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Two-post-Newtonian light propagation in the scalar-tensor theory: An N-point mass case
| 25-10-24 | 【 【打印】【关闭】

On August 3,  2012, the Physcial Review D published a paper which mainly investigated  2PN light deflection in the saclar-tensor theory (STT) with an N-point  mass case in order to meet the needs of some future space missions at  the level of few or higher nano-arcsecond precision. This work is done  by Dr. Xue-Mei Deng of Purple Mountain Observatory who is collaborated  with Dr. Yi Xie of Department of Astronomy in Nanjing University.

Some future  space missions will measure distances of laser links and angles among  these links with very high precision. For example, LATOR mission will  reach a level of 0.1 pico-arcsecond. And when light ray passes the limb  of the Sun, the 2PN deflection contributed by the Sun is about few  micro-arcsecond. So, a whole 2PN light propagation should be considered.  On the other hand, although Einstein’s general relativity (GR) has  passed nearly all the tests in the Solar System, there are many  important reasons to question it. Especially, in the cosmological scale,  two big problems challenge the GR. So, testing and distinguishing  different gravity theories is needed. Among these theories, STT is the  simplest and most natural way to modify GR. And deviation of the PPN  parameter γ from 1 might range for 10-7 to 10-5. And this deviation  needs to be considered at 2PN order. From the practial and theoretical  points of view, it is a natural development to build a 2PN theory of a  N-body system for its dynamics and light propagation within it which  might show some subtle but interesting effects due to the coupling terms  in the 2PN order.

This research  shows the 2PN 2-body effect in the Solar System is one order of  magnitude less than future ~1 nano-arcsecond experiments, while this  effect could be comparable with first post-Newtonian component of δθSTT  in a binary system with two Sun-like stars and separation by ~0.1 AU if  an experiment would be able to measureγ-1 down to ~10-6. Besides, the  deviation from the general relativity δθSTT does not depend on the PPN  parameter β at 2PN level in a case that the light propagation time is  much less than the time scale of its orbital motion. For more details,  please see the following link:

http://prd.aps.org/abstract/PRD/v86/i4/e044007

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