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- W3100367130 endingPage "075008" @default.
- W3100367130 startingPage "075008" @default.
- W3100367130 abstract "We recently suggested a nonlocal modification of Einstein's field equations in which Newton's constant G was promoted to a covariant differential operator . The latter contains two independent contributions which operate respectively in the infrared (IR) and ultraviolet (UV) energy regimes. In the light of the recent direct gravitational radiation measurements we aim to determine the UV-modified 1.5 post-Newtonian radiative quadrupole moment of a generic n-body system. We eventually use these preliminary results in the context of a binary system and observe that in the limit vanishing UV parameters we precisely recover the corresponding general relativistic results. Moreover we notice that the leading order deviation of the UV-modified radiative quadrupole moment numerically coincides with findings obtained in the framework of calculations performed previously in the context of the perihelion precession of Mercury." @default.
- W3100367130 created "2020-11-23" @default.
- W3100367130 creator A5027969969 @default.
- W3100367130 date "2018-03-06" @default.
- W3100367130 modified "2023-10-10" @default.
- W3100367130 title "The 1.5 post-Newtonian radiative quadrupole moment in the context of a nonlocal field theory of gravity" @default.
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- W3100367130 doi "https://doi.org/10.1088/1361-6382/aaafa6" @default.
- W3100367130 hasPublicationYear "2018" @default.
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