. As a result, the emergence and the characteristic of the critical point… 

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References

SHOWING 1-10 OF 12 REFERENCES
The generalized Poynting-Robertson effect
The special relativistic equations of motion for a particle and the general relativistic equations of motion for a fluid in an arbitrary radiation field are formulated. The Poynting-Robertson forces
The General relativistic Poynting-Robertson effect
The general relativistic version is developed for Robertson's discussion of the Poynting–Robertson effect that he based on special relativity and Newtonian gravity for point radiation sources like
Relativistic effects in superluminal jets and neutron star winds
A complete solution is given for the problem of radial motion of a test particle through the combined gravitational and radiation field of a spherical star. The star is assumed to radiate
Critical radiation fluxes and luminosities of black holes and relativistic stars
The critial luminosity at which the outward force of radiation balances the inward force of gravity plays an important role in many astrophysical systems. We present expressions for the radiation
Effect of radiation forces on disk accretion by weakly magnetic neutron stars
Radiation forces are shown to be more important than general relativistic corrections to Newtonian gravitational forces in determining the motion of particles accreting onto a slowly rotating neutron
Astrophys
  • J. 178, 347
  • 1972
Astrophys
  • J. 162, 71
  • 1970
...
1
2
...