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Spin-orbit coupling can be described in two approaches. The method known as "the MacDonald torque" is often combined with an assumption that the quality factor Q is frequency-independent. This makes the method inconsistent, because the…

地球与行星天体物理 · 物理学 2019-08-28 Michael Efroimsky

Spin-orbit coupling is often described in the "MacDonald torque" approach which has become the textbook standard. Within this method, a concise expression for the additional tidal potential, derived by MacDonald (1964; Rev. Geophys. 2,…

地球与行星天体物理 · 物理学 2013-01-22 James G. Williams , Michael Efroimsky

Tidal torques play a key role in rotational dynamics of celestial bodies. They govern these bodies' tidal despinning, and also participate in the subtle process of entrapment of these bodies into spin-orbit resonances. This makes tidal…

地球与行星天体物理 · 物理学 2015-06-11 Michael Efroimsky , Valeri V. Makarov

We expand the equations used in MacDonald's 1964 theory and Fourier analyze the tidal variations of the height at one point on the Earth surface, and also the tidal potential at such point. It is shown that no intrinsic law is relating the…

地球与行星天体物理 · 物理学 2013-01-24 S. Ferraz-Mello

This report is a review of Darwin's classical theory of bodily tides in which we present the analytical expressions for the orbital and rotational evolution of the bodies and for the energy dissipation rates due to their tidal interaction.…

天体物理学 · 物理学 2009-06-19 Sylvio Ferraz-Mello , Adrián Rodríguez , Hauke Hussmann

The Darwin-Kaula theory of bodily tides is intended for celestial bodies rotating without libration. We demonstrate that this theory, in its customary form, is inapplicable to a librating body. Specifically, in the presence of libration in…

地球与行星天体物理 · 物理学 2017-08-28 Julien Frouard , Michael Efroimsky

A formula for the tidal dissipation rate in a spherical body is derived from first principles, to correct some mathematical inaccuracies found in the literature. The development is combined with the Darwin-Kaula formalism for tides. Our…

地球与行星天体物理 · 物理学 2015-12-22 Michael Efroimsky , Valeri V. Makarov

This paper presents a new theory of the dynamical tides of celestial bodies. It is founded on a Newtonian creep instead of the classical delaying approach of the standard viscoelastic theories and the results of the theory derive mainly…

地球与行星天体物理 · 物理学 2015-06-04 Sylvio Ferraz-Mello

Any model of tides is based on a specific hypothesis of how lagging depends on the tidal-flexure frequency. For example, Gerstenkorn (1955), MacDonald (1964), and Kaula (1964) assumed constancy of the geometric lag angle, while Singer…

天体物理学 · 物理学 2012-12-04 Michael Efroimsky , Valery Lainey

In geophysics and seismology, it is a common knowledge that the quality factors Q of the mantle and crust materials scale as the tidal frequency to a positive fractional power (Karato 2007, Efroimsky and Lainey 2007). In astronomy, there…

天体物理学 · 物理学 2012-03-19 Michael Efroimsky

We derive from first principles equations governing (a) the quadrupole tensor of a star distorted by both rotation and the presence of a companion in a possibly eccentric orbit, (b) a functional form for the dissipative force of tidal…

天体物理学 · 物理学 2009-10-30 Peter P. Eggleton , Ludmila G. Kiseleva , Piet Hut

We address the expressions for the rates of the Keplerian orbital elements within a two-body problem perturbed by the tides in both partners. The formulae for these rates have appeared in the literature in various forms, at times with…

地球与行星天体物理 · 物理学 2022-06-22 Gwenaël Boué , Michael Efroimsky

Hydrodynamic modelling is an important tool for the development of tidal stream energy projects. Many hydrodynamic models incorporate the effect of tidal turbines through an enhanced bottom drag. In this paper we show that although for…

计算工程、金融与科学 · 计算机科学 2015-06-12 Stephan C Kramer , Matthew D Piggott

We discuss the linear response to low-frequency tidal forcing of fluid bodies that are slowly and uniformly rotating, are neutrally stratified and may contain a solid or fluid core. This problem may be regarded as a simplified model of…

地球与行星天体物理 · 物理学 2015-06-12 Gordon I. Ogilvie

Description of tides is based on the form of dependence of the geometric lag on the tidal frequency. Some authors assume the lag angle to be constant, others set it to be linear in the frequency. The actual dependence of the lag on the…

天体物理学 · 物理学 2012-08-28 Michael Efroimsky

Thermal atmospheric tides have a strong impact on the rotation of terrestrial planets. They can lock these planets into an asynchronous rotation state of equilibrium. We aim at characterizing the dependence of the tidal torque resulting…

地球与行星天体物理 · 物理学 2019-04-10 Pierre Auclair-Desrotour , Jérémy Leconte , Cyril Mergny

While the seismic quality factor and phase lag are defined solely by the bulk properties of the mantle, their tidal counterparts are determined both by the bulk properties and self-gravitation of a body as a whole. For a qualitative…

地球与行星天体物理 · 物理学 2012-12-03 Michael Efroimsky

Time-reversal (TR) refocusing of waves is one of fundamental principles in wave physics. Using the TR approach, "Time-reversal mirrors" can physically create a time-reversed wave that exactly refocus back, in space and time, to its original…

流体动力学 · 物理学 2016-09-23 G. Ducrozet , M. Fink , A. Chabchoub

We prove a reducibility result for a class of quasi-periodically forced linear wave equations on the $d$-dimensional torus $\mathbb{T}^d$ of the form $$ \partial_{tt} v - \Delta v + \varepsilon {\cal P}(\omega t)[v] = 0 $$ where the…

偏微分方程分析 · 数学 2017-08-10 Riccardo Montalto

Many new models of wave turbulence -- frozen, mesoscopic, laminated, decaying, sand-pile, etc. -- have been developed in the last decade aiming to solve problems seemingly not solvable in the framework of the existing wave turbulence theory…

流体动力学 · 物理学 2014-06-17 Elena Tobisch
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