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Journal ArticleDOI

Derivation of the Equations of Motion of a Gyroscope from the Quantum Theory of Gravitation

B. M. Barker, +1 more
- 15 Oct 1970 - 
- Vol. 2, Iss: 8, pp 1428-1435
TLDR
In this article, a new approach based on a gravitational potential energy derived from Gupta's quantum theory of gravitation was proposed to carry out the calculations using only the familiar tools of Newtonian mechanics and the Euler-Lagrange equations.
Abstract
Previous work on the gravitational two-body problem is surveyed Next, we present a new approach, which we consider to be simpler and more transparent than the usual methods because it is based on a gravitational potential energy This enables us to carry out our calculations using only the familiar tools of Newtonian mechanics and the Euler-Lagrange equations Starting from a gravitational potential energy derived from Gupta's quantum theory of gravitation, the classical motion of a spherical gyroscope in the gravitational field of a much larger mass with a quadrupole moment is found The results of the precession of the spin are compared with those of Schiff, and a detailed derivation of the results of O'Connell for the effect of a quadrupole moment (and higher moments) on the precession of the spin is presented In addition, we present some new results First, we show that the quadrupole moment manifests its presence in another way, which also contributes to the precession of the gyroscope a term that is about ten times larger than what could be detected Second, with regard to the precession of the orbit, in addition to the usual contributions, our results include the effects of the spin of both particles (which enables us to calculate the effect of the rotation of Mercury on the precession of its perihelion)

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Journal ArticleDOI

Higher Order Relativistic Periastron Advances and Binary Pulsars

TL;DR: In this article, the contributions of relativistic dynamical effects of order higher than the usual first post-Newtonian (1PN) equations of motion are investigated, and the spin-orbit contribution to the secular precession of the orbit in space is derived in a streamlined way by making full use of Hamiltonian methods.
Journal ArticleDOI

The effective field theorist’s approach to gravitational dynamics

TL;DR: In this article, effective field theory (EFT) was used for the study of cosmological large-scale structures, focusing on extended objects in long-wavelength backgrounds and gravitational wave emission from spinning binary systems.
Journal ArticleDOI

Phenomenology of the Lense-Thirring effect in the solar system

TL;DR: In this paper, the authors review the performed or proposed attempts to detect the Lense-thirring effect affecting the orbital motions of natural and artificial bodies in the gravitational fields of the Sun, Earth, Mars and Jupiter.
Journal ArticleDOI

The Effective Field Theorist's Approach to Gravitational Dynamics

TL;DR: In this article, effective field theory (EFT) was used for the study of cosmological large-scale structures, focusing on extended objects in long-wavelength backgrounds and gravitational wave emission from spinning binary systems.
Journal ArticleDOI

Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling

TL;DR: The spin-dependent EOB Hamiltonian is constructed from four main ingredients: (i) a transformation between the effective Hamiltonian and the real one; (ii) a generalized effective Hamilton-Jacobi equation involving higher powers of the momenta; (iii) a Kerr-type effective metric (with Pad\'e-resummed coefficients) which depends on the choice of some basic ''effective spin vector'' ${\mathbf{S}}_{\mathrm{eff}}$ and which is deformed by comparable-mass effects; and (iv) an additional effective
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