z-logo
open-access-imgOpen Access
Do Relativistic Corrections Affect Microlensing Amplification?
Author(s) -
J. Ebina,
Takafumi Osuga,
Hideki Asada,
M. Kasai
Publication year - 2000
Publication title -
progress of theoretical physics
Language(s) - English
Resource type - Journals
eISSN - 1347-4081
pISSN - 0033-068X
DOI - 10.1143/ptp.104.1317
Subject(s) - gravitational microlensing , physics , amplification factor , gravitational lens , order (exchange) , lens (geology) , astrophysics , quantum electrodynamics , theoretical physics , particle physics , stars , optics , galaxy , amplifier , optoelectronics , redshift , cmos , finance , economics
Studies of gravitational microlensing are usually based on the lens equation,which is valid only to first order in the gravitational constant $G$. However,the amplification factor of microlensing is a second-order quantity withrespect to $G$. Despite this fact, conventional studies are still based on thelowest-order lens equation. Then the question naturally arises: Why are theseconventional studies justified? We carefully study the relativistic correctionto the amplification factor at $O(G^2)$. We show that the amplification factorfor each image is corrected. However, the total amplification remains unchangedat this order.Comment: 4 pages (PTPTeX); accepted for publication in Prog. Theor. Phy

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom