Planetary orbital precession in pseudo-Newtonian potentials: reproduction of the general relativity orbital effect

2019 ◽  
Vol 40 (6) ◽  
pp. 065601
Author(s):  
Jia-Fan Wang ◽  
Zhao-Yu Zuo
2019 ◽  
Vol 17 (1, spec.issue) ◽  
pp. 11-20
Author(s):  
Vesna Borka-Jovanovic ◽  
Predrag Jovanovic ◽  
Dusko Borka ◽  
Salvatore Capozziello ◽  
Stefania Gravina ◽  
...  

The aim of our investigation is to derive a particular theory among the class of scalar-tensor(ST) theories of gravity, and then to test it by studying kinematics and dynamics of S-stars around a supermassive black hole (BH) at Galactic Center (GC). We also discuss the Newtonian limit of this class of ST theories of gravity, as well as its parameters. We compare the observed orbit of S2 star with our simulated orbit which we obtained theoretically with the derived ST potential and constrained parameters. Using the obtained best-fit parameters we calculated orbital precession of S2 star in ST gravity and found that it has the same direction as in General Relativity (GR) but causes much larger pericenter shift.


Author(s):  
M. P. Hobson ◽  
G. P. Efstathiou ◽  
A. N. Lasenby
Keyword(s):  

2012 ◽  
Vol 182 (8) ◽  
pp. 894 ◽  
Author(s):  
Vladimir N. Lukash ◽  
Elena V. Mikheeva ◽  
Vladimir N. Strokov
Keyword(s):  

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