Envelope Bright- and Dark-Soliton Solutions for the Gerdjikov–Ivanov Model

Total Page:16

File Type:pdf, Size:1020Kb

Envelope Bright- and Dark-Soliton Solutions for the Gerdjikov–Ivanov Model Nonlinear Dyn (2015) 82:1211–1220 DOI 10.1007/s11071-015-2227-6 ORIGINAL PAPER Envelope bright- and dark-soliton solutions for the Gerdjikov–Ivanov model Xing Lü · Wen-Xiu Ma · Jun Yu · Fuhong Lin · Chaudry Masood Khalique Received: 20 April 2015 / Accepted: 14 June 2015 / Published online: 11 July 2015 © Springer Science+Business Media Dordrecht 2015 Abstract Within the context of the Madelung fluid which possesses bright- and dark-type (including gray description, investigation has been carried out on the and black) solitary waves due to associated parametric connection between the envelope soliton-like solu- constraints, and finally envelope solitons are found cor- tions of a wide family of nonlinear Schrödinger equa- respondingly for the Gerdjikov–Ivanov model. More- tions and the soliton-like solutions of a wide fam- over, this approach may be useful for studying other ily of Korteweg–de Vries or Korteweg–de Vries-type nonlinear Schrödinger-type equations. equations. Under suitable hypothesis for the current velocity, the Gerdjikov–Ivanov envelope solitons are Keywords Gerdjikov–Ivanov model · Madelung derived and discussed in this paper. For a motion with fluid description · Solitary wave · Envelope soliton the stationary profile current velocity, the fluid den- sity satisfies a generalized stationary Gardner equation, Mathematics Subject Classification 35Q51 · 35Q55 · 37K40 Xing Lü (B) Department of Mathematics, Beijing Jiao Tong University, Beijing 100044, China 1 Introduction e-mail: [email protected]; [email protected] The proposal of the concept “quantum potential” is a X. Lü · W.-X. Ma · J. Yu Department of Mathematics and Statistics, University valuable and seminal contribution to quantum mechan- of South Florida, Tampa, FL 33620, USA ics [1,2]. The Madelung fluid description of quan- tum mechanics plays an important role in a number of J. Yu applications, e.g., from stochastic mechanics to quan- Institute of Nonlinear Science, Shaoxing University, Shaoxing 312000, China tum cosmology and from the pilot waves theory to the hidden variables theory [3–5]. It has been employed F. Lin to describe quantum effects in mesoscopic systems School of Computer and Communication Engineering, and in plasma physics and discuss quantum aspects of University of Science and Technology Beijing, Beijing 100083, China beam dynamics in high-intensity accelerators (see [6,7] and references therein). It has also been applied to C. M. Khalique such situations where the quantum formalism is a International Institute for Symmetry Analysis and useful tool for describing the evolution of quantum- Mathematical Modelling, Department of Mathematical Sciences, North-West University, Mafikeng Campus, like systems or solving classical nonlinear evolution Private Bag X 2046, Mmabatho 2735, South Africa equations [8–24]. 123 1212 X. Lü et al. Within the context of Madelung fluid description, cubic nonlinear Schrödinger equation can be put the complex wave function (say Ψ ) is represented in in correspondence with the standard Korteweg–de terms of modulus and phase, and submitted into the Vries equation in such a way that the soliton solu- Schrödinger equation to lead to the possible achieve- tions of the latter are the squared modulus of the ment of a pair of nonlinear fluid equations for the envelope soliton solution of the former. The condi- “density” ρ =|Ψ |2 and the “current velocity” v = tions for different types of envelope solitons (bright, ∇Arg(Ψ ): one is the continuity equation (taking into dark or gray ones) are also discussed. account probability conservation) and the other one is • In Ref. [16], a modified nonlinear Schrödinger a Navier-Stokes-like equation√ of motion [6,7,15–20]. equation with a quartic nonlinear potential in the i Θ(x,t) Substitution of Ψ(x, t) = ρ(x, t) e h¯ into the modulus of the wave function has been studied one-dimensional Schrödinger equation within the framework of Madelung fluid descrip- tion, i.e., setting U |Ψ |2 = q |Ψ |2 +q |Ψ |4 with ∂Ψ(x, t) h¯ 2 ∂2Ψ(x, t) 1 2 i h¯ =− +mU(x)Ψ (x, t), (1) q and q as real constants in Eq. (3). By consider- ∂ ∂ 2 1 2 t 2 m x ing different boundary conditions, up-shifted bright results in the following pair of coupled Madelung fluid soliton, upper-shifted bright soliton, gray soliton equations and dark soliton are finally found and can be cast ∂ρ ∂ + (ρ v) = 0, (2a) into envelope solitons conversely. ∂t ∂x • In Ref. [17], the existence of envelope soliton-like √ ∂v ∂v h¯ 2 ∂ 1 ∂2 ρ ∂U solutions of a nonlinear Schrödinger equation con- + v − √ + = 0, |Ψ |−4Ψ ∂t ∂x 2 m2 ∂x ρ ∂x2 ∂x taining an anti-cubic nonlinearity ( )plus a ‘regular’ nonlinear part is investigated. In par- (2b) ticular, in the case that the regular nonlinear part ρ =|Ψ |2 v = 1 ∂Θ where is the fluid density and m ∂x consists of a sum of cubic and quintic nonlineari- 2 −4 2 is the current velocity. Equation (2a) is a continuity ties, i.e., setting U |Ψ | = Q0|Ψ | + q1|Ψ | + 4 equation for the fluid density, while Eq. (2b) is an Euler q2|Ψ | with Q0, q1 and q2 as real constants in equation or equation of motion for the fluid velocity and Eq. (3), an upper-shifted bright envelope soliton- contains a force term proportional to√ the gradient of the like solution is explicitly found. 2 ∂ ∂2 ρ “quantum potential”, h¯ √1 . • In Ref. [18], a review is given on the results of inves- 2 m2 ∂x ρ ∂x2 Madelung fluid description has been used to dis- tigations dealing with the connection between the cuss families of generalized one-dimensional nonlinear envelope soliton-like solutions of a wide family of Schrödinger equations [15–19], as follows: nonlinear Schrödinger equations and the soliton- like solutions of a wide family of Korteweg– • In Ref. [15], the following nonlinear Schrödinger- de Vries equations. In two different fluid motion like equation regimes (uniform current velocity and stationary ∂Ψ μ2 ∂2Ψ profile current velocity variation, respectively), i μ =− + U |Ψ |2 Ψ, (3) ∂ ∂ 2 t 2 x bright- and gray-/dark-soliton-like solutions of where U |Ψ |2 and μ are as an arbitrary real func- those equations are found. tional of the complex wave function Ψ and an arbi- • In Ref. [19], a similar discussion is given for a class trary real dispersion/diffraction coefficient, respec- of derivative nonlinear Schrödinger-type equations. tively, has been cast as For a motion with the stationary profile current ∂ρ ∂ velocity, the fluid density satisfies a generalized sta- + (ρv) = , ∂ ∂ 0 (4a) tionary Gardner equation, and solitary wave solu- t x ∂v ∂ρ ∂v ∂ρ tions are found. For the completely integrable cases, −ρ + v + 2 c (t) − dx these solutions are compared with existing solu- ∂t ∂t 0 ∂t ∂x tions in the literature. dU ∂ρ μ2 ∂3ρ − ρ + 2U + = 0, (4b) dρ ∂x 4 ∂x3 In the present paper, we will investigate the with c0(t) as an arbitrary function of t. Under the Gerdjikov–Ivanov envelope solitons with the frame- hypothesis of stationary fluid, it is revealed that the work of Madelung fluid description. Various optical 123 Envelope bright- and dark-soliton solutions for the Gerdjikov–Ivanov model 1213 √ envelope soliton problems have been proposed and ∂v 2 ∂v ∂ 1 ∂2 ρ + v = k √ studied in the series literature [25–34]. In Sect. 2,we ∂t k ∂x ∂x ρ ∂x2 will pay attention to the Gerdjikov–Ivanov model and ∂ 2 derive the basic equations of Madelung fluid: the conti- + ρv+ ρ2 . ∂ (6b) nuity equation for the fluid density and motion equation x k for the fluid velocity. Symbolic-computation manipulation on Eq. (6b)gives It will be found in Sect. 3 that for a motion with rise to the stationary profile current velocity, the fluid den- ∂ρ ∂v ∂ρ ∂v ∂ρ sity satisfies a generalized stationary Gardner equation. − v + ρ − ρv − ρ2 − k ρ2 ∂ ∂ 2 ∂ ∂ 2 ∂ Under suitable hypothesis for the current velocity and t t x x x k ∂3ρ ∂ρ ∂ρ ∂v due to associated parametric constraints, in Sect. 4,we − + 2 c (t) + 2 dx = 0, (6c) ∂ 3 0 ∂ ∂ ∂ will present bright- and dark-type (including gray and 2 x x x t black) solitary waves for the stationary Gardner equa- where c (t) is an arbitrary function of t. tion, and finally, associated envelope solitons will be 0 Hereby, Eqs. (6a) and (6c) constitute the basic equa- constructed correspondingly for the Gerdjikov–Ivanov tions for the subsequent discussion. model. Sect. 5 will be our conclusions. 3 Motion with the stationary profile current 2 Gerdjikov–Ivanov model and basic equations velocity ρ v The Gerdjikov–Ivanov model studied hereby is given Assuming that both the quantities and involved as [35–38] in Eqs. (6a) and (6b) are functions of the combined variable ξ = x − u0 t with u0 being a real constant, we ∗ ∂Ψ ∂2Ψ ∂Ψ 1 can cast Eq. (6a)into i + − i Ψ 2 + |Ψ |4Ψ = 0, (5) ∂t ∂x2 ∂x 2 dρ d 2 1 where ∗ denotes the complex conjugation and Ψ = −u + ρv− ρ2 = , 0 ξ ξ 0 (7) Ψ(x, t) is the complex wave function. Eq. (5)isalso d d k 2 called the derivative nonlinear Schrödinger III equation and integrate once of Eq. (7) with respect to ξ to obtain and can be transformed into the Kaup–Newell or the Chen–Lee–Liu equation by corresponding gauge trans- k 1 A0 formations [37,38]. With the help of gauge transfor- v = u0 + ρ + , (8) 2 2 ρ mation of the spectral problem, a Darboux transforma- tion for Eq. (5) has been constructed with the achieve- by taking the integration constant as A0.
Recommended publications
  • First-Principles Envelope-Function Theory for Lattice-Matched Semiconductor Heterostructures
    PHYSICAL REVIEW B 72, 165345 ͑2005͒ First-principles envelope-function theory for lattice-matched semiconductor heterostructures Bradley A. Foreman* Department of Physics, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, China ͑Received 17 June 2005; revised manuscript received 26 August 2005; published 28 October 2005͒ In this paper a multiband envelope-function Hamiltonian for lattice-matched semiconductor heterostructures is derived from first-principles self-consistent norm-conserving pseudopotentials. The theory is applicable to isovalent or heterovalent heterostructures with macroscopically neutral interfaces and no spontaneous bulk polarization. The key assumption—proved in earlier numerical studies—is that the heterostructure can be treated as a weak perturbation with respect to some periodic reference crystal, with the nonlinear response small in comparison to the linear response. Quadratic response theory is then used in conjunction with k·p perturbation theory to develop a multiband effective-mass Hamiltonian ͑for slowly varying envelope functions͒ in which all interface band-mixing effects are determined by the linear response. To within terms of the same order as the position dependence of the effective mass, the quadratic response contributes only a bulk band offset term and an interface dipole term, both of which are diagonal in the effective-mass Hamiltonian. The interface band mixing is therefore described by a set of bulklike parameters modulated by a structure factor that determines the distribution of atoms in the heterostructure. The same linear parameters determine the interface band-mixing Hamiltonian for slowly varying and ͑sufficiently large͒ abrupt heterostructures of arbitrary shape and orientation. Long-range multipole Coulomb fields arise in quantum wires or dots, but have no qualitative effect in two-dimensional systems beyond a dipole contribution to the band offsets.
    [Show full text]
  • Laser Envelope Model In
    Laser Envelope model in Maison de la Simulation Francesco– March 2019 Massimo Francesco Massimo Outline I. Motivations II. Modeling Laser Wakefield Acceleration with a laser envelope III. Case study: Laser Wakefield Acceleration with external injection IV. Perspectives and future developments Laser Wakefield Acceleration (LWFA): Characteristic Scales 1.5 Laser Beam Duration: 28 fs Transverse 1.2 Electric Field Ponderomotive (A.U.) Force: 0.9 F= - ILaser 0.6 Electrons Immobile Ions Mi >>me 0.003 Plasma density: 3.1018 cm-3 0.002 Electron Charge Density Plasma 0.001 (A.U.) wavelength: ~20 μm 0.000 Laser Wakefield Acceleration (LWFA): Characteristic Scales E > 100 GV/m 0.04 Longitudinal Electric Field Electrons 0.00 (A.U.) injected here on propagation axis are accelerated -0.04 0.003 Laser wavelength: Electron ~1 μm 0.002 Charge Laser duration ~ Density Plasma wavelength: 0.001 (A.U.) ~20 μm 0.000 0.000 LWFA PIC simulations are cumbersome X. Davoine, Physics of Plasmas 15, 113102 (2008) 2D cartesian simulations are not accurate enough for LWFA! 3D LWFA simulations: 1 mm plasma ~ 320 kcpu-heures ~ 10.2 k€ Laser Envelopes need less sampling points Spatial variation scales: Laser Envelope Laser length ~ Plasma wavelength (10-100 μm) Laser wavelength Laser “Standard” (~1 μm) Points sampling Laser “Standard” = 10 Points sampling Laser Envelope Larger Δx and Δt can be used! Structure of a PIC code with Laser Envelope Standard PIC Envelope (/Ponderomotive) PIC ~ E, B field E,B field Envelope A (laser) (plasma fields+laser fields) (plasma fields) Lorentz Lorentz Force Ponderomotive Force Force Plasma Current Current Density J Density J Susceptibility Particles Particles The Laser Envelope evolution: wave equation D.
    [Show full text]
  • The K·P Method Lokc.Lewyanvoon· Morten Willatzen
    The k·p Method LokC.LewYanVoon· Morten Willatzen The k·p Method Electronic Properties of Semiconductors 123 Dr. Lok C. Lew Yan Voon Dr. Morten Willatzen Wright State University University of Southern Denmark Physics Dept. Mads Clausen Institute for 3640 Colonel Glenn Highway Product Innovation Dayton OH 45435 Alsion 2 USA 6400 Soenderborg [email protected] Denmark [email protected] ISBN 978-3-540-92871-3 e-ISBN 978-3-540-92872-0 DOI 10.1007/978-3-540-92872-0 Springer Dordrecht Heidelberg London New York Library of Congress Control Number: 2009926838 c Springer-Verlag Berlin Heidelberg 2009 This work is subject to copyright. All rights are reserved, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilm or in any other way, and storage in data banks. Duplication of this publication or parts thereof is permitted only under the provisions of the German Copyright Law of September 9, 1965, in its current version, and permission for use must always be obtained from Springer. Violations are liable to prosecution under the German Copyright Law. The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. Cover design: WMXDesign GmbH Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) Uber¨ Halbleiter sollte man nicht arbeiten, das ist eine Schweinerei; wer weiss ob es uberhaupt¨ Halbleiter gibt.
    [Show full text]
  • Introducing the Rossby Wave Packet Tool
    Introducing the Rossby Wave Packet Tool Mike Bodner HPC/DTB 25 August 2011 Acknowledgements The work on developing a wave packet tool is a collaborative effort between HPC and Stony Brook University, and is part of C-Star funding. Special thanks to Brian Colle and Edmund Chang for leading this effort, and to Matt Souders for sharing computer code and his research materials with HPC. Gratitude extended to Bob Daniels from OPC for assistance in configuring Matlab. Training Outline • Overview of Wave Packets • How to View Wave Packets • Methods of Computing Wave Packet Envelopes • Wave Packet Climatology • Utilization of Wave Packets Why Wave Packets? • High impact weather has been found to be associated with wave packets (Archambault et al. 2010) • 500 hPa geopotential heights move with phase velocity, while wave packets propagate with group velocity which can be an indicator of downstream development • Potential indicator of uncertainty – forecast errors can develop and propagate like wave packets (Hakim 2005) What are Wave Packets ? • Baroclinic waves propogate chaotically and are driven primarily by phase speed • A wave packet encompasses several waves and will propagate with the group velocity which is much faster than the phase speed of individual troughs ▪ Red curves are two sine curves which can represent troughs and ridges ▪ Blue curve is the wave packet which encompasses the toughs/ridges The figure on the right shows 300 hPa geopotenital heights for the period 18-28 December, 1985 (Chang 1993). ▪ Wave packets are useful in forecasting because since they propagate with this much faster group velocity, the packets will often result in downstream development.
    [Show full text]
  • Wavepacket and Dispersion
    Wavepacket and Dispersion Andreas Wacker1 Mathematical Physics, Lund University September 18, 2017 1 Motivation A wave is a periodic structure in space and time with periods λ and T , respectively. Common examples are water waves, electromagnetic waves, or sound waves. The spatial structure is 2π 2π A cos(kz − !t + ') = RefA~ei(kz−!t)g with A~ = ei'A; k = and ! = (1) λ T where the complex representation often simplifies the maths significantly. The angular fre- quency ! and the angular wavenumber k (Note that the term wavenumber refers to 1/λ in spectroscopy) are related to each other by a dispersion relation !disp(k), which is a property of the material considered. For linear media considered here, the dispersion relation is indepen- dent of the amplitude A and different waves can be superimposed (i.e. added) without affecting each other. The structure of waves is described by the phase φ = kz − !t + ', where certain values, such as φ = 0 or φ = π=2, correspond to positions of maximal or vanishing amplitude, respectively. If we considers the position zp for a point with constant phase in time, we find dzp=dt = !=k = vp, which defines the phase velocity vp = !disp(k)=k. This is the velocity of the maxima in a single monochromatic wave as given by Eq. (1). In order to transmit any information between two places, the recipient cannot handle a single wave, as all peaks look the same. Thus we require some modulation, so that characteristic spatial structures are transmitted. This can be achieved by interfering waves with different wavenumbers/frequencies.
    [Show full text]
  • Laser Wakefield Simulation Using a Speed-Of-Light Frame Envelope Model
    Lawrence Berkeley National Laboratory Lawrence Berkeley National Laboratory Title Laser wakefield simulation using a speed-of-light frame envelope model Permalink https://escholarship.org/uc/item/41h1k8kf Author Cowan, B. Publication Date 2009-01-22 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Laser wakefield simulation using a speed-of-light frame envelope model , B. Cowan∗, D. Bruhwiler∗, E. Cormier-Michely, E. Esareyy ∗∗, C. G. R. Geddesy, P. Messmer∗ and K. Paul∗ ∗Tech-X Corporation, 5621 Arapahoe Ave., Boulder, CO 80303 yLOASIS program, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 ∗∗University of Nevada, Reno, Reno, NV 89557 Abstract. Simulation of laser wakefield accelerator (LWFA) experiments is computationally inten- sive due to the disparate length scales involved. Current experiments extend hundreds of laser wave- lengths transversely and many thousands in the propagation direction, making explicit PIC simula- tions enormously expensive and requiring massively parallel execution in 3D. We can substantially improve the performance of laser wakefield simulations by modeling the envelope modulation of the laser field rather than the field itself. This allows for much coarser grids, since we need only resolve the plasma wavelength and not the laser wavelength, and therefore larger timesteps. Thus an envelope model can result in savings of several orders of magnitude in computational resources. By propagating the laser envelope in a frame moving at the speed of light, dispersive errors can be avoided and simulations over long distances become possible. Here we describe the model and its implementation, and show simulations and benchmarking of laser wakefield phenomena such as channel propagation, self-focusing, wakefield generation, and downramp injection using the model.
    [Show full text]
  • Laser Wakefield Simulation Using a Speed-Of-Light Frame Envelope Model
    Laser wakefield simulation using a speed-of-light frame envelope model , B. Cowan∗, D. Bruhwiler∗, E. Cormier-Michely, E. Esareyy ∗∗, C. G. R. Geddesy, P. Messmer∗ and K. Paul∗ ∗Tech-X Corporation, 5621 Arapahoe Ave., Boulder, CO 80303 yLOASIS program, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 ∗∗University of Nevada, Reno, Reno, NV 89557 Abstract. Simulation of laser wakefield accelerator (LWFA) experiments is computationally inten- sive due to the disparate length scales involved. Current experiments extend hundreds of laser wave- lengths transversely and many thousands in the propagation direction, making explicit PIC simula- tions enormously expensive and requiring massively parallel execution in 3D. We can substantially improve the performance of laser wakefield simulations by modeling the envelope modulation of the laser field rather than the field itself. This allows for much coarser grids, since we need only resolve the plasma wavelength and not the laser wavelength, and therefore larger timesteps. Thus an envelope model can result in savings of several orders of magnitude in computational resources. By propagating the laser envelope in a frame moving at the speed of light, dispersive errors can be avoided and simulations over long distances become possible. Here we describe the model and its implementation, and show simulations and benchmarking of laser wakefield phenomena such as channel propagation, self-focusing, wakefield generation, and downramp injection using the model. INTRODUCTION Laser-driven plasma wakefield accelerators (LWFAs) are capable of producing acceler- ating gradients several orders of magnitude higher than conventional accelerators. Sev- eral years ago, high-quality electron beams were produced by self-trapping and acceler- ated to 100MeV in a few millimeters [1, 2, 3].
    [Show full text]
  • The Influence of a Pressure Wavepacket's Characteristics on Its
    The influence of a pressure wavepacket’s characteristics on its acoustic radiation R. Serré, Jean-Christophe Robinet, F. Margnat To cite this version: R. Serré, Jean-Christophe Robinet, F. Margnat. The influence of a pressure wavepacket’s character- istics on its acoustic radiation. Journal of the Acoustical Society of America, Acoustical Society of America, 2015, 137 (6), pp.3178-3189. 10.1121/1.4921031. hal-02569482 HAL Id: hal-02569482 https://hal.archives-ouvertes.fr/hal-02569482 Submitted on 11 May 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. The influence of a pressure wavepacket’s characteristics on its acoustic radiation R. Serre and J.-C. Robinet Arts et Metiers ParisTech, DynFluid, 151 Boulevard de l’Hopital, 75013 Paris, France a) F. Margnat Institut PPRIME, Department of Fluid Flow, Heat Transfer and Combustion, Universite de Poitiers - ENSMA - CNRS, Building B17 - 6 rue Marcel Dore, TSA 41105, 86073 Poitiers Cedex 9, France Noise generation by flows is modeled using a pressure wavepacket to excite the acoustic medium via a boundary condition of the homogeneous wave equation. The pressure wavepacket is a generic representation of the flow unsteadiness, and is characterized by a space envelope of pseudo- Gaussian shape and by a subsonic phase velocity.
    [Show full text]
  • 2.2 the Nonlinear Schrödinger Equation As an Envelope Equation
    20 V. Hakim Another interesting elementary example of application of the multiscale method is the computation of the size of the limit cycle of a Van der Pol oscillator: x¨ + ǫ x2 1 x˙ + x =0 for ǫ 1 (2 .13) − ≪ The zeroth order solution is x0 = A cos( t + φ) (2 .14) With an arbitrary amplitude A. Introducing a slow time scale like in (2.6), the cancellation of secular terms at first order gives the evolution of the amplitude dA A3 2 = A (2 .15) dT − 4 This shows that the amplitude of the limit cycle is equal to 2 and that (2.15) describes the approach to the limit cycle on a time scale that is long compared to the oscillation frequency. At next order, the change of the period of the limit cycle appears 1 ω = 1 ǫ2 (2 .16) − 16 This computation is left as an exercise to the reader. It is described in detail in S. Fauve’s lectures. 2.2 The nonlinear Schr¨odinger equation as an envelope equation for small amplitude gravity waves in deep water 2.2.1 A short introduction to water waves The problem of water waves has played a central role in the development of nonlinear physics, with Stokes’s discovery that dispersion relation in- volves the amplitude for periodic nonlinear wave trains, Russell’s first observation of a solitary wave, the derivation of model equations by Boussinesq, Rayleigh and Korteweg-de Vries . Moreover, the observa- tion of water waves is a common but fascinating experience. A good introduction to the subject can be found in Stoker (1957) and Whitham (1974).
    [Show full text]
  • A Spatial Envelope Soliton
    A Soliton Model of the Electron with an internal Nonlinearity cancelling the de Broglie-Bohm Quantum Potential ROALD EKHOLDT§ Abstract The paper proposes an envelope soliton model of the electron that propagates as a protuberance on a fictitious waveguide, which acts as trajectory. The model is based on de Broglie’s original electron wave-particle relativistic theory, and on the observation that the Klein-Gordon equation governs the propagation mode of a common microwave waveguide—with the Schrödinger equation as a low group velocity approximation. This analogy opened for practical physical models, including solitons. In the linear case a conceived corpuscle zigzags within the fictitious waveguide—a zigzagging that resembles Penrose’s picture of Dirac’s electron theory. The soliton envelope is defined by a special nonlinear version of the Schrödinger equation. The nonlinearity cancels the de Broglie/Bohm Quantum Potential of the envelope. The wavefunction is confined by the envelope, and thus the concept of the collapse of the wavefunction is eliminated. Since the electron model is based directly on the Special theory of relativity it also illustrates that theory. The corpuscle, incorporating spin and charge, which moves at the speed of light, needs further study relating it to the photon. A nonlinear model of the photon, based on mutual coupling of two modes of an optical fiber at the Planck scale, is suggested. One of these modes is thought to carry two orthogonal polarized electromagnetic external fields, while the other, internal, mode carries a corpuscle that moves helically and thus represents the spin. A single photon is considered to have one linear polarization only, without any possibility for a circular polarization; hence, the concept of collapse in a polarization measurement is eliminated.
    [Show full text]
  • The Hydrodynamic Nonlinear Schrödinger Equation: Space and Time
    fluids Article The Hydrodynamic Nonlinear Schrödinger Equation: Space and Time Amin Chabchoub 1,2,†,* and Roger H. J. Grimshaw 3,† 1 Graduate School of Frontier Sciences, The University of Tokyo, Chiba 277-8563, Japan 2 Department of Mechanical Engineering, Aalto University, Espoo 02150, Finland 3 Department of Mathematics, University College London, London, WC1E 6BT, UK; [email protected] * Correspondence: [email protected]; Tel./Fax: +81-7136-4880 † These authors contributed equally to this work. Academic Editor: Pavel Berloff Received: 11 April 2016; Accepted: 11 July 2016; Published: 19 July 2016 Abstract: The nonlinear Schrödinger equation (NLS) is a canonical evolution equation, which describes the dynamics of weakly nonlinear wave packets in time and space in a wide range of physical media, such as nonlinear optics, cold gases, plasmas and hydrodynamics. Due to its integrability, the NLS provides families of exact solutions describing the dynamics of localised structures which can be observed experimentally in applicable nonlinear and dispersive media of interest. Depending on the co-ordinate of wave propagation, it is known that the NLS can be either expressed as a space- or time-evolution equation. Here, we discuss and examine in detail the limitation of the first-order asymptotic equivalence between these forms of the water wave NLS. In particular, we show that the the equivalence fails for specific periodic solutions. We will also emphasise the impact of the studies on application in geophysics and ocean engineering. We expect the results to stimulate similar studies for higher-order weakly nonlinear evolution equations and motivate numerical as well as experimental studies in nonlinear dispersive media.
    [Show full text]
  • CHAPTER 7 Envelope Solitary Waves
    CHAPTER 7 Envelope solitary waves R.H.J. Grimshaw Department of Mathematical Sciences, Loughborough University, Loughborough, UK. Abstract In this chapter, we discuss envelope solitary waves that arise when a plane peri- odic wave is amplitude modulated. In general, the modulation leads to a rapidly oscillating carrier wave with a slowly varying envelope. In the weakly nonlinear regime, envelope waves are described by the nonlinear Schrödinger equation when attention is confined to just one spatial dimension. We shall focus our attention on capillary–gravity waves, although envelope waves can arise in many other fluid flow situations. When the nonlinear Schrödinger equation is of the focusing type, it supports solitary waves (solitons). However, these solitary waves do not lead to a steady solution of the full physical system, as the carrier’s phase speed and the envelope’s group velocity are not usually equal. But in the special circumstances when the phase and group velocities do coincide, there is a bifurcation to a steady envelope solitary wave. Our main interest is in capillary–gravity waves, and for these we give many details. Extensions to waves in more than one space dimension is based on the Benney–Roskes system, and leads to ‘lump’ solitary waves. 1 Linear waves and group velocity As noted in Chapter 1, there are two classes of solitary waves of interest, each of which can be regarded as a bifurcation from those points in the linear spec- trum where the group velocity and phase velocity are equal. When this bifurcation occurs in the long-wave limit, it leads typically to the Korteweg–de Vries equation and its solitary wave solutions.
    [Show full text]