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• W3100013274 abstract "The Galactic Center star cluster, known as S-stars, is a perfect source of relativistic phenomena observations. The stars are located in the strong field of relativistic compact object Sgr A* and are moving with very high velocities at pericenters of their orbits. In this work we consider motion of several S-stars by using the Parameterized Post-Newtonian (PPN) formalism of General Relativity (GR) and Post-Newtonian (PN) equations of motion of the Feynman's quantum-field gravity theory, where the positive energy density of the gravity field can be measured via the relativistic pericenter shift. The PPN parameters $beta$ and $gamma$ are constrained using the S-stars data. The positive value of the $T_g^{00}$ component of the gravity energy-momentum tensor is confirmed for condition of S-stars motion." @default.
• W3100013274 created "2020-11-23" @default.
• W3100013274 creator A5066993598 @default.
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• W3100013274 date "2020-10-14" @default.
• W3100013274 modified "2023-10-14" @default.
• W3100013274 title "Relativistic Effects in Orbital Motion of the S-Stars at the Galactic Center" @default.
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• W3100013274 doi "https://doi.org/10.3390/universe6100177" @default.
• W3100013274 hasPublicationYear "2020" @default.
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