Results 11 to 20 of about 62,721 (327)
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
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Spin–orbit-driven ferromagnetic resonance [PDF]
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
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Dynamics and Origins of the Near-resonant Kepler Planets
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
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RESONANCES IN ASTEROID SYSTEMS
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
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Holonomy invariance, orbital resonances, and kilohertz QPOs [PDF]
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
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Eccentricity Evolution for Planets in Gaseous Disks [PDF]
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
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Covariant orbital-spin scheme for any spin based on irreducible tensor
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
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Quantized Orbits and Resonant Transport [PDF]
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
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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
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DISSIPATIVE DIVERGENCE OF RESONANT ORBITS [PDF]
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
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