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With the great development of theory, experiment, and manipulation of micro/nanoscale thermal radiation, several advanced applications emerge and show promising prospects in high-efficiency energy harvest/conversion such as angular/spectral selective or wideband absorber, thermophotovoltaics, or heat management implements such as radiative cooling, thermal camouflage, cloaking, and illusion. This chapter will give a brief introduction of these state-of-art technologies on the basis of theory of micro/nanoscale thermal radiation.
In this chapter, a summary of numerical algorithms solving the radiative transfer equation (RTE) is presented. These algorithms could be roughly classified into two categories. The one is ray-tracing methods, including the Zone method, Monte Carlo method, and discrete transfer method. The stochastic approach of Monte Carlo codes is widely used, since its flexible applicability to arbitrary multidimensional configurations. The others are methods based on the discretization of the differential form of RTE, including the spherical harmonics method, discrete ordinates method, and finite volume method.
At micro/nanoscale, the general principles of the thermal radiation are failed to solve or explain the majority of radiative problems or phenomena. This chapter will first point out the limitations and reasons of the general principles of thermal radiation by introducing a typical example. Then, some basic concepts, including the role of energy carriers such as photons, electrons, and phonon will be introduced first, followed by the brief introduction of the corresponding governing equations and the influence mechanism in radiative properties. Next, we would like to give a fundamental framework and chart review from macro- to nanoscalethermal radiation, aiming to make the relation and difference between macro- and nanothermal radiation more distinct. Finally, the development of micro/nanoscale thermal radiation in the last decades will be summarized as well.
The radiative transfer equation (RTE) is the governing equation of radiation propagation in participating media, which plays a central role in the analysis of radiative transfer in gases, semitransparent liquids and solids, porous materials, and particulate media, and is important in many scientific and engineering disciplines. This chapter will give a detailed introduction of the RTE. The microphysical derivation and the physical meaning of the relating quantities will be given. Besides, the relationship between the RTE and Maxwell’s equation will also be discussed and deduced as well, to build a comprehensive understanding of the RTE.
Thermal radiation is a ubiquitous aspect of nature, and this subject has developed for several centuries. In order to build a framework of macroscale thermal radiation, this chapter will give brief introductions of some fundamental theories and definitions of basic concepts of thermal radiation, such as blackbody radiation, radiative interactions at a surface, and radiative exchange between two or more surfaces. Besides, gas radiation as an important direction of thermal radiation will be introduced, including the molecular radiation theory, some gas spectral models, and some useful results in engineering applications.
Macrothermal radiation theory and analysis methods have been widely used in several real applications, such as heat transfer processes in the industrial boiler, radiant heat exchanger design, solar-thermal conversion in solar power plants, and so on. This chapter will cover the applications associated with macrothermal properties control, and some typical application examples will be given, hoping to offer a guidance in engineering applications.
This chapter focuses on experimental techniques in macroscale thermal radiation. The contents mainly involve the Fourier transform infrared spectrometer, the UV-Vis-NIR spectrophotometer, and the bidirectional reflectance distribution function (BRDF) instrument. We will review some outstanding experiments performed by different research groups for measuring the properties of macroscale thermal radiation. This chapter can be served as a guideline for researchers to design the experimental setups.
The pth ($p\geq 1$) moment exponential stability, almost surely exponential stability and stability in distribution for stochastic McKean–Vlasov equation are derived based on some distribution-dependent Lyapunov function techniques.
Master the fundamentals of complex marine systems with this introduction to marine dynamics, vibrations, hydrodynamics, and stochastic processes. It connects key theoretical concepts, including as the velocity potential, impulsive force and L'Hôpital's Rule, to real-world marine engineering applications such as such as marine platform dynamics, extreme motions and exceedance probabilities, and includes over 60 multi-part end-of-chapter problems, building from simplified questions to advanced exercises, enabling students to grow in confidence towards solving complex questions. Students will gain a deep understanding effective design and safe operation of offshore systems and ocean resources; and is supported by downloadable Matlab code, and online solutions for instructors. Including over 300 full-colour illustrations and worked examples, drawing on the author's 45 years of teaching experience in marine dynamics, this textbook provides the ideal introduction to marine dynamics for senior undergraduate and graduate students in marine engineering, and is a comprehensive reference for practitioners in industry.
Thermal radiation studies have progressed rapidly, not only in theoretical and experimental exploration beyond the conventional use but also in advanced applications. This is a one-stop resource for capturing and discussing these cutting-edge developments exploring the theory, experiments, and applications of thermal radiation from macro- to nanoscale. Presented in a systematic framework, this book is divided into two parts: the first on macroscopic thermal radiation and the second on micro- and nanoscale thermal radiation. Each part delivers basic theory, numerical methods, advanced experimental techniques, and promising applications, making this an easy-to-follow guide meeting both basic and advanced needs. Supported by more than 180 colorful illustrations, readers can clearly visualize the theory, experiments, and applications in practice. A book for all, written at a graduate level but undoubtedly a useful tool for researchers, professionals, and even engineers who are interested in this fast-developing area.
This concise and rigorous textbook introduces students to continuum thermodynamics, combining a complete treatment of the subject with practical applications to material modelling. It presents mathematical prerequisites and the foundations of continuum mechanics, then introduces more advanced topics such as theories for the investigation of material models. Taking the student step-by-step through the subject, it allows full understanding of the theory and how it relates to real-world practical applications. Packed with examples and illustrations to describe complex concepts and mathematical derivations, and including end-of-chapter problems with helpful hints, this is the ideal, accessible introduction to continuum thermodynamics for senior undergraduate and graduate students in mechanical, aeronautical and civil engineering.
We derive and analyse well-posed boundary conditions for the linear shallow water wave equation. The analysis is based on the energy method and it identifies the number, location and form of the boundary conditions so that the initial boundary value problem is well-posed. A finite-volume method is developed based on the summation-by-parts framework with the boundary conditions implemented weakly using penalties. Stability is proven by deriving a discrete energy estimate analogous to the continuous estimate. The continuous and discrete analysis covers all flow regimes. Numerical experiments are presented verifying the analysis.
Assuming linear theory, the phenomenon of scattering of waves by a circular arc shaped barrier with nonuniform porosity is studied. The water region is considered to be of infinite or finite depth. Based on a judicious application of Green’s integral theorem, the corresponding boundary value problem is reduced to a hypersingular integral equation of second kind. The boundary element method and the collocation method are adopted to solve the hypersingular integral equation, and we ensure a good matching of the solutions obtained by the two methods. The reflection coefficient and energy dissipation are evaluated by using the solution of the integral equation which is then studied graphically. Different choices of distributions of pores on the barrier are considered, and we observe that the nonuniform porosity of the barrier has significant effect on the reflected wave and the energy dissipation.
The behaviour of an axisymmetric bubble in a pure liquid forced by an acoustic pressure field is analysed. The bubble is assumed to have a sharp deformable interface, which is subject both to surface tension and to Rayleigh viscosity damping. Two modelling regimes are considered. The first is a linearized solution, based on the assumption of small axisymmetric deformations to an otherwise spherical bubble. The second involves a semi-numerical solution of the fully nonlinear problem, using a novel spectral method of high accuracy. For large-amplitude nonspherical bubble oscillations, the fully nonlinear solutions show that a complicated resonance structure is possible and that curvature singularities may occur at the interface, even in the presence of surface tension. Rayleigh viscosity at the interface prevents singularity formation, but eventually causes the bubble to become purely spherical unless shape-mode resonances occur. An extended analysis is also presented for purely spherical bubbles, which allows for a more detailed study of the effects of resonance and the Rayleigh viscosity at the bubble surface.
We propose a novel time-asymptotically stable, implicit–explicit, adaptive, time integration method (denoted by the $\theta $-method) for the solution of the fractional advection–diffusion-reaction (FADR) equations. The spectral analysis of the method (involving the group velocity and the phase speed) indicates a region of favourable dispersion for a limited range of Péclet number. The numerical inversion of the coefficient matrix is avoided by exploiting the sparse structure of the matrix in the iterative solver for the Poisson equation. The accuracy and the efficacy of the method is benchmarked using (a) the two-dimensional fractional diffusion equation, originally proposed by researchers earlier, and (b) the incompressible, subdiffusive dynamics of a planar viscoelastic channel flow of the Rouse chain melts (FADR equation with fractional time-derivative of order ) and the Zimm chain solution (). Numerical simulations of the viscoelastic channel flow effectively capture the nonhomogeneous regions of high viscosity at low fluid inertia (or the so-called “spatiotemporal macrostructures”), experimentally observed in the flow-instability transition of subdiffusive flows.
We study the influence of a low-frequency harmonic vibration on the formation of the two-dimensional rolling solitary waves in vertically co-flowing two-layer liquid films. The system consists of two adjacent layers of immiscible fluids with the first layer being sandwiched between a vertical solid plate and the second fluid layer. The solid plate oscillates harmonically in the horizontal direction inducing Faraday waves at the liquid–liquid and liquid–air interfaces. We use a reduced hydrodynamic model derived from the Navier–Stokes equations in the long-wave approximation. Linear stability of the base flow in a flat two-layer film is determined semi-analytically using Floquet theory. We consider sub-millimetre-thick films and focus on the competition between the long-wavelength gravity-driven and finite wavelength Faraday instabilities. In the linear regime, the range of unstable wave vectors associated with the gravity-driven instability broadens at low and shrinks at high vibration frequencies. In nonlinear regimes, we find multiple metastable states characterized by solitary-like travelling waves and short pulsating waves. In particular, we find the range of the vibration parameters at which the system is multistable. In this regime, depending on the initial conditions, the long-time dynamics is dominated either by the fully developed solitary-like waves or by the shorter pulsating Faraday waves.
We devise schemes for producing, in the least possible time, p identical objects with n agents that work at differing speeds. This involves halting the process to transfer production across agent types. For the case of two types of agent, we construct schemes based on the Euclidean algorithm that seeks to minimize the number of pauses in production.
For microscale heterogeneous partial differential equations (PDEs), this article further develops novel theory and methodology for their macroscale mathematical/asymptotic homogenization. This article specifically encompasses the case of quasi-periodic heterogeneity with finite scale separation: no scale separation limit is required. A key innovation herein is to analyse the ensemble of all phase-shifts of the heterogeneity. Dynamical systems theory then frames the homogenization as a slow manifold of the ensemble. Depending upon any perceived scale separation within the quasi-periodic heterogeneity, the homogenization may be done in either one step or two sequential steps: the results are equivalent. The theory not only assures us of the existence and emergence of an exact homogenization at finite scale separation, it also provides a practical systematic method to construct the homogenization to any specified order. For a class of heterogeneities, we show that the macroscale homogenization is potentially valid down to lengths which are just twice that of the microscale heterogeneity! This methodology complements existing well-established results by providing a new rigorous and flexible approach to homogenization that potentially also provides correct macroscale initial and boundary conditions, treatment of forcing and control, and analysis of uncertainty.
We construct a new stochastic interest rate model with two stochastic factors, by introducing a stochastic long-run equilibrium level into the Vasicek interest rate model which follows another Ornstein–Uhlenbeck process. With the interest rate under the Black–Scholes model being assumed to follow the newly proposed model, a closed-form representation of European option prices is successfully presented, when the analytical characteristic function of the underlying log-price under a forward measure is derived. To assess the model performance, a preliminary empirical study is conducted using S&P 500 index and its options, with the Vasicek model and an alternative two-factor Vasicek model taken as benchmarks.