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Physical Vacuum Is a Special Superfluid Medium
Physical vacuum is a special superfluid medium Valeriy I. Sbitnev∗ St. Petersburg B. P. Konstantinov Nuclear Physics Institute, NRC Kurchatov Institute, Gatchina, Leningrad district, 188350, Russia; Department of Electrical Engineering and Computer Sciences, University of California, Berkeley, Berkeley, CA 94720, USA (Dated: August 9, 2016) The Navier-Stokes equation contains two terms which have been subjected to slight modification: (a) the viscosity term depends of time (the viscosity in average on time is zero, but its variance is non-zero); (b) the pressure gradient contains an added term describing the quantum entropy gradient multiplied by the pressure. Owing to these modifications, the Navier-Stokes equation can be reduced to the Schr¨odingerequation describing behavior of a particle into the vacuum being as a superfluid medium. Vortex structures arising in this medium show infinitely long life owing to zeroth average viscosity. The non-zero variance describes exchange of the vortex energy with zero-point energy of the vacuum. Radius of the vortex trembles around some average value. This observation sheds the light to the Zitterbewegung phenomenon. The long-lived vortex has a non-zero core where the vortex velocity vanishes. Keywords: Navier-Stokes; Schr¨odinger; zero-point fluctuations; superfluid vacuum; vortex; Bohmian trajectory; interference I. INTRODUCTION registered. Instead, the wave function represents it existence within an experimental scene [13]. A dramatic situation in physical understand- Another interpretation was proposed by Louis ing of the nature emerged in the late of 19th cen- de Broglie [18], which permits to explain such an tury. Observed phenomena on micro scales came experiment. In de Broglie's wave mechanics and into contradiction with the general positions of the double solution theory there are two waves. -
Conformal Field Theory out of Equilibrium: a Review Denis Bernard
Conformal field theory out of equilibrium: a review Denis Bernard| and Benjamin Doyon♠ | Laboratoire de Physique Th´eoriquede l'Ecole Normale Sup´erieurede Paris, CNRS, ENS & PSL Research University, UMPC & Sorbonne Universit´es,France. ♠ Department of Mathematics, King's College London, London, United Kingdom. We provide a pedagogical review of the main ideas and results in non-equilibrium conformal field theory and connected subjects. These concern the understanding of quantum transport and its statistics at and near critical points. Starting with phenomenological considerations, we explain the general framework, illustrated by the example of the Heisenberg quantum chain. We then introduce the main concepts underlying conformal field theory (CFT), the emergence of critical ballistic transport, and the CFT scattering construction of non-equilibrium steady states. Using this we review the theory for energy transport in homogeneous one-dimensional critical systems, including the complete description of its large deviations and the resulting (extended) fluctuation relations. We generalize some of these ideas to one-dimensional critical charge transport and to the presence of defects, as well as beyond one-dimensional criticality. We describe non-equilibrium transport in free-particle models, where connections are made with generalized Gibbs ensembles, and in higher-dimensional and non-integrable quantum field theories, where the use of the powerful hydrodynamic ideas for non-equilibrium steady states is explained. We finish with a list of open questions. The review does not assume any advanced prior knowledge of conformal field theory, large-deviation theory or hydrodynamics. March 24, 2016 Contents 1 Introduction 1 2 Mesoscopic electronic transport: basics 3 2.1 Elementary phenomenology . -
Stochastic Hydrodynamic Analogy of Quantum Mechanics
The mass lowest limit of a black hole: the hydrodynamic approach to quantum gravity Piero Chiarelli National Council of Research of Italy, Area of Pisa, 56124 Pisa, Moruzzi 1, Italy Interdepartmental Center “E.Piaggio” University of Pisa Phone: +39-050-315-2359 Fax: +39-050-315-2166 Email: [email protected]. Abstract: In this work the quantum gravitational equations are derived by using the quantum hydrodynamic description. The outputs of the work show that the quantum dynamics of the mass distribution inside a black hole can hinder its formation if the mass is smaller than the Planck's one. The quantum-gravitational equations of motion show that the quantum potential generates a repulsive force that opposes itself to the gravitational collapse. The eigenstates in a central symmetric black hole realize themselves when the repulsive force of the quantum potential becomes equal to the gravitational one. The work shows that, in the case of maximum collapse, the mass of the black hole is concentrated inside a sphere whose radius is two times the Compton length of the black hole. The mass minimum is determined requiring that the gravitational radius is bigger than or at least equal to the radius of the state of maximum collapse. PACS: 04.60.-m Keywords: quantum gravity, minimum black hole mass, Planck's mass, quantum Kaluza Klein model 1. Introduction One of the unsolved problems of the theoretical physics is that of unifying the general relativity with the quantum mechanics. The former theory concerns the gravitation dynamics on large cosmological scale in a fully classical ambit, the latter one concerns, mainly, the atomic or sub-atomic quantum phenomena and the fundamental interactions [1-9]. -
Giuseppe Gaeta – List of Publications∗
Giuseppe Gaeta { List of publications∗ Books [B1 ] G. Gaeta: \Nonlinear symmetries and nonlinear equations" (series: Math- ematics and Its Application, vol. 299); Kluwer Academic Publishers (Dor- drecht) 1994; ISBN 0-7923-3048-X [B2 ] G. Gaeta and G. Cicogna: \Symmetry and perturbation theory in non- linear dynamics" (series: Lecture Notes in Physics, vol. M57); Springer (Berlin) 1999; ISBN 3-540-65904 Monographs [M1 ] G. Gaeta: \Bifurcation and symmetry breaking"; Physics Reports 189 (1990), n. 1, 1-87 [M2 ] G. Gaeta, C. Reiss, M. Peyrard and T. Dauxois: \Simple models of DNA nonlinear dynamics"; Rivista del Nuovo Cimento 17 (1994), n.4, 1-48 Edited volumes [E1 ] D. Bambusi and G. Gaeta (eds.): \Symmetry and Perturbation Theory" (Proceedings of Torino Workshop, I.S.I., December 1996); G.N.F.M. { C.N.R. (Gruppo Nazionale di Fisica Matematica { Consiglio Nazionale delle Ricerche), Roma, 1997 [E2 ] A. Degasperis and G. Gaeta (eds.): \Symmetry and Perturbation Theory II { SPT98" (Proceedings of Roma Workshop, Universit´a\La Sapienza", December 1998); World Scientific, Singapore, 1999; ISBN 981-02-4166-6 ∗Only research and review papers and monographs are listed; in particular, this list does not include contributions to conferences or schools proceedings (as these reproduce results obtained in research papers). Note that books and monographs (not edited volumes nor textbook) also appear in the list of published research works. Last modified 5/12/2015. 1 [E3 ] D. Bambusi, G. Gaeta and M. Cadoni (eds.): \Symmetry and Pertur- bation Theory { SPT2001" (Proceedings of the international conference SPT2001, Cala Gonone, Sardinia, Italy, 6-13 May 2001); World Scientific, Singapore, 2001; ISBN 981-02-4793-1 [E4 ] G. -
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News 6/2013 Physics H. Friedrich, TU München, Germany R. Gendler, Rob Gendler Astropics, Avon, CT, USA G. Ghisellini, The Astronomical Observatory of Brera, Scattering Theory (Ed) Merate, Italy Lessons from the Masters Radiative Processes in High This book presents a concise and modern coverage of scattering theory. It is motivated by the fact that Current Concepts in Astronomical Image Energy Astrophysics experimental advances have shifted and broad- Processing This book grew out of the author’s notes from his ened the scope of applications where concepts course on Radiative Processes in High Energy from scattering theory are used, e.g. to the field of There are currently thousands of amateur astrono- Astrophysics. The course provides fundamental ultracold atoms and molecules, which has been mers around the world engaged in astrophotogra- definitions of radiative processes and serves as a experiencing enormous growth in recent years, phy at a sophisticated level. brief introduction to Bremsstrahlung and black largely triggered by the successful realization of Features body emission, relativistic beaming, synchrotron Bose-Einstein condensates of dilute atomic gases 7 Written by a brilliant body of recognized emission and absorption, Compton scattering, in 1995. In the present treatment, special atten- leaders 7 Contains the most current, sophisti- synchrotron self-compton emission, pair creation tion is given to the role played by the long-range cated and useful information on astrophotogra- and emission. The final chapter discusses the ob- behaviour of the projectile-target interaction, phy 7 Covers all types of astronomical image served features of Active Galactic Nuclei and their and a theory is developed, which is well suited processing, including processing of events such interpretation based on the radiative processes to describe near-threshold bound and continuum as eclipses, using DSLRs, and deep sky, planetary, presented in the book. -
Arxiv:2105.05054V2 [Cond-Mat.Stat-Mech] 1 Sep 2021 2
Exact entanglement growth of a one-dimensional hard-core quantum gas during a free expansion Stefano Scopa1, Alexandre Krajenbrink1, Pasquale Calabrese1;2 and Jer´ omeˆ Dubail3 1 SISSA and INFN, via Bonomea 265, 34136 Trieste, Italy 2 International Centre for Theoretical Physics (ICTP), I-34151, Trieste, Italy 3 Universite´ de Lorraine, CNRS, LPCT, F-54000 Nancy, France Abstract. We consider the non-equilibrium dynamics of the entanglement entropy of a one- dimensional quantum gas of hard-core particles, initially confined in a box potential at zero temperature. At t = 0 the right edge of the box is suddenly released and the system is let free to expand. During this expansion, the initially correlated region propagates with a non-homogeneous profile, leading to the growth of entanglement entropy. This setting is investigated in the hydrodynamic regime, with tools stemming from semi-classical Wigner function approach and with recent developments of quantum fluctuating hydrodynamics. Within this framework, the entanglement entropy can be associated to a correlation function of chiral twist-fields of the conformal field theory that lives along the Fermi contour and it can be exactly determined. Our predictions for the entanglement evolution are found in agreement with and generalize previous results in literature based on numerical calculations and heuristic arguments. arXiv:2105.05054v2 [cond-mat.stat-mech] 1 Sep 2021 2 Contents 1 Introduction3 2 Setup and main result5 2.1 The model: free expansion of a lattice hard-core gas . .5 2.2 Previous results in the literature . .6 2.3 Main result of this paper . .7 3 Classical and quantum fluctuating hydrodynamic description8 3.1 Continuum limit and regularization of the problem . -
Emergent Hydrodynamics in a 1D Bose-Fermi Mixture
Emergent Hydrodynamics in a 1D Bose-Fermi Mixture PACS numbers: INTRODUCTION OF MY LECTURE scale, all the densities and currents of local observables are the functions of ξ = x=t. Here the evolution can be Nonequilibrium dynamics of one dimensional (1D) intuitively understood by the transport of the quasipar- integrable systems is very insightful in understanding ticles in integrable systems. Within the light core the transport of many-body systems. Significantly differ- quasiparticles can arrive and leave that totally depends ent behaviours are observed from that of the higher di- on their local velocities. Moreover, the GH method has mensional systems since the existence of many conserved been adapted to study the evolution of 1D systems con- quantities in 1D. For example, 1D integrable systems do fined by the external field [8,9], also see experiment [10]. not thermalize to a usual state of thermodynamic equi- Beyond the Euler type of hydrodynamics, diffusion has librium [1], where after a long time evolution there is a also been studied by the GH [11, 12]. maximal entropy state constrained by all the conserved On the other hand, at low temperatures, universal phe- quantities[2]. When we consider such a process of time nomena emerge in quantum many-body systems. In high evolution, it is extremely hard to solve the Schrodinger dimensions, the low energy physics can be described by equation of the system with large number particles. Landau's Fermi liquids theory. However, for 1D sys- tems, the elementary excitations form collective motions of bosons. Thus the low energy physics of 1D systems is elegantly descried by the theory of Luttinger liquids [13{ 15]. -
Birds and Frogs Equation
Notices of the American Mathematical Society ISSN 0002-9920 ABCD springer.com New and Noteworthy from Springer Quadratic Diophantine Multiscale Principles of Equations Finite Harmonic of the American Mathematical Society T. Andreescu, University of Texas at Element Analysis February 2009 Volume 56, Number 2 Dallas, Richardson, TX, USA; D. Andrica, Methods A. Deitmar, University Cluj-Napoca, Romania Theory and University of This text treats the classical theory of Applications Tübingen, quadratic diophantine equations and Germany; guides readers through the last two Y. Efendiev, Texas S. Echterhoff, decades of computational techniques A & M University, University of and progress in the area. The presenta- College Station, Texas, USA; T. Y. Hou, Münster, Germany California Institute of Technology, tion features two basic methods to This gently-paced book includes a full Pasadena, CA, USA investigate and motivate the study of proof of Pontryagin Duality and the quadratic diophantine equations: the This text on the main concepts and Plancherel Theorem. The authors theories of continued fractions and recent advances in multiscale finite emphasize Banach algebras as the quadratic fields. It also discusses Pell’s element methods is written for a broad cleanest way to get many fundamental Birds and Frogs equation. audience. Each chapter contains a results in harmonic analysis. simple introduction, a description of page 212 2009. Approx. 250 p. 20 illus. (Springer proposed methods, and numerical 2009. Approx. 345 p. (Universitext) Monographs in Mathematics) Softcover examples of those methods. Softcover ISBN 978-0-387-35156-8 ISBN 978-0-387-85468-7 $49.95 approx. $59.95 2009. X, 234 p. (Surveys and Tutorials in The Strong Free Will the Applied Mathematical Sciences) Solving Softcover Theorem Introduction to Siegel the Pell Modular Forms and ISBN: 978-0-387-09495-3 $44.95 Equation page 226 Dirichlet Series Intro- M. -
Arxiv:1904.12388V2 [Gr-Qc] 5 Oct 2019 [email protected] Orsodn Uhr .Gregori G
Draft version October 8, 2019 Typeset using LATEX twocolumn style in AASTeX62 Modified Friedmann equations via conformal Bohm – De Broglie gravity G. Gregori,1 B. Reville,2 and B. Larder1 1Department of Physics, University of Oxford, Parks Road, Oxford OX1 3PU, UK 2Max-Planck-Institut f¨ur Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany ABSTRACT We use an alternative interpretation of quantum mechanics, based on the Bohmian trajectory ap- proach, and show that the quantum effects can be included in the classical equation of motion via a conformal transformation on the background metric. We apply this method to the Robertson-Walker metric to derive a modified version of Friedmann’s equations for a Universe consisting of scalar, spin- zero, massive particles. These modified equations include additional terms that result from the non- local nature of matter and appear as an acceleration in the expansion of the Universe. We see that the same effect may also be present in the case of an inhomogeneous expansion. Keywords: cosmology: theory — cosmology: dark matter — cosmology: dark energy 1. INTRODUCTION de Broglie-Bohm trajectories can have a sound phys- The equations governing quantum mechanics have been ical interpretation if full non-locality is accounted for known for nearly 100 years, but yet the task of reconcil- (Mahler et al. 2016). Extensions to quantum fluids ing them with the equations of classical motions remains (Haas 2011; Cross et al. 2014), field theory (D¨urr et al. unsolved (see e.g., Ref. Hiley and Muft (1995)). The 2004; Carroll 2007) and curved space-time (D¨urr et al. -
Bekenstein Bound of Information Number N and Its Relation to Cosmological Parameters in a Universe with and Without Cosmological Constant
Wilfrid Laurier University Scholars Commons @ Laurier Physics and Computer Science Faculty Publications Physics and Computer Science 2013 Bekenstein Bound of Information Number N and its Relation to Cosmological Parameters in a Universe with and without Cosmological Constant Ioannis Haranas Wilfrid Laurier University, [email protected] Ioannis Gkigkitzis East Carolina University, [email protected] Follow this and additional works at: https://scholars.wlu.ca/phys_faculty Part of the Mathematics Commons, and the Physics Commons Recommended Citation Haranas, I., Gkigkitzis, I. Bekenstein Bound of Information Number N and its Relation to Cosmological Parameters in a Universe with and without Cosmological Constant. Modern Physics Letters A 28:19 (2013). DOI: 10.1142/S0217732313500776 This Article is brought to you for free and open access by the Physics and Computer Science at Scholars Commons @ Laurier. It has been accepted for inclusion in Physics and Computer Science Faculty Publications by an authorized administrator of Scholars Commons @ Laurier. For more information, please contact [email protected]. Bekestein Bound of Information Number N and its Relation to Cosmological Parameters in a Universe with and without Cosmological Constant 1 2 Ioannis Haranas Ioannis Gkigkitzis 1 Department of Physics and Astronomy, York University 4700 Keele Street, Toronto, Ontario, M3J 1P3, Canada E-mail:[email protected] 1 Departments of Mathematics, East Carolina University 124 Austin Building, East Fifth Street, Greenville NC 27858-4353, USA E-mail: [email protected] Abstract Bekenstein has obtained is an upper limit on the entropy S, and from that, an information number bound N is deduced. In other words, this is the information contained within a given finite region of space that includes a finite amount of energy. -
Bokulich- Forest for the Ψ-Preprint
Forthcoming in S. French and J. Saatsi (eds.) Scientific Realism and the Quantum. Oxford: Oxford University Press Losing Sight of the Forest for the Ψ: Beyond the Wavefunction Hegemony Alisa Bokulich Philosophy Department Boston University [email protected] Abstract: Traditionally Ψ is used to stand in for both the mathematical wavefunction (the representation) and the quantum state (the thing in the world). This elision has been elevated to a metaphysical thesis by advocates of the view known as wavefunction realism. My aim in this paper is to challenge the hegemony of the wavefunction by calling attention to a little-known formulation of quantum theory that does not make use of the wavefunction in representing the quantum state. This approach, called Lagrangian quantum hydrodynamics (LQH), is not an approximation scheme, but rather a full alternative formulation of quantum theory. I argue that a careful consideration of alternative formalisms is an essential part of any realist project that attempts to read the ontology of a theory off of the mathematical formalism. In particular, I show that LQH undercuts the central presumption of wavefunction realism and falsifies the claim that one must represent the many-body quantum state as living in a 3n-dimensional configuration space. I conclude by briefly sketching three different realist approaches one could take toward LQH, and argue that both models of the quantum state should be admitted. When exploring quantum realism, regaining sight of the proverbial forest of quantum representations beyond the Ψ is just the first step. I. Introduction II. Quantum Realism a. Wavefunction Realism b. A Few Cautionary Tales III. -
On an Interpolative Schr\"{O} Dinger Equation and an Alternative
UQ Theory: October1992 On an interpolative Schr¨odinger equation and an alternative classical limit ∗ K. R. W. Jones Physics Department, University of Queensland, St Lucia 4072, Brisbane, Australia. (Revised version 13/10/92) Abstract We introduce a simple deformed quantization prescription that interpolates the classical and quantum sectors of Weinberg’s nonlinear quantum theory. The result is a novel classical limit where ¯h is kept fixed while a dimensionless mesoscopic parameter, λ ∈ [0, 1], goes to zero. Unlike the standard classical limit, which holds good up to a certain timescale, ours is a precise limit incorporating true dynamical chaos, no dispersion, an absence of macroscopic superpositions and a complete recovery of the symplectic geometry of classical phase space. We develop the formalism, and discover that energy levels suffer a generic perturbation. Exactly, they become E(λ2¯h), where λ = 1 gives the standard prediction. Exact interpolative eigenstates can be similarly constructed. Unlike the linear case, these need no longer be orthogonal. A formal solution for the interpolative dynamics is given, and we exhibit the free particle as one exactly soluble case. Dispersion is reduced, to vanish at λ = 0. We conclude by discussing some possible empirical signatures, and explore the obstructions to a satisfactory physical interpretation. arXiv:1312.4195v1 [math-ph] 15 Dec 2013 PACS numbers: 03.65.Bz, 02.30.+g, 03.20.+i, 0.3.65.Db ∗ Author’s note: Archival version of an old preprint restored from obsolete electronic media. This was first submitted to Phys. Rev. D back in 1992 but rejected as being of “insufficient interest”.