The Decay Rates of Ps Species and Bound Muon to Bound Electron Decay Behaviour by Md Samiur Rahman Mir a Thesis Submitted In
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The Particle Zoo
219 8 The Particle Zoo 8.1 Introduction Around 1960 the situation in particle physics was very confusing. Elementary particlesa such as the photon, electron, muon and neutrino were known, but in addition many more particles were being discovered and almost any experiment added more to the list. The main property that these new particles had in common was that they were strongly interacting, meaning that they would interact strongly with protons and neutrons. In this they were different from photons, electrons, muons and neutrinos. A muon may actually traverse a nucleus without disturbing it, and a neutrino, being electrically neutral, may go through huge amounts of matter without any interaction. In other words, in some vague way these new particles seemed to belong to the same group of by Dr. Horst Wahl on 08/28/12. For personal use only. particles as the proton and neutron. In those days proton and neutron were mysterious as well, they seemed to be complicated compound states. At some point a classification scheme for all these particles including proton and neutron was introduced, and once that was done the situation clarified considerably. In that Facts And Mysteries In Elementary Particle Physics Downloaded from www.worldscientific.com era theoretical particle physics was dominated by Gell-Mann, who contributed enormously to that process of systematization and clarification. The result of this massive amount of experimental and theoretical work was the introduction of quarks, and the understanding that all those ‘new’ particles as well as the proton aWe call a particle elementary if we do not know of a further substructure. -
Positronium and Positronium Ions from T
674 Nature Vol. 292 20 August 1981 antigens, complement allotyping and Theoretically the reasons for expecting of HLA and immunoglobulin allotyping additional enzyme markers would clarify HLA and immunoglobulin-gene linked data together with other genetic markers the point. associations with immune response in and environmental factors should allow Although in the face of the evidence general and autoimmune disease in autoimmune diseases to be predicted presented one tends to think of tissue particular are overwhelming: HLA-DR exactly. However, there is still a typing at birth (to predict the occurrence of antigens (or antigens in the same considerable amount of analysis of both autoimmune disease) or perhaps even chromosome area) are necessary for H LA-region genes and lgG-region genes to before one goes to the computer dating antigen handling and presentation by a be done in order to achieve this goal in the service, there are practical scientific lymphoid cell subset; markers in this region general population. reasons for being cautious. For example, (by analogy with the mouse) are important In Japanese families, the occurrence of Uno et a/. selected only 15 of the 30 for interaction ofT cells during a response; Graves' disease can be exactly predicted on families studied for inclusion without immunoglobulin genes are also involved in the basis of HLA and immunoglobulin saying how or why this selection was made. T-cell recognition and control; HLA-A,-B allotypes, but it is too early to start wearing Second, lgG allotype frequencies are very and -C antigens are important at the "Are you my H LA type?" badges outside different in Caucasoid and Japanese effector arm of the cellular response; and Japan. -
First Search for Invisible Decays of Ortho-Positronium Confined in A
First search for invisible decays of ortho-positronium confined in a vacuum cavity C. Vigo,1 L. Gerchow,1 L. Liszkay,2 A. Rubbia,1 and P. Crivelli1, ∗ 1Institute for Particle Physics and Astrophysics, ETH Zurich, 8093 Zurich, Switzerland 2IRFU, CEA, University Paris-Saclay F-91191 Gif-sur-Yvette Cedex, France (Dated: March 20, 2018) The experimental setup and results of the first search for invisible decays of ortho-positronium (o-Ps) confined in a vacuum cavity are reported. No evidence of invisible decays at a level Br (o-Ps ! invisible) < 5:9 × 10−4 (90 % C. L.) was found. This decay channel is predicted in Hidden Sector models such as the Mirror Matter (MM), which could be a candidate for Dark Mat- ter. Analyzed within the MM context, this result provides an upper limit on the kinetic mixing strength between ordinary and mirror photons of " < 3:1 × 10−7 (90 % C. L.). This limit was obtained for the first time in vacuum free of systematic effects due to collisions with matter. I. INTRODUCTION A. Mirror Matter The origin of Dark Matter is a question of great im- Mirror matter was originally discussed by Lee and portance for both cosmology and particle physics. The Yang [12] in 1956 as an attempt to preserve parity as existence of Dark Matter has very strong evidence from an unbroken symmetry of Nature after their discovery cosmological observations [1] at many different scales, of parity violation in the weak interaction. They sug- e.g. rotational curves of galaxies [2], gravitational lens- gested that the transformation in the particle space cor- ing [3] and the cosmic microwave background CMB spec- responding to the space inversion x! −x was not the trum. -
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. -
Collision of a Positron with the Capture of an Electron from Lithium and the Effect of a Magnetic Field on the Particles Balance
chemosensors Article Collision of a Positron with the Capture of an Electron from Lithium and the Effect of a Magnetic Field on the Particles Balance Elena V. Orlenko 1,* , Alexandr V. Evstafev 1 and Fedor E. Orlenko 2 1 Theoretical Physics Department, Institute of Physics, Nanotechnology and Telecommunication, Peter the Great Saint Petersburg Polytechnic University, 195251 St. Petersburg, Russia; [email protected] 2 Scientific and Educational Center for Biophysical Research in the Field of Pharmaceuticals, Saint Petersburg State Chemical Pharmaceutical University (SPCPA), 197376 St. Petersburg, Russia; [email protected] * Correspondence: [email protected]; Tel.: +7-911-762-7228 Abstract: The processes of scattering slow positrons with the possible formation of positronium play an important role in the diagnosis of both composite materials, including semiconductor materials, and for the analysis of images obtained by positron tomography of living tissues. In this paper, we consider the processes of scattering positrons with the capture of an electron and the formation of positronium. When calculating the cross-section for the capture reaction, exchange effects caused by the rearrangement of electrons between colliding particles are taken into account. Comparison of the results of calculating the cross-section with a similar problem of electron capture by a proton showed that the mass effect is important in such a collision process. The loss of an electron by a lithium atom is more effective when it collides with a positron than with a proton or alpha particles. The dynamic equilibrium of the formation of positronium in the presence of a strong magnetic Citation: Orlenko, E.V.; Evstafev, A.V.; field is considered. -
Particle Nature of Matter
Solved Problems on the Particle Nature of Matter Charles Asman, Adam Monahan and Malcolm McMillan Department of Physics and Astronomy University of British Columbia, Vancouver, British Columbia, Canada Fall 1999; revised 2011 by Malcolm McMillan Given here are solutions to 5 problems on the particle nature of matter. The solutions were used as a learning-tool for students in the introductory undergraduate course Physics 200 Relativity and Quanta given by Malcolm McMillan at UBC during the 1998 and 1999 Winter Sessions. The solutions were prepared in collaboration with Charles Asman and Adam Monaham who were graduate students in the Department of Physics at the time. The problems are from Chapter 3 The Particle Nature of Matter of the course text Modern Physics by Raymond A. Serway, Clement J. Moses and Curt A. Moyer, Saunders College Publishing, 2nd ed., (1997). Coulomb's Constant and the Elementary Charge When solving numerical problems on the particle nature of matter it is useful to note that the product of Coulomb's constant k = 8:9876 × 109 m2= C2 (1) and the square of the elementary charge e = 1:6022 × 10−19 C (2) is ke2 = 1:4400 eV nm = 1:4400 keV pm = 1:4400 MeV fm (3) where eV = 1:6022 × 10−19 J (4) Breakdown of the Rutherford Scattering Formula: Radius of a Nucleus Problem 3.9, page 39 It is observed that α particles with kinetic energies of 13.9 MeV or higher, incident on copper foils, do not obey Rutherford's (sin φ/2)−4 scattering formula. • Use this observation to estimate the radius of the nucleus of a copper atom. -
Quantum Mechanics
Quantum Mechanics Richard Fitzpatrick Professor of Physics The University of Texas at Austin Contents 1 Introduction 5 1.1 Intendedaudience................................ 5 1.2 MajorSources .................................. 5 1.3 AimofCourse .................................. 6 1.4 OutlineofCourse ................................ 6 2 Probability Theory 7 2.1 Introduction ................................... 7 2.2 WhatisProbability?.............................. 7 2.3 CombiningProbabilities. ... 7 2.4 Mean,Variance,andStandardDeviation . ..... 9 2.5 ContinuousProbabilityDistributions. ........ 11 3 Wave-Particle Duality 13 3.1 Introduction ................................... 13 3.2 Wavefunctions.................................. 13 3.3 PlaneWaves ................................... 14 3.4 RepresentationofWavesviaComplexFunctions . ....... 15 3.5 ClassicalLightWaves ............................. 18 3.6 PhotoelectricEffect ............................. 19 3.7 QuantumTheoryofLight. .. .. .. .. .. .. .. .. .. .. .. .. .. 21 3.8 ClassicalInterferenceofLightWaves . ...... 21 3.9 QuantumInterferenceofLight . 22 3.10 ClassicalParticles . .. .. .. .. .. .. .. .. .. .. .. .. .. .. 25 3.11 QuantumParticles............................... 25 3.12 WavePackets .................................. 26 2 QUANTUM MECHANICS 3.13 EvolutionofWavePackets . 29 3.14 Heisenberg’sUncertaintyPrinciple . ........ 32 3.15 Schr¨odinger’sEquation . 35 3.16 CollapseoftheWaveFunction . 36 4 Fundamentals of Quantum Mechanics 39 4.1 Introduction .................................. -
On the Possibility of Generating a 4-Neutron Resonance with a {\Boldmath $ T= 3/2$} Isospin 3-Neutron Force
On the possibility of generating a 4-neutron resonance with a T = 3/2 isospin 3-neutron force E. Hiyama Nishina Center for Accelerator-Based Science, RIKEN, Wako, 351-0198, Japan R. Lazauskas IPHC, IN2P3-CNRS/Universite Louis Pasteur BP 28, F-67037 Strasbourg Cedex 2, France J. Carbonell Institut de Physique Nucl´eaire, Universit´eParis-Sud, IN2P3-CNRS, 91406 Orsay Cedex, France M. Kamimura Department of Physics, Kyushu University, Fukuoka 812-8581, Japan and Nishina Center for Accelerator-Based Science, RIKEN, Wako 351-0198, Japan (Dated: September 26, 2018) We consider the theoretical possibility to generate a narrow resonance in the four neutron system as suggested by a recent experimental result. To that end, a phenomenological T = 3/2 three neutron force is introduced, in addition to a realistic NN interaction. We inquire what should be the strength of the 3n force in order to generate such a resonance. The reliability of the three-neutron force in the T = 3/2 channel is exmined, by analyzing its consistency with the low-lying T = 1 states of 4H, 4He and 4Li and the 3H+ n scattering. The ab initio solution of the 4n Schr¨odinger equation is obtained using the complex scaling method with boundary conditions appropiate to the four-body resonances. We find that in order to generate narrow 4n resonant states a remarkably attractive 3N force in the T = 3/2 channel is required. I. INTRODUCTION ergy axis (physical domain) it will have no significant impact on a physical process. The possibility of detecting a four-neutron (4n) structure of Following this line of reasoning, some calculations based any kind – bound or resonant state – has intrigued the nuclear on semi-realistic NN forces indicated null [13] or unlikely physics community for the last fifty years (see Refs. -
TO the POSSIBILITY of BOUND STATES BETWEEN TWO ELECTRONS Alexander A
WEPPP031 Proceedings of IPAC2012, New Orleans, Louisiana, USA TO THE POSSIBILITY OF BOUND STATES BETWEEN TWO ELECTRONS Alexander A. Mikhailichenko, Cornell University, LEPP, Ithaca, NY 14853, USA Abstract spins for reduction of minimal emittance restriction arisen from Eq. 1. In some sense it is an attempt to prepare the We analyze the possibility to compress dynamically the pure quantum mechanical state between just two polarized electron bunch so that the distance between electrons. What is important here is that the distance some electrons in the bunch comes close to the Compton between two electrons should be of the order of the wavelength, arranging a bound state, as the attraction by Compton wavelength. We attracted attention in [2,3] that the magnetic momentum-induced force at this distance attraction between two electrons determined by the dominates repulsion by the electrostatic force for the magnetic force of oppositely oriented magnetic moments. appropriately prepared orientation of the magnetic In this case the resulting spin is zero. Another possibility moments of the electron-electron pair. This electron pair considered below. behaves like a boson now, so the restriction for the In [4], it was suggested a radical explanation of minimal emittance of the beam becomes eliminated. structure of all elementary particles caused by magnetic Some properties of such degenerated electron gas attraction at the distances of the order of Compton represented also. wavelength. In [5], motion of charged particle in a field OVERVIEW of magnetic dipole was considered. In [4] and [5] the term in Hamiltonian responsible for the interaction Generation of beams of particles (electrons, positrons, between magnetic moments is omitted, however as it protons, muons) with minimal emittance is a challenging looks like problem in contemporary beam physics. -
Bound and Quasi Bound States in the Continuum
Bound and Quasi-Bound States in the Continuum One-dimensional models of square-integrable states embedded in continua, first offered by von Neumann and Wigner, can stabilize ordinary resonance levels and have gained importance in connection with solid state heterostructure semi conductor devices. General continuum bound state theories for many-particle systems do not exist, but models for continuum crossings of bound states suggest possible long-lived states, including some double charged anions. Nonlinear varia tional calculations can provide estimates of resonance energies and of the rapid onset of instability in various atomic and molecular ionization phenomena, typifying results found in mathematical "catastrophe theory". One-Dimensional Models :Many years ago von Neumann and Wignerl pointed out that local potentials could have bound (i.e. square-integrable) eigenstates with positive energies. These states are embedded in the continuum of scattering states with the same symmetry, but nevertheless would fail to "ionize". Thus it would be proper to regard these continuum bound states as infinitely sharp resonances. The example offered by von Neumann and Wigner (subsequently corrected by Simon2) was one-dimensional, and involved an oscillatory potential V(x) which behaved essentially as (sin x)/x for large lxl. Likewise the square-integ rable wavefunction l/;(x) for the positive energy bound state was oscillatory but, owing to diffractive interference induced by V(x), the amplitude of l/1 was driven toward zero as lxl increased, so that particle binding resulted. The exist ence of this elementary example naturally raises questions about whether similar continuum bound states could exist in physically more realistic cases. -
Two Dimensional Supersymmetric Models and Some of Their Thermodynamic Properties from the Context of Sdlcq
TWO DIMENSIONAL SUPERSYMMETRIC MODELS AND SOME OF THEIR THERMODYNAMIC PROPERTIES FROM THE CONTEXT OF SDLCQ DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Yiannis Proestos, B.Sc., M.Sc. ***** The Ohio State University 2007 Dissertation Committee: Approved by Stephen S. Pinsky, Adviser Stanley L. Durkin Adviser Gregory Kilcup Graduate Program in Robert J. Perry Physics © Copyright by Yiannis Proestos 2007 ABSTRACT Supersymmetric Discrete Light Cone Quantization is utilized to derive the full mass spectrum of two dimensional supersymmetric theories. The thermal properties of such models are studied by constructing the density of states. We consider pure super Yang–Mills theory without and with fundamentals in large-Nc approximation. For the latter we include a Chern-Simons term to give mass to the adjoint partons. In both of the theories we find that the density of states grows exponentially and the theories have a Hagedorn temperature TH . For the pure SYM we find that TH at infi- 2 g Nc nite resolution is slightly less than one in units of π . In this temperature range, q we find that the thermodynamics is dominated by the massless states. For the system with fundamental matter we consider the thermal properties of the mesonic part of the spectrum. We find that the meson-like sector dominates the thermodynamics. We show that in this case TH grows with the gauge coupling. The temperature and coupling dependence of the free energy for temperatures below TH are calculated. As expected, the free energy for weak coupling and low temperature grows quadratically with the temperature. -
An Introduction to Supersymmetric Quantum Mechanics
MIT Physics 8.05 Nov. 12, 2007 SUPPLEMENTARY NOTES ON SOLVING THE RADIAL WAVE EQUATION USING OPERATOR METHODS Alternative title: An Introduction to Supersymmetric Quantum Mechanics 1 Introduction In lecture this week we reduced the problem of finding the energy eigenstates and eigenvalues of hydrogenic atoms to finding the eigenstates and eigenvalues of the Coulomb Hamiltonians d2 HCoul = + V (x) (1) ℓ −dx2 ℓ where ℓ(ℓ + 1) 1 V (x)= . (2) ℓ x2 − x (You will review this procedure on a Problem Set.) That is, we are looking for the eigenstates u (x) and eigenvalues κ2 satisfying νℓ − νℓ HCoul u (x)= κ2 u (x) . (3) ℓ νℓ − νℓ νℓ Here the dimensionless variable x and dimensionless eigenvalue constants κνℓ are related to r and the energy by a 2µe4Z2 r = x , E = κ2 , (4) 2Z νℓ − h¯2 νℓ 2 2 −1 where a =¯h /(me ) is the Bohr radius, the nuclear charge is Ze, and µ = (1/m +1/mN ) is the reduced mass in terms of the electron mass m and nuclear mass mN . Even though Coul the Hamiltonians Hℓ secretly all come from a single three-dimensional problem, for our present purposes it is best to think of them as an infinite number of different one-dimensional Hamiltonians, one for each value of ℓ, each with different potentials Vℓ(x). The Hilbert space for these one-dimensional Hamiltonians consists of complex functions of x 0 that vanish ≥ for x 0. The label ν distinguishes the different energy eigenstates and eigenvalues for a →Coul given Hℓ .