Results 11 to 20 of about 2,165 (257)

The theory of secondary resonances in the spin–orbit problem [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
We study the resonant dynamics in a simple one degree of freedom, time dependent Hamiltonian model describing spin-orbit interactions. The equations of motion admit periodic solutions associated with resonant motions, the most important being the synchronous one in which most evolved satellites of the Solar system, including the Moon, are observed ...
GKOLIAS, IOANNIS   +3 more
openaire   +3 more sources

The Origin of Jupiter’s Obliquity

open access: yesThe Planetary Science Journal, 2023
The origin of the 3.°12 obliquity of Jupiter’s spin axis to its orbit normal is unknown. Improved estimates of Jupiter’s moment of inertia rule out a previously proposed explanation involving a resonance with the precession of the inclined orbit of ...
Rola Dbouk, Jack Wisdom
doaj   +1 more source

Tilting Uranus: Collisions versus Spin–Orbit Resonance

open access: yesThe Planetary Science Journal, 2021
Abstract In this paper, we investigate whether Uranus’s 98° obliquity was a by-product of a secular spin–orbit resonance assuming that the planet originated closer to the Sun. In this position, Uranus’s spin precession frequency is fast enough to resonate with another planet located beyond Saturn.
Zeeve Rogoszinski, Douglas P. Hamilton
openaire   +2 more sources

Collision‐induced spin‐orbit relaxation of highly vibrationally excited NO near 1 K

open access: yesNatural Sciences, 2022
State‐to‐state scattering studies of vibrationally excited molecules in the cold regime extend inelastic scattering investigations into a new territory. Here, we present differential cross‐sections for superelastic scattering of spin‐orbit excited nitric
Chandika Amarasinghe   +8 more
doaj   +1 more source

Magnetotunneling in resonant tunneling structures with spin − orbit interaction [PDF]

open access: yesJournal of Applied Physics, 2011
Magnetotunneling spectroscopy of resonant tunneling structures provides information on the nature of the two-dimensional electron gas in the well. We describe a model based on nonequilibrium Green’s functions that allows for a comprehensive study of the density of states, tunneling currents and current spin polarization.
Isić, Goran   +5 more
openaire   +2 more sources

RESONANCES IN ASTEROID SYSTEMS

open access: yesOdessa Astronomical Publications, 2016
Today the following types of resonances in the rotation of celestial bodies in the solar system are known, namely orbital, spin-orbit and spin-spin resonances.
V. Troianskyi
doaj   +1 more source

Spin-orbit qubit on a multiferroic insulator in a superconducting resonator [PDF]

open access: yesPhysical Review B, 2014
6 pages, 3 ...
Zhang, P., Xiang, Ze-Liang, Nori, Franco
openaire   +2 more sources

Magnetic Topology in Coupled Binaries, Spin-orbital Resonances, and Flares [PDF]

open access: yesThe Astrophysical Journal, 2021
Abstract We consider topological configurations of the magnetically coupled spinning stellar binaries (e.g., merging neutron stars or interacting star–planet systems). We discuss conditions when the stellar spins and the orbital motion nearly “compensate” each other, leading to very slow overall winding of the coupled magnetic fields ...
Sergey A. Cherkis, Maxim Lyutikov
openaire   +2 more sources

Probing evolution of binaries influenced by the spin–orbit resonances [PDF]

open access: yesClassical and Quantum Gravity, 2014
We evolve isolated comparable mass spinning compact binaries experiencing Schnittman's post-Newtonian spin-orbit resonances in an inertial frame associated with $j_0$, the initial direction of the total angular momentum. We argue that accurate gravitational wave (GW) measurements of the initial orientations of the two spins and orbital angular momentum
Gupta, Anuradha, Gopakumar, Achamveedu
openaire   +2 more sources

Tidal Dissipation Regimes among the Short-period Exoplanets

open access: yesThe Astrophysical Journal Letters, 2023
The efficiency of tidal dissipation provides a zeroth-order link to a planet’s physical properties. For super-Earth and sub-Neptune planets in the range R _⊕ ≲ R _p ≲ 4 R _⊕ , particularly efficient dissipation (i.e., low tidal quality factors) may ...
Emma M. Louden   +2 more
doaj   +1 more source

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