Unsolved Problems in Special and General Relativity
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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. -
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. -
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. -
Council for Innovative Research Peer Review Research Publishing System
ISSN 2347-3487 Einstein's gravitation is Einstein-Grossmann's equations Alfonso Leon Guillen Gomez Independent scientific researcher, Bogota, Colombia E-mail: [email protected] Abstract While the philosophers of science discuss the General Relativity, the mathematical physicists do not question it. Therefore, there is a conflict. From the theoretical point view “the question of precisely what Einstein discovered remains unanswered, for we have no consensus over the exact nature of the theory's foundations. Is this the theory that extends the relativity of motion from inertial motion to accelerated motion, as Einstein contended? Or is it just a theory that treats gravitation geometrically in the spacetime setting?”. “The voices of dissent proclaim that Einstein was mistaken over the fundamental ideas of his own theory and that their basic principles are simply incompatible with this theory. Many newer texts make no mention of the principles Einstein listed as fundamental to his theory; they appear as neither axiom nor theorem. At best, they are recalled as ideas of purely historical importance in the theory's formation. The very name General Relativity is now routinely condemned as a misnomer and its use often zealously avoided in favour of, say, Einstein's theory of gravitation What has complicated an easy resolution of the debate are the alterations of Einstein's own position on the foundations of his theory”, (Norton, 1993) [1]. Of other hand from the mathematical point view the “General Relativity had been formulated as a messy set of partial differential equations in a single coordinate system. People were so pleased when they found a solution that they didn't care that it probably had no physical significance” (Hawking and Penrose, 1996) [2]. -
Herbert P Ster Markus King the Fundamental Nature and Structure
Lecture Notes in Physics 897 Herbert P ster Markus King Inertia and Gravitation The Fundamental Nature and Structure of Space-Time Lecture Notes in Physics Volume 897 Founding Editors W. Beiglböck J. Ehlers K. Hepp H. Weidenmüller Editorial Board B.-G. Englert, Singapore, Singapore P. Hänggi, Augsburg, Germany W. Hillebrandt, Garching, Germany M. Hjorth-Jensen, Oslo, Norway R.A.L. Jones, Sheffield, UK M. Lewenstein, Barcelona, Spain H. von Löhneysen, Karlsruhe, Germany M.S. Longair, Cambridge, UK J.-F. Pinton, Lyon, France J.-M. Raimond, Paris, France A. Rubio, Donostia, San Sebastian, Spain M. Salmhofer, Heidelberg, Germany S. Theisen, Potsdam, Germany D. Vollhardt, Augsburg, Germany J.D. Wells, Geneva, Switzerland The Lecture Notes in Physics The series Lecture Notes in Physics (LNP), founded in 1969, reports new devel- opments in physics research and teaching-quickly and informally, but with a high quality and the explicit aim to summarize and communicate current knowledge in an accessible way. Books published in this series are conceived as bridging material between advanced graduate textbooks and the forefront of research and to serve three purposes: • to be a compact and modern up-to-date source of reference on a well-defined topic • to serve as an accessible introduction to the field to postgraduate students and nonspecialist researchers from related areas • to be a source of advanced teaching material for specialized seminars, courses and schools Both monographs and multi-author volumes will be considered for publication. Edited volumes should, however, consist of a very limited number of contributions only. Proceedings will not be considered for LNP. -
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. -
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. -
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 -
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). -
Spontaneous Symmetry Breaking in the Higgs Mechanism
Spontaneous symmetry breaking in the Higgs mechanism August 2012 Abstract The Higgs mechanism is very powerful: it furnishes a description of the elec- troweak theory in the Standard Model which has a convincing experimental ver- ification. But although the Higgs mechanism had been applied successfully, the conceptual background is not clear. The Higgs mechanism is often presented as spontaneous breaking of a local gauge symmetry. But a local gauge symmetry is rooted in redundancy of description: gauge transformations connect states that cannot be physically distinguished. A gauge symmetry is therefore not a sym- metry of nature, but of our description of nature. The spontaneous breaking of such a symmetry cannot be expected to have physical e↵ects since asymmetries are not reflected in the physics. If spontaneous gauge symmetry breaking cannot have physical e↵ects, this causes conceptual problems for the Higgs mechanism, if taken to be described as spontaneous gauge symmetry breaking. In a gauge invariant theory, gauge fixing is necessary to retrieve the physics from the theory. This means that also in a theory with spontaneous gauge sym- metry breaking, a gauge should be fixed. But gauge fixing itself breaks the gauge symmetry, and thereby obscures the spontaneous breaking of the symmetry. It suggests that spontaneous gauge symmetry breaking is not part of the physics, but an unphysical artifact of the redundancy in description. However, the Higgs mechanism can be formulated in a gauge independent way, without spontaneous symmetry breaking. The same outcome as in the account with spontaneous symmetry breaking is obtained. It is concluded that even though spontaneous gauge symmetry breaking cannot have physical consequences, the Higgs mechanism is not in conceptual danger. -
DARK ENERGY and ACCELERATING UNIVERSE PHONGSAPHAT RANGDEE a Thesis Submitted to Graduate School of Naresuan University in Partia
DARK ENERGY AND ACCELERATING UNIVERSE PHONGSAPHAT RANGDEE A Thesis Submitted to Graduate School of Naresuan University in Partial Fulfillment of the Requirements of the Doctor of Philosophy Degree in Theoretical Physics December 2015 Copyright 2015 by Naresuan University Thesis entitled \Dark Energy and Accelerating Universe" By Mr.Phongsaphat Rangdee Has been approved by the Graduate School as partial fulfillment of the requirements for the Doctor of Philosophy Degree in Theoretical Physics of Naresuan University. Oral Defense Committee ........................................................... Chair (Seckson Sukhasena, Ph.D.) ........................................................... Advisor (Associate Professor Burin Gumjudpai, Ph.D.) ........................................................... Co-Advisor (Khamphee Karwan, Ph.D.) ........................................................... Co-Advisor (Pitayuth Wongjun, Ph.D.) ........................................................... External Examiner (Professor David Wands, D.Phil.) Approved ........................................................................... (Panu Putthawong, Ph.D.) Associate Dean for Administration and Planning For Dean of the Graduate School December 2015 ACKNOWLEDGMENT I would like to thank my advisor, Associate Professor Burin Gumjudpai for giving me the motivations, discussions and suggestions, also useful knowledge and knowhow to do research and thank you for all additional knowledge in everything. I would like to thank all of committee for giving their time to become my viva voce examination's committee. All the past and present of people at IF that have been imparted their knowledge to me. I ought to be thanked Mr.Narakorn Kaewkhao for his discussions, suggestions, and new insights on Physics. I would like to thank all people at IF whom I had the chance to interact; lecturers, staffs, friends. All people that made me happy during I was a student at IF. It's my pleasure and my great time to spend with all of them. -
Holography Inspired Stringy Hadrons Arxiv:1602.00704V4 [Hep-Th] 20
Holography Inspired Stringy Hadrons Jacob Sonnenschein The Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Ramat Aviv 69978, Israel November 22, 2016 Abstract Holography inspired stringy hadrons (HISH) is a set of models that describe hadrons: mesons, baryons and glueballs as strings in flat four dimensional space time. The models are based on a \map" from stringy hadrons of holographic confining backgrounds. In this note we review the 5 \derivation" of the models. We start with a brief reminder of the passage from the AdS5 ×S string theory to certain flavored confining holographic models. We then describe the string configurations in holographic backgrounds that correspond to a Wilson line,a meson,a baryon and a glueball. The key ingredients of the four dimensional picture of hadrons are the \string endpoint mass" and the \baryonic string vertex". We determine the classical trajectories of the HISH. We review the current understanding of the quantization of the hadronic strings. We end with a summary of the comparison of the outcome of the HISH models with the PDG data about mesons and baryons. We extract the values of the tension, masses and intercepts from best fits, write down certain predictions for higher excited hadrons and present attempts to identify glueballs. arXiv:1602.00704v4 [hep-th] 20 Nov 2016 1 Contents 1 Introduction 3 5 2 From AdS5 × S to confining string backgrounds 5 2.1 Confining background . 5 2.2 Introducing fundamental quarks . 6 2.3 Review of the Witten-Sakai-Sugimoto model . 6 3 Hadrons as strings in holographic background 10 3.1 The holographic Wilson line .