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Negative Energies and Time Reversal in Quantum Field Theory F
Negative Energies and Time Reversal in Quantum Field Theory F. Henry-Couannier To cite this version: F. Henry-Couannier. Negative Energies and Time Reversal in Quantum Field Theory. Global Journal of Science Research, Global Journals™ Incorporated, 2012, 12, pp.39-58. in2p3-00865527 HAL Id: in2p3-00865527 http://hal.in2p3.fr/in2p3-00865527 Submitted on 18 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License NEGATIVE ENERGIES AND TIME REVERSAL IN QUANTUM FIELD THEORY Frederic Henry-Couannier CPPM, 163 Avenue De Luminy, Marseille 13009 France. [email protected] Abstract The theoretical and phenomenological status of negative energies is reviewed in Quantum Field Theory leading to the conclusion that hope- fully their rehabilitation might only be completed in a modified general relativistic model. 1 Introduction With recent cosmological observations related to supernovae, CMB and galactic clustering the evidence is growing that our universe is undergoing an accelerated expansion at present. Though the most popular way to account for this unex- pected result has been the reintroduction of a cosmological constant or a new kind of dark matter with negative pressure, scalar fields with negative kinetic energy, so-called phantom fields, have recently been proposed [1] [2] [3] as new sources leading to the not excluded possibility that the equation of state param- eter be less than minus one. -
The Negative Energy in Generalized Vaidya Spacetime
universe Communication The Negative Energy in Generalized Vaidya Spacetime Vitalii Vertogradov 1,2 1 Department of the Theoretical Physics and Astronomy, Herzen State Pedagogical University, 191186 St. Petersburg, Russia; [email protected] 2 The SAO RAS, Pulkovskoe Shosse 65, 196140 St. Petersburg, Russia Received: 17 August 2020; Accepted: 17 September 2020; Published: 22 September 2020 Abstract: In this paper we consider the negative energy problem in generalized Vaidya spacetime. We consider several models where we have the naked singularity as a result of the gravitational collapse. In these models we investigate the geodesics for particles with negative energy when the II type of the matter field satisfies the equation of the state P = ar (a 2 [0 , 1]). Keywords: generalized Vaidya spacetime; naked singularity; black hole; negative energy 1. Introduction In 1969 R. Penrose theoretically predicted the effect of the negative energy formation in the Kerr metric during the process of the decay or the collision. Furthermore, the nature of the geodesics for particles with negative energy was investigated [1,2]. It was shown that in the ergosphere of a rotating black hole closed orbits for such particles are absent. This geodesics must appear from the region inside the gravitational radius. Moreover, there was research devoted to the particles with negative energy in Schwarzschild spacetime which was conducted by A. A. Grib and Yu. V. Pavlov [3]. They showed that the particles with negative energy can exist only in the region inside of the event horizon. However, the Schwarzschild black hole is the eternal one and we must consider the gravitational collapse to speak about the past of the geodesics for particles with negative energy. -
The Penrose and Hawking Singularity Theorems Revisited
Classical singularity thms. Interlude: Low regularity in GR Low regularity singularity thms. Proofs Outlook The Penrose and Hawking Singularity Theorems revisited Roland Steinbauer Faculty of Mathematics, University of Vienna Prague, October 2016 The Penrose and Hawking Singularity Theorems revisited 1 / 27 Classical singularity thms. Interlude: Low regularity in GR Low regularity singularity thms. Proofs Outlook Overview Long-term project on Lorentzian geometry and general relativity with metrics of low regularity jointly with `theoretical branch' (Vienna & U.K.): Melanie Graf, James Grant, G¨untherH¨ormann,Mike Kunzinger, Clemens S¨amann,James Vickers `exact solutions branch' (Vienna & Prague): Jiˇr´ıPodolsk´y,Clemens S¨amann,Robert Svarcˇ The Penrose and Hawking Singularity Theorems revisited 2 / 27 Classical singularity thms. Interlude: Low regularity in GR Low regularity singularity thms. Proofs Outlook Contents 1 The classical singularity theorems 2 Interlude: Low regularity in GR 3 The low regularity singularity theorems 4 Key issues of the proofs 5 Outlook The Penrose and Hawking Singularity Theorems revisited 3 / 27 Classical singularity thms. Interlude: Low regularity in GR Low regularity singularity thms. Proofs Outlook Table of Contents 1 The classical singularity theorems 2 Interlude: Low regularity in GR 3 The low regularity singularity theorems 4 Key issues of the proofs 5 Outlook The Penrose and Hawking Singularity Theorems revisited 4 / 27 Theorem (Pattern singularity theorem [Senovilla, 98]) In a spacetime the following are incompatible (i) Energy condition (iii) Initial or boundary condition (ii) Causality condition (iv) Causal geodesic completeness (iii) initial condition ; causal geodesics start focussing (i) energy condition ; focussing goes on ; focal point (ii) causality condition ; no focal points way out: one causal geodesic has to be incomplete, i.e., : (iv) Classical singularity thms. -
A Unifying Theory of Dark Energy and Dark Matter: Negative Masses and Matter Creation Within a Modified ΛCDM Framework J
Astronomy & Astrophysics manuscript no. theory_dark_universe_arxiv c ESO 2018 November 5, 2018 A unifying theory of dark energy and dark matter: Negative masses and matter creation within a modified ΛCDM framework J. S. Farnes1; 2 1 Oxford e-Research Centre (OeRC), Department of Engineering Science, University of Oxford, Oxford, OX1 3QG, UK. e-mail: [email protected]? 2 Department of Astrophysics/IMAPP, Radboud University, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands. Received February 23, 2018 ABSTRACT Dark energy and dark matter constitute 95% of the observable Universe. Yet the physical nature of these two phenomena remains a mystery. Einstein suggested a long-forgotten solution: gravitationally repulsive negative masses, which drive cosmic expansion and cannot coalesce into light-emitting structures. However, contemporary cosmological results are derived upon the reasonable assumption that the Universe only contains positive masses. By reconsidering this assumption, I have constructed a toy model which suggests that both dark phenomena can be unified into a single negative mass fluid. The model is a modified ΛCDM cosmology, and indicates that continuously-created negative masses can resemble the cosmological constant and can flatten the rotation curves of galaxies. The model leads to a cyclic universe with a time-variable Hubble parameter, potentially providing compatibility with the current tension that is emerging in cosmological measurements. In the first three-dimensional N-body simulations of negative mass matter in the scientific literature, this exotic material naturally forms haloes around galaxies that extend to several galactic radii. These haloes are not cuspy. The proposed cosmological model is therefore able to predict the observed distribution of dark matter in galaxies from first principles. -
Classical and Semi-Classical Energy Conditions Arxiv:1702.05915V3 [Gr-Qc] 29 Mar 2017
Classical and semi-classical energy conditions1 Prado Martin-Morunoa and Matt Visserb aDepartamento de F´ısica Te´orica I, Ciudad Universitaria, Universidad Complutense de Madrid, E-28040 Madrid, Spain bSchool of Mathematics and Statistics, Victoria University of Wellington, PO Box 600, Wellington 6140, New Zealand E-mail: [email protected]; [email protected] Abstract: The standard energy conditions of classical general relativity are (mostly) linear in the stress-energy tensor, and have clear physical interpretations in terms of geodesic focussing, but suffer the significant drawback that they are often violated by semi-classical quantum effects. In contrast, it is possible to develop non-standard energy conditions that are intrinsically non-linear in the stress-energy tensor, and which exhibit much better well-controlled behaviour when semi-classical quantum effects are introduced, at the cost of a less direct applicability to geodesic focussing. In this chapter we will first review the standard energy conditions and their various limitations. (Including the connection to the Hawking{Ellis type I, II, III, and IV classification of stress-energy tensors). We shall then turn to the averaged, nonlinear, and semi-classical energy conditions, and see how much can be done once semi-classical quantum effects are included. arXiv:1702.05915v3 [gr-qc] 29 Mar 2017 1Draft chapter, on which the related chapter of the book Wormholes, Warp Drives and Energy Conditions (to be published by Springer) will be based. Contents 1 Introduction1 2 Standard energy conditions2 2.1 The Hawking{Ellis type I | type IV classification4 2.2 Alternative canonical form8 2.3 Limitations of the standard energy conditions9 3 Averaged energy conditions 11 4 Nonlinear energy conditions 12 5 Semi-classical energy conditions 14 6 Discussion 16 1 Introduction The energy conditions, be they classical, semiclassical, or \fully quantum" are at heart purely phenomenological approaches to deciding what form of stress-energy is to be considered \physically reasonable". -
Can Mass Be Negative?
Can Mass Be Negative? Vladik Kreinovich1 and Sergei Soloviev2 1Department of Computer Science University of Texas at El Paso El Paso, TX 7996058, USA [email protected] 2Institut de Recherche en Informatique de Toulouse (IRIT) IRIT, porte 426 118 route de Narbonne 31062 Toulouse cedex 4, France [email protected] Abstract Overcoming the force of gravity is an important part of space travel and a significant obstacle preventing many seemingly reasonable space travel schemes to become practical. Science fiction writers like to imagine materials that may help to make space travel easier. Negative mass { supposedly causing anti-gravity { is one of the popular ideas in this regard. But can mass be negative? In this paper, we show that negative masses are not possible { their existence would enable us to create energy out of nothing, which contradicts to the energy conservation law. 1 Formulation of the Problem Overcoming the force of gravity is an important part of space travel and a significant obstacle preventing many seemingly reasonable space travel schemes to become practical. Science fiction writers like to imagine materials that may help to make space travel easier. Negative mass { supposedly causing anti- gravity { is one of the popular ideas in this regard. But can mass be negative? 2 Reminder: There Are Different Types of Masses To properly answer the question of whether negative masses are possible, it is important to take into account that there are, in principle, three types of masses: 1 • inertial mass mI that describes how an object reacts to a force F : the object's acceleration a is determined by Newton's law mI · a = F ; and • active and passive gravitational mass mA and mP : gravitation force ex- erted by Object 1 with active mass m on Object 2 with passive mass m · m A1 m is equal to F = G · A1 P 2 ; where r is the distance between the P 2 r2 two objects; see, e.g., [1, 3]. -
Light Rays, Singularities, and All That
Light Rays, Singularities, and All That Edward Witten School of Natural Sciences, Institute for Advanced Study Einstein Drive, Princeton, NJ 08540 USA Abstract This article is an introduction to causal properties of General Relativity. Topics include the Raychaudhuri equation, singularity theorems of Penrose and Hawking, the black hole area theorem, topological censorship, and the Gao-Wald theorem. The article is based on lectures at the 2018 summer program Prospects in Theoretical Physics at the Institute for Advanced Study, and also at the 2020 New Zealand Mathematical Research Institute summer school in Nelson, New Zealand. Contents 1 Introduction 3 2 Causal Paths 4 3 Globally Hyperbolic Spacetimes 11 3.1 Definition . 11 3.2 Some Properties of Globally Hyperbolic Spacetimes . 15 3.3 More On Compactness . 18 3.4 Cauchy Horizons . 21 3.5 Causality Conditions . 23 3.6 Maximal Extensions . 24 4 Geodesics and Focal Points 25 4.1 The Riemannian Case . 25 4.2 Lorentz Signature Analog . 28 4.3 Raychaudhuri’s Equation . 31 4.4 Hawking’s Big Bang Singularity Theorem . 35 5 Null Geodesics and Penrose’s Theorem 37 5.1 Promptness . 37 5.2 Promptness And Focal Points . 40 5.3 More On The Boundary Of The Future . 46 1 5.4 The Null Raychaudhuri Equation . 47 5.5 Trapped Surfaces . 52 5.6 Penrose’s Theorem . 54 6 Black Holes 58 6.1 Cosmic Censorship . 58 6.2 The Black Hole Region . 60 6.3 The Horizon And Its Generators . 63 7 Some Additional Topics 66 7.1 Topological Censorship . 67 7.2 The Averaged Null Energy Condition . -
Negative Matter, Repulsion Force, Dark Matter, Phantom And
Negative Matter, Repulsion Force, Dark Matter, Phantom and Theoretical Test Their Relations with Inflation Cosmos and Higgs Mechanism Yi-Fang Chang Department of Physics, Yunnan University, Kunming, 650091, China (e-mail: [email protected]) Abstract: First, dark matter is introduced. Next, the Dirac negative energy state is rediscussed. It is a negative matter with some new characteristics, which are mainly the gravitation each other, but the repulsion with all positive matter. Such the positive and negative matters are two regions of topological separation in general case, and the negative matter is invisible. It is the simplest candidate of dark matter, and can explain some characteristics of the dark matter and dark energy. Recent phantom on dark energy is namely a negative matter. We propose that in quantum fluctuations the positive matter and negative matter are created at the same time, and derive an inflation cosmos, which is created from nothing. The Higgs mechanism is possibly a product of positive and negative matter. Based on a basic axiom and the two foundational principles of the negative matter, we research its predictions and possible theoretical tests, in particular, the season effect. The negative matter should be a necessary development of Dirac theory. Finally, we propose the three basic laws of the negative matter. The existence of four matters on positive, opposite, and negative, negative-opposite particles will form the most perfect symmetrical world. Key words: dark matter, negative matter, dark energy, phantom, repulsive force, test, Dirac sea, inflation cosmos, Higgs mechanism. 1. Introduction The speed of an object surrounded a galaxy is measured, which can estimate mass of the galaxy. -
The Quantum Negative Energy Problem Revisited
Annales Fondation Louis de Broglie, Volume 30, no 3-4, 2005 381 The Quantum Negative Energy Problem Revisited MENDEL SACHS Department of Physics, University at Buffalo, State University of New York 1 Introduction The aim of this note is to revisit the problem of the negative energy levels in the early Dirac electron theory. It is a problem that was not resolved satisfactorily in the context of Dirac’s relativistic quantum theory, or in its extension to quantum electrodynamics, according to Dirac’s own view. It will be my contention that this problem is automatically resolved in any continuous field theory of microscopic matter, as in the author’s demonstration of quantum mechanics as a linear, asymptotic limit of a continuous, nonlinear field theory of the inertia of matter, rooted in the theory of general relativity, [1]. 2 Review of the Quantum Electron Problem In Dirac’s generalization of Schrodinger’s nonrelativistic wave mechanics, to a spinor form in special relativity, he was left with the problem of the existence of negative energy levels E-, accompanying the positive energy levels E+ of the electron. It was a problem not encountered in classical field theory or in nonrelativistic wave mechanics. According to Dirac [2], “In the quantum theory, since in general a perturbation will cause transitions from states with E positive to states with E negative, such transitions would appear experimentally as the electron (whose charge) suddenly changes from –e to +e, a phenomenon which has not been observed”. In time, it was recognized that +e (the positron) in the Dirac theory, is an elementary particle that is independent of the elementary particle –e (electron). -
General Relativistic Energy Conditions: the Hubble Expansion in the Epoch of Galaxy Formation
General Relativistic Energy Conditions: The Hubble expansion in the epoch of galaxy formation. Matt Visser† Physics Department Washington University Saint Louis Missouri 63130-4899 USA 26 May 1997; gr-qc/9705070 Abstract The energy conditions of Einstein gravity (classical general relativity) are designed to extract as much information as possible from classical general relativity without enforcing a particular equation of state for the stress-energy. This systematic avoidance of the need to specify a particular equation of state is particularly useful in a cosmological setting — since the equation of state for the cosmological fluid in a Friedmann–Robertson– Walker type universe is extremely uncertain. I shall show that the energy conditions provide simple and robust bounds on the behaviour of both the density and look-back time as a function of red-shift. I shall show that current observations suggest that the so-called strong energy condition (SEC) is violated sometime between the epoch of galaxy formation and the present. This implies that no possible combination of “normal” matter is capable of fitting the observational data. PACS: 98.80.-k; 98.80.Bp; 98.80.Hw; 04.90.+e † E-mail: [email protected] 1 1 Introduction The discussion presented in this paper is a model-independent analysis of the misnamed age-of-the-universe problem, this really being an age-of-the-oldest- stars problem. In this paper I trade off precision against robustness: I sacrifice the precision that comes from assuming a particular equation of state, for the robustness that arises from model independence. A briefer presentation of these ideas can be found in [1], while a related analysis is presented in [2]. -
Black Holes and Black Hole Thermodynamics Without Event Horizons
General Relativity and Gravitation (2011) DOI 10.1007/s10714-008-0739-9 RESEARCHARTICLE Alex B. Nielsen Black holes and black hole thermodynamics without event horizons Received: 18 June 2008 / Accepted: 22 November 2008 c Springer Science+Business Media, LLC 2009 Abstract We investigate whether black holes can be defined without using event horizons. In particular we focus on the thermodynamic properties of event hori- zons and the alternative, locally defined horizons. We discuss the assumptions and limitations of the proofs of the zeroth, first and second laws of black hole mechan- ics for both event horizons and trapping horizons. This leads to the possibility that black holes may be more usefully defined in terms of trapping horizons. We also review how Hawking radiation may be seen to arise from trapping horizons and discuss which horizon area should be associated with the gravitational entropy. Keywords Black holes, Black hole thermodynamics, Hawking radiation, Trapping horizons Contents 1 Introduction . 2 2 Event horizons . 4 3 Local horizons . 8 4 Thermodynamics of black holes . 14 5 Area increase law . 17 6 Gravitational entropy . 19 7 The zeroth law . 22 8 The first law . 25 9 Hawking radiation for trapping horizons . 34 10 Fluid flow analogies . 36 11 Uniqueness . 37 12 Conclusion . 39 A. B. Nielsen Center for Theoretical Physics and School of Physics College of Natural Sciences, Seoul National University Seoul 151-742, Korea [email protected] 2 A. B. Nielsen 1 Introduction Black holes play a central role in physics. In astrophysics, they represent the end point of stellar collapse for sufficiently large stars. -
Negative Energy: Why Interdisciplinary Physics Requires Multiple Ontologies
Negative Energy: Why Interdisciplinary Physics Requires Multiple Ontologies Benjamin W. Dreyfus, Benjamin D. Geller, Julia Gouvea, Vashti Sawtelle, Chandra Turpen, and Edward F. Redish Department of Physics, University of Maryland, College Park MD 20742 Abstract. Much recent work in physics education research has focused on ontological metaphors for energy, particularly the substance ontology and its pedagogical affordances. The concept of negative energy problematizes the substance on- tology for energy, but in many instructional settings, the specific difficulties around negative energy are outweighed by the general advantages of the substance ontology. However, we claim that our interdisciplinary setting (a physics class that builds deep connections to biology and chemistry) leads to a different set of considerations and conclusions. In a course designed to draw interdisciplinary connections, the centrality of chemical bond energy in biology necessitates foregrounding negative energy from the beginning. We argue that the emphasis on negative energy requires a combina- tion of substance and location ontologies. The location ontology enables energies both "above" and "below" zero. We present preliminary student data that illustrate difficulties in reasoning about negative energy, and the affordances of the location metaphor. Keywords: physics education research, biology education, interdisciplinary, energy, ontology, metaphor PACS: 01.40.-d, 01.40.Fk, 01.30.Cc INTRODUCTION likewise here we focus primarily on the substance and location metaphors, both of which are commonly used Energy is a central concept in physics, chemistry, by expert physicists. and biology, and has been widely promoted [1] as a Scherr et al. go on to focus on the substance ontol- way to connect physics and chemistry to biology.