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UNIVERSITY of CALIFORNIA, SAN DIEGO Exciton Transport
UNIVERSITY OF CALIFORNIA, SAN DIEGO Exciton Transport Phenomena in GaAs Coupled Quantum Wells A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Jason R. Leonard Committee in charge: Professor Leonid V. Butov, Chair Professor John M. Goodkind Professor Shayan Mookherjea Professor Charles W. Tu Professor Congjun Wu 2016 Copyright Jason R. Leonard, 2016 All rights reserved. The dissertation of Jason R. Leonard is approved, and it is acceptable in quality and form for publication on microfilm and electronically: Chair University of California, San Diego 2016 iii TABLE OF CONTENTS Signature Page . iii Table of Contents . iv List of Figures . vi Acknowledgements . viii Vita........................................ x Abstract of the Dissertation . xii Chapter 1 Introduction . 1 1.1 Semiconductor introduction . 2 1.1.1 Bulk GaAs . 3 1.1.2 Single Quantum Well . 3 1.1.3 Coupled-Quantum Wells . 5 1.2 Transport Physics . 7 1.3 Spin Physics . 8 1.3.1 D'yakanov and Perel' spin relaxation . 10 1.3.2 Dresselhaus Interaction . 10 1.3.3 Electron-Hole Exchange Interaction . 11 1.4 Dissertation Overview . 11 Chapter 2 Controlled exciton transport via a ramp . 13 2.1 Introduction . 13 2.2 Experimental Methods . 14 2.3 Qualitative Results . 14 2.4 Quantitative Results . 16 2.5 Theoretical Model . 17 2.6 Summary . 19 2.7 Acknowledgments . 19 Chapter 3 Controlled exciton transport via an optically controlled exciton transistor . 22 3.1 Introduction . 22 3.2 Realization . 22 3.3 Experimental Methods . 23 3.4 Results . 25 3.5 Theoretical Model . -
Understanding a Warped Cosmos
Lisa Randall. “One challenge today is to see what you can do with large amounts of data, to study fundamental properties, not just questions of how electromagnetism gives rise to certain things. Can we actually see deviations from what you would predict in conventional theories?” Rami Shllush Understanding a warped cosmos What’s the connection between dinosaurs and dark matter? What is the glue that holds the universe together? Is there a fourth - and fifth - dimension? These are just some of the questions that occupy Lisa Randall, the first female physicist to get tenure at Princeton, Harvard and MIT ■ ״ ״r* י •• 1 י׳ The CERN facility, near Geneva. “We need higher-energy machines and particle Illustration of a large asteroid colliding with Earth over the Yucatan Peninsula, in accelerators,” says Randall, “but to really see new things, we need even more Mexico. The impact of such occurrences are thought to have led to the death of the powerful machines.” Richard Juillian/AFP dinosaurs some 65 million years ago. Mark Garlick/Science Photo Libra Ido Efrati in the sciences. In 2016 he mystery of the universe,be seen as evidence that dark matter Over the years, studies have specializes interview with The New she and the many riddles that re- interacted in some way with hydrogen mapped the presence of dark matter Yorker, related that in her teens she had fre- main open about itcan be ex- atoms, thus leadingto the loweringof in various placesin the universe,in- the of the dark matter. our emplifiedin myriad ways. temperature eludingin the center of galaxy,the quent confrontations with her mother, to One of the most frustratingPhysicistsresponding the article Milky Way. -
Solo Journey to a Fifth Dimension with More Than 100 Parameters of Digital Trans- Formation, Which Evolve As the Plot Progresses
NATURE|Vol 460|9 July 2009 OPINION French, and Spanish pillaging of native Ameri- eties for the same reason everyone else does: familiar world is confined to a four-dimensional can resources in the sixteenth and seventeenth economic success. space-time ‘brane’ that lies, in her theory, within centuries, during the heyday of piracy. The Invisible Hook is a good addition to a larger five-dimensional ‘hyperspace’. Moving Sovereign governments may have legalized the genre of popular economics: a fun and into the fifth dimension takes the fictional trav- such plundering, but they were not necessarily enlightening read, and rock solid in its schol- eller into regions of vastly magnified gravity that more moral than the pirates who re-plundered arly bona fides. ■ distorts other attributes of reality and experi- that same wealth. Both used the threat of force, Michael Shermer is publisher of Skeptic magazine, ence: time, distance, energy and mass. as Leeson reminds us. He does not argue for a columnist for Scientific American, and author of The challenge was to depict this exotic jour- moral equivalency, rather he explains that The Mind of the Market. ney as a beautiful experience for the audience. pirates form their own versions of civil soci- e-mail: [email protected] Parra samples the sounds produced by the sing- ers and instruments and passes them through an elaborate digital system of real-time signal processing and synthesis. The instrumental and vocal scores are of stunning complexity, Solo journey to a fifth dimension with more than 100 parameters of digital trans- formation, which evolve as the plot progresses. -
Chapter 09584
Author's personal copy Excitons in Magnetic Fields Kankan Cong, G Timothy Noe II, and Junichiro Kono, Rice University, Houston, TX, United States r 2018 Elsevier Ltd. All rights reserved. Introduction When a photon of energy greater than the band gap is absorbed by a semiconductor, a negatively charged electron is excited from the valence band into the conduction band, leaving behind a positively charged hole. The electron can be attracted to the hole via the Coulomb interaction, lowering the energy of the electron-hole (e-h) pair by a characteristic binding energy, Eb. The bound e-h pair is referred to as an exciton, and it is analogous to the hydrogen atom, but with a larger Bohr radius and a smaller binding energy, ranging from 1 to 100 meV, due to the small reduced mass of the exciton and screening of the Coulomb interaction by the dielectric environment. Like the hydrogen atom, there exists a series of excitonic bound states, which modify the near-band-edge optical response of semiconductors, especially when the binding energy is greater than the thermal energy and any relevant scattering rates. When the e-h pair has an energy greater than the binding energy, the electron and hole are no longer bound to one another (ionized), although they are still correlated. The nature of the optical transitions for both excitons and unbound e-h pairs depends on the dimensionality of the e-h system. Furthermore, an exciton is a composite boson having integer spin that obeys Bose-Einstein statistics rather than fermions that obey Fermi-Dirac statistics as in the case of either the electrons or holes by themselves. -
Amplitude/Higgs Modes in Condensed Matter Physics
Amplitude / Higgs Modes in Condensed Matter Physics David Pekker1 and C. M. Varma2 1Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15217 and 2Department of Physics and Astronomy, University of California, Riverside, CA 92521 (Dated: February 10, 2015) Abstract The order parameter and its variations in space and time in many different states in condensed matter physics at low temperatures are described by the complex function Ψ(r; t). These states include superfluids, superconductors, and a subclass of antiferromagnets and charge-density waves. The collective fluctuations in the ordered state may then be categorized as oscillations of phase and amplitude of Ψ(r; t). The phase oscillations are the Goldstone modes of the broken continuous symmetry. The amplitude modes, even at long wavelengths, are well defined and decoupled from the phase oscillations only near particle-hole symmetry, where the equations of motion have an effective Lorentz symmetry as in particle physics, and if there are no significant avenues for decay into other excitations. They bear close correspondence with the so-called Higgs modes in particle physics, whose prediction and discovery is very important for the standard model of particle physics. In this review, we discuss the theory and the possible observation of the amplitude or Higgs modes in condensed matter physics – in superconductors, cold-atoms in periodic lattices, and in uniaxial antiferromagnets. We discuss the necessity for at least approximate particle-hole symmetry as well as the special conditions required to couple to such modes because, being scalars, they do not couple linearly to the usual condensed matter probes. -
Exciton Binding Energy in Small Organic Conjugated Molecule
1 Exciton Binding Energy in small organic conjugated molecule. Pabitra K. Nayak* Department of Materials and Interfaces, Weizmann Institute of Science, Rehovot, 76100, Israel Email: [email protected] Abstract: For small organic conjugated molecules the exciton binding energy can be calculated treating molecules as conductor, and is given by a simple relation BE ≈ 2 e /(4πε0εR), where ε is the dielectric constant and R is the equivalent radius of the molecule. However, if the molecule deviates from spherical shape, a minor correction factor should be added. 1. Introduction An understanding of the energy levels in organic semiconductors is important for designing electronic devices and for understanding their function and performance. The absolute hole transport level and electron transport level can be obtained from theoretical calculations and also from photoemission experiments [1][2][3]. The difference between the two transport levels is referred to as the transport gap (Et). The transport gap is different from the optical gap (Eopt) in organic semiconductors. This is because optical excitation gives rise to excitons rather than free carriers. These excitons are Frenkel excitons and localized to the molecule, hence an extra amount of energy, termed as exciton binding energy (Eb) is needed to produce free charge carriers. What is the magnitude of Eb in organic semiconductors? Answer to this question is more relevant in emerging field of Organic Photovoltaic cells (OPV), due to their impact in determining the output voltage of the solar cells. A lot of efforts are also going on to develop new absorbing material for OPV. It is also important to guess the magnitude of exciton binding energy before the actual synthesis of materials. -
Pion-Induced Transport of Π Mesons in Nuclei
Central Washington University ScholarWorks@CWU All Faculty Scholarship for the College of the Sciences College of the Sciences 2-8-2000 Pion-induced transport of π mesons in nuclei S. G. Mashnik R. J. Peterson A. J. Sierk Michael R. Braunstein Follow this and additional works at: https://digitalcommons.cwu.edu/cotsfac Part of the Atomic, Molecular and Optical Physics Commons, and the Nuclear Commons PHYSICAL REVIEW C, VOLUME 61, 034601 Pion-induced transport of mesons in nuclei S. G. Mashnik,1,* R. J. Peterson,2 A. J. Sierk,1 and M. R. Braunstein3 1T-2, Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 2Nuclear Physics Laboratory, University of Colorado, Boulder, Colorado 80309 3Physics Department, Central Washington University, Ellensburg, Washington 98926 ͑Received 28 May 1999; published 8 February 2000͒ A large body of data for pion-induced neutral pion continuum spectra spanning outgoing energies near 180 MeV shows no dip there that might be ascribed to internal strong absorption processes involving the formation of ⌬’s. This is the same observation previously made for the charged pion continuum spectra. Calculations in an intranuclear cascade model or a cascade exciton model with free-space parameters predict such a dip for both neutral and charged pions. We explore several medium modifications to the interactions of pions with internal nucleons that are able to reproduce the data for nuclei from 7Li through Bi. PACS number͑s͒: 25.80.Hp, 25.80.Gn, 25.80.Ls, 21.60.Ka I. INTRODUCTION the NCX data at angles forward of 90° by a factor of 2 ͓3͔. -
Phonon-Exciton Interactions in Wse2 Under a Quantizing Magnetic Field
ARTICLE https://doi.org/10.1038/s41467-020-16934-x OPEN Phonon-exciton Interactions in WSe2 under a quantizing magnetic field Zhipeng Li1,10, Tianmeng Wang 1,10, Shengnan Miao1,10, Yunmei Li2,10, Zhenguang Lu3,4, Chenhao Jin 5, Zhen Lian1, Yuze Meng1, Mark Blei6, Takashi Taniguchi7, Kenji Watanabe 7, Sefaattin Tongay6, Wang Yao 8, ✉ Dmitry Smirnov 3, Chuanwei Zhang2 & Su-Fei Shi 1,9 Strong many-body interaction in two-dimensional transitional metal dichalcogenides provides 1234567890():,; a unique platform to study the interplay between different quasiparticles, such as prominent phonon replica emission and modified valley-selection rules. A large out-of-plane magnetic field is expected to modify the exciton-phonon interactions by quantizing excitons into dis- crete Landau levels, which is largely unexplored. Here, we observe the Landau levels origi- nating from phonon-exciton complexes and directly probe exciton-phonon interaction under a quantizing magnetic field. Phonon-exciton interaction lifts the inter-Landau-level transition selection rules for dark trions, manifested by a distinctively different Landau fan pattern compared to bright trions. This allows us to experimentally extract the effective mass of both holes and electrons. The onset of Landau quantization coincides with a significant increase of the valley-Zeeman shift, suggesting strong many-body effects on the phonon-exciton inter- action. Our work demonstrates monolayer WSe2 as an intriguing playground to study phonon-exciton interactions and their interplay with charge, spin, and valley. 1 Department of Chemical and Biological Engineering, Rensselaer Polytechnic Institute, Troy, NY 12180, USA. 2 Department of Physics, The University of Texas at Dallas, Richardson, TX 75080, USA. -
Chapter 10 Dynamic Condensation of Exciton-Polaritons
Chapter 10 Dynamic condensation of exciton-polaritons 1 REVIEWS OF MODERN PHYSICS, VOLUME 82, APRIL–JUNE 2010 Exciton-polariton Bose-Einstein condensation Hui Deng Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA Hartmut Haug Institut für Theoretische Physik, Goethe Universität Frankfurt, Max-von-Laue-Street 1, D-60438 Frankfurt am Main, Germany Yoshihisa Yamamoto Edward L. Ginzton Laboratory, Stanford University, Stanford, California 94305, USA; National Institute of Informatics, Hitotsubashi, Chiyoda-ku, Tokyo 101-8430, Japan; and NTT Basic Research Laboratories, NTT Corporation, Atsugi, Kanagawa 243-0198, Japan ͑Published 12 May 2010͒ In the past decade, a two-dimensional matter-light system called the microcavity exciton-polariton has emerged as a new promising candidate of Bose-Einstein condensation ͑BEC͒ in solids. Many pieces of important evidence of polariton BEC have been established recently in GaAs and CdTe microcavities at the liquid helium temperature, opening a door to rich many-body physics inaccessible in experiments before. Technological progress also made polariton BEC at room temperatures promising. In parallel with experimental progresses, theoretical frameworks and numerical simulations are developed, and our understanding of the system has greatly advanced. In this article, recent experiments and corresponding theoretical pictures based on the Gross-Pitaevskii equations and the Boltzmann kinetic simulations for a finite-size BEC of polaritons are reviewed. DOI: 10.1103/RevModPhys.82.1489 PACS number͑s͒: 71.35.Lk, 71.36.ϩc, 42.50.Ϫp, 78.67.Ϫn CONTENTS A. Polariton-phonon scattering 1500 B. Polariton-polariton scattering 1500 1. Nonlinear polariton interaction coefficients 1500 I. Introduction 1490 2. Polariton-polariton scattering rates 1502 II. -
Amplitude Modes in Cold Atoms
T01 Amplitude modes in cold atoms S.D. Huber, Institute for Theoretical Physics, ETH Zurich E-mail address: [email protected] The Bose Hubbard model exhibits a quantum phase transition between an insulating Mott state and a superfluid. We aim at the determination of the excitation spectrum of the superfluid phase, in particular its evolution from the vicinity of the Mott phase towards the weakly interacting regime. Furthermore, we discuss a method allowing to observe our findings in an experiment. We make the link between our microscopic findings and the notion of a “Higgs” mode. Specifically, we highlight the role of emergent symmetries. Recent developments in the description of amplitude modes in exotic chiral Mott insulators will be mentioned. [1] S.D. Huber, E. Altman, H.P. Buchler,¨ and G. Blatter, Phys. Rev. B, 75 085106 (2007) [2] S.D. Huber, B. Theiler, E. Altman, G. Blatter, Phys. Rev. Lett., 100 050404 (2008) [3] S.D. Huber and N.H. Lindner, Proc. Natl. Acad. Sci. USA, 108 19925 (2011) T02 Higgs mode and universal dynamics near quantum criticality D. Podolsky Department of Physics, Technion – Israel Institute of Technology, Haifa 32000, Israel E-mail address: [email protected] The Higgs mode is a ubiquitous collective excitation in condensed matter systems with broken continuous symmetry. Its detection is a valuable test of the corresponding field theory, and its mass gap measures the proximity to a quantum critical point. However, since the Higgs mode can decay into low energy Goldstone modes, its experimental visibility has been questioned. In this talk, I will show that the visibility of the Higgs mode depends on the symmetry of the measured susceptibility. -
Speed of Light and Rates of Clocks in the Space Generation Model of Gravitation, Part 1
GravitationLab.com Speed of Light and Rates of Clocks in the Space Generation Model of Gravitation, Part 1 1 R. BENISH( ) (1) Eugene, Oregon, USA, [email protected] Abstract. — General Relativity’s Schwarzschild solution describes a spherically symmetric gravi- tational field as an utterly static thing. The Space Generation Model (SGM) describes it as an absolutely moving thing. The SGM nevertheless agrees equally well with observations made in the fields of the Earth and Sun, because it predicts almost ex- actly the same spacetime curvature. This success of the SGM motivates deepening the context—especially with regard to the fundamental concepts of motion. The roots of Einstein’s relativity theories thus receive critical examination. A particularly illumi- nating and widely applicable example is that of uniform rotation, which was used to build General Relativity (GR). Comparing Einstein’s logic to that of the SGM, the most significant difference concerns the interpretation of the readings of accelerom- eters and the rates of clocks. Where Einstein infers relativity of motion and space- time symmetry, it is argued to be more logical to infer absoluteness of motion and spacetime asymmetry. This approach leads to reassessments of the essential nature of matter, time, and the dimensionality of space, which lead in turn to some novel cos- mological consequences. Special emphasis is given to the model’s deviations from standard predictions inside matter, which have never been tested, but could be tested by conducting a simple experiment. PACS 04.80.Cc – Experimental tests of gravitational theories. 1. – Introduction; Intended Audience Beware ye, all those bold of spirit who want to suggest new ideas. -
Arxiv:2006.01140V3 [Cond-Mat.Str-El] 28 Jul 2020
arXiv:2006.01140 Deconfined criticality and ghost Fermi surfaces at the onset of antiferromagnetism in a metal Ya-Hui Zhang and Subir Sachdev Department of Physics, Harvard University, Cambridge, MA 02138, USA (Dated: July 29, 2020) Abstract We propose a general theoretical framework, using two layers of ancilla qubits, for deconfined criticality between a Fermi liquid with a large Fermi surface, and a pseudogap metal with a small Fermi surface of electron-like quasiparticles. The pseudogap metal can be a magnetically ordered metal, or a fractionalized Fermi liquid (FL*) without magnetic order. A critical `ghost' Fermi surface emerges (alongside the large electron Fermi surface) at the transition, with the ghost fermions carrying neither spin nor charge, but minimally coupled to (U(1) × U(1))=Z2 or (SU(2) × U(1))=Z2 gauge fields. The (U(1) × U(1))=Z2 case describes simultaneous Kondo breakdown and onset of magnetic order: the two gauge fields induce nearly equal attractive and repulsive interactions between ghost Fermi surface excitations, and this competition controls the quantum criticality. Away from the transition on the pseudogap side, the ghost Fermi surface absorbs part of the large electron Fermi surface, and leads to a jump in the Hall co-efficient. We also find an example of an \unnecessary quantum critical point" between a metal with spin density wave order, and a metal with local moment magnetic order. The ghost fermions contribute an enhanced specific heat near the transition, and could also be detected in other thermal probes. We relate our results to the phases of correlated electron compounds.