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Some optimal choices for a parameter of the Dai–Liao conjugate gradient method are proposed by conducting matrix analyses of the method. More precisely, first the $\ell _{1}$ and $\ell _{\infty }$ norm condition numbers of the search direction matrix are minimized, yielding two adaptive choices for the Dai–Liao parameter. Then we show that a recent formula for computing this parameter which guarantees the descent property can be considered as a minimizer of the spectral condition number as well as the well-known measure function for a symmetrized version of the search direction matrix. Brief convergence analyses are also carried out. Finally, some numerical experiments on a set of test problems related to constrained and unconstrained testing environment, are conducted using a well-known performance profile.
We introduce a model for the execution of large market orders in limit order books, and use a linear combination of self-exciting Hawkes processes to model asset-price dynamics, with the addition of a price-impact function that is concave in the order size. A criterion for a general price-impact function is introduced, which is used to show how specification of a concave impact function affects order execution. Using our model, we examine the immediate and permanent impacts of large orders, analyse the potential for price manipulation, and show the effectiveness of the time-weighted average price strategy. Our model shows that price depends on the balance between the intensities of the Hawkes process, which can be interpreted as a dependence on order-flow imbalance.
We analyse the vorticity production of lake-scale circulation in wind-induced shallow flows using a linear elliptic partial differential equation. The linear equation is derived from the vorticity form of the shallow-water equation using a linear bed friction formula. The features of the wind-induced steady-state flow are analysed in a circular basin with topography as a concave paraboloid, having a quadratic pile in the middle of the basin. In our study, the size of the pile varies by a size parameter. The vorticity production due to the gradient in the topography (and the distance of the boundary) makes the streamlines parallel to topographical contours, and beyond a critical size parameter, it results in a secondary vortex pair. We compare qualitatively and quantitatively the steady-state circulation patterns and vortex evolution of the flow fields calculated by our linear vorticity model and the full, nonlinear shallow-water equations. From these results, we hypothesize that the steady-state topographical vorticity production in lake-scale wind-induced circulations can be described by the equilibrium of the wind friction field and the bed friction field. Moreover, the latter can also be considered as a linear function of the velocity vector field, and hence the problem can be described by a linear equation.
Written in lucid language, this valuable text discusses fundamental concepts of von Neumann algebras including bounded linear operators in Hilbert spaces, finite von Neumann algebras, linear forms on algebra of operators, geometry of projections and classification of von Neumann algebras in an easy to understand manner. The revised text covers new material including the first two examples of factors of type II^1, an example of factor of type III and theorems for von Neumann algebras with a cyclic and separating vector. Pedagogical features including solved problems and exercises are interspersed throughout the book.
Dynamo theory is introduced as the theory of the spontaneous generation of magnetic fields by internal inductive motions in planets, stars and galaxies. The historical background to dynamo theory is described, focussing mainly on the magnetic fields of the Earth and the Sun. The simplest self-exciting dynamo model (the homopolar disc dynamo) is described, and its limitations are indicated. Cowling’s anti-dynamo theorem is touched on, and the resulting need for departures from axisymmetry in the internal fluid motions is discussed. For flows that are turbulent (whether strongly nonlinear or weak, as in a field of random waves), the `mean-field’ approach is described, and the need for a lack of reflectional symmetry (or ‘chirality’) in the flow is stressed. Other highlights in the historical development since the 1950s are described: the analogy with vorticity in turbulence, the first rigorous examples of dynamo action in a simply connected fluid domain (the two-sphere model of Herzenberg and the stasis model of Backus), the early computational attack on the geodynamo problem by Bullard and Gellman, the `cyclonic events’ theory of E. N. Parker, and the incorporation of dynamic constraints imposed by the Navier–Stokes equation in a strongly rotating fluid.
The gross properties of the magnetic fields of the Earth and of Mercury, Venus, Mars, Jupiter, Saturn, Uranus and Neptune are described. Strong rotation and a liquid conducting interior, at least in part, are indicated as necessary requirements for the existence of a significant magnetic field. The magnetic fields of planetary satellites are briefly described. The interior structure of the Earth is described, conditions in the outer liquid core being of particular relevance for dynamo theory. The time variation of the dipole moment of the Earth over the last few thousand years, as inferred from archaeomagnetic studies, is discussed, and the random reversals of the dipole moment over periods of the order of millions of years, that are inferred from palaeomagnetic studies of rock magnetism, are described. The need for a dynamo theory for the Earth to explain the persistence and time-variation of its magnetic field over past millennia is established. Conditions at the core-mantle boundary are discussed, and the possible relevance of precession of the Earth’s angular velocity vector as the source of energy for the core motions responsible for dynamo action is briefly considered.
Dynamic effects are introduced via the theory of Alfvén waves in a perfectly conducting fluid, the associated invariants and their relation with ‘cross-helicity’. Lehnert waves in a rotating fluid with an ambient magnetic field are then considered, and the dispersion relation is obtained. The important helicity-related concepts of `up-down symmetry breaking’ and the magnetostrophic limit are introduced. Transitory dynamo action associated with decaying Lehnert waves leading to a ‘fossil magnetic field’ is explained. Quenching of the α-effect due to the back-reaction of the Lorentz force and resulting magnetic equilibration are treated, first for waves generated by helical forcing, then for forced Lehnert waves, for which a resonant response in the presence of a growing magnetic field can occur. Boundary forcing is also considered. The generation of helicity is analysed, first due to the interaction of buoyancy and Coriolis forces, then due to magnetostrophic waves in an unstably stratified medium, then through instability due to ‘magnetic buoyancy’, and finally due to flow over the core–mantle interface, for which up-down symmetry is clearly broken.
Alfvén’s theorem, the analogue of Kelvin’s circulation theorem, is proved. The concept of a ‘frozen-in’ field in a perfectly conducting fluid is described, and the associated conservation of magnetic helicity is proved. The analogy with vorticity in an ideal fluid under Euler evolution is presented. The evolution of a magnetic field subjected to uniform strain is considered, and the possibility of accelerated ohmic diffusion is described. Flux expulsion is introduced through the example of uniform shearing of a space-periodic field; magnetic instability associated with oscillating shear flow and with steadily rotating shear flow is described. Flux expulsion associated with differential rotation is then analysed, with focus on the initial distortion, the intermediate phase and the ultimate steady state. The law of isorotation and the generation of toroidal field by differential rotation are also analysed, with emphasis again on the initial phase and the ultimate steady state. The concept of topological pumping resulting from asymmetry between upward and downward convective flow is introduced, and the behaviour as a function of the magnetic Reynolds number is described.