Quantum Mechanics Condensed Matter Physics
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978-1-62808-450-4 Ch1.Pdf
In: Recent Advances in Magnetism Research ISBN: 978-1-62808-450-4 Editor: Keith Pace © 2013 Nova Science Publishers, Inc. No part of this digital document may be reproduced, stored in a retrieval system or transmitted commercially in any form or by any means. The publisher has taken reasonable care in the preparation of this digital document, but makes no expressed or implied warranty of any kind and assumes no responsibility for any errors or omissions. No liability is assumed for incidental or consequential damages in connection with or arising out of information contained herein. This digital document is sold with the clear understanding that the publisher is not engaged in rendering legal, medical or any other professional services. Chapter 1 TOWARDS A FIELD THEORY OF MAGNETISM Ulrich Köbler FZ-Jülich, Institut für Festkörperforschung, Jülich, Germany ABSTRACT Experimental tests of conventional spin wave theory reveal two serious shortcomings of this typical local or atomistic theory: first, spin wave theory is unable to explain the universal temperature dependence of the thermodynamic observables and, second, spin wave theory does not distinguish between the dynamics of magnets with integer and half- integer spin quantum number. As experiments show, universality is not restricted to the critical dynamics but holds for all temperatures in the long range ordered state including the low temperature regime where spin wave theory is widely believed to give an adequate description. However, a rigorous and convincing test that spin wave theory gives correct description of the thermodynamics of ordered magnets has never been delivered. Quite generally, observation of universality unequivocally calls for a continuum or field theory instead of a local theory. -
Rutherford's Nuclear World: the Story of the Discovery of the Nuc
Rutherford's Nuclear World: The Story of the Discovery of the Nuc... http://www.aip.org/history/exhibits/rutherford/sections/atop-physic... HOME SECTIONS CREDITS EXHIBIT HALL ABOUT US rutherford's explore the atom learn more more history of learn about aip's nuclear world with rutherford about this site physics exhibits history programs Atop the Physics Wave ShareShareShareShareShareMore 9 RUTHERFORD BACK IN CAMBRIDGE, 1919–1937 Sections ← Prev 1 2 3 4 5 Next → In 1962, John Cockcroft (1897–1967) reflected back on the “Miraculous Year” ( Annus mirabilis ) of 1932 in the Cavendish Laboratory: “One month it was the neutron, another month the transmutation of the light elements; in another the creation of radiation of matter in the form of pairs of positive and negative electrons was made visible to us by Professor Blackett's cloud chamber, with its tracks curled some to the left and some to the right by powerful magnetic fields.” Rutherford reigned over the Cavendish Lab from 1919 until his death in 1937. The Cavendish Lab in the 1920s and 30s is often cited as the beginning of modern “big science.” Dozens of researchers worked in teams on interrelated problems. Yet much of the work there used simple, inexpensive devices — the sort of thing Rutherford is famous for. And the lab had many competitors: in Paris, Berlin, and even in the U.S. Rutherford became Cavendish Professor and director of the Cavendish Laboratory in 1919, following the It is tempting to simplify a complicated story. Rutherford directed the Cavendish Lab footsteps of J.J. Thomson. Rutherford died in 1937, having led a first wave of discovery of the atom. -
Sounds of a Supersolid A
NEWS & VIEWS RESEARCH hypothesis came from extensive population humans, implying possible mosquito exposure long-distance spread of insecticide-resistant time-series analysis from that earlier study5, to malaria parasites and the potential to spread mosquitoes, worsening an already dire situ- which showed beyond reasonable doubt that infection over great distances. ation, given the current spread of insecticide a mosquito vector species called Anopheles However, the authors failed to detect resistance in mosquito populations. This would coluzzii persists locally in the dry season in parasite infections in their aerially sampled be a matter of great concern because insecticides as-yet-undiscovered places. However, the malaria vectors, a result that they assert is to be are the best means of malaria control currently data were not consistent with this outcome for expected given the small sample size and the low available8. However, long-distance migration other malaria vectors in the study area — the parasite-infection rates typical of populations of could facilitate the desirable spread of mosqui- species Anopheles gambiae and Anopheles ara- malaria vectors. A problem with this argument toes for gene-based methods of malaria-vector biensis — leaving wind-powered long-distance is that the typical infection rates they mention control. One thing is certain, Huestis and col- migration as the only remaining possibility to are based on one specific mosquito body part leagues have permanently transformed our explain the data5. (salivary glands), rather than the unknown but understanding of African malaria vectors and Both modelling6 and genetic studies7 undoubtedly much higher infection rates that what it will take to conquer malaria. -
Current Status of Equation of State in Nuclear Matter and Neutron Stars
Open Issues in Understanding Core Collapse Supernovae June 22-24, 2004 Current Status of Equation of State in Nuclear Matter and Neutron Stars J.R.Stone1,2, J.C. Miller1,3 and W.G.Newton1 1 Oxford University, Oxford, UK 2Physics Division, ORNL, Oak Ridge, TN 3 SISSA, Trieste, Italy Outline 1. General properties of EOS in nuclear matter 2. Classification according to models of N-N interaction 3. Examples of EOS – sensitivity to the choice of N-N interaction 4. Consequences for supernova simulations 5. Constraints on EOS 6. High density nuclear matter (HDNM) 7. New developments Equation of State is derived from a known dependence of energy per particle of a system on particle number density: EA/(==En) or F/AF(n) I. E ( or Boltzman free energy F = E-TS for system at finite temperature) is constructed in a form of effective energy functional (Hamiltonian, Lagrangian, DFT/EFT functional or an empirical form) II. An equilibrium state of matter is found at each density n by minimization of E (n) or F (n) III. All other related quantities like e.g. pressure P, incompressibility K or entropy s are calculated as derivatives of E or F at equilibrium: 2 ∂E ()n ∂F ()n Pn()= n sn()=− | ∂n ∂T nY, p ∂∂P()nnEE() ∂2 ()n Kn()==9 18n +9n2 ∂∂nn∂n2 IV. Use as input for model simulations (Very) schematic sequence of equilibrium phases of nuclear matter as a function of density: <~2x10-4fm-3 ~2x10-4 fm-3 ~0.06 fm-3 Nuclei in Nuclei in Neutron electron gas + ‘Pasta phase’ Electron gas ~0.1 fm-3 0.3-0.5 fm-3 >0.5 fm-3 Nucleons + n,p,e,µ heavy baryons Quarks ??? -
Bose-Einstein Condensation
Physics monitor The oldest galaxy, as seen by the European Southern Observatory's NTT telescope. The left picture shows the target quasar, with right, the quasar image removed to make the galaxy, situated just to the north-west of the quasar, easier to see. superfluidity. Condensates could also play an important role in particle physics and cosmology, explaining, for example, why the pion as a bound quark-antiquark state is so much lighter than the three-quark proton. A hunt to create a pure Bose- Einstein condensate has been underway for over 15 years, with different groups employing different techniques to cool their bosons. The two recent successes have been achieved by incorporating several techniques. In both cases, the bosons have been atoms. In Colo just 2 arcsec away from the quasar. led to Einstein's prediction. Unlike rado, rubidium-87 was used, whilst at This tiny angular separation corre fermions, which obey the Pauli Rice University, the condensate was sponds to a distance 'on the ground' exclusion principle of only one formed from lithium-7. Both teams of 40,000 light-years. resident particle per allowed quantum started with the technique of laser There are strong indications that state, any number of bosons can cooling. This works by pointing finely this galaxy contains all the necessary pack into an identical quantum state. tuned laser beams at the sample nuclei to produce the observed This led Einstein to suggest that such that any atoms moving towards absorption effects. Only hydrogen under certain conditions, bosons a beam are struck by a photon, which and helium were produced in the Big would lose their individual identities, slows them down. -
Download Report 2010-12
RESEARCH REPORt 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Cover: Aurora borealis paintings by William Crowder, National Geographic (1947). The International Geophysical Year (1957–8) transformed research on the aurora, one of nature’s most elusive and intensely beautiful phenomena. Aurorae became the center of interest for the big science of powerful rockets, complex satellites and large group efforts to understand the magnetic and charged particle environment of the earth. The auroral visoplot displayed here provided guidance for recording observations in a standardized form, translating the sublime aesthetics of pictorial depictions of aurorae into the mechanical aesthetics of numbers and symbols. Most of the portait photographs were taken by Skúli Sigurdsson RESEARCH REPORT 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Introduction The Max Planck Institute for the History of Science (MPIWG) is made up of three Departments, each administered by a Director, and several Independent Research Groups, each led for five years by an outstanding junior scholar. Since its foundation in 1994 the MPIWG has investigated fundamental questions of the history of knowl- edge from the Neolithic to the present. The focus has been on the history of the natu- ral sciences, but recent projects have also integrated the history of technology and the history of the human sciences into a more panoramic view of the history of knowl- edge. Of central interest is the emergence of basic categories of scientific thinking and practice as well as their transformation over time: examples include experiment, ob- servation, normalcy, space, evidence, biodiversity or force. -
Universal Scaling Behavior of Non-Equilibrium Phase Transitions
Universal scaling behavior of non-equilibrium phase transitions HABILITATIONSSCHRIFT der FakultÄat furÄ Naturwissenschaften der UniversitÄat Duisburg-Essen vorgelegt von Sven LubÄ eck aus Duisburg Duisburg, im Juni 2004 Zusammenfassung Kritische PhÄanomene im Nichtgleichgewicht sind seit Jahrzehnten Gegenstand inten- siver Forschungen. In Analogie zur Gleichgewichtsthermodynamik erlaubt das Konzept der UniversalitÄat, die verschiedenen NichtgleichgewichtsphasenubÄ ergÄange in unterschied- liche Klassen einzuordnen. Alle Systeme einer UniversalitÄatsklasse sind durch die glei- chen kritischen Exponenten gekennzeichnet, und die entsprechenden Skalenfunktionen werden in der NÄahe des kritischen Punktes identisch. WÄahrend aber die Exponenten zwischen verschiedenen UniversalitÄatsklassen sich hÄau¯g nur geringfugigÄ unterscheiden, weisen die Skalenfunktionen signi¯kante Unterschiede auf. Daher ermÄoglichen die uni- versellen Skalenfunktionen einerseits einen emp¯ndlichen und genauen Nachweis der UniversalitÄatsklasse eines Systems, demonstrieren aber andererseits in ubÄ erzeugender- weise die UniversalitÄat selbst. Bedauerlicherweise wird in der Literatur die Betrachtung der universellen Skalenfunktionen gegenubÄ er der Bestimmung der kritischen Exponen- ten hÄau¯g vernachlÄassigt. Im Mittelpunkt dieser Arbeit steht eine bestimmte Klasse von Nichtgleichgewichts- phasenubÄ ergÄangen, die sogenannten absorbierenden PhasenubÄ ergÄange. Absorbierende PhasenubÄ ergÄange beschreiben das kritische Verhalten von physikalischen, chemischen sowie biologischen -
Universal Scaling Behavior of Non-Equilibrium Phase Transitions
Universal scaling behavior of non-equilibrium phase transitions Sven L¨ubeck Theoretische Physik, Univerit¨at Duisburg-Essen, 47048 Duisburg, Germany, [email protected] December 2004 arXiv:cond-mat/0501259v1 [cond-mat.stat-mech] 11 Jan 2005 Summary Non-equilibrium critical phenomena have attracted a lot of research interest in the recent decades. Similar to equilibrium critical phenomena, the concept of universality remains the major tool to order the great variety of non-equilibrium phase transitions systematically. All systems belonging to a given universality class share the same set of critical exponents, and certain scaling functions become identical near the critical point. It is known that the scaling functions vary more widely between different uni- versality classes than the exponents. Thus, universal scaling functions offer a sensitive and accurate test for a system’s universality class. On the other hand, universal scaling functions demonstrate the robustness of a given universality class impressively. Unfor- tunately, most studies focus on the determination of the critical exponents, neglecting the universal scaling functions. In this work a particular class of non-equilibrium critical phenomena is considered, the so-called absorbing phase transitions. Absorbing phase transitions are expected to occur in physical, chemical as well as biological systems, and a detailed introduc- tion is presented. The universal scaling behavior of two different universality classes is analyzed in detail, namely the directed percolation and the Manna universality class. Especially, directed percolation is the most common universality class of absorbing phase transitions. The presented picture gallery of universal scaling functions includes steady state, dynamical as well as finite size scaling functions. -
Solid State Insurrection
INTRODUCTION WHAT IS SOLID STATE PHYSICS AND WHY DOES IT MATTER? Solid state physics sounds kind of funny. —GREGORY H. WANNIER, 1943 The Superconducting Super Collider (SSC), the largest scientific instrument ever proposed, was also one of the most controversial. The enormous parti- cle accelerator’s beam pipe would have encircled hundreds of square miles of Ellis County, Texas. It was designed to produce evidence for the last few elements of the standard model of particle physics, and many hoped it might generate unexpected discoveries that would lead beyond. Advocates billed the SSC as the logical apotheosis of physical research. Opponents raised their eyebrows at the facility’s astronomical price tag, which stood at $11.8 billion by the time Congress yanked its funding in 1993. Skeptics also objected to the reductionist rhetoric used to justify the project—which suggested that knowledge of the very small was the only knowledge that could be truly fun- damental—and grew exasperated when SSC boosters ascribed technological developments and medical advances to high energy physics that they thought more justly credited to other areas of science. To the chagrin of the SSC’s supporters, many such skeptics were fellow physicists. The most prominent among them was Philip W. Anderson, a No- bel Prize–winning theorist. Anderson had risen to prominence in the new field known as solid state physics after he joined the Bell Telephone Labora- tories in 1949, the ink on his Harvard University PhD still damp. In a House of Representatives committee hearing in July 1991, Anderson, by then at © 2018 University of Pittsburgh Press. -
A Modern View of the Equation of State in Nuclear and Neutron Star Matter
S S symmetry Article A Modern View of the Equation of State in Nuclear and Neutron Star Matter G. Fiorella Burgio * , Hans-Josef Schulze , Isaac Vidaña and Jin-Biao Wei INFN Sezione di Catania, Dipartimento di Fisica e Astronomia, Università di Catania, Via Santa Sofia 64, 95123 Catania, Italy; [email protected] (H.-J.S.); [email protected] (I.V.); [email protected] (J.-B.W.) * Correspondence: fi[email protected] Abstract: Background: We analyze several constraints on the nuclear equation of state (EOS) cur- rently available from neutron star (NS) observations and laboratory experiments and study the existence of possible correlations among properties of nuclear matter at saturation density with NS observables. Methods: We use a set of different models that include several phenomenological EOSs based on Skyrme and relativistic mean field models as well as microscopic calculations based on different many-body approaches, i.e., the (Dirac–)Brueckner–Hartree–Fock theories, Quantum Monte Carlo techniques, and the variational method. Results: We find that almost all the models considered are compatible with the laboratory constraints of the nuclear matter properties as well as with the +0.10 largest NS mass observed up to now, 2.14−0.09 M for the object PSR J0740+6620, and with the upper limit of the maximum mass of about 2.3–2.5 M deduced from the analysis of the GW170817 NS merger event. Conclusion: Our study shows that whereas no correlation exists between the tidal deformability and the value of the nuclear symmetry energy at saturation for any value of the NS mass, very weak correlations seem to exist with the derivative of the nuclear symmetry energy and with the nuclear incompressibility. -
Memorial Tributes: Volume 15
THE NATIONAL ACADEMIES PRESS This PDF is available at http://nap.edu/13160 SHARE Memorial Tributes: Volume 15 DETAILS 444 pages | 6 x 9 | HARDBACK ISBN 978-0-309-21306-6 | DOI 10.17226/13160 CONTRIBUTORS GET THIS BOOK National Academy of Engineering FIND RELATED TITLES Visit the National Academies Press at NAP.edu and login or register to get: – Access to free PDF downloads of thousands of scientific reports – 10% off the price of print titles – Email or social media notifications of new titles related to your interests – Special offers and discounts Distribution, posting, or copying of this PDF is strictly prohibited without written permission of the National Academies Press. (Request Permission) Unless otherwise indicated, all materials in this PDF are copyrighted by the National Academy of Sciences. Copyright © National Academy of Sciences. All rights reserved. Memorial Tributes: Volume 15 Memorial Tributes NATIONAL ACADEMY OF ENGINEERING Copyright National Academy of Sciences. All rights reserved. Memorial Tributes: Volume 15 Copyright National Academy of Sciences. All rights reserved. Memorial Tributes: Volume 15 NATIONAL ACADEMY OF ENGINEERING OF THE UNITED STATES OF AMERICA Memorial Tributes Volume 15 THE NATIONAL ACADEMIES PRESS Washington, D.C. 2011 Copyright National Academy of Sciences. All rights reserved. Memorial Tributes: Volume 15 International Standard Book Number-13: 978-0-309-21306-6 International Standard Book Number-10: 0-309-21306-1 Additional copies of this publication are available from: The National Academies Press 500 Fifth Street, N.W. Lockbox 285 Washington, D.C. 20055 800–624–6242 or 202–334–3313 (in the Washington metropolitan area) http://www.nap.edu Copyright 2011 by the National Academy of Sciences. -
Supersolid State of Matter Nikolai Prokof 'Ev University of Massachusetts - Amherst, [email protected]
University of Massachusetts Amherst ScholarWorks@UMass Amherst Physics Department Faculty Publication Series Physics 2005 Supersolid State of Matter Nikolai Prokof 'ev University of Massachusetts - Amherst, [email protected] Boris Svistunov University of Massachusetts - Amherst, [email protected] Follow this and additional works at: https://scholarworks.umass.edu/physics_faculty_pubs Part of the Physical Sciences and Mathematics Commons Recommended Citation Prokof'ev, Nikolai and Svistunov, Boris, "Supersolid State of Matter" (2005). Physics Review Letters. 1175. Retrieved from https://scholarworks.umass.edu/physics_faculty_pubs/1175 This Article is brought to you for free and open access by the Physics at ScholarWorks@UMass Amherst. It has been accepted for inclusion in Physics Department Faculty Publication Series by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. On the Supersolid State of Matter Nikolay Prokof’ev and Boris Svistunov Department of Physics, University of Massachusetts, Amherst, MA 01003 and Russian Research Center “Kurchatov Institute”, 123182 Moscow We prove that the necessary condition for a solid to be also a superfluid is to have zero-point vacancies, or interstitial atoms, or both, as an integral part of the ground state. As a consequence, superfluidity is not possible in commensurate solids which break continuous translation symmetry. We discuss recent experiment by Kim and Chan [Nature, 427, 225 (2004)] in the context of this theorem, question its bulk supersolid interpretation, and offer an alternative explanation in terms of superfluid helium interfaces. PACS numbers: 67.40.-w, 67.80.-s, 05.30.-d Recent discovery by Kim and Chan [1, 2] that solid 4He theorem.