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• W1970931569 endingPage "1021" @default.
• W1970931569 startingPage "1019" @default.
• W1970931569 abstract "The evolution of the orbit of a binary pulsar under the action of gravitational radiation reaction is calculated. No approximation is made of weak gravity inside the individual stars; the details of the orbital motion are given directly (to order ${c}^{ensuremath{-}5}$ and ${G}^{3}$). The calculation reveals no acceleration of the center of mass of the system, and a secular decrease of the time of return to periastron. The quantitative results agree both with the well-known quadrupole formula and with observations." @default.
• W1970931569 created "2016-06-24" @default.
• W1970931569 creator A5075603241 @default.
• W1970931569 date "1983-09-19" @default.
• W1970931569 modified "2023-10-18" @default.
• W1970931569 title "Gravitational Radiation Reaction in the Binary Pulsar and the Quadrupole-Formula Controversy" @default.
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• W1970931569 doi "https://doi.org/10.1103/physrevlett.51.1019" @default.
• W1970931569 hasPublicationYear "1983" @default.
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