Post-Newtonian effect on the variation of time of periastron passage of binary stars in three gravitational theories
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Publication:973705
DOI10.1007/s10509-010-0267-4zbMath1187.85010OpenAlexW2026559624MaRDI QIDQ973705
Publication date: 26 May 2010
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-010-0267-4
Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (4)
Influence of the gravitational radiation damping on the time of periastron passage of binary stars ⋮ Yukawa-type potential effects in the anomalistic period of celestial bodies ⋮ Higher-order corrections to the relativistic perihelion advance and the mass of binary pulsars ⋮ Solar system's bounds on the extra acceleration of \(f(R,T)\) gravity revisited
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