Do relativistic corrections affect microlensing amplification?
arXiv:astro-ph/0011314 · doi:10.1143/PTP.104.1317
Abstract
Studies of gravitational microlensing are usually based on the lens equation, which is valid only to first order in the gravitational constant . However, the amplification factor of microlensing is a second-order quantity with respect to . Despite this fact, conventional studies are still based on the lowest-order lens equation. Then the question naturally arises: Why are these conventional studies justified? We carefully study the relativistic correction to the amplification factor at . We show that the amplification factor for each image is corrected. However, the total amplification remains unchanged at this order.
4 pages (PTPTeX); accepted for publication in Prog. Theor. Phys
Cited by in corpus (8)
- Gravitational Lensing by Black Holes
- Formalism for Testing Theories of Gravity Using Lensing by Compact Objects. I: Static, Spherically Symmetric Case
- Formalism for testing theories of gravity using lensing by compact objects. II: Probing Post-Post-Newtonian metrics
- Weak field limit of Reissner-Nordstrom black hole lensing
- On Relativistic Corrections to Microlensing Effects: Applications to the Galactic Black Hole
- Constraints on the black-hole charges of M87* and Sagittarius A* by changing rates of photon spheres can be relaxed
- Gravitational Wave detection through microlensing?
- Perturbative Approach to the Gravitational Lensing by a Non-spherically Distorted Compact Object