Spontaneous Symmetry Breaking and Mass Generation As Built-In Phenomena in Logarithmic Nonlinear Quantum Theory
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Lecture Notes: BCS Theory of Superconductivity
Lecture Notes: BCS theory of superconductivity Prof. Rafael M. Fernandes Here we will discuss a new ground state of the interacting electron gas: the superconducting state. In this macroscopic quantum state, the electrons form coherent bound states called Cooper pairs, which dramatically change the macroscopic properties of the system, giving rise to perfect conductivity and perfect diamagnetism. We will mostly focus on conventional superconductors, where the Cooper pairs originate from a small attractive electron-electron interaction mediated by phonons. However, in the so- called unconventional superconductors - a topic of intense research in current solid state physics - the pairing can originate even from purely repulsive interactions. 1 Phenomenology Superconductivity was discovered by Kamerlingh-Onnes in 1911, when he was studying the transport properties of Hg (mercury) at low temperatures. He found that below the liquifying temperature of helium, at around 4:2 K, the resistivity of Hg would suddenly drop to zero. Although at the time there was not a well established model for the low-temperature behavior of transport in metals, the result was quite surprising, as the expectations were that the resistivity would either go to zero or diverge at T = 0, but not vanish at a finite temperature. In a metal the resistivity at low temperatures has a constant contribution from impurity scattering, a T 2 contribution from electron-electron scattering, and a T 5 contribution from phonon scattering. Thus, the vanishing of the resistivity at low temperatures is a clear indication of a new ground state. Another key property of the superconductor was discovered in 1933 by Meissner. -
Path Integral Formulation of Loop Quantum Cosmology
Path Integral Formulation of Loop Quantum Cosmology Adam D. Henderson Institute for Gravitation and the Cosmos Pennsylvania State University International Loop Quantum Gravity Seminar March 17 2008 Motivations 1. There have been arguments against the singularity resolution in LQC using path integrals. The canonical quantization is well understood and the singularity resolution is robust, so where do the path integral arguments break down? 2. Recent developements have allowed for the construction of new spin foam models that are more closely related to the canonical theory. It is important to make connections to spin-foams by building path integrals from the canonical theory when possible. 3. A path integral representation of Loop Quantum Cosmology will aid in studying the physics of more complicated LQC models (k = 1, Λ = 0, Bianchi). Using standard path integral techniques one can 6 argue why the effective equations are so surprisingly accurate. Introduction We construct a path integral for the exactly soluble Loop Quantum • Cosmology starting with the canonical quantum theory. The construction defines each component of the path integral. Each • has non-trivial changes from the standard path integral. We see the origin of singularity resolution in the path integral • representation of LQC. The structure of the path integral features similarities to spin foam • models. The path integral can give an argument for the surprising accuracy • of the effective equations used in more complicated models. Outline Standard Construction Exactly Soluble LQC LQC Path Integral Other Forms of Path Integral Singularity Resolution/Effective Equations Conclusion Path Integrals - Overview Path Integrals: Covariant formulation of quantum theory expressed • as a sum over paths Formally the path integral can be written as • qeiS[q]/~ or q peiS[q,p]/~ (1) D D D Z Z To define a path integral directly involves defining the components • of these formal expressions: 1. -
Conformal Symmetry in Field Theory and in Quantum Gravity
universe Review Conformal Symmetry in Field Theory and in Quantum Gravity Lesław Rachwał Instituto de Física, Universidade de Brasília, Brasília DF 70910-900, Brazil; [email protected] Received: 29 August 2018; Accepted: 9 November 2018; Published: 15 November 2018 Abstract: Conformal symmetry always played an important role in field theory (both quantum and classical) and in gravity. We present construction of quantum conformal gravity and discuss its features regarding scattering amplitudes and quantum effective action. First, the long and complicated story of UV-divergences is recalled. With the development of UV-finite higher derivative (or non-local) gravitational theory, all problems with infinities and spacetime singularities might be completely solved. Moreover, the non-local quantum conformal theory reveals itself to be ghost-free, so the unitarity of the theory should be safe. After the construction of UV-finite theory, we focused on making it manifestly conformally invariant using the dilaton trick. We also argue that in this class of theories conformal anomaly can be taken to vanish by fine-tuning the couplings. As applications of this theory, the constraints of the conformal symmetry on the form of the effective action and on the scattering amplitudes are shown. We also remark about the preservation of the unitarity bound for scattering. Finally, the old model of conformal supergravity by Fradkin and Tseytlin is briefly presented. Keywords: quantum gravity; conformal gravity; quantum field theory; non-local gravity; super- renormalizable gravity; UV-finite gravity; conformal anomaly; scattering amplitudes; conformal symmetry; conformal supergravity 1. Introduction From the beginning of research on theories enjoying invariance under local spacetime-dependent transformations, conformal symmetry played a pivotal role—first introduced by Weyl related changes of meters to measure distances (and also due to relativity changes of periods of clocks to measure time intervals). -
Identical Particles
8.06 Spring 2016 Lecture Notes 4. Identical particles Aram Harrow Last updated: May 19, 2016 Contents 1 Fermions and Bosons 1 1.1 Introduction and two-particle systems .......................... 1 1.2 N particles ......................................... 3 1.3 Non-interacting particles .................................. 5 1.4 Non-zero temperature ................................... 7 1.5 Composite particles .................................... 7 1.6 Emergence of distinguishability .............................. 9 2 Degenerate Fermi gas 10 2.1 Electrons in a box ..................................... 10 2.2 White dwarves ....................................... 12 2.3 Electrons in a periodic potential ............................. 16 3 Charged particles in a magnetic field 21 3.1 The Pauli Hamiltonian ................................... 21 3.2 Landau levels ........................................ 23 3.3 The de Haas-van Alphen effect .............................. 24 3.4 Integer Quantum Hall Effect ............................... 27 3.5 Aharonov-Bohm Effect ................................... 33 1 Fermions and Bosons 1.1 Introduction and two-particle systems Previously we have discussed multiple-particle systems using the tensor-product formalism (cf. Section 1.2 of Chapter 3 of these notes). But this applies only to distinguishable particles. In reality, all known particles are indistinguishable. In the coming lectures, we will explore the mathematical and physical consequences of this. First, consider classical many-particle systems. If a single particle has state described by position and momentum (~r; p~), then the state of N distinguishable particles can be written as (~r1; p~1; ~r2; p~2;:::; ~rN ; p~N ). The notation (·; ·;:::; ·) denotes an ordered list, in which different posi tions have different meanings; e.g. in general (~r1; p~1; ~r2; p~2)6 = (~r2; p~2; ~r1; p~1). 1 To describe indistinguishable particles, we can use set notation. -
Neutrino Mass Models: a Road Map
Neutrino Mass Models: a road map S.F.King School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK E-mail: [email protected] Abstract. In this talk we survey some of the recent promising developments in the search for the theory behind neutrino mass and mixing, and indeed all fermion masses and mixing. The talk is organized in terms of a neutrino mass models road map according to which the answers to experimental questions provide sign posts to guide us through the maze of theoretical models eventually towards a complete theory of flavour and uni¯cation. 1. Introduction It has been one of the long standing goals of theories of particle physics beyond the Standard Model (SM) to predict quark and lepton masses and mixings. With the discovery of neutrino mass and mixing, this quest has received a massive impetus. Indeed, perhaps the greatest advance in particle physics over the past decade has been the discovery of neutrino mass and mixing involving two large mixing angles commonly known as the atmospheric angle θ23 and the solar angle θ12, while the remaining mixing angle θ13, although unmeasured, is constrained to be relatively small [1]. The largeness of the two large lepton mixing angles contrasts sharply with the smallness of the quark mixing angles, and this observation, together with the smallness of neutrino masses, provides new and tantalizing clues in the search for the origin of quark and lepton flavour. However, before trying to address such questions, it is worth recalling why neutrino mass forces us to go beyond the SM. -
Quantum Gravity from the QFT Perspective
Quantum Gravity from the QFT perspective Ilya L. Shapiro Universidade Federal de Juiz de Fora, MG, Brazil Partial support: CNPq, FAPEMIG ICTP-SAIFR/IFT-UNESP – 1-5 April, 2019 Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 Lecture 5. Advances topics in QG Induced gravity concept. • Effective QG: general idea. • Effective QG as effective QFT. • Where we are with QG?. • Bibliography S.L. Adler, Rev. Mod. Phys. 54 (1982) 729. S. Weinberg, Effective Field Theory, Past and Future. arXive:0908.1964[hep-th]; J.F. Donoghue, The effective field theory treatment of quantum gravity. arXive:1209.3511[gr-qc]; I.Sh., Polemic notes on IR perturbative quantum gravity. arXiv:0812.3521 [hep-th]. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 I. Induced gravity. The idea of induced gravity is simple, while its realization may be quite non-trivial, depending on the theory. In any case, the induced gravity concept is something absolutely necessary if we consider an interaction of gravity with matter and quantum theory concepts. I. Induced gravity from cut-off Original simplest version. Ya.B. Zeldovich, Sov. Phys. Dokl. 6 (1967) 883. A.D. Sakharov, Sov. Phys. Dokl. 12 (1968) 1040. Strong version of induced gravity is like that: Suppose that the metric has no pre-determined equations of motion. These equations result from the interaction to matter. Main advantage: Since gravity is not fundamental, but induced interaction, there is no need to quantize metric. Ilya Shapiro, Quantum Gravity from the QFT perspective April - 2019 And we already know that the semiclassical approach has no problems with renormalizability! Suppose we have a theory of quantum matter fields Φ = (ϕ, ψ, Aµ) interacting to the metric gµν . -
Electron-Phonon Interaction in Conventional and Unconventional Superconductors
Electron-Phonon Interaction in Conventional and Unconventional Superconductors Pegor Aynajian Max-Planck-Institut f¨ur Festk¨orperforschung Stuttgart 2009 Electron-Phonon Interaction in Conventional and Unconventional Superconductors Von der Fakult¨at Mathematik und Physik der Universit¨at Stuttgart zur Erlangung der W¨urde eines Doktors der Naturwissenschaften (Dr. rer. nat.) genehmigte Abhandlung vorgelegt von Pegor Aynajian aus Beirut (Libanon) Hauptberichter: Prof. Dr. Bernhard Keimer Mitberichter: Prof. Dr. Harald Giessen Tag der m¨undlichen Pr¨ufung: 12. M¨arz 2009 Max-Planck-Institut f¨ur Festk¨orperforschung Stuttgart 2009 2 Deutsche Zusammenfassung Die Frage, ob ein genaueres Studium der Phononen-Spektren klassischer Supraleiter wie Niob und Blei mittels inelastischer Neutronenstreuung der M¨uhe wert w¨are, w¨urde sicher von den meisten Wissenschaftlern verneint werden. Erstens erk¨art die ber¨uhmte mikroskopische Theorie von Bardeen, Cooper und Schrieffer (1957), bekannt als BCS Theorie, nahezu alle Aspekte der klassischen Supraleitung. Zweitens ist das aktuelle Interesse sehr stark auf die Hochtemperatur-Supraleitung in Kupraten und Schwere- Fermionen Systemen fokussiert. Daher waren die ersten Experimente dieser Arbeit, die sich mit der Bestimmung der Phononen-Lebensdauern in supraleitendem Niob und Blei befaßten, nur als ein kurzer Test der Aufl¨osung eines neuen hochaufl¨osenden Neutronen- spektrometers am Forschungsreaktor FRM II geplant. Dieses neuartige Spektrometer TRISP (triple axis spin echo) erm¨oglicht die Bestimmung von Phononen-Linienbreiten uber¨ große Bereiche des Impulsraumes mit einer Energieaufl¨osung im μeV Bereich, d.h. zwei Gr¨oßenordnungen besser als an klassische Dreiachsen-Spektrometern. Philip Allen hat erstmals dargelegt, daß die Linienbreite eines Phonons proportional zum Elektron-Phonon Kopplungsparameter λ ist. -
Prediction in Quantum Cosmology
Prediction in Quantum Cosmology James B. Hartle Department of Physics University of California Santa Barbara, CA 93106, USA Lectures at the 1986 Carg`esesummer school publshed in Gravitation in As- trophysics ed. by J.B. Hartle and B. Carter, Plenum Press, New York (1987). In this version some references that were `to be published' in the original have been supplied, a few typos corrected, but the text is otherwise unchanged. The author's views on the quantum mechanics of cosmology have changed in important ways from those originally presented in Section 2. See, e.g. [107] J.B. Hartle, Spacetime Quantum Mechanics and the Quantum Mechan- ics of Spacetime in Gravitation and Quantizations, Proceedings of the 1992 Les Houches Summer School, ed. by B. Julia and J. Zinn-Justin, Les Houches Summer School Proceedings Vol. LVII, North Holland, Amsterdam (1995).) The general discussion and material in Sections 3 and 4 on the classical geom- etry limit and the approximation of quantum field theory in curved spacetime may still be of use. 1 Introduction As far as we know them, the fundamental laws of physics are quantum mechanical in nature. If these laws apply to the universe as a whole, then there must be a description of the universe in quantum mechancial terms. Even our present cosmological observations require such a description in principle, although in practice these observations are so limited and crude that the approximation of classical physics is entirely adequate. In the early universe, however, the classical approximation is unlikely to be valid. There, towards the big bang singularity, at curvatures characterized by the Planck length, 3 1 (¯hG=c ) 2 , quantum fluctuations become important and eventually dominant. -
TASI 2008 Lectures: Introduction to Supersymmetry And
TASI 2008 Lectures: Introduction to Supersymmetry and Supersymmetry Breaking Yuri Shirman Department of Physics and Astronomy University of California, Irvine, CA 92697. [email protected] Abstract These lectures, presented at TASI 08 school, provide an introduction to supersymmetry and supersymmetry breaking. We present basic formalism of supersymmetry, super- symmetric non-renormalization theorems, and summarize non-perturbative dynamics of supersymmetric QCD. We then turn to discussion of tree level, non-perturbative, and metastable supersymmetry breaking. We introduce Minimal Supersymmetric Standard Model and discuss soft parameters in the Lagrangian. Finally we discuss several mech- anisms for communicating the supersymmetry breaking between the hidden and visible sectors. arXiv:0907.0039v1 [hep-ph] 1 Jul 2009 Contents 1 Introduction 2 1.1 Motivation..................................... 2 1.2 Weylfermions................................... 4 1.3 Afirstlookatsupersymmetry . .. 5 2 Constructing supersymmetric Lagrangians 6 2.1 Wess-ZuminoModel ............................... 6 2.2 Superfieldformalism .............................. 8 2.3 VectorSuperfield ................................. 12 2.4 Supersymmetric U(1)gaugetheory ....................... 13 2.5 Non-abeliangaugetheory . .. 15 3 Non-renormalization theorems 16 3.1 R-symmetry.................................... 17 3.2 Superpotentialterms . .. .. .. 17 3.3 Gaugecouplingrenormalization . ..... 19 3.4 D-termrenormalization. ... 20 4 Non-perturbative dynamics in SUSY QCD 20 4.1 Affleck-Dine-Seiberg -
Magnetic Materials I
5 Magnetic materials I Magnetic materials I ● Diamagnetism ● Paramagnetism Diamagnetism - susceptibility All materials can be classified in terms of their magnetic behavior falling into one of several categories depending on their bulk magnetic susceptibility χ. without spin M⃗ 1 χ= in general the susceptibility is a position dependent tensor M⃗ (⃗r )= ⃗r ×J⃗ (⃗r ) H⃗ 2 ] In some materials the magnetization is m / not a linear function of field strength. In A [ such cases the differential susceptibility M is introduced: d M⃗ χ = d d H⃗ We usually talk about isothermal χ susceptibility: ∂ M⃗ χ = T ( ∂ ⃗ ) H T Theoreticians define magnetization as: ∂ F⃗ H[A/m] M=− F=U−TS - Helmholtz free energy [4] ( ∂ H⃗ ) T N dU =T dS− p dV +∑ μi dni i=1 N N dF =T dS − p dV +∑ μi dni−T dS−S dT =−S dT − p dV +∑ μi dni i=1 i=1 Diamagnetism - susceptibility It is customary to define susceptibility in relation to volume, mass or mole: M⃗ (M⃗ /ρ) m3 (M⃗ /mol) m3 χ= [dimensionless] , χρ= , χ = H⃗ H⃗ [ kg ] mol H⃗ [ mol ] 1emu=1×10−3 A⋅m2 The general classification of materials according to their magnetic properties μ<1 <0 diamagnetic* χ ⃗ ⃗ ⃗ ⃗ ⃗ ⃗ B=μ H =μr μ0 H B=μo (H +M ) μ>1 >0 paramagnetic** ⃗ ⃗ ⃗ χ μr μ0 H =μo( H + M ) → μ r=1+χ μ≫1 χ≫1 ferromagnetic*** *dia /daɪə mæ ɡˈ n ɛ t ɪ k/ -Greek: “from, through, across” - repelled by magnets. We have from L2: 1 2 the force is directed antiparallel to the gradient of B2 F = V ∇ B i.e. -
5.1 Two-Particle Systems
5.1 Two-Particle Systems We encountered a two-particle system in dealing with the addition of angular momentum. Let's treat such systems in a more formal way. The w.f. for a two-particle system must depend on the spatial coordinates of both particles as @Ψ well as t: Ψ(r1; r2; t), satisfying i~ @t = HΨ, ~2 2 ~2 2 where H = + V (r1; r2; t), −2m1r1 − 2m2r2 and d3r d3r Ψ(r ; r ; t) 2 = 1. 1 2 j 1 2 j R Iff V is independent of time, then we can separate the time and spatial variables, obtaining Ψ(r1; r2; t) = (r1; r2) exp( iEt=~), − where E is the total energy of the system. Let us now make a very fundamental assumption: that each particle occupies a one-particle e.s. [Note that this is often a poor approximation for the true many-body w.f.] The joint e.f. can then be written as the product of two one-particle e.f.'s: (r1; r2) = a(r1) b(r2). Suppose furthermore that the two particles are indistinguishable. Then, the above w.f. is not really adequate since you can't actually tell whether it's particle 1 in state a or particle 2. This indeterminacy is correctly reflected if we replace the above w.f. by (r ; r ) = a(r ) (r ) (r ) a(r ). 1 2 1 b 2 b 1 2 The `plus-or-minus' sign reflects that there are two distinct ways to accomplish this. Thus we are naturally led to consider two kinds of identical particles, which we have come to call `bosons' (+) and `fermions' ( ). -
BCS Thermal Vacuum of Fermionic Superfluids and Its Perturbation Theory
www.nature.com/scientificreports OPEN BCS thermal vacuum of fermionic superfuids and its perturbation theory Received: 14 June 2018 Xu-Yang Hou1, Ziwen Huang1,4, Hao Guo1, Yan He2 & Chih-Chun Chien 3 Accepted: 30 July 2018 The thermal feld theory is applied to fermionic superfuids by doubling the degrees of freedom of the Published: xx xx xxxx BCS theory. We construct the two-mode states and the corresponding Bogoliubov transformation to obtain the BCS thermal vacuum. The expectation values with respect to the BCS thermal vacuum produce the statistical average of the thermodynamic quantities. The BCS thermal vacuum allows a quantum-mechanical perturbation theory with the BCS theory serving as the unperturbed state. We evaluate the leading-order corrections to the order parameter and other physical quantities from the perturbation theory. A direct evaluation of the pairing correlation as a function of temperature shows the pseudogap phenomenon, where the pairing persists when the order parameter vanishes, emerges from the perturbation theory. The correspondence between the thermal vacuum and purifcation of the density matrix allows a unitary transformation, and we found the geometric phase associated with the transformation in the parameter space. Quantum many-body systems can be described by quantum feld theories1–4. Some available frameworks for sys- tems at fnite temperatures include the Matsubara formalism using the imaginary time for equilibrium systems1,5 and the Keldysh formalism of time-contour path integrals3,6 for non-equilibrium systems. Tere are also alterna- tive formalisms. For instance, the thermal feld theory7–9 is built on the concept of thermal vacuum.