Results 11 to 20 of about 62,721 (327)

Scaling, Mirror Symmetries and Musical Consonances Among the Distances of the Planets of the Solar System

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Orbital systems are often self-organized and/or characterized by harmonic relations. Inspired by music theory, we rewrite the Geddes and King-Hele (QJRAS, 24, 10–13, 1983) equations for mirror symmetries among the distances of the planets of the Solar ...
Michael J. Bank, Nicola Scafetta
doaj   +1 more source

Spin–orbit-driven ferromagnetic resonance [PDF]

open access: yesNature Nanotechnology, 2011
Ferromagnetic resonance is the most widely used technique for characterizing ferromagnetic materials. However, its use is generally restricted to wafer-scale samples or specific micro-magnetic devices, such as spin valves, which have a spatially varying magnetization profile and where ferromagnetic resonance can be induced by an alternating current ...
D. Fang1   +10 more
openaire   +3 more sources

Dynamics and Origins of the Near-resonant Kepler Planets

open access: yesThe Astrophysical Journal, 2023
Short-period super-Earths and mini-Neptunes encircle more than ∼50% of Sun-like stars and are relatively amenable to direct observational characterization.
Max Goldberg, Konstantin Batygin
doaj   +1 more source

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

Holonomy invariance, orbital resonances, and kilohertz QPOs [PDF]

open access: yes, 2002
Quantized orbital structures are typical for many aspects of classical gravity (Newton's as well as Einstein's). The astronomical phenomenon of orbital resonances is a well-known example.
A V Thampan   +18 more
core   +2 more sources

Eccentricity Evolution for Planets in Gaseous Disks [PDF]

open access: yes, 2002
We investigate the hypothesis that interactions between a giant planet and the disk from which it forms promote eccentricity growth. These interactions are concentrated at discrete Lindblad and corotation resonances.
Borderies N.   +4 more
core   +2 more sources

Covariant orbital-spin scheme for any spin based on irreducible tensor

open access: yesJournal of High Energy Physics, 2023
In hadron spectrum physics, the partial wave analysis is a primary method used to extract properties of hadronic resonances. The covariant orbital-spin coupling scheme holds unique advantages over other partial wave methods due to its Lorentz covariant ...
Hao-Jie Jing   +4 more
doaj   +1 more source

Quantized Orbits and Resonant Transport [PDF]

open access: yesPhysical Review Letters, 2000
A tight binding representation of the kicked Harper model is used to obtain an integrable semiclassical Hamiltonian consisting of degenerate "quantized" orbits. New orbits appear when renormalized Harper parameters cross integer multiples of $ /2$. Commensurability relations between the orbit frequencies are shown to correlate with the emergence of ...
Satija, Indubala I., Sundaram, Bala
openaire   +3 more sources

DYNAMIC EVOLUTION EXOPLANET SYSTEMS, MOVING IN ORBITAL RESONANCES WITH THE ACCOUNT OF SECULAR PERTURBATION FROM N BODIES

open access: yesOdessa Astronomical Publications, 2017
Equations of exoplanet's motion connected with orbital Lindblad resonances with the account of secular terms caused by gravitational non-resonant perturbation are derived. Qualitative researches of orbital evolution modeling exoplanet systems are carried
B. R. Mushailov, A. K. Chuyas
doaj   +1 more source

DISSIPATIVE DIVERGENCE OF RESONANT ORBITS [PDF]

open access: yesThe Astronomical Journal, 2012
A considerable fraction of multi-planet systems discovered by the observational surveys of extrasolar planets reside in mild proximity to first-order mean motion resonances. However, the relative remoteness of such systems from nominal resonant period ratios (e.g. 2:1, 3:2, 4:3) has been interpreted as evidence for lack of resonant interactions.
Batygin, Konstantin   +1 more
openaire   +3 more sources

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