The Casimir Effect

Total Page:16

File Type:pdf, Size:1020Kb

The Casimir Effect IFPA, AGO Department University of Liège THE CASIMIR EFFECT J. Cugnon University of Liège HLPW10, Spa, 6-8 April 2011 ● Dark energy ● The Casimir effect as a manifestation of quantum vacuum energy ● Dependence upon the fine structure constant ● The Casimir effect as a van der Waals force between giant « molecules » ● « Reality » of quantum fluctuations in the vacuum? ● Conclusion H, Wroclaw, 9-11 July 2009 DARK ENERGY from Hubble plot at large red shifts and CMB fluctuations Dark energy has a constant energy density and a negative pressure 3 DE≃3/4c≃4GeV /m Dark matter energyzero point energy of quantum fields - first proposed by Zeldovitch (1957) - confirmed by Casimir effect, according... S. Weinberg, 1987 Perhaps surprisingly, it was a long time before particle physicists began seriously to worry about [quantum zero point fluctuations contribution to L] despite the demonstration in the Casimir effect of the reality of zero-point energies. S. M. Carroll, 2001 ... and the vacuum fluctuations themselves are very real, as evidenced by the Casimir effect. D. Perkins, « Particle Astrophysics », Oxford Univ. Press, 2008 That this concept [the vacuum energy] is not a figment of the physicist©s imagination was already demonstrated many years ago, when Casimir predicted that by modifying boundary conditions on the vacuum state, the change of the vacuum energy would lead to a measurable force, subsequently detected and measured by... For a free bosonic field: k cut 3 ∫ d k 1 4 =∑ 1/2 ℏ=ℏ c k= ℏ c kcut 2 3 82 121 3 For kcut ~1/ℓPL , e ~10 GeV/m For a free fermionic field: =−∑ 1/2 ℏ ... and there are plenty of condensates in the SM ! THE CASIMIR FORCE and the ZERO POINT ENERGY of the ELECTROMAGNETIC FIELD The modes in the cavity are not the same as in free space, especially at low frequency Interaction energy=difference of zero-point energies ik x ik y ik z −i t ik x ik y −i t x y z k x y k E= e e e e ⇔ E= e e sin k z z e k z=nz /d for nz=1,2,3,.... Rm: for nz=0, only one mode E E cav E free = − S S S ∞ ∞ ∞ ∞ ∞ ℏ c2 1 = 2− 2 3 ∫ du u ∑∫ du u n ∫ dx∫ du u x 4 d {2 0 n=1 0 0 0 } 2 Rm: regularized by integration factor e− ux , 0 Euler-McLaurin theorem: ∞ ∞ 1 1 1 1 f 0∑ f n−∫ f x =− f ∞ [ f © 0− f © ∞]− [ f © © © 0− f © © © ∞] 2 n=1 0 2 12 720 E ℏ c2 =− See Itzykson and Zuber S 720 d3 The Casimir force 2 F ℏ c − =− =4×10 4 N /m2 at d=1 m S 240 d 4 has been calculated for many « geometries » has been verified experimentally - M. J. Sparnaay, Physica 24 (1958) 751 parallelism, impurities, residual charges - M. J. Spaarnay, P. W. J. Jochems, 1960 - B. V. Darjaguin et al, « Surface forces », Plenum, 1987 - S. K. Lamoreaux, PRL 78 (1997) 5 - T. Ederth (2001?) 1% Now, a blooming field in MEMS technology -from attractive to repulsive -turned to be a control tool A field of its own DEPENDANCE on the FINE STRUCTURE CONSTANT Universality? Independence of a? Real conductors are characterized by: - plasma frequency wpl : no propagation for w < wpl - skin depth d; d-2 = 2p w|s| /c : penetration depth of incident waves Drude model: free electrons with friction force (f=-gv) −1/2 2 2 4 e n 1 pl = =c pl m 2 22 e Limit of perfect conductor: wpl ∞, d 0 Perfect metal hypothesis is justified if characteristic frequencies c/d << wpl i.e. m c ≫ e 4 ℏ n d2 For typical cases (Cu, d=1mm), rhs ~ 10-6 - This condition is comfortably satisfied for the physical value of a - Casimir©s result = the a ∞ limit !!!! - corrections appears as powers of 1/a E ℏ c2 ℏ c2 ≈− ≈− 1−6 ⋯ S 720d2 3 720 d3 d Small a limit 2 ℏ 3 2 2 aB= 2 ∝1/ , n∝ , pl ∝ , ∝1/ me e Conducting plates become transparent and Casimir effect goes away The only distinctive feature: goes to a constant in the strong coupling limit CASIMIR EFFECT as a VAN DER WAALS FORCE between MACROSCOPIC NEUTRAL OBJECTS Two neutral atoms at distance r : effects of Coulomb forces 2 London (1937) : 2d order in a and in Rat/r 4 2 2 1 2 e ∣a ∣ ∣a ∣ 2 =− k0 l0 , a = k∣ z ∣0 E 6 6 ∑∑ 2 2 1 1 k0 〈 ∑ i 〉 r k≠0 l≠0 E k −E0 El −E 0 Atom 2 1 ∣ai∣2 = 2 k0 =14 n Static atomic polarizability i e ∑ i i at k≠0 E k −E 0 -Known for: Casimir operator, hyperfine interactions, cooling by adiabatic demagnetization (mK), etc -PhD of Erhenfest, assistant of Pauli, position in Leiden -In 1940, moved to Philips gloeilampenfabriek NV in Eindhoven In 1947, EJW Verwey and JTG Overbeek : dilute colloidal suspensions HBG Casimir and D. Polder, Phys. Rev 73 (1948) 360: Interaction between atoms through Coulomb forces and the coupling to the radiation field (retardation effects) Perturbation theory at the second order in a ● ● L r For small r, London©s expression is recovered For r >> ako : ℏ 2 23 c (1) E =− 1 2 4r 7 In the same paper, interaction of a atom with a conducting plane 2 e 2 =− ∣ ∣2 For small d : E atom−wall 3 ∑ ak0 4 d k d ℏ For d >> ako : 2 3 c (2) E atom−wall=− 1 8 d 4 Perturbation theory at the first order in a (first order in Coulomb forces, second order in atom-radiation coupling) Niels Bohr: « Why don©t you calculate the effect by evaluating the differences of zero point energies of the electromagnetic field? » Casimir rederived results (1) and (2) by this method (in some approximation) : Colloque sur la théorie de la liaison chimique, Paris, 12-17 avril 1948 He calculated by the same method the interaction between parallel conducting planes H.B.G. Casimir, Proceedings of the Koninglijke Nederlandse Akademie van Wetenschappen B51, 793 (1948) 3 Limit of VdW-Casimir-Polder : lim ai / r = 1 London-VdW Casimir-Polder Order 4 2 2 1 2 2 e ∣ak0 ∣ ∣al0 ∣ E =−6 ∑ ∑ 2 23 ℏ c 6 2 2 1 1 E =− 1 2 r k≠0 l≠0 E −E E −E 7 k 0 l 0 4 r α2 2 2 e 2 3ℏ c E =− ∣a ∣ 2 =− α atom−wall 3 ∑ k0 E atom−wall 4 1 4 d k 8 d Replacing an atom by a plate : ℏ c2 −infinite volume withconstant n E=− Sd d 4 α0 −ni −1/ 720 − ∞ ai disappears, a power of a is absorbed !! replaced by a volume ! Same results by Casimir©s method ConclusionConclusion :: CasimirCasimir effecteffect == limitlimit ofof vanvan derder WaalsWaals forceforce forfor «« macroscopicmacroscopic moleculesmolecules »» inin thethe idealideal conductorconductor (infinitely(infinitely polarisable)polarisable) limitlimit The « REALITY » of QUANTUM FLUCTUATIONS in the VACUUM 1. Casimir©s result is « heuristic »: that the interaction energy is given by the difference of zero point energies is accidental and does not reveal the « reality » of quantum fluctuation energy 1 rr © 1 for a diffuse charge: W= ∫ dr∫ dr © = ∫∣E r∣2 dr 2 ∣r−r ©∣ 8 Rm: « reality » of the field coming from light, pair production, etc 2. Zero-point energy coming from an « obscure » choice of ordering fields in the classical lagrangian (giving negative energy for fermion fields) 3. Interaction between neutral objects gives no more (or less) support to the « reality » of the vacuum energy of fluctuating quantum fields than the other one-loop effects in quantum electrodynamics, like vacuum polarisation contribution in the Lamb shift (R. Jaffe, PR D72 (2005) 021301) : the effect vanishes as a 0 4. Casimir effect can be derived without reference to zero-point motion -general theory of fluctuations (Lifshitz, Zhur. eksp. i teor. fiz. 29 (1955) 9, Landau and Lifshitz, Electrodynamics of continuous media) 1 〈 Ei rEj r〉= f ,...W = ∫∣E∣2∣H∣2 8 no field quantization calculation of the interaction between semi-infinite pieces of dielectrics; Casimir force obtained as the e ∞ limit - field theory without reference to zero-point fluctuations: Schwinger, 1975, scalar field Schwinger, DeRaad, Milton, 1978, for QED ℏ E= ℑ∫ d Tr∫ d3 x[G x , x ,i −G x , x ,i ] 2 0 G is the full Green©s function in the background (plates) d N 1 E∝∫ d i.e. ∑ ℏ −ℏ d 2 0 G can be expanded in series of G0 and a Rm: all features of QED can be reformulated from the point of view of zero point fluctuations (Milonni, « The Quantum Vacuum », Acad. Press, 1994) CONCLUSIONS ● Casimir effect often advocated as a manifestation of the quantum fluctuations of the vacuum and the support of the latter as a candidate for DM. But... ● Casimir force can (should) be viewed as a vdW force between gigantic molecules in the strong coupling limit ● Casimir forces are real in the micro- to nano-world ● Not a demonstration of the « reality » of the zero-point energy (no more than vacuum polarisation, ...): vanishes in weak coupling, formulation without reference to zero-point energy ● Reality of vacuum energy? .
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]
  • 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.
    [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]