The Antiparticles of Neutral Bosons
Total Page:16
File Type:pdf, Size:1020Kb

Load more
Recommended publications
-
On the Mass Spectrum of Exotic Protonium Atom in Oscillator Representation Method
International Journal of Advanced Science and Technology Vol.74 (2015), pp.43-48 http://dx.doi.org/10.14257/ijast.2015.74.05 On the Mass Spectrum of Exotic Protonium Atom in Oscillator Representation Method Arezu Jahanshir Assistant professor and faculty member of Bueinzahra Technical University, Iran [email protected] Abstract In the given paper one determines the constituent mass of the bound state and binding energy of hadronic exotic system, according to the basis investigation of the asymptotically behavior of the loop function of scalar particles in the external electromagnet field are analytically determined exploration of these states through relativistic and non-perturbative corrections. It is shown that, the mass spectrum of a relativistic bound state of protonium consisting from proton and anti-proton is differing from a mass of initial particles. Keywords: protonium, constituent mass, Hamiltonian, Green function, scalar particles 1. Introduction All of theoretical high energy physician by using mathematical methods and new theories try to understand how bound state arise in the formalism of quantum field theory and to work out effective methods to calculate all characteristics of these bound states, especially their masses, binding energy and spin interactions. The analysis of a bound state is difficult when the interaction have to be considered as relativistic, i.e. when they travel at speeds considerably near the "c". The theoretical criterion is that the coupling constant should be strong [1-6] and masses of intermediate particles gluons in quantum chromodynamic should be big in comparison with masses of constituents. New importance to the exotic hadronic bound state physics was given by the development of quantum chromodynamic, the modern theory of strong interactions. -
The Neutrino Theory of Light
THE NEUTRINO THEORY OF LIGHT. BY MAx BORN AND N. ~. I~AGENDRA N/kT~I. (From the Department of Physics, Indian Institute o[ Science, Bangalore.) Received March 18, 1936. 7. Introduction. TI~E most important contribution during the last years to the fundamental conceptions of theoretical physics seems to be the development of a new theory of light which contains the acknowledged one as a limiting case, but connects the optical phenomena with those of a very different kind, radio- activity. The idea that the photon is not an elementary particle but a secondary one, composed of simpler particles, has been first mentioned by p. Jordan 1. His argument was a statistical one, based on the fact, that photons satisfy the Bose-Einstein statistics. It is known from the theory of composed particles as nuclei, atoms or molecules, that this statistics may appear for such systems, which are compounds of elementary particles satisfying the Fermi-Dirac statistics (e.g., electrons or protons). After the discovery of the neutrino, de Broglie2 suggested that a photon hv is composed of a " neutrino " and an " anti-neutrino," each having the energy He has developed some interesting mathematical relations between the wave equation of a neutrino (which he assumed to be Dirac's equation for a vanish- {ngly small rest;mass) and Maxwell's field equations. But de Broglie has not touched the central problem, namely, as to how the Bose-Einstein statistics of the photons arises from the Fermi-statistics of the neutrinos. This ques- tion cannot be solved in the same way as in the cases mentioned above (material particles) Where it is a consequence of considering the composed system as a whole neglecting internal motions. -
Progress and Simulations for Intranuclear Neutron-Antineutron 40Ar Transformations in 18 Joshua L
PHYSICAL REVIEW D 101, 036008 (2020) Progress and simulations for intranuclear neutron-antineutron 40Ar transformations in 18 Joshua L. Barrow * The University of Tennessee at Knoxville, Department of Physics and Astronomy, † 1408 Circle Drive, Knoxville, Tennessee 37996, USA ‡ Elena S. Golubeva and Eduard Paryev§ Institute for Nuclear Research, Russian Academy of Sciences, Prospekt 60-letiya Oktyabrya 7a, Moscow 117312, Russia ∥ Jean-Marc Richard Institut de Physique des 2 Infinis de Lyon, Universit´e de Lyon, CNRS-IN2P3–UCBL, 4 rue Enrico Fermi, Villeurbanne 69622, France (Received 10 June 2019; accepted 29 January 2020; published 18 February 2020) With the imminent construction of the Deep Underground Neutrino Experiment (DUNE) and Hyper- Kamiokande, nucleon decay searches as a means to constrain beyond standard model extensions are once again at the forefront of fundamental physics. Abundant neutrons within these large experimental volumes, along with future high-intensity neutron beams such as the European Spallation Source, offer a powerful, high-precision portal onto this physics through searches for B and B − L violating processes such as neutron-antineutron transformations (n → n¯), a key prediction of compelling theories of baryogenesis. With this in mind, this paper discusses a novel and self-consistent intranuclear simulation of this process 40 within 18Ar, which plays the role of both detector and target within the DUNE’s gigantic liquid argon time projection chambers. An accurate and independent simulation of the resulting intranuclear annihilation respecting important physical correlations and cascade dynamics for this large nucleus is necessary to understand the viability of such rare searches when contrasted against background sources such as atmospheric neutrinos. -
Exotic Double-Charm Molecular States with Hidden Or Open Strangeness and Around 4.5 ∼ 4.7 Gev
PHYSICAL REVIEW D 102, 094006 (2020) Exotic double-charm molecular states with hidden or open strangeness and around 4.5 ∼ 4.7 GeV † Fu-Lai Wang and Xiang Liu * School of Physical Science and Technology, Lanzhou University, Lanzhou 730000, China and Research Center for Hadron and CSR Physics, Lanzhou University and Institute of Modern Physics of CAS, Lanzhou 730000, China (Received 1 September 2020; accepted 16 October 2020; published 10 November 2020) à In this work, we investigate the interactions between the charmed-strange meson (Ds;Ds )inH-doublet à and the (anti-)charmed-strange meson (Ds1;Ds2)inT-doublet, where the one boson exchange model is adopted by considering the S-D wave mixing and the coupled-channel effects. By extracting the effective ¯ potentials for the discussed HsTs and HsTs systems, we try to find the bound state solutions for the corresponding systems. We predict the possible hidden-charm hadronic molecular states with hidden à ¯ PC 0−− 0−þ à ¯ à strangeness, i.e., the Ds Ds1 þ c:c: states with J ¼ ; and the Ds Ds2 þ c:c: states with PC −− −þ J ¼ 1 ; 1 . Applying the same theoretical framework, we also discuss the HsTs systems. Unfortunately, the existence of the open-charm and open-strange molecular states corresponding to the HsTs systems can be excluded. DOI: 10.1103/PhysRevD.102.094006 ¯ ðÞ I. INTRODUCTION strong evidence to support these Pc states as the ΣcD - – Studying exotic hadronic states, which are very type hidden-charm pentaquark molecules [10 16]. different from conventional mesons and baryons, is an Before presenting our motivation, we first need to give a intriguing research frontier full of opportunities and chal- brief review of how these observed XYZ states were lenges in hadron physics. -
Antiproton–Proton Scattering Experiments with Polarization ( Collaboration) PAX Abstract
Technical Proposal for Antiproton–Proton Scattering Experiments with Polarization ( Collaboration) PAX arXiv:hep-ex/0505054v1 17 May 2005 J¨ulich, May 2005 2 Technical Proposal for PAX Frontmatter 3 Technical Proposal for Antiproton–Proton Scattering Experiments with Polarization ( Collaboration) PAX Abstract Polarized antiprotons, produced by spin filtering with an internal polarized gas target, provide access to a wealth of single– and double–spin observables, thereby opening a new window to physics uniquely accessible at the HESR. This includes a first measurement of the transversity distribution of the valence quarks in the proton, a test of the predicted opposite sign of the Sivers–function, related to the quark dis- tribution inside a transversely polarized nucleon, in Drell–Yan (DY) as compared to semi–inclusive DIS, and a first measurement of the moduli and the relative phase of the time–like electric and magnetic form factors GE,M of the proton. In polarized and unpolarized pp¯ elastic scattering, open questions like the contribution from the odd charge–symmetry Landshoff–mechanism at large t and spin–effects in the extraction | | of the forward scattering amplitude at low t can be addressed. The proposed de- | | tector consists of a large–angle apparatus optimized for the detection of DY electron pairs and a forward dipole spectrometer with excellent particle identification. The design and performance of the new components, required for the polarized antiproton program, are outlined. A low–energy Antiproton Polarizer Ring (APR) yields an antiproton beam polarization of Pp¯ = 0.3 to 0.4 after about two beam life times, which is of the order of 5–10 h. -
Interpreted History of Neutrino Theory of Light and Its Futureprovided by CERN Document Server
View metadata, citation and similar papers at core.ac.uk brought to you by CORE Interpreted History Of Neutrino Theory Of Light And Its Futureprovided by CERN Document Server W. A. Perkins Perkins Advanced Computing Systems, 12303 Hidden Meadows Circle, Auburn, CA 95603, USA E-mail: [email protected] De Broglie's original idea that a photon is composed of a neutrino- antineutrino pair bound by some interaction was severely modified by Jor- dan. Although Jordan addressed an important problem (photon statistics) that de Broglie had not considered, his modifications may have been detri- mental to the development of a composite photon theory. His obsession with obtaining Bose statistics for the composite photon made it easy for Pryce to prove his theory untenable. Pryce also indicated that forming transversely- polarized photons from neutrino-antineutrino pairs was impossible, but oth- ers have shown that this is not a problem. Following Pryce, Berezinskii has proven that any composite photon theory (using fermions) is impossible if one accepts five assumptions. Thus, any successful composite theory must show which of Berezinskii's assumptions is not valid. A method of forming composite particles based on Fermi and Yang's model will be discussed. Such composite particles have properties similar to conventional photons. However, unlike the situation with conventional photon theory, Lorentz invariance can be satisfied without the need for gauge invariance or introducing non-physical photons. PACS numbers: 14.70.Bh,12.60.Rc,12.20.Ds I. INTRODUCTION The theoretical development of a composite photon theory (based on de Broglie’s idea that the photon is composed of a neutrino-antineutrino pair [1] bound by some interaction) has had a stormy history with many negative papers. -
Plasma Physics and Fusion Research Royal Institute of Technology S-100 44 Stockholm Sweden Trita-Pfu-91-05
ISSN 0348-7644 TRITA-PFU-91-05 NEUTRON TIME-OF-FLIGHT COUNTERS AND SPECTROMETERS FOR DIAGNOSTICS OF BURNING FUSION PLASMAS T. Elevant and M. Olsson Research and Training Programme on CONTROLLED THERMONUCLEAR FUSION AND PLASMA PHYSICS (EUR-NFR) PLASMA PHYSICS AND FUSION RESEARCH ROYAL INSTITUTE OF TECHNOLOGY S-100 44 STOCKHOLM SWEDEN TRITA-PFU-91-05 NEUTRON TIME-OF-FLIGHT COUNTERS AND SPECTROMETERS FOR DIAGNOSTICS OF BURNING FUSION PLASMAS T. Elevant and M. Olsson Stockholm, February 1991 Department of Plasma Physics and Fusion Research Royal Institute of Technology 5-100 44 Stockholm, Sweden Neutron Time-of-Flight Counters and Spectrometers for Diagnostics of burning Fusion Plasmas. T. Elevant and M. Olsson. Department of Plasma Physics and Fusion Research, The Royal Institute of Technology, S-10044 Stockholm, Sweden. ABSTRACT Experiment with burning fusion plasmas in tokamaks will place particular requirements on neutron measurements from radiation resistance-, physics-, burn control- and reliability considerations. The possibility to meet these needs by measurements of neutron fluxes and energy spectra by means of time-of-flight techniques are described. Reference counters and spectrometers are proposed and characterized with respect to efficiency, count-rate capabilities, energy resolution and tolerable neutron and y-radiation background levels. The instruments can be used in a neutron camera and are capable to operate in collimated neutron fluxes up to levels corresponding to full nuclear output power in the next generation of experiments. Energy resolutions of the spectrometers enables determination of ion temperatures from 3 [keV] through analysis of the Doppler broadening. Primarily, the instruments are aimed for studies of 14 [MeV] neutrons produced in [d,t]-plasmas but can, after minor modifications, be used for analysis of 2.45 [McV] neutrons produced in [d,d]-plasmas. -
Printed Here
PHYSICAL REVIEW C, VOLUME 66, NUMBER 3 Selected Abstracts from Other Physical Review Journals Abstracts of papers which are published in other Physical Review journals and may be of interest to Physical Review C readers are printed here. The Editors of Physical Review C routinely scan the abstracts of Physical Review D papers. Appropriate abstracts of papers in other Physical Review journals may be included upon request. Supernova neutrinos and the LSND evidence for neutrino oscil- We present a study of inhomogeneous big bang nucleosynthesis lations. Michel Sorel and Janet Conrad, Department of Physics, with emphasis on transport phenomena. We combine a hydrody- Columbia University, New York, New York 10027. ͑Received 15 namic treatment to a nuclear reaction network and compute the light December 2001; published 23 August 2002͒ element abundances for a range of inhomogeneity parameters. We ®nd that shortly after annihilation of electron-positron pairs, Thom- Å The observation of the e energy spectrum from a supernova son scattering on background photons prevents the diffusion of the burst can provide constraints on neutrino oscillations. We derive remaining electrons. Protons and multiply charged ions then tend to formulas for adiabatic oscillations of supernova antineutrinos for a diffuse into opposite directions so that no net charge is carried. Ions variety of 3- and 4-neutrino mixing schemes and mass hierarchies with ZϾ1 get enriched in the overdense regions, while protons which are consistent with the Liquid Scintillation Neutrino Detector diffuse out into regions of lower density. This leads to a second Å →Å ͑LSND͒ evidence for e oscillations. Finally, we explore the burst of nucleosynthesis in the overdense regions at TϽ20 keV, constraints on these models and LSND given by the supernova SN leading to enhanced destruction of deuterium and lithium. -
Relativistic Kinematics of Particle Interactions Introduction
le kin rel.tex Relativistic Kinematics of Particle Interactions byW von Schlipp e, March2002 1. Notation; 4-vectors, covariant and contravariant comp onents, metric tensor, invariants. 2. Lorentz transformation; frequently used reference frames: Lab frame, centre-of-mass frame; Minkowski metric, rapidity. 3. Two-b o dy decays. 4. Three-b o dy decays. 5. Particle collisions. 6. Elastic collisions. 7. Inelastic collisions: quasi-elastic collisions, particle creation. 8. Deep inelastic scattering. 9. Phase space integrals. Intro duction These notes are intended to provide a summary of the essentials of relativistic kinematics of particle reactions. A basic familiarity with the sp ecial theory of relativity is assumed. Most derivations are omitted: it is assumed that the interested reader will b e able to verify the results, which usually requires no more than elementary algebra. Only the phase space calculations are done in some detail since we recognise that they are frequently a bit of a struggle. For a deep er study of this sub ject the reader should consult the monograph on particle kinematics byByckling and Ka jantie. Section 1 sets the scene with an intro duction of the notation used here. Although other notations and conventions are used elsewhere, I present only one version which I b elieveto b e the one most frequently encountered in the literature on particle physics, notably in such widely used textb o oks as Relativistic Quantum Mechanics by Bjorken and Drell and in the b o oks listed in the bibliography. This is followed in section 2 by a brief discussion of the Lorentz transformation. -
NEW ENTITIES, OLD PARADIGMS: ELEMENTARY PARTICLES in the 1930S1
LUE,, vol. 27,2004,435-464 NEW ENTITIES, OLD PARADIGMS: ELEMENTARY PARTICLES IN THE 1930s1 JAUME NAVARRO Cambridge University RESUMEN Al3STRACT En este artículo pretendo analizar los The aim of this paper is to analyse the procesos por los cuales se descubrieron y processes by which a number of new ele- aceptaron nuevas partículas elementales mentary particles were discovered and en los años anteriores a la segunda guerra accepted by the scientific community in the mundiaL Muchos libros de divulgación de years before World War 11. Many popular física de partículas elementales suelen accounts of particle physics depict a linear narrar una historia lineal sobre la bŭsque- history of the search for the ultimate con- da de las ŭltimas partículas constitutivas stituents of matter, which would start in de la materia. Ésta empezaría en 1897, 1897, with the discovery of the electron, con el descubrimiento del electrón, y and move on to an increasing number of avanzaría linealmente añadiendo nuevas new particles: photon, proton, neutron, partículas: fotones, protones, neutrones, positron, neutrino... Nevertheless, the positrones, neutrinos, etc. Sin embargo, el question about the building-blocks of the problema de los elementos constitutivos material world seems to have been a sec- de la materia no era un tema central de la ondary concern for physidsts who were fisica en la década de 1930. En sentido involved in the discovery of the new ele- estricto, se puede asegurar que antes de la mentary particles in the 1930s. In the segunda guerra mundial no existz'a una strong sense, one can argue that there was nueva disciplina de partículas elementales no such thing as a new discipline of particle en física. -
A Conjectural Preon Theory and Its Implications
A Conjectural Preon Theory and its Implications Rupert Gerritsen Copyright © - Rupert Gerritsen Batavia Online Publishing A Conjectural Preon Theory and its Implications Batavia Online Publishing Canberra, Australia Published by Batavia Online Publishing 2012 Copyright © Rupert Gerritsen National Library of Australia Cataloguing-in-Publication Data Author: Gerritsen, Rupert, 1953- Title: A Conjectural Preon Theory ISBN: 978-0-9872141-5-7 (pbk.) Notes: Includes bibliographic references Subjects: Particles (Nuclear physics) Dewey Number: 539.72 Copyright © - Rupert Gerritsen 1 A Conjectural Preon Theory and its Implications At present the dominant paradigm in particle physics is the Standard Model. This theory has taken hold over the last 30 years as its predictions of new particles have been dramatically borne out in increasingly sophisticated experiments. Despite this it would seem that the Standard Model has some shortcomings and leaves a number of questions unanswered. The number of arbitrary constants and parameters incorporated in the Model is one unsatisfactory aspect, as is its inability to explain the masses of the quarks and leptons. Another problematic area often cited is the Model’s failure to account for the number of generations of quarks and leptons. The plethora of “fundamental” particles also appears to represent a major weakness in the Standard Model. There are 16 “fundamental” or “elementary” particles, as well as their anti-particles, engendered in the Standard Model, along with 8 types of gluons. This difficulty may be further compounded by theorizing based on supersymmetry, as an extension of the Standard Model, because it requires heavier twins for the known particles. Furthermore the Higgs mechanism, postulated to generate mass in particles, has not as yet been validated experimentally. -
Birth of the Neutrino, from Pauli to the Reines-Cowan Experiment 1
Birth of the neutrino, from Pauli to the Reines-Cowan experiment C. Jarlskog Division of Mathematical Physics, LTH, Lund University Box 118, S-22100 Lund, Sweden Fifty years after the introduction of the neutrino hypothesis, Bruno Pontecorvo praised its inventor stating 1: \It is difficult to find a case where the word \intuition" characterizes a human achievement better than in the case of the neutrino invention by Pauli". The neutrino a hypothesis generated a huge amount of excitement in physics. Several hundred papers were written about the neutrino before its discovery in the Reines-Cowan experiment. My task here is to share some of that excitement with you. 1 Introduction I would like to start by expressing my gratitude to the organizers for having invited me to give this talk. Indeed I am \Super Glad" to be here because of a very special reason. A few years ago I produced a book in honor of my supervisor Professor Gunnar K¨all´en (1926-1968) 2. Because I lacked the necessary experience, it took me about three years to produce the book. First I had to locate K¨all´en'sscholarly belongings, among them his scientific correspondence. Due to tragic events that took place after his death, the search took some time. Eventually, I found 18 boxes which had been deposited at the Manuscripts & Archives section of the Lund University's Central Library. To my great surprise, this “K¨all´enCollection" contained about 160 letters exchanged between him and Pauli - almost all in German. After Pauli's death in 1958 his widow Franziska (called Franka) collected his scientific belongings and donated them to CERN and not to ETH in Z¨urich, where Pauli had been a professor since 1928, i.e., for 30 years.