Overcoming the Bradyon–Tachyon Barrier
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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. -
Limits on New Physics from Black Holes Arxiv:1309.0530V1
Limits on New Physics from Black Holes Clifford Cheung and Stefan Leichenauer California Institute of Technology, Pasadena, CA 91125 Abstract Black holes emit high energy particles which induce a finite density potential for any scalar field φ coupling to the emitted quanta. Due to energetic considerations, φ evolves locally to minimize the effective masses of the outgoing states. In theories where φ resides at a metastable minimum, this effect can drive φ over its potential barrier and classically catalyze the decay of the vacuum. Because this is not a tunneling process, the decay rate is not exponentially suppressed and a single black hole in our past light cone may be sufficient to activate the decay. Moreover, decaying black holes radiate at ever higher temperatures, so they eventually probe the full spectrum of particles coupling to φ. We present a detailed analysis of vacuum decay catalyzed by a single particle, as well as by a black hole. The former is possible provided large couplings or a weak potential barrier. In contrast, the latter occurs much more easily and places new stringent limits on theories with hierarchical spectra. Finally, we comment on how these constraints apply to the standard model and its extensions, e.g. metastable supersymmetry breaking. arXiv:1309.0530v1 [hep-ph] 2 Sep 2013 1 Contents 1 Introduction3 2 Finite Density Potential4 2.1 Hawking Radiation Distribution . .4 2.2 Classical Derivation . .6 2.3 Quantum Derivation . .8 3 Catalyzed Vacuum Decay9 3.1 Scalar Potential . .9 3.2 Point Particle Instability . 10 3.3 Black Hole Instability . 11 3.3.1 Tadpole Instability . -
Tachyon-Dilaton Inflation As an Α'-Non Perturbative Solution in First
Anna Kostouki Work in progress with J. Alexandre and N. Mavromatos TachyonTachyon --DilatonDilaton InflationInflation asas anan αα''--nonnon perturbativeperturbative solutionsolution inin firstfirst quantizedquantized StringString CosmologyCosmology Oxford, 23 September 2008 A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 1 OutlineOutline • Motivation : String Inflation in 4 dimensions • Closed Bosonic String in Graviton, Dilaton and Tachyon Backgrounds; a non – perturbative configuration • Conformal Invariance of this model • Cosmological Implications of this model: FRW universe & inflation (under conditions) • Open Issues: Exit from the inflationary phase; reheating A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 2 MotivationMotivation Inflation : • elegant & simple idea • explains many cosmological observations (e.g. “horizon problem”, large - scale structure) Inflation in String Theory: • effective theory • in traditional string theories: compactification of extra dimensions of space-time is needed • other models exist too, but no longer “simple & elegant” A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 3 ProposalProposal • Closed Bosonic String • graviton, dilaton and tachyon background • field configuration non-perturbative in Does it satisfy conformal invariance conditions? A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 4 ConformalConformal propertiesproperties ofof thethe configurationconfiguration General field redefinition: • Theory is invariant • The Weyl anomaly coefficients transform : ( ) A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 5 ConformalConformal propertiesproperties ofof thethe configurationconfiguration • 1-loop beta-functions: homogeneous dependence on X0, besides one term in the tachyon beta-function • Power counting → Every other term that appears at higher loops in the beta-functions is homogeneous A. Kostouki 2 nd UniverseNet School, Oxford, 23/09/08 6 ConformalConformal propertiesproperties ofof thethe configurationconfiguration One can find a general field redefinition , that: 1. -
Tachyonic Dark Matter
Tachyonic dark matter P.C.W. Davies Australian Centre for Astrobiology Macquarie University, New South Wales, Australia 2109 [email protected] Abstract Recent attempts to explain the dark matter and energy content of the universe have involved some radical extensions of standard physics, including quintessence, phantom energy, additional space dimensions and variations in the speed of light. In this paper I consider the possibility that some dark matter might be in the form of tachyons. I show that, subject to some reasonable assumptions, a tachyonic cosmological fluid would produce distinctive effects, such as a surge in quantum vacuum energy and particle creation, and a change in the conventional temperature-time relation for the normal cosmological material. Possible observational consequences are discussed. Keywords: tachyons, cosmological models, dark matter 1 1. Tachyons in an expanding universe In this section I consider the behaviour of a tachyon in an expanding universe, following the treatment in Davies (1975). A tachyon is a particle with imaginary mass iµ (µ real and positive), velocity v > c and momentum and energy given in a local inertial frame by p = µv(v2 – 1)-1/2 (1.1) E = µ(v2 – 1)-1/2 (1.2) where here and henceforth I choose units with c = ħ =1. Consider such a particle moving in a Friedmann-Roberston-Walker (FRW) universe with scale factor a(t), t being the cosmic time. In a short time dt, the particle will have moved a distance vdt to a point where the local comoving frame is retreating at a speed dv = (a′/a)vdt, where a′ = da/dt. -
Non-Tachyonic Semi-Realistic Non-Supersymmetric Heterotic-String Vacua
Eur. Phys. J. C (2016) 76:208 DOI 10.1140/epjc/s10052-016-4056-2 Regular Article - Theoretical Physics Non-tachyonic semi-realistic non-supersymmetric heterotic-string vacua Johar M. Ashfaquea, Panos Athanasopoulosb, Alon E. Faraggic, Hasan Sonmezd Department of Mathematical Sciences, University of Liverpool, Liverpool L69 7ZL, UK Received: 1 December 2015 / Accepted: 31 March 2016 / Published online: 15 April 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com Abstract The heterotic-string models in the free fermionic 1 Introduction formulation gave rise to some of the most realistic-string models to date, which possess N = 1 spacetime supersym- The discovery of the agent of electroweak symmetry break- metry. Lack of evidence for supersymmetry at the LHC insti- ing at the LHC [1,2] is a pivotal moment in particle physics. gated recent interest in non-supersymmetric heterotic-string While confirmation of this agent as the Standard Model vacua. We explore what may be learned in this context from electroweak doublet representation will require experimental the quasi-realistic free fermionic models. We show that con- scrutiny in the decades to come, the data to date seems to vin- structions with a low number of families give rise to pro- dicate this possibility. Substantiation of this interpretation of liferation of a priori tachyon producing sectors, compared to the data will reinforce the view that the electroweak symme- the non-realistic examples, which typically may contain only try breaking mechanism is intrinsically perturbative, and that one such sector. The reason being that in the realistic cases the SM provides a viable perturbative parameterisation up to the internal six dimensional space is fragmented into smaller the Planck scale. -
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). -
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. -
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. -
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]. -
Stability of a Tachyon Braneworld
Stability of a tachyon braneworld Gabriel Germán,a Alfredo Herrera-Aguilar,b;c André Martorano Kuerten,a;d Dagoberto Malagón–Morejón,a and Roldão da Rochae aInstituto de Ciencias Físicas, Universidad Nacional Autónoma de México, Apartado Postal 48-3, 62251, Cuernavaca, Morelos, México bInstituto de Física, Benemérita Universidad Autónoma de Puebla, Apartado Postal J-48, 72570, Puebla, Puebla, México cInstituto de Física y Matemáticas, Universidad Michoacana de San Nicolás de Hidalgo, Ciudad Universitaria, CP 58040, Morelia, Michoacán, México dCentro de Ciências Naturais e Humanas, Universidade Federal do ABC, 09210-580, Santo André, SP, Brazil eCentro de Matemática, Computação e Cognição, Universidade Federal do ABC, 09210-580, Santo André, SP, Brazil E-mail: gabriel@fis.unam.mx, malagon@fis.unam.mx, [email protected], [email protected], [email protected] Abstract. Within the braneworld paradigm the tachyonic scalar field has been used to gener- ate models that attempt to solve some of the open problems that physics faces nowadays, both in cosmology and high energy physics as well. When these field configurations are produced by the interplay of higher dimensional warped gravity with some matter content, braneworld models must prove to be stable under the whole set of small fluctuations of the gravitational and matter fields background, among other consistency tests. Here we present a complete proof of the stability under scalar perturbations of tachyonic thick braneworlds with an em- bedded maximally symmetric 4D space-time, revealing its physical consistency. This family of models contains a recently reported tachyonic de Sitter thick braneworld which possesses a series of appealing properties. -
Annulus Amplitudes and ZZ Branes in Minimal String Theory
EFI-04-19 PUPT-2121 Annulus Amplitudes and ZZ Branes in Minimal String Theory David Kutasov,1 Kazumi Okuyama,1 Jongwon Park,1 Nathan Seiberg2 and David Shih3 1Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA 2School of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540 USA 3Department of Physics, Princeton University, Princeton, NJ 08544 USA We study the annulus amplitudes of (p, q) minimal string theory. Focusing on the ZZ-FZZT annulus amplitude as a target-space probe of the ZZ brane, we use it to confirm that the ZZ branes are localized in the strong-coupling region. Along the way we learn that the ZZ-FZZT open strings are fermions, even though our theory is bosonic! We also provide arXiv:hep-th/0406030v2 22 Jun 2004 a geometrical interpretation of the annulus amplitudes in terms of the Riemann surface that emerges from the FZZT branes. The ZZ-FZZT annulus amplitude measures the Mp,q deformation of due to the presence of background ZZ branes; each kind of ZZ-brane Mp,q deforms only one A-period of the surface. Finally, we use the annulus amplitudes to argue that the ZZ branes can be regarded as “wrong-branch” tachyons which violate the bound α<Q/2. June, 2004 1. Introduction Minimal string theories are string theories based on the (p, q) minimal conformal field theories coupled to Liouville. They were first solved using their description in terms of matrix models [1-8] (for reviews, see e.g. [9,10]). This tractable description allows explicit calculations of many physical quantities of interest. -
The Physics of Tachyons I. Tachyon Kinematics
Aust. J. Phys., 1992, 45, 591-620 The Physics of Tachyons I. Tachyon Kinematics Ross L. Dawe A and Kenneth C. Hines School of Physics, University of Melbourne, Parkville, Vic. 3052, Australia. A Present address: Maritime Operations Division, Materials Research Laboratory, P.O. Box 1750, Salisbury, S.A. 5108, Australia. Abstract A new formulation of the theory of tachyons is developed using the same two postulates as in special relativity. Use is made of a 'switching principle' to show how tachyons automatically obey the laws of conservation of energy, momentum and electric charge. Tachyonic mechanics is further developed by a consideration of tachyonic rods and clocks. There follows a discussion of the conservation of electric charge and the apparent visual appearance of a tachyonic cube. 1. Introduction The question of whether or not tachyons can exist has been a subject of considerable theoretical interest in recent decades. The most notable formulations of a theory of tachyons at the classical relativistic level have been provided by Bilaniuk et al. (1962, 1969), Recami and Mignani (1974), Recami (1986)* and Corben (1975, 1976, 1978). Recami has built up a detailed formulation based on symmetry arguments within special relativity, while Corben takes a more rigorous approach but has not completed all of the details. Tachyon theories are prone to misinterpretation, and the resulting fallacies and paradoxes have often proved difficult to resolve. It is the purpose of this and subsequent papers to build upon the work by these authors by presenting a rigorous formulation of the theory of tachyons in which the particles are able to interact with ordinary matter via the laws of mechanics and electrodynamics.