Effect of Quantum Fluctuations on Structural Phase Transitions In

Total Page:16

File Type:pdf, Size:1020Kb

Effect of Quantum Fluctuations on Structural Phase Transitions In PHYSICAL REVIEW B VOLUME 53, NUMBER 9 1 MARCH 1996-I Effect of quantum fluctuations on structural phase transitions in SrTiO 3 and BaTiO 3 W. Zhong and David Vanderbilt Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08855-0849 ~Received 20 September 1995! Using path-integral Monte Carlo simulations and an ab initio effective Hamiltonian, we study the effects of quantum fluctuations on structural phase transitions in the cubic perovskite compounds SrTiO 3 and BaTiO 3 . We find quantum fluctuations affect ferroelectric ~FE! transitions more strongly than antiferrodistor- tive ~AFD! ones, even though the effective mass of a single FE local mode is larger. For SrTiO 3 we find that the quantum fluctuations suppress the FE transition completely, and reduce the AFD transition temperature from 130 to 110 K. For BaTiO 3 , quantum fluctuations do not affect the order of the transition, but do reduce the transition temperature by 35–50 K. The implications of the calculations are discussed. 12,13 Quantum fluctuations typically have a very important ef- BaTiO 3 ~Refs. 10 and 11! and SrTiO 3 , giving good fect on the structural and thermodynamic properties of ma- agreement with experimental observations. Treating atomic terials consisting of light atoms like hydrogen and helium. motion classically, it predicted FE phase transitions for For example, quantum effects introduce large corrections to SrTiO3 at low temperature, thus giving indirect support for the calculated hydrogen density distribution in the Nb:H the notion that quantum fluctuations ~not included in the system.1 For materials with heavier atoms, however, the theory! must be responsible for the observed absence of a quantum fluctuation can have only a small effect on the dis- low-temperature FE phase. tribution of atomic displacements, and thus typically do not In the present work, we have extended the previous treat- have a noticeable effect on the structural and thermodynamic ment of the first-principles based effective Hamiltonian to properties of the material. However, exceptions may occur. include quantum fluctuations. In particular, we use path- As we shall see, the cubic perovskites can exhibit decisive integral ~PI! quantum Monte Carlo simulations to study the quantum-fluctuation effects, despite the fact that the lightest effect of quantum fluctuations on the structural phase transi- constituent is oxygen. This can occur because these materials tions in SrTiO and BaTiO . For SrTiO , we find that the have several competing structures with very small structural 3 3 3 quantum fluctuations have only a modest effect on the AFD and energetic differences.2 transition temperature, while the FE transition is suppressed A good example is SrTiO . While it has the simple cubic 3 entirely. We discuss the relative importance of AFD and FE perovskite structure at high temperature, SrTiO goes 3 quantum fluctuations in some detail, and examine the poten- through an antiferrodistortive ~AFD! transition at 105 K to a tetragonal phase in which the oxygen octahedra have rotated tial implications of our results for understanding the low- in opposite senses in neighboring unit cells. The observed temperature behavior of the material. For BaTiO 3 , in which softening of the ferroelectric ~FE! polar phonons with further the FE transitions occur at higher temperature, we find that reduction of temperature in the range 50–100 K would ap- the quantum effects are less dramatic. pear to extrapolate to a FE transition close to 20 K, but We start by reviewing the effective Hamiltonian and its instead the softening saturates and no such transition is construction. Two approximations are involved. First, since observed.3 The absence of a true FE transition is suggested to both the FE and AFD transitions involve only small struc- be suppressed by quantum fluctuations, giving rise to a tural distortions, we represent the energy surface by a Taylor ‘‘quantum paraelectric’’ phase at very low temperature.4 expansion around the high-symmetry cubic perovskite struc- Some experiments appear to suggest a sharp transition to this ture, including up to fourth-order anharmonic terms. Second, low-temperature phase at about 40 K, perhaps indicating the because only low-energy distortions are important to the formation of some kind quantum coherent state.5,6 However, structural properties, we include only three such distortions until a plausible candidate for the order parameter of the in our expansion: the soft FE mode, the AFD mode, and an low-temperature phase is put forward, these ideas must re- elastic mode. These are represented, respectively, by local- main highly speculative. mode amplitudes fi , ai , and ui , where i is a cell index. The These developments have stimulated many theoretical ef- local modes are constructed in such a way that a uniform ~or, 4,7–9 forts to understand the quantum effects in SrTiO 3 . How- for AFD, a uniformly staggered! arrangement of the mode ever, the previous work has all been qualitative or empirical vectors represents the desired low-energy excitation.11 Thus, in approach. Although it was shown that quantum zero-point we work with local-mode vectors instead of atomic displace- motion is capable of suppressing phase transitions,9 a de- ments. This reduces the number of degrees of freedom from tailed microscopic approach is needed to gain a quantitative 15 to 9 per cell and greatly reduces the complexity of the and detailed understanding of the quantum effects at finite Taylor expansion. The Hamiltonian is specified by a set of temperature. Recently, an ab initio effective-Hamiltonian expansion parameters determined using highly accurate first- scheme has been developed to study structural phase transi- principles calculations with Vanderbilt ultrasoft tions of cubic perovskites. It has been successfully applied to pseudopotentials.14 The details of the Hamiltonian, the first- 0163-1829/96/53~9!/5047~4!/$10.0053 5047 © 1996 The American Physical Society 5048 BRIEF REPORTS 53 principles calculations, and the values of the expansion pa- Here, i and j are the cell indices, while a and b denote rameters have been reported elsewhere.10–13 Cartesian components. j(ia) is the eigenvector describing In our previous work, we have used this effective Hamil- atomic displacements associated with local mode f ia , and M tonian by applying Monte Carlo simulation techniques to is a ~diagonal! mass matrix in the 15L3-dimensional space of study the thermodynamics of the system in the classical atomic displacements of our L3L3L supercell. Similarly, limit. Assuming the ionic motions are classical is usually a mass matrix elements connecting different kinds of local good approximation for systems such as cubic perovskites vectors, such as those between fi and ai , are also included. containing atoms no less massive than oxygen. However, the The entire mass matrix can be calculated once and for all, structural differences and energy barriers between the cubic and the extension of the PI technique to handle a nondiago- structure and the possible ~rhombohedral or tetragonal! dis- nal mass matrix is straightforward. torted structures are very small. A rough estimate of the im- The study of the thermodynamic properties of the classi- portance of quantum fluctuations can be obtained from the cal system is performed using Monte Carlo ~MC! Heisenberg uncertainty principle Dp•Dq>\/2, or equiva- simulations.18 The original simulation cell is an L3L3L lently, cube, with three vectors fi , ai , and ui at each lattice point i. 2 2 Periodic boundary conditions are used, and homogeneous DE>\ /~8mDq !. ~1! strains of the entire supercell are included. Each local vector 3 Here, Dq denotes the uncertainty in the structural coordinate, is converted to a string of P beads, so that we have 9PL which is related to the structural difference between phases. degrees of freedom per simulation supercell. We use a DE is the energy uncertainty, or zero-point energy, which single-flip algorithm, making trial moves of the vectors at may prevent the occurrence of the distorted phase if it is each site in turn and testing acceptance after each move. We larger than the classical free-energy reduction. So if the say that one Monte Carlo sweep ~MCS! has been completed structural and energetic differences between phases are small when all vectors on all sites have been tried once. Because of enough, quantum suppression may occur even for fairly mas- the 1% lattice-constant error in our local-density approxima- sive ions. For a quantitative understanding, we need to per- tion ~LDA! calculations and the strong sensitivity of the form statistical simulations that treat the ionic motion quan- structural transitions to the lattice constant, all our simula- tum mechanically. tions are performed at a negative pressure to restore the ex- 10–13 Here, we adopt the path-integral ~PI! technique15 of quan- periment lattice constant, as in our previous work. tum simulations, which has proven to be a very successful The Trotter number P should be large enough to ensure method for studying H- and He-related systems.1,16 The that the quantum effects are correctly accounted for. On the method is based on Feynman’s PI formulation of quantum other hand, the computational load increases rapidly with mechanics.17 This formulation states that the partition func- increasing P, because of both larger system size and longer tion of the original quantum-statistical systems of particles correlation time with larger P. In our simulation, the proper can be approximated by the partition function of P sub- Trotter number for each temperature is chosen empirically. systems of classical particles with each quantum particle re- For a certain temperature, we simulate systems with increas- placed by a cyclic chain of P beads coupled by harmonic ing Trotter number P51,2,4,8,16,.... We equilibrate springs. Each subsystem ~comprising one bead from each systems with each P and monitor their order parameters.
Recommended publications
  • The Union of Quantum Field Theory and Non-Equilibrium Thermodynamics
    The Union of Quantum Field Theory and Non-equilibrium Thermodynamics Thesis by Anthony Bartolotta In Partial Fulfillment of the Requirements for the degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 Defended May 24, 2018 ii c 2018 Anthony Bartolotta ORCID: 0000-0003-4971-9545 All rights reserved iii Acknowledgments My time as a graduate student at Caltech has been a journey for me, both professionally and personally. This journey would not have been possible without the support of many individuals. First, I would like to thank my advisors, Sean Carroll and Mark Wise. Without their support, this thesis would not have been written. Despite entering Caltech with weaker technical skills than many of my fellow graduate students, Mark took me on as a student and gave me my first project. Mark also granted me the freedom to pursue my own interests, which proved instrumental in my decision to work on non-equilibrium thermodynamics. I am deeply grateful for being provided this priviledge and for his con- tinued input on my research direction. Sean has been an incredibly effective research advisor, despite being a newcomer to the field of non-equilibrium thermodynamics. Sean was the organizing force behind our first paper on this topic and connected me with other scientists in the broader community; at every step Sean has tried to smoothly transition me from the world of particle physics to that of non-equilibrium thermody- namics. My research would not have been nearly as fruitful without his support. I would also like to thank the other two members of my thesis and candidacy com- mittees, John Preskill and Keith Schwab.
    [Show full text]
  • Path Integral and Asset Pricing
    Path Integral and Asset Pricing Zura Kakushadze§†1 § Quantigicr Solutions LLC 1127 High Ridge Road #135, Stamford, CT 06905 2 † Free University of Tbilisi, Business School & School of Physics 240, David Agmashenebeli Alley, Tbilisi, 0159, Georgia (October 6, 2014; revised: February 20, 2015) Abstract We give a pragmatic/pedagogical discussion of using Euclidean path in- tegral in asset pricing. We then illustrate the path integral approach on short-rate models. By understanding the change of path integral measure in the Vasicek/Hull-White model, we can apply the same techniques to “less- tractable” models such as the Black-Karasinski model. We give explicit for- mulas for computing the bond pricing function in such models in the analog of quantum mechanical “semiclassical” approximation. We also outline how to apply perturbative quantum mechanical techniques beyond the “semiclas- sical” approximation, which are facilitated by Feynman diagrams. arXiv:1410.1611v4 [q-fin.MF] 10 Aug 2016 1 Zura Kakushadze, Ph.D., is the President of Quantigicr Solutions LLC, and a Full Professor at Free University of Tbilisi. Email: [email protected] 2 DISCLAIMER: This address is used by the corresponding author for no purpose other than to indicate his professional affiliation as is customary in publications. In particular, the contents of this paper are not intended as an investment, legal, tax or any other such advice, and in no way represent views of Quantigic Solutions LLC, the website www.quantigic.com or any of their other affiliates. 1 Introduction In his seminal paper on path integral formulation of quantum mechanics, Feynman (1948) humbly states: “The formulation is mathematically equivalent to the more usual formulations.
    [Show full text]
  • Critical Notice: the Quantum Revolution in Philosophy (Richard Healey; Oxford University Press, 2017)
    Critical notice: The Quantum Revolution in Philosophy (Richard Healey; Oxford University Press, 2017) DAVID WALLACE Richard Healey’s The Quantum Revolution in Philosophy is a terrific book, and yet I disagree with nearly all its main substantive conclusions. The purpose of this review is to say why the book is well worth your time if you have any interest in the interpretation of quantum theory or in the general philosophy of science, and yet why in the end I think Healey’s ambitious project fails to achieve its full goals. The quantum measurement problem is the central problem in philosophy of quantum mechanics, and arguably the most important issue in philosophy of physics more generally; not coincidentally, it has seen some of the field’s best work, and some of its most effective engagement with physics. Yet the debate in the field largely now appears deadlocked: the last few years have seen developments in our understanding of many of the proposed solutions, but not much movement in the overall dialectic. This is perhaps clearest with a little distance: metaphysicians who need to refer to quantum mechanics increasingly tend to talk of “the three main interpretations” (they mean: de Broglie and Bohm’s hidden variable theory; Ghirardi, Rimini and Weber’s (‘GRW’) dynamical-collapse theory; Everett’s many- universes theory) and couch their discussions so as to be, as much as possible, equally valid for any of those three. It is not infrequent for philosophers of physics to use the familiar framework of underdetermination of theory by evidence to discuss the measurement problem.
    [Show full text]
  • The Path Integral Approach to Quantum Mechanics Lecture Notes for Quantum Mechanics IV
    The Path Integral approach to Quantum Mechanics Lecture Notes for Quantum Mechanics IV Riccardo Rattazzi May 25, 2009 2 Contents 1 The path integral formalism 5 1.1 Introducingthepathintegrals. 5 1.1.1 Thedoubleslitexperiment . 5 1.1.2 An intuitive approach to the path integral formalism . .. 6 1.1.3 Thepathintegralformulation. 8 1.1.4 From the Schr¨oedinger approach to the path integral . .. 12 1.2 Thepropertiesofthepathintegrals . 14 1.2.1 Pathintegralsandstateevolution . 14 1.2.2 The path integral computation for a free particle . 17 1.3 Pathintegralsasdeterminants . 19 1.3.1 Gaussianintegrals . 19 1.3.2 GaussianPathIntegrals . 20 1.3.3 O(ℏ) corrections to Gaussian approximation . 22 1.3.4 Quadratic lagrangians and the harmonic oscillator . .. 23 1.4 Operatormatrixelements . 27 1.4.1 Thetime-orderedproductofoperators . 27 2 Functional and Euclidean methods 31 2.1 Functionalmethod .......................... 31 2.2 EuclideanPathIntegral . 32 2.2.1 Statisticalmechanics. 34 2.3 Perturbationtheory . .. .. .. .. .. .. .. .. .. .. 35 2.3.1 Euclidean n-pointcorrelators . 35 2.3.2 Thermal n-pointcorrelators. 36 2.3.3 Euclidean correlators by functional derivatives . ... 38 0 0 2.3.4 Computing KE[J] and Z [J] ................ 39 2.3.5 Free n-pointcorrelators . 41 2.3.6 The anharmonic oscillator and Feynman diagrams . 43 3 The semiclassical approximation 49 3.1 Thesemiclassicalpropagator . 50 3.1.1 VanVleck-Pauli-Morette formula . 54 3.1.2 MathematicalAppendix1 . 56 3.1.3 MathematicalAppendix2 . 56 3.2 Thefixedenergypropagator. 57 3.2.1 General properties of the fixed energy propagator . 57 3.2.2 Semiclassical computation of K(E)............. 61 3.2.3 Two applications: reflection and tunneling through a barrier 64 3 4 CONTENTS 3.2.4 On the phase of the prefactor of K(xf ,tf ; xi,ti) ....
    [Show full text]
  • Quantum Fluctuation
    F EATURE Kavli IPMU Principal Investigator Eiichiro Komatsu Research Area: Theoretical Physics Quantum Fluctuation The 20th century has seen the remarkable is not well known to the public. This ingredient development of the Standard Model of elementary is not contained in the name of ΛCDM, but is particles and elds. The last piece, the Higgs particle, an indispensable part of the Standard Model of was discovered in 2012. In the 21st century, we are cosmology. It is the idea that our ultimate origin is witnessing the similarly remarkable development the quantum mechanical uctuation generated in of the Standard Model of cosmology. In his 2008 the early Universe. However remarkable it may sound, book on“ Cosmology” Steven Weinberg, who led this idea is consistent with all the observational data the development of particle physics, wrote“: This that have been collected so far for the Universe. new excitement in cosmology came as if on cue Furthermore, the evidence supporting this idea keeps for elementary particle physicists. By the 1980s the accumulating and is strengthened as we collect more Standard Model of elementary particles and elds data! It is likely that all the structures we see today in had become well established. Although signicant the Universe, such as galaxies, stars, planets, and lives, theoretical and experimental work continued, there ultimately originated from the quantum uctuation was now little contact between experiment and new in the early Universe. theoretical ideas, and without this contact, particle physics lost much of its liveliness. Cosmology now Borrowing energy from the vacuum offered the excitement that particle physicists had experienced in the 1960s and 1970s.” In quantum mechanics, we can borrow energy The Standard Model of cosmology is known from the vacuum if we promise to return it as the“ ΛCDM model”.
    [Show full text]
  • Electronic Zero-Point Fluctuation Forces Inside Circuit Components Arxiv
    Electronic zero-point fluctuation forces inside circuit components Ephraim Shahmoon1 and Ulf Leonhardt2 1Department of Physics, Harvard University, Cambridge MA 02138, USA 2Department of Physics of Complex Systems, Weizmann Institute of Science, Rehovot 761001, Israel May 1, 2018 One of the most intriguing manifestations of quantum zero-point fluctuations are the van der Waals and Casimir forces, often associated with vacuum fluc- tuations of the electromagnetic field. Here we study generalized fluctuation potentials acting on internal degrees of freedom of components in electrical circuits. These electronic Casimir-like potentials are induced by the zero-point current fluctuations of any general conductive circuit. For realistic examples of an electromechanical capacitor and a superconducting qubit, our results re- veal the possibility of tunable forces between the capacitor plates, or the level shifts of the qubit, respectively. Our analysis suggests an alternative route to- wards the exploration of Casimir-like fluctuation potentials, namely, by char- acterizing and measuring them as a function of parameters of the environ- ment. Such tunable potentials may be useful for future nanoelectromechanical and quantum technologies. arXiv:1612.03250v2 [quant-ph] 29 Apr 2018 Introduction Understanding the role of quantum phenomena in electrical circuits has opened numerous pos- sibilities in quantum information and optics (1, 2). In this article we show how conceptually simple systems, such as linear electrical circuits, provide a new direction in the study and appli- cation of quantum fluctuation phenomena, in analogy to the van der Waals (vdW) and Casimir forces (3, 4, 5). A key element of the ensuing discussion is the generalization of the familiar Casimir force in three aspects; namely, the source of the quantum fluctuations, the physical effect they entail and, most importantly, how the effect is measured and manipulated.
    [Show full text]
  • Quantum Fluctuations of Vector Fields and the Primordial Curvature Perturbation in the Universe
    Quantum Fluctuations of Vector Fields and the Primordial Curvature Perturbation in the Universe Mindaugas Karčiauskas MSc, BSc December 2009 This thesis is submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy. No part of this thesis has been previously submitted for the award of a higher degree. arXiv:1009.1779v1 [astro-ph.CO] 9 Sep 2010 “What he [a scientist] is really seeking is to learn something new that has a cer- tain fundamental kind of significance: a hitherto unknown lawfulness in the order of nature, which exhibits unity in a broad range of phenomena. Thus, he wishes to find in the reality in which he lives a cer- tain oneness and totality, or wholeness, constituting a kind of harmony that is felt to be beautiful. In this respect, the scientist is perhaps not basically differ- ent from the artist, the architect, the music composer, etc., who all want to create this sort of thing in their work.” David Bohm Acknowledgments This thesis is a culmination of more than three years spend in England as a PhD student, which signify not only my scientific achievements but also people I met and moments experienced together. Although written by me, these pages include contributions from all these people without whom this would be just a collection of blank paper. Some of contributions are too subtle to put into words, but each of them is essential and invaluable. It is impossible to name everyone, so I sincerely apologize those whose name is not mentioned here. First and foremost I want to say thank you to Milda Beišyt˙e.
    [Show full text]
  • On Heisenberg Uncertainty Relationship, Its Extension, and the Quantum Issue of Wave-Particle Duality
    Int. J. Mol. Sci. 2010, 11, 4124-4139; doi:10.3390/ijms11104124 OPEN ACCESS International Journal of Molecular Sciences ISSN 1422-0067 www.mdpi.com/journal/ijms Article On Heisenberg Uncertainty Relationship, Its Extension, and the Quantum Issue of Wave-Particle Duality Mihai V. Putz 1,2 1 Laboratory of Computational and Structural Physical Chemistry, Chemistry Department, West University of Timişoara, Pestalozzi Street No.16, Timişoara, RO-300115, Romania; E-Mail: [email protected] or [email protected]; Tel.: ++40-256-592-633; Fax: ++40-256-592-620; Web: www.mvputz.iqstorm.ro 2 Theoretical Physics Institute, Free University Berlin, Arnimallee 14, 14195 Berlin, Germany Received: 11 August 2010; in revised form: 27 September 2010 / Accepted: 17 October 2010 / Published: 22 October 2010 Abstract: Within the path integral Feynman formulation of quantum mechanics, the fundamental Heisenberg Uncertainty Relationship (HUR) is analyzed in terms of the quantum fluctuation influence on coordinate and momentum estimations. While introducing specific particle and wave representations, as well as their ratio, in quantifying the wave-to-particle quantum information, the basic HUR is recovered in a close analytical manner for a large range of observable particle-wave Copenhagen duality, although with the dominant wave manifestation, while registering its progressive modification with the factor 1 n2 , in terms of magnitude n0,1 of the quantum fluctuation, for the free quantum evolution around the exact wave-particle equivalence. The practical implications of the present particle-to-wave ratio as well as of the free-evolution quantum picture are discussed for experimental implementation, broken symmetry and the electronic localization function.
    [Show full text]
  • Quantum Fluctuations, Decoherence of the Mean Field, and Structure
    Quantum Fluctuations, Decoherence of the Mean Field, and Structure Formation in the Early Universe E. Calzetta IAFE and FCEN, University of Buenos Aires, Argentina B. L. Hu Department of Physics, University of Maryland, College Park, MD 20742, USA School of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540, USA (IASSNS-HEP-95/38, UMDPP 95-083, May 9, 1995) arXiv:gr-qc/9505046v1 24 May 1995 1 1 Introduction and Summary In this paper we shall examine, starting from first principles, under what circumstances the fluctuations of a quantum field transmute into classical, stochastic fluctuations. To do so we shall analyze the relationship between the phenomena of dissipation, fluctuation, noise and decoherence [1], first in an interacting scalar field theory in flat space time [2], and then in the more complex but realistic case of a scalar field interacting with gravitons in an expanding Universe. The main motivation for this work is to develop the necessary tools to analyze the quan- tum to classical transition of primordial density fluctuations in the early universe. Indeed, this is the third of a series of papers by the authors and collaborators on the quantum statistical theory of structure formation. The first one [3] calls into question conventional treatments of this issue, and focuses on decoherence and the quantum origin of noise in stochastic inflation. The second one [4] explains how noise and fluctuations originate from particle creation in semiclassical gravity, and casts doubt on the conventional practise of simplistically identifying quantum and classical fluctuations. In this paper we will discuss how a quantum mean field can be decohered by its own quantum fluctuations, turning into a classical stochastic field.
    [Show full text]
  • Chapter 3 Feynman Path Integral
    Chapter 3 Feynman Path Integral The aim of this chapter is to introduce the concept of the Feynman path integral. As well as developing the general construction scheme, particular emphasis is placed on establishing the interconnections between the quantum mechanical path integral, classical Hamiltonian mechanics and classical statistical mechanics. The practice of path integration is discussed in the context of several pedagogical applications: As well as the canonical examples of a quantum particle in a single and double potential well, we discuss the generalisation of the path integral scheme to tunneling of extended objects (quantum fields), dissipative and thermally assisted quantum tunneling, and the quantum mechanical spin. In this chapter we will temporarily leave the arena of many–body physics and second quantisation and, at least superficially, return to single–particle quantum mechanics. By establishing the path integral approach for ordinary quantum mechanics, we will set the stage for the introduction of functional field integral methods for many–body theories explored in the next chapter. We will see that the path integral not only represents a gateway to higher dimensional functional integral methods but, when viewed from an appropriate perspective, already represents a field theoretical approach in its own right. Exploiting this connection, various techniques and concepts of field theory, viz. stationary phase analyses of functional integrals, the Euclidean formulation of field theory, instanton techniques, and the role of topological concepts in field theory will be motivated and introduced in this chapter. 3.1 The Path Integral: General Formalism Broadly speaking, there are two basic approaches to the formulation of quantum mechan- ics: the ‘operator approach’ based on the canonical quantisation of physical observables Concepts in Theoretical Physics 64 CHAPTER 3.
    [Show full text]
  • Fundamental Aspects of Quantum Brownian Motion
    CHAOS 15, 026105 ͑2005͒ Fundamental aspects of quantum Brownian motion Peter Hänggi and Gert-Ludwig Ingold Institut für Physik, Universität Augsburg, 86135 Augsburg, Germany ͑Received 1 December 2004; accepted 9 December 2004; published online 17 June 2005͒ With this work we elaborate on the physics of quantum noise in thermal equilibrium and in stationary nonequilibrium. Starting out from the celebrated quantum fluctuation-dissipation theorem we discuss some important consequences that must hold for open, dissipative quantum systems in thermal equilibrium. The issue of quantum dissipation is exemplified with the fundamental problem of a damped harmonic quantum oscillator. The role of quantum fluctuations is discussed in the context of both, the nonlinear generalized quantum Langevin equation and the path integral ap- proach. We discuss the consequences of the time-reversal symmetry for an open dissipative quan- tum dynamics and, furthermore, point to a series of subtleties and possible pitfalls. The path integral methodology is applied to the decay of metastable states assisted by quantum Brownian noise. © 2005 American Institute of Physics. ͓DOI: 10.1063/1.1853631͔ This work deals with the description of quantum Brown- the substitution of the energy kBT from the classical equipar- ian motion in linear and nonlinear quantum systems that tition law4 by the thermally averaged quantum energy ͑but exhibit frictional influences. The symmetries of thermal leaving out the zero point energy contribution͒ of the har- equilibrium impose severe constraints on the time evolu- monic oscillator. Nyquist’s remark thus constitutes a precur- tion properties of open quantum systems. These lead to a sor of the celebrated work by Callen and Welton5 who gen- quantum generalization of the classical Einstein relation eralized the relations by Einstein, Nyquist, and Johnson to that connects friction with the strength of thermal quan- include quantum effects: In their work they put forward a tum fluctuations.
    [Show full text]
  • 5 Fluctuations from Inflation
    may well not move very much during the last phases – our observations relate only to a small piece of the potential, and we cannot hope to recover its form without substantial a priori knowledge; stimulating, because observations even on very large scales must relate to a period where the simple concepts of exponential inflation and scale-invariant density fluctuations were coming close to breaking down. This opens the possibility of testing inflation theories in a way that would not be possible with data relating to only the simpler early phases. These tests take the form of tilt and gravitational waves in the final perturbation spectrum, to be discussed further below. 5 Fluctuations from inflation Topics to be covered: Description of inhomogeneity • Mechanisms for fluctuation generation • Tilt and tensor modes • Eternal inflation • 5.1 The perturbed universe We now need to consider the greatest achievement of inflation, which was not anticipated when the theory was first put forward: it provides a concrete mechanism for generating the seeds of structure in the universe. In essence, the idea is that the inevitable small quantum fluctuations in the inflaton field φ are transformed into residual classical fluctuations in density when inflation is over. The details of this process can be technical, and could easily fill a lecture course. The following treatment is therefore simplified as far as possible, while still making contact with the full results. quantifying inhomogeneity The first issue we have to deal with is how to quantify departures from uniform density. Frequently, an intuitive Newtonian approach can be used, and we will adopt this wherever possible.
    [Show full text]