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This work presents a generalized physical interpretation of unconventional dispersion asymmetries associated moving elastic solids. By shifting the notion from systems with time-variant material fields to physically traveling materials, the…

应用物理 · 物理学 2019-01-15 M. A. Attarzadeh , M. Nouh

An approximate dispersion relation is derived and presented for linear surface waves atop a shear current whose magnitude and direction can vary arbitrarily with depth. The approximation, derived to first order of deviation from potential…

流体动力学 · 物理学 2019-01-21 Simen Å. Ellingsen , Yan Li

Origin of hydrodynamic turbulence in rotating shear flows is investigated. The particular emphasis is the flows whose angular velocity decreases but specific angular momentum increases with increasing radial coordinate. Such flows are…

高能天体物理现象 · 物理学 2013-02-19 Banibrata Mukhopadhyay , Amit K. Chattopadhyay

Accretion disc turbulence is investigated in the framework of the shearing box approximation. The turbulence is either driven by the magneto-rotational instability or, in the non-magnetic case, by an explicit and artificial forcing term in…

天体物理学 · 物理学 2008-11-26 Axel Brandenburg

We numerically study the precessing disk model for superhump in the SU~UMa subclass of cataclysmic variables, using a two dimensional SPH code specifically designed for thin disk problems. Two disk simulations for a binary with mass ratio…

天体物理学 · 物理学 2015-06-24 James R. Murray

We revisit linear tidal excitation of spiral density waves in the disks of cataclysmic variables (CVs), focusing on scalings with orbital Mach number in order to bridge the gap between numerical simulations and real systems. If an inner…

太阳与恒星天体物理 · 物理学 2018-08-15 Wenrui Xu , Jeremy Goodman

We perform a linear analysis of the stability of isothermal, rotating, magnetic, self-gravitating sheets that are weakly ionized. The magnetic field and rotation axis are perpendicular to the sheet. We include a self-consistent treatment of…

太阳与恒星天体物理 · 物理学 2021-05-17 Indrani Das , Shantanu Basu

Bending waves are perhaps the most fundamental and analytically tractable phenomena in warped disc dynamics. In this work we conduct 3D grid-based, numerical experiments of bending waves in laminar, viscous hydrodynamic and turbulent,…

太阳与恒星天体物理 · 物理学 2025-01-28 Callum W. Fairbairn

Motivated by the recent results of \citet{Lesur_Ogilvie10} on the transport properties of incompressible convection in protoplanetary discs, in this paper we study the role of compressibility and hence of another basic mode -- spiral…

太阳与恒星天体物理 · 物理学 2015-05-28 G. R. Mamatsashvili , W. K. M. Rice

We investigate the two-point correlations in the band spectra of spatially periodic systems that exhibit chaotic diffusion in the classical limit. By including level pairs pertaining to non-identical quasimomenta, we define form factors…

chao-dyn · 物理学 2009-10-30 T. Dittrich , B. Mehlig , H. Schanz , U. Smilansky

The dispersing equation was derived from system of the hydrodynamic equations that take into account the gravity, and from boundary conditions of shock front. The dispersing equation made it possible to study unstable stability of front not…

等离子体物理 · 物理学 2010-05-21 V. V. Lyahov , V. M. Neshchadim

We have applied an eccentric accretion disc theory in simplified form to the case of an accretion disc in a binary system, where the disc contains the 3:1 Lindblad resonance. This is relevant to the case of superhumps in SU Ursae Majoris…

天体物理学 · 物理学 2009-11-11 Simon Goodchild , Gordon Ogilvie

We numerically study the tidal instability of accretion discs in close binary systems using a two-dimensional SPH code. We find that the precession rate of tidally unstable, eccentric discs does not only depend upon the binary mass ratio q.…

天体物理学 · 物理学 2009-10-30 James Murray

We study and elucidate the mechanism of spiral density wave excitation in a differentially rotating turbulent flow. We formulate a set of wave equations with sources that are only non-zero in the presence of turbulent fluctuations. We solve…

天体物理学 · 物理学 2015-05-13 T. Heinemann , J. C. B. Papaloizou

We investigate the properties of spiral shocks in a steady, adiabatic, non-axisymmetric, self-gravitating, mass-outflowing accretion disk around a compact object. We obtain the accretion-ejection solutions in a gaseous galactic disk and…

星系天体物理 · 物理学 2023-12-06 Ramiz Aktar , Li Xue , Li-Xin Zhang , Jing-Yi Luo

Using hydrodynamic approach, it is shown that the properties of a marginally stable collisionless stellar disc resemble those of a thermodynamic system undergoing a gas--liquid phase transition. The maximum in Toomre's stability diagram,…

星系天体物理 · 物理学 2010-01-04 E. I. Ivannikova , M. N. Maksumov

Using a novel approximation scheme within the convective diffusion (two body Smoluchowski) equation framework, we unveil the shear-driven aggregation mechanism at the origin of structure-formation in sheared colloidal systems. The theory,…

软凝聚态物质 · 物理学 2010-02-24 Alessio Zaccone , Daniele Gentili , Hua Wu , Massimo Morbidelli

We construct a linear response theory of applying shear deformations from boundary walls in the film geometry in Kubo's theoretical scheme. Our method is applicable to any solids and fluids. For glasses, we assume quasi-equilibrium around a…

软凝聚态物质 · 物理学 2018-12-27 Akira Onuki , Takeshi Kawasaki

If the Electroweak Symmetry Breaking Sector turns out to be strongly interacting, the actively investigated effective theory for longitudinal gauge bosons plus Higgs can be efficiently extended to cover the regime of saturation of unitarity…

高能物理 - 唯象学 · 物理学 2015-05-06 Rafael L. Delgado , Antonio Dobado , Felipe J. Llanes-Estrada

Starting from the beam wave equation, which has a Schr\"odinger structure, on a hypercubic lattice of size $L$, with weak nonlinearity of strength $\lambda$, we show that the two point correlation function can be asymptotically expressed as…

偏微分方程分析 · 数学 2023-01-30 Gigliola Staffilani , Minh-Binh Tran