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25.3 MB
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4939B6F3E4B05F6BF42D56CCD1F2631D2E0626CB
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April 20, 2026, 12:53 p.m.
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(Last updated: April 20, 2026, 12:57 p.m.)
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| Iorio L. General Post-Newtonian Orbital Effects. From Earth's Satellites...2025.pdf | 25.3 MB |
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SOURCE: Iorio L. General Post-Newtonian Orbital Effects. From Earth's Satellites...2025
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MEDIAINFO
Textbook in PDF format Orbital motions have always been used to test gravitational theories which, from time to time, have challenged the then-dominant paradigms. This book provides a unified treatment for calculating a wide variety of orbital effects due to general relativity and modified models of gravity, to its first and second post-Newtonian orders, in full generality. It gives explicit results valid for arbitrary orbital configurations and spin axes of the sources, without a priori simplifying assumptions on either the orbital eccentricity or inclination. These general results apply to a range of phenomena, from Earth's artificial satellites to the S-stars orbiting the supermassive black hole in the Galactic Centre to binary and triple pulsars, exoplanets, and interplanetary probes. Readers will become acquainted with working out a variety of orbital effects other than the time-honoured perihelion precession, designing their own space-based tests, performing effective sensitivity analyses, and assessing realistic error budgets
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