Theoretical Investigation of Subluminal Particles Endowed with Imaginary Mass

Total Page:16

File Type:pdf, Size:1020Kb

Theoretical Investigation of Subluminal Particles Endowed with Imaginary Mass Article Theoretical Investigation of Subluminal Particles Endowed with Imaginary Mass Luca Nanni Faculty of Natural Science, University of Ferrara, 44122 Ferrara, Italy; [email protected] Abstract: In this article, the general solution of the tachyonic Klein–Gordon equation is obtained as a Fourier integral performed on a suitable path in the complex w-plane. In particular, it is proved that this solution does not contain any superluminal components under the given boundary conditions. On the basis of this result, we infer that all possible spacelike wave equations describe the dynamics of subluminal particles endowed with imaginary mass. This result is validated for the Chodos equation, used to describe the hypothetical superluminal behaviour of the neutrino. In this specific framework, it is proved that the wave packet propagates in spacetime with subluminal group velocities and that it behaves as a localized wave for sufficiently small energies. Keywords: tachyons; Klein–Gordon equation; tachyon-like Dirac equation; relativistic wave packet PACS: 03.65.Pm; 03.65.Ge; 03.65.Db 1. Introduction The physics of tachyons is an intriguing and fascinating subject that has attracted the attention of physicists in both the pre-relativistic [1–3] and post-relativistic epochs [4–10]. Citation: Nanni, L. Theoretical However, the majority of the scientific community still considers it a speculative theory, and Investigation of Subluminal Particles Endowed with Imaginary Mass. there are only a few efforts aimed at finding the experimental evidence that could make it a Particles 2021, 4, 325–332. https:// candidate for extending the current Standard Model [11]. A comprehensive overview of the doi.org/10.3390/particles4020027 most relevant experiments dealing with the superluminal behaviour of waves and particles is detailed in [9,12–15]. If considered in the framework of quantum mechanics, tachyons Academic Editor: Kazuharu Bamba exhibit completely unexpected behaviours [16–18]. In particular, half-integer free fermions endowed with imaginary mass behave like wave trains propagating with subluminal group Received: 29 May 2021 velocities. The aim of this study is to verify whether this result can be generalized for any Accepted: 15 June 2021 particle regardless of its spin. The basic idea is that the individual components of spinor Published: 18 June 2021 wave functions, which are solutions of the tachyonic wave equations, must satisfy the tachyonic Klein–Gordon (TKG) equation as well [19]. Finding a general solution of the Publisher’s Note: MDPI stays neutral TKG equation without spacelike components means proving that any solution of the wave with regard to jurisdictional claims in equations of particles with negative mass squared represents a wave packet that propagates published maps and institutional affil- with subluminal group velocity. As proposed by Salesi, these particles are called pseudo- iations. tachyons (PTs), namely particles travelling with slower-than-light velocity but fulfilling the tachyonic energy-momentum relation E2 = p2c2 + m2c4, where m = im denotes the imaginary mass. The obtained result will be validated for the Chodos equation [20] which 1 describes the behaviour of a 2 -spin tachyon using a more different analytical approach Copyright: © 2021 by the author. than that discussed in [18]. Licensee MDPI, Basel, Switzerland. This article is an open access article 2. Preliminary Notions on the Fourier Transforms in the Complex Plane distributed under the terms and To facilitate the reading of Section3 of this article, a brief review on the theory of the conditions of the Creative Commons Fourier transform in the complex plane is presented [21]. Attribution (CC BY) license (https:// creativecommons.org/licenses/by/ 4.0/). Particles 2021, 4, 325–332. https://doi.org/10.3390/particles4020027 https://www.mdpi.com/journal/particles Particles 2021, 4 326 Let f (x) be an integrable function; its Fourier transform is defined as: ¥ Z F[ f (x)] = fe(w) = f (x)eiwxdx, (1) −¥ while the inverse Fourier transform is: ¥ h i 1 Z F −1 fe(w) = fe(w)e−iwxdw. (2) 2p −¥ Definitions (1) and (2) can be generalized by allowing w to take complex values. To this end, let us suppose that f (x) grows at most exponentially at infinity, i.e., f (x) = O ecjxj as x ! ±¥ and c > 0. Moreover, we split up f (x) as follows: f (x) = f+(x) + f−(x) : f+(x) = 0 8x< 0 and f−(x) = 0 8x >0 (3) The Fourier transform of the component f+(x) is: ¥ Z iRe(w)x −Im(w)x fe+(w) = f+(x)e e dx. (4) 0 It is evident that: ¥ Z −Im(w)x fe+(w) ≤ j f+(x)je dx, (5) 0 and the integral converges provided Im(w) > c. Therefore, fe+(w) exists and is holomor- phic for Im(w) > c. Next, we need to extend the Fourier inversion theorem to recover f+(x) from fe+(w). −ax h i To this end, let F+(x) = f+(x)e , where a > c, so that Fe+(w) = fe+(w + ia) exists and is holomorphic for Im(w) > c − a, in particular for w 2 R, since a > c. Thus, we can apply the Fourier transform inversion theorem obtaining: ¥ ¥ 1 R −iwx −ax 1 R −iwx F+(x) = 2p Fe+(w)e dw ) f+(x)e = 2p fe+(w + ia)e dw −¥ −¥ ¥ (6) 1 R −i(w+ia)x ) f+(x) = 2p fe+(w + ia)e dw. −¥ The final integral corresponds to an integration along a horizontal contour in the complex w-plane: ¥+ia Z 1 −iwx f+(x) = fe+(w)e dw. (7) 2p −¥+ia Suppose fe+(w) can be continued below Im(w) = c, so that it is holomorphic in some region W+ ⊃ fw : Im(w) > cg except for singularities at w = a1, a2, ··· . By the deformation theory, the inversion contour G+ = fx + ia : −¥ < x < ¥g may be deformed into W+ provided it passes above the singularities of fe+(w). Since the singularities of fe+(w) are below the inversion contour, for x < 0, we can close the contour at +i¥. This gives the expected result that f+(x) = 0 for x < 0. For x > 0, we would need to close the contour in Im(w) < 0, picking up the contributions from the singularities in fe+(w) and giving a nonzero value of f+(x). The same procedure works for f−(x) with everything upside down, namely fe−(w) can be continued above Im(w) = −c, so that it is holomorphic in some region W− ⊃ Particles 2021, 4 327 fw : Im(w) < −cg except for singularities at w = b1, b2, ··· . If there is a non-empty overlap region W = W+ \ W−nfaig [ bj , where faig are the singularities of fe+(w) and bj are the singularities of fe−(w), then the Fourier transform of f (x) is defined as: fe(w) = fe+(w) + fe−(w), (8) for w 2 W. Moreover, if G+ and G− can be deformed into the same contour G ⊂ W, with G above the singularities of fe+(w) and below the singularities of fe−(w), then: 1 Z f (x) = fe(w)e−iwxdw. (9) 2p G What is discussed in this section represents the method that will be implemented below to solve the TKG equation. 3. Dynamics of Wave Packets in the TKG Equation The TKG equation can be obtained by quantizing the tachyonic energy-momentum relation using the operators E ! i}¶/¶t and p ! −i}cr : ¶2 }2 − }2c2r2 − m2c4 y(r, t) = 0. (10) ¶t2 For free scalar particles, Equation (10) can be solved by Fourier transform in time, which allows decomposing the wave function y(r, t) in its monochromatic temporal com- ponents, using the initial conditions given for y(r, t)jr=0 and ¶y(r, t)/¶rjr=0. To simplify the following discussion, we suppose that the motion of the particle takes place along the z-axis. The solution is a wave packet represented by the following inverse Fourier transform: 1 Z h i y(z, t) = A(w)eiK(w)z + B(w)e−iK(w)z e−iwtdw, (11) 2p G where G is a path in the w-plane. The quantity w is defined as w = ±E/}, and, for a tachyon, it is always a real quantity except when E = ±mc2 (this last statement will be clarified in Section4 where we calculate the group velocity of the tachyonic wave packet). In fact: −1/2 −1/2 u2 u2 E = ±gmc2 = ± 1 − imc2 = ± − 1 mc2, (12) c2 c2 where g is the tachyonic Lorentz factor and u > c is the classical tachyonic velocity. Returning to Equation (11), the term K(w) is the dispersion relation whose characteristic equation is: w2 − w2 K2(w) = 0 where w2 = −m2c4/}2. (13) c2 0 Equation (13) is obtained from Equation (10) upon factorisation y(z, t) = j(z)e−iwt. The aim is to prove that Equation (1) admits a general solution in which no spacelike components arise. In other words, we want to prove that this solution is completely analogous to the one that solves the ordinary KG equation, where w is always real, and tends to the solution of the d’Alembert wave equation as the mass energy tends to zero. We point out that the spacelike components are those associated with complex values of w, and therefore of K(w). The coefficients A(w) and B(w) are calculated once the following boundary conditions have been set [21]: 0 f (t) = y(0, t) and f (t) = ¶y(z, t)/¶zjz=0. (14) Particles 2021, 4 328 As we will see, these conditions determine the choice of the path G of integration. Using the boundary conditions in Equation (14), we obtain [21]: 8 h 0 i ( ) = 1 R ¥ ( ) − f (t) iwt < A w 2 −¥ f t i K(w) e dt h 0 i (15) ( ) = 1 R ¥ ( ) + f (t) iwt : B w 2 −¥ f t i K(w) e dt The computation of the integrals in Equation (15) can be simplified if we consider f (t) as a semi-infinite wave train with a sharp edge.
Recommended publications
  • Off-Shell Interactions for Closed-String Tachyons
    Preprint typeset in JHEP style - PAPER VERSION hep-th/0403238 KIAS-P04017 SLAC-PUB-10384 SU-ITP-04-11 TIFR-04-04 Off-Shell Interactions for Closed-String Tachyons Atish Dabholkarb,c,d, Ashik Iqubald and Joris Raeymaekersa aSchool of Physics, Korea Institute for Advanced Study, 207-43, Cheongryangri-Dong, Dongdaemun-Gu, Seoul 130-722, Korea bStanford Linear Accelerator Center, Stanford University, Stanford, CA 94025, USA cInstitute for Theoretical Physics, Department of Physics, Stanford University, Stanford, CA 94305, USA dDepartment of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India E-mail:[email protected], [email protected], [email protected] Abstract: Off-shell interactions for localized closed-string tachyons in C/ZN super- string backgrounds are analyzed and a conjecture for the effective height of the tachyon potential is elaborated. At large N, some of the relevant tachyons are nearly massless and their interactions can be deduced from the S-matrix. The cubic interactions be- tween these tachyons and the massless fields are computed in a closed form using orbifold CFT techniques. The cubic interaction between nearly-massless tachyons with different charges is shown to vanish and thus condensation of one tachyon does not source the others. It is shown that to leading order in N, the quartic contact in- teraction vanishes and the massless exchanges completely account for the four point scattering amplitude. This indicates that it is necessary to go beyond quartic inter- actions or to include other fields to test the conjecture for the height of the tachyon potential. Keywords: closed-string tachyons, orbifolds.
    [Show full text]
  • Meson Spectra from a Dynamical Three-Field Model of Ads/QCD
    Meson Spectra from a Dynamical Three-Field Model of AdS/QCD A THESIS SUBMITTED TO THE FACULTY OF THE GRADUATE SCHOOL OF THE UNIVERSITY OF MINNESOTA BY Sean Peter Bartz IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY Joseph I. Kapusta, Adviser August, 2014 c Sean Peter Bartz 2014 ALL RIGHTS RESERVED Acknowledgements There are many people who have earned my gratitude for their contribution to mytime in graduate school. First, I would like to thank my adviser, Joe Kapusta, for giving me the opportunity to begin my research career, and for guiding my research during my time at Minnesota. I would also like to thank Tom Kelley, who helped guide me through the beginnings of my research and helped me understand the basics of the AdS/CFT correspondence. My graduate school experience was shaped by my participation in the Department of Energy Office of Science Graduate Fellowship for three years. The research support for travel made my graduate career a great experience, and the camaraderie with the other fellows was also fulfilling. I would like to thank Dr. Ping Ge, Cayla Stephenson, Igrid Gregory, and everyone else who made the DOE SCGF program a fulfilling, eye-opening experience. Finally, I would like to thank the members of my thesis defense committee: Ron Poling, Tony Gherghetta, and Tom Jones. This research is supported by the Department of Energy Office of Science Graduate Fellowship Program (DOE SCGF), made possible in part by the American Recovery and Reinvestment Act of 2009, administered by ORISE-ORAU under contract no.
    [Show full text]
  • Arxiv:2012.15102V2 [Hep-Ph] 13 May 2021 T > Tc
    Confinement of Fermions in Tachyon Matter at Finite Temperature Adamu Issifu,1, ∗ Julio C.M. Rocha,1, y and Francisco A. Brito1, 2, z 1Departamento de F´ısica, Universidade Federal da Para´ıba, Caixa Postal 5008, 58051-970 Jo~aoPessoa, Para´ıba, Brazil 2Departamento de F´ısica, Universidade Federal de Campina Grande Caixa Postal 10071, 58429-900 Campina Grande, Para´ıba, Brazil We study a phenomenological model that mimics the characteristics of QCD theory at finite temperature. The model involves fermions coupled with a modified Abelian gauge field in a tachyon matter. It reproduces some important QCD features such as, confinement, deconfinement, chiral symmetry and quark-gluon-plasma (QGP) phase transitions. The study may shed light on both light and heavy quark potentials and their string tensions. Flux-tube and Cornell potentials are developed depending on the regime under consideration. Other confining properties such as scalar glueball mass, gluon mass, glueball-meson mixing states, gluon and chiral condensates are exploited as well. The study is focused on two possible regimes, the ultraviolet (UV) and the infrared (IR) regimes. I. INTRODUCTION Confinement of heavy quark states QQ¯ is an important subject in both theoretical and experimental study of high temperature QCD matter and quark-gluon-plasma phase (QGP) [1]. The production of heavy quarkonia such as the fundamental state ofcc ¯ in the Relativistic Heavy Iron Collider (RHIC) [2] and the Large Hadron Collider (LHC) [3] provides basics for the study of QGP. Lattice QCD simulations of quarkonium at finite temperature indicates that J= may persists even at T = 1:5Tc [4] i.e.
    [Show full text]
  • On the Reality of Quantum Collapse and the Emergence of Space-Time
    Article On the Reality of Quantum Collapse and the Emergence of Space-Time Andreas Schlatter Burghaldeweg 2F, 5024 Küttigen, Switzerland; [email protected]; Tel.: +41-(0)-79-870-77-75 Received: 22 February 2019; Accepted: 22 March 2019; Published: 25 March 2019 Abstract: We present a model, in which quantum-collapse is supposed to be real as a result of breaking unitary symmetry, and in which we can define a notion of “becoming”. We show how empirical space-time can emerge in this model, if duration is measured by light-clocks. The model opens a possible bridge between Quantum Physics and Relativity Theory and offers a new perspective on some long-standing open questions, both within and between the two theories. Keywords: quantum measurement; quantum collapse; thermal time; Minkowski space; Einstein equations 1. Introduction For a hundred years or more, the two main theories in physics, Relativity Theory and Quantum Mechanics, have had tremendous success. Yet there are tensions within the respective theories and in their relationship to each other, which have escaped a satisfactory explanation until today. These tensions have also prevented a unified view of the two theories by a more fundamental theory. There are, of course, candidate-theories, but none has found universal acceptance so far [1]. There is a much older debate, which concerns the question of the true nature of time. Is reality a place, where time, as we experience it, is a mere fiction and where past, present and future all coexist? Is this the reason why so many laws of nature are symmetric in time? Or is there really some kind of “becoming”, where the present is real, the past irrevocably gone and the future not yet here? Admittedly, the latter view only finds a minority of adherents among today’s physicists, whereas philosophers are more balanced.
    [Show full text]
  • Tachyons and the Preferred Frames
    Tachyons and the preferred frames∗ Jakub Rembieli´nski† Katedra Fizyki Teoretycznej, UniwersytetL´odzki ul. Pomorska 149/153, 90–236L´od´z, Poland Abstract Quantum field theory of space-like particles is investigated in the framework of absolute causality scheme preserving Lorentz symmetry. It is related to an appropriate choice of the synchronization procedure (defi- nition of time). In this formulation existence of field excitations (tachyons) distinguishes an inertial frame (privileged frame of reference) via sponta- neous breaking of the so called synchronization group. In this scheme relativity principle is broken but Lorentz symmetry is exactly preserved in agreement with local properties of the observed world. It is shown that tachyons are associated with unitary orbits of Poincar´emappings induced from SO(2) little group instead of SO(2, 1) one. Therefore the corresponding elementary states are labelled by helicity. The cases of the ± 1 helicity λ = 0 and λ = 2 are investigated in detail and a correspond- ing consistent field theory is proposed. In particular, it is shown that the Dirac-like equation proposed by Chodos et al. [1], inconsistent in the standard formulation of QFT, can be consistently quantized in the pre- sented framework. This allows us to treat more seriously possibility that neutrinos might be fermionic tachyons as it is suggested by experimental data about neutrino masses [2, 3, 4]. arXiv:hep-th/9607232v2 1 Aug 1996 1 Introduction Almost all recent experiments, measuring directly or indirectly the electron and muon neutrino masses, have yielded negative values for the mass square1 [2, 3, 4]. It suggests that these particles might be fermionic tachyons.
    [Show full text]
  • Confinement and Screening in Tachyonic Matter
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Open Access Repository Eur. Phys. J. C (2014) 74:3202 DOI 10.1140/epjc/s10052-014-3202-y Regular Article - Theoretical Physics Confinement and screening in tachyonic matter F. A. Brito 1,a,M.L.F.Freire2, W. Serafim1,3 1 Departamento de Física, Universidade Federal de Campina Grande, 58109-970 Campina Grande, Paraíba, Brazil 2 Departamento de Física, Universidade Estadual da Paraíba, 58109-753 Campina Grande, Paraíba, Brazil 3 Instituto de Física, Universidade Federal de Alagoas, 57072-970 Maceió, Alagoas, Brazil Received: 26 August 2014 / Accepted: 19 November 2014 © The Author(s) 2014. This article is published with open access at Springerlink.com Abstract In this paper we consider confinement and way in which hadronic matter lives. In three spatial dimen- screening of the electric field. We study the behavior of sions this effect is represented by Coulomb and confinement a static electric field coupled to a dielectric function with potentials describing the potential between quark pairs. Nor- v ( ) =−a + the intent of obtaining an electrical confinement similar to mally the potential of Cornell [1], c r r br, is used, what happens with the field of gluons that bind quarks in where a and b are positive constants, and r is the distance hadronic matter. For this we use the phenomenon of ‘anti- between the heavy quarks. In QED (Quantum Electrodynam- screening’ in a medium with exotic dielectric. We show that ics), the effective electrical charge increases when the dis- tachyon matter behaves like in an exotic way whose associ- tance r between a pair of electron–anti-electron decreases.
    [Show full text]
  • Relativistic Quantum Mechanics 1
    Relativistic Quantum Mechanics 1 The aim of this chapter is to introduce a relativistic formalism which can be used to describe particles and their interactions. The emphasis 1.1 SpecialRelativity 1 is given to those elements of the formalism which can be carried on 1.2 One-particle states 7 to Relativistic Quantum Fields (RQF), which underpins the theoretical 1.3 The Klein–Gordon equation 9 framework of high energy particle physics. We begin with a brief summary of special relativity, concentrating on 1.4 The Diracequation 14 4-vectors and spinors. One-particle states and their Lorentz transforma- 1.5 Gaugesymmetry 30 tions follow, leading to the Klein–Gordon and the Dirac equations for Chaptersummary 36 probability amplitudes; i.e. Relativistic Quantum Mechanics (RQM). Readers who want to get to RQM quickly, without studying its foun- dation in special relativity can skip the first sections and start reading from the section 1.3. Intrinsic problems of RQM are discussed and a region of applicability of RQM is defined. Free particle wave functions are constructed and particle interactions are described using their probability currents. A gauge symmetry is introduced to derive a particle interaction with a classical gauge field. 1.1 Special Relativity Einstein’s special relativity is a necessary and fundamental part of any Albert Einstein 1879 - 1955 formalism of particle physics. We begin with its brief summary. For a full account, refer to specialized books, for example (1) or (2). The- ory oriented students with good mathematical background might want to consult books on groups and their representations, for example (3), followed by introductory books on RQM/RQF, for example (4).
    [Show full text]
  • The Unitary Representations of the Poincaré Group in Any Spacetime Dimension Abstract Contents
    SciPost Physics Lecture Notes Submission The unitary representations of the Poincar´egroup in any spacetime dimension X. Bekaert1, N. Boulanger2 1 Institut Denis Poisson, Unit´emixte de Recherche 7013, Universit´ede Tours, Universit´e d'Orl´eans,CNRS, Parc de Grandmont, 37200 Tours (France) [email protected] 2 Service de Physique de l'Univers, Champs et Gravitation, Universit´ede Mons, UMONS Research Institute for Complex Systems, Place du Parc 20, 7000 Mons (Belgium) [email protected] December 31, 2020 1 Abstract 2 An extensive group-theoretical treatment of linear relativistic field equations 3 on Minkowski spacetime of arbitrary dimension D > 3 is presented. An exhaus- 4 tive treatment is performed of the two most important classes of unitary irre- 5 ducible representations of the Poincar´egroup, corresponding to massive and 6 massless fundamental particles. Covariant field equations are given for each 7 unitary irreducible representation of the Poincar´egroup with non-negative 8 mass-squared. 9 10 Contents 11 1 Group-theoretical preliminaries 2 12 1.1 Universal covering of the Lorentz group 2 13 1.2 The Poincar´egroup and algebra 3 14 1.3 ABC of unitary representations 4 15 2 Elementary particles as unitary irreducible representations of the isom- 16 etry group 5 17 3 Classification of the unitary representations 7 18 3.1 Induced representations 7 19 3.2 Orbits and stability subgroups 8 20 3.3 Classification 10 21 4 Tensorial representations and Young diagrams 12 22 4.1 Symmetric group 12 23 4.2 General linear
    [Show full text]
  • Supercritical Stability, Transitions and (Pseudo)Tachyons
    hep-th/0612031 SU-ITP-06/32 SLAC-PUB-12243 WIS/18/06-NOV-DPP Supercritical Stability, Transitions and (Pseudo)tachyons Ofer Aharonya,b, and Eva Silversteinc,d aDepartment of Particle Physics, Weizmann Institute of Science, Rehovot 76100, Israel. bSchool of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540, USA. cSLAC and Department of Physics, Stanford University, Stanford, CA 94305-4060, USA. dKavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106-4030, USA. Highly supercritical strings (c 15) with a time-like linear dilaton provide a large class ≫ of solutions to string theory, in which closed string tachyon condensation is under control (and follows the worldsheet renormalization group flow). In this note we analyze the late-time stability of such backgrounds, including transitions between them. The large friction introduced by the rolling dilaton and the rapid decrease of the string coupling suppress the back-reaction of naive instabilities. In particular, although the graviton, dilaton, and other light fields have negative effective mass squared in the linear dilaton background, the decaying string coupling ensures that their condensation does not cause large back-reaction. Similarly, the copious particles produced in transitions between highly supercritical theories do not back-react significantly on the solution. We discuss these features also in a somewhat more general class of time-dependent backgrounds with stable late-time asymptotics. December 2006 Submitted to Physical Review D Work supported in part by the US Department of Energy contract DE-AC02-76SF00515 1. Introduction It is of interest to understand cosmological solutions of string theory. Most solutions of general relativity coupled to quantum field theory evolve non-trivially with time, leading to a weakly coupled description only (at best) at asymptotically late times (or only at early times).
    [Show full text]
  • New Varying Speed of Light Theories
    New varying speed of light theories Jo˜ao Magueijo The Blackett Laboratory,Imperial College of Science, Technology and Medicine South Kensington, London SW7 2BZ, UK ABSTRACT We review recent work on the possibility of a varying speed of light (VSL). We start by discussing the physical meaning of a varying c, dispelling the myth that the constancy of c is a matter of logical consistency. We then summarize the main VSL mechanisms proposed so far: hard breaking of Lorentz invariance; bimetric theories (where the speeds of gravity and light are not the same); locally Lorentz invariant VSL theories; theories exhibiting a color dependent speed of light; varying c induced by extra dimensions (e.g. in the brane-world scenario); and field theories where VSL results from vacuum polarization or CPT violation. We show how VSL scenarios may solve the cosmological problems usually tackled by inflation, and also how they may produce a scale-invariant spectrum of Gaussian fluctuations, capable of explaining the WMAP data. We then review the connection between VSL and theories of quantum gravity, showing how “doubly special” relativity has emerged as a VSL effective model of quantum space-time, with observational implications for ultra high energy cosmic rays and gamma ray bursts. Some recent work on the physics of “black” holes and other compact objects in VSL theories is also described, highlighting phenomena associated with spatial (as opposed to temporal) variations in c. Finally we describe the observational status of the theory. The evidence is slim – redshift dependence in alpha, ultra high energy cosmic rays, and (to a much lesser extent) the acceleration of the universe and the WMAP data.
    [Show full text]
  • MITOCW | L0.8 Introduction to Nuclear and Particle Physics: Relativistic Kinematics
    MITOCW | L0.8 Introduction to Nuclear and Particle Physics: Relativistic Kinematics MARKUS Now back to 8.701. So in this section, we'll talk about relativistic kinematics. Let me start by saying that one of KLUTE: my favorite classes here at MIT is a class called 8.20, special relativity, where we teach students about special relativity, of course, but Einstein and paradoxes. And it's one of my favorite classes. And in their class, there's a component on particle physics, which has to do with just using relativistic kinematics in order to understand how to create antimatter, how to collide beams, how we can analyze decays. And in this introductory section, we're going to do a very similar thing. I trust that you all had some sort of class introduction of special relativity, some of you maybe general relativity. What we want to do here is review this content very briefly, but then more use it in a number of examples. So in particle physics, nuclear physics, we often deal particles who will travel close to the speed of light. The photon travels at the speed of light. We typically define the velocity as v/c in natural units. Beta is the velocity, gamma is defined by 1 over square root 1 minus the velocity squared. Beta is always smaller or equal to 1, smaller for massive particle. And gamma is always equal or greater than 1. The total energy of a particle with 0 mass-- sorry, with non-zero mass, is then given by gamma times m c squared.
    [Show full text]
  • Fully Symmetric Relativistic Quantum Mechanics and Its Physical Implications
    mathematics Article Fully Symmetric Relativistic Quantum Mechanics and Its Physical Implications Bao D. Tran and Zdzislaw E. Musielak * Departmemt of Physics, University of Texas at Arlington, Arlington, TX 76019, USA; [email protected] * Correspondence: [email protected] Abstract: A new formulation of relativistic quantum mechanics is presented and applied to a free, massive, and spin-zero elementary particle in the Minkowski spacetime. The reformulation requires that time and space, as well as the timelike and spacelike intervals, are treated equally, which makes the new theory fully symmetric and consistent with the special theory of relativity. The theory correctly reproduces the classical action of a relativistic particle in the path integral formalism, and allows for the introduction of a new quantity called vector-mass, whose physical implications for nonlocality, the uncertainty principle, and quantum vacuum are described and discussed. Keywords: relativistic quantum mechanics; generalized Klein–Gordon equation; path integral formulation; nonlocality; quantum measurement; uncertainty principle; quantum vacuum 1. Introduction Relativistic quantum mechanics (RQM) primarily concerns free relativistic fields [1,2] Citation: Tranl, B.D.; Musielak, Z.E. described by the Klein–Gordon [3,4], Dirac [5], Proca [6], and Rarita–Schwinger [7] wave Fully Symmetric Relativistic equations, whereas the fundamental interactions and their unification are considered by Quantum Mechanics and Its Physical the gauge invariant quantum field theory (QFT) [8,9]. The above equations of RQM are Implications. Mathematics 2021, 9, P = SO( ) ⊗ 1213. https://doi.org/10.3390/ invariant with respect to all transformations that form the Poincaré group 3, 1 s ( + ) ( ) math9111213 T 3 1 , where SO 3, 1 is a non-invariant Lorentz group of rotations and boosts and T(3 + 1) an invariant subgroup of spacetime translations, and this structure includes Academic Editor: Rami Ahmad reversal of parity and time [10].
    [Show full text]