Aspects of Riemannian Geometry in Quantum Field Theories Ricardo
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2-Loop $\Beta $ Function for Non-Hermitian PT Symmetric $\Iota
2-Loop β Function for Non-Hermitian PT Symmetric ιgφ3 Theory Aditya Dwivedi1 and Bhabani Prasad Mandal2 Department of Physics, Institute of Science, Banaras Hindu University Varanasi-221005 INDIA Abstract We investigate Non-Hermitian quantum field theoretic model with ιgφ3 interaction in 6 dimension. Such a model is PT-symmetric for the pseudo scalar field φ. We analytically calculate the 2-loop β function and analyse the system using renormalization group technique. Behavior of the system is studied near the different fixed points. Unlike gφ3 theory in 6 dimension ιgφ3 theory develops a new non trivial fixed point which is energetically stable. 1 Introduction Over the past two decades a new field with combined Parity(P)-Time rever- sal(T) symmetric non-Hermitian systems has emerged and has been one of the most exciting topics in frontier research. It has been shown that such theories can lead to the consistent quantum theories with real spectrum, unitary time evolution and probabilistic interpretation in a different Hilbert space equipped with a positive definite inner product [1]-[3]. The huge success of such non- Hermitian systems has lead to extension to many other branches of physics and interdisciplinary areas. The novel idea of such theories have been applied in arXiv:1912.07595v1 [hep-th] 14 Dec 2019 numerous systems leading huge number of application [4]-[21]. Several PT symmetric non-Hermitian models in quantum field theory have also been studied in various context [16]-[26]. Deconfinment to confinment tran- sition is realised by PT phase transition in QCD model using natural but uncon- ventional hermitian property of the ghost fields [16]. -
Effective Quantum Field Theories Thomas Mannel Theoretical Physics I (Particle Physics) University of Siegen, Siegen, Germany
Generating Functionals Functional Integration Renormalization Introduction to Effective Quantum Field Theories Thomas Mannel Theoretical Physics I (Particle Physics) University of Siegen, Siegen, Germany 2nd Autumn School on High Energy Physics and Quantum Field Theory Yerevan, Armenia, 6-10 October, 2014 T. Mannel, Siegen University Effective Quantum Field Theories: Lecture 1 Generating Functionals Functional Integration Renormalization Overview Lecture 1: Basics of Quantum Field Theory Generating Functionals Functional Integration Perturbation Theory Renormalization Lecture 2: Effective Field Thoeries Effective Actions Effective Lagrangians Identifying relevant degrees of freedom Renormalization and Renormalization Group T. Mannel, Siegen University Effective Quantum Field Theories: Lecture 1 Generating Functionals Functional Integration Renormalization Lecture 3: Examples @ work From Standard Model to Fermi Theory From QCD to Heavy Quark Effective Theory From QCD to Chiral Perturbation Theory From New Physics to the Standard Model Lecture 4: Limitations: When Effective Field Theories become ineffective Dispersion theory and effective field theory Bound Systems of Quarks and anomalous thresholds When quarks are needed in QCD É. T. Mannel, Siegen University Effective Quantum Field Theories: Lecture 1 Generating Functionals Functional Integration Renormalization Lecture 1: Basics of Quantum Field Theory Thomas Mannel Theoretische Physik I, Universität Siegen f q f et Yerevan, October 2014 T. Mannel, Siegen University Effective Quantum -
Hep-Th] 27 May 2021
Higher order curvature corrections and holographic renormalization group flow Ahmad Ghodsi∗and Malihe Siahvoshan† Department of Physics, Faculty of Science, Ferdowsi University of Mashhad, Mashhad, Iran September 3, 2021 Abstract We study the holographic renormalization group (RG) flow in the presence of higher-order curvature corrections to the (d+1)-dimensional Einstein-Hilbert (EH) action for an arbitrary interacting scalar matter field by using the superpotential approach. We find the critical points of the RG flow near the local minima and maxima of the potential and show the existence of the bounce solutions. In contrast to the EH gravity, regarding the values of couplings of the bulk theory, superpoten- tial may have both upper and lower bounds. Moreover, the behavior of the RG flow controls by singular curves. This study may shed some light on how a c-function can exist in the presence of these corrections. arXiv:2105.13208v1 [hep-th] 27 May 2021 ∗[email protected] †[email protected] Contents 1 Introduction1 2 The general setup4 3 Holographic RG flow: κ1 = 0 theories5 3.1 Critical points for κ2 < 0...........................7 3.1.1 Local maxima of the potential . .7 3.1.2 Local minima of potential . .9 3.1.3 Bounces . .9 3.2 Critical points for κ2 > 0........................... 11 3.2.1 Critical points for W 6= WE ..................... 12 3.2.2 Critical points near W = WE .................... 13 4 Holographic RG flow: General case 15 4.1 Local maxima of potential . 18 4.2 Local minima of potential . 22 4.3 Bounces . -
The Euler Legacy to Modern Physics
ENTE PER LE NUOVE TECNOLOGIE, L'ENERGIA E L'AMBIENTE THE EULER LEGACY TO MODERN PHYSICS G. DATTOLI ENEA -Dipartimento Tecnologie Fisiche e Nuovi Materiali Centro Ricerche Frascati M. DEL FRANCO - ENEA Guest RT/2009/30/FIM This report has been prepared and distributed by: Servizio Edizioni Scientifiche - ENEA Centro Ricerche Frascati, C.P. 65 - 00044 Frascati, Rome, Italy The technical and scientific contents of these reports express the opinion of the authors but not necessarily the opinion of ENEA. THE EULER LEGACY TO MODERN PHYSICS Abstract Particular families of special functions, conceived as purely mathematical devices between the end of XVIII and the beginning of XIX centuries, have played a crucial role in the development of many aspects of modern Physics. This is indeed the case of the Euler gamma function, which has been one of the key elements paving the way to string theories, furthermore the Euler-Riemann Zeta function has played a decisive role in the development of renormalization theories. The ideas of Euler and later those of Riemann, Ramanujan and of other, less popular, mathematicians have therefore provided the mathematical apparatus ideally suited to explore, and eventually solve, problems of fundamental importance in modern Physics. The mathematical foundations of the theory of renormalization trace back to the work on divergent series by Euler and by mathematicians of two centuries ago. Feynman, Dyson, Schwinger… rediscovered most of these mathematical “curiosities” and were able to develop a new and powerful way of looking at physical phenomena. Keywords: Special functions, Euler gamma function, Strin theories, Euler-Riemann Zeta function, Mthematical curiosities Riassunto Alcune particolari famiglie di funzioni speciali, concepite come dispositivi puramente matematici tra la fine del XVIII e l'inizio del XIX secolo, hanno svolto un ruolo cruciale nello sviluppo di molti aspetti della fisica moderna. -
August to December 2011 ALTERNATIVE COSMOLOGY GROUP
1 ALTERNATIVE COSMOLOGY GROUP www.cosmology.info Monthly Notes of the Alternative Cosmology Group – 2011 Part Two: August to December 2011 The ACG Webmaster who distributes this newsletter to subscribers would prefer not to receive related correspondence. Please address all correspondence to MNACG Editor, Hilton Ratcliffe: [email protected]. The ACG newsletter is distributed gratis to subscribers. Get onto our mailing list without obligation at www.cosmology.info/newsletter. The current newsletter is a review of more than 12,000 papers published on arXiv under astro-ph, together with 6500 under gen-phys, for the months of April to December, 2011. We now include papers archived elsewhere, provided access is full and open. The Alternative Cosmology Group draws its mandate from the open letter published in New Scientist, 2004 (www.cosmologystatement.org), and these monthly notes seek to publicise recently published empirical results that are aligned with that ethos. In other words, what observations seem anomalous in terms of the Standard Model of Cosmology? We prefer observational results and tend to avoid complete cosmologies and purely theoretical work. Discussion of method is welcome. If you would like to suggest recently published or archived papers for inclusion, please send the arXiv, viXra or other direct reference and a brief exposition to Hilton Ratcliffe ([email protected]). Note that our spam filter rejects slash and colon in the text, so please write web addresses commencing “www”. I. Editorial comment I apologise most profusely again for the delay in getting the MNACG out to you. This newsletter and one that preceded it cover several months each, so please pardon their lengthiness. -
MAP-Fis Essay Proposal, 2014-2015 (Please Write in English)
MAP-fis Essay Proposal, 2014-2015 (please write in English) Supervisor Name: Orfeu Bertolami Neto E-mail: [email protected] Co-supervisor Name: João Pedro Trancoso Gomes Rosa E-mail: [email protected] Title Interaction of dark energy and dark matter to Standard Model States Area (Materials, Optics, Condensed Theory, High Energy Theory,....); Cosmology, Particle Physics Summary of Proposal In this proposal it is intended to build and to examine the implications of the interaction between dark energy, dark matter and states of the Standard Model. We will be particularly interested in the study of the coupling to the Higgs and the neutrino sectors. This is a very interesting and relevant research topic that combines several research fields, Particle Physics, Astrophysics and Cosmology, for which there is a rich literature [1-9]. (continue if necessary) MAP-fis Physics Doctoral Program – [email protected] – http://www.map.edu.pt/fis Departamento e Física e Astronomia, Faculdade de Ciências da Universidade do Porto, 4169-007 Porto Portugal - Tel: +351 220402393 References (to allow students first look at topic) [1] N. Bilic, G. B. Tupper, R. D. Viollier, “Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas”, Phys. Lett. B535 (2002) 17-21. [2] M. C. Bento, O. Bertolami, A. A. Sen, "Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification", Phys.Rev. D66 (2002) 043507. [3] M.C. Bento, O. Bertolami, R. Rosenfeld, L. Teodoro, "Self-interacting Dark Matter and Invisibly Decaying Higgs", Phys. Rev. D62 (2000) 041302. [4] M.C. Bento, O. Bertolami, R. -
1.3 Self-Dual/Chiral Gauge Theories 23 1.3.1 PST Approach 27
Durham E-Theses Chiral gauge theories and their applications Berman, David Simon How to cite: Berman, David Simon (1998) Chiral gauge theories and their applications, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/5041/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk Chiral gauge theories and their applications by David Simon Berman A thesis submitted for the degree of Doctor of Philosophy Department of Mathematics University of Durham South Road Durham DHl 3LE England June 1998 The copyright of this tliesis rests with tlie author. No quotation from it should be published without the written consent of the author and information derived from it should be acknowledged. 3 0 SEP 1998 Preface This thesis summarises work done by the author between October 1994 and April 1998 at the Department of Mathematical Sciences of the University of Durham and at CERN theory division under the supervision of David FairUe. -
Dimensional Reduction, Regularisation
PoS(LL2012)011 Dimensional Reduction (and all that) Tim Jones∗ Liverpool University E-mail: [email protected] I summarise the salient features of regularisation by dimensional reduction, and its relationship with the original form of dimensional regularisation. “Loops and Legs in Quantum Field Theory", 11th DESY Workshop on Elementary Particle Physics April 15-20, 2012 Wernigerode, Germany ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. http://pos.sissa.it/ Dimensional Reduction (and all that) Tim Jones 1. Introduction Siegel [1] introduced regularisation by dimensional reduction (DRED) as a variation of di- mensional regularisation, DREG [2], to maintain the equality of Bose-Fermi degrees of freedom characteristic of supersymmetry, an equality not preserved by DREG. As a consequence, for exam- ple, the relationship between the quark-quark-gluon and quark-squark-gluino couplings in SQCD is not preserved when DREG is used. Which is not to say that DREG cannot be used in supersym- metric theories; but it lacks convenience. For a formal discussion of the equivalence of DRED and DREG (modulo DRED ambiguities to be discussed below) see [3],[4]. A pedagogical introduction PoS(LL2012)011 to Siegel’s proposal, and a first discussion of its application to the non-supersymmetric case appears in Ref. [5]. Essentially DRED amounts to defining xµ ≡ (xi,0) pµ ≡ (pi,0) j j Wµ ≡ Wi(x ),Wσ (x ) (1.1) where µ and i, j are 4-dimensional and D-dimensional indices respectively, and D < 4. It is useful to define hatted quantities with µ,ν ··· indices whose only non-vanishing components are in the D-dimensional subspace; in particular,g ˆµν = (gi j,0). -
Department of Physics and Astronomy University of Heidelberg
Department of Physics and Astronomy University of Heidelberg Diploma thesis in Physics submitted by Kher Sham Lim born in Pulau Pinang, Malaysia 2011 This page is intentionally left blank Planck Scale Boundary Conditions And The Standard Model This diploma thesis has been carried out by Kher Sham Lim at the Max Planck Institute for Nuclear Physics under the supervision of Prof. Dr. Manfred Lindner This page is intentionally left blank Fakult¨atf¨urPhysik und Astronomie Ruprecht-Karls-Universit¨atHeidelberg Diplomarbeit Im Studiengang Physik vorgelegt von Kher Sham Lim geboren in Pulau Pinang, Malaysia 2011 This page is intentionally left blank Randbedingungen der Planck-Skala und das Standardmodell Die Diplomarbeit wurde von Kher Sham Lim ausgef¨uhrtam Max-Planck-Institut f¨urKernphysik unter der Betreuung von Herrn Prof. Dr. Manfred Lindner This page is intentionally left blank Randbedingungen der Planck-Skala und das Standardmodell Das Standardmodell (SM) der Elementarteilchenphysik k¨onnte eine effektive Quan- tenfeldtheorie (QFT) bis zur Planck-Skala sein. In dieser Arbeit wird diese Situ- ation angenommen. Wir untersuchen, ob die Physik der Planck-Skala Spuren in Form von Randbedingungen des SMs hinterlassen haben k¨onnte. Zuerst argumen- tieren wir, dass das SM-Higgs-Boson kein Hierarchieproblem haben k¨onnte, wenn die Physik der Planck-Skala aus einem neuen, nicht feld-theoretischen Konzept bestehen w¨urde. Der Higgs-Sektor wird bez¨uglich der theoretischer und experimenteller Ein- schr¨ankungenanalysiert. Die notwendigen mathematischen Methoden aus der QFT, wie z.B. die Renormierungsgruppe, werden eingef¨uhrtum damit das Laufen der Higgs- Kopplung von der Planck-Skala zur elektroschwachen Skala zu untersuchen. -
Running Coupling and Anomalous Dimension of SU(3) Gauge Theory with Adjoint Fermions
Running coupling and anomalous dimension of SU(3) gauge theory with adjoint fermions Thomas DeGranda, Yigal Shamirb and Benjamin Svetitskyb Department of Physics, University of Colorado, Boulder, CO 80309, USA cRaymond and Beverly Sackler School of Physics and Astronomy Tel-Aviv University, Ramat Aviv, 69978 Israel ABSTRACT We propose to measure the running coupling and pseudoscalar renormalization constant of the SU(3) gauge theory with two flavors of adjoint fermions on 124 and 164 lattices. This will be combined with data from smaller lattices to give the beta func- tion and mass anomalous dimension of the theory, which is a technicolor candidate. The total time requested is 3.3 million Jpsi-equivalent core-hours on the Fermilab clusters. 1 1 Physics goals Gauge theories with groups other than SU(3), or with light fermions in representations higher than the fundamental, are a staple of theories that go beyond the Standard Model. Among the mechanisms proposed to connect these theories to the Standard Model at low energies are technicolor and tumbling, with many associated variants. Both of these depend largely on weak-coupling pictures for their dynamics: a perturbative β function to take technicolor from weak to strong coupling as the energy scale drops, and a most-attractive-channel argument for scale separation and selection of the condensed channel in tumbling. Nonperturbative tests of these pictures, long overdue, have appear only in the last four years—for reviews, see [1–3]. In the past four years we have carried out a program of lattice studies of theories with SU(N) gauge fields and fermions in the two-index symmetric representation of the gauge group [4–9]. -
Exact Solutions and Black Hole Stability in Higher Dimensional Supergravity Theories
Exact Solutions and Black Hole Stability in Higher Dimensional Supergravity Theories by Sean Michael Anton Stotyn A thesis presented to the University of Waterloo in fulfillment of the thesis requirement for the degree of Doctor of Philosophy in Physics Waterloo, Ontario, Canada, 2012 c Sean Michael Anton Stotyn 2012 ! I hereby declare that I am the sole author of this thesis. This is a true copy of the thesis, including any required final revisions, as accepted by my examiners. I understand that my thesis may be made electronically available to the public. iii Abstract This thesis examines exact solutions to gauged and ungauged supergravity theories in space-time dimensions D 5 as well as various instabilities of such solutions. ≥ I begin by using two solution generating techniques for five dimensional minimal un- gauged supergravity, the first of which exploits the existence of a Killing spinor to gener- ate supersymmetric solutions, which are time-like fibrations over four dimensional hyper- K¨ahlerbase spaces. I use this technique to construct a supersymmetric solution with the Atiyah-Hitchin metric as the base space. This solution has three independent parameters and possesses mass, angular momentum, electric charge and magnetic charge. Via an anal- ysis of a congruence of null geodesics, I determine that the solution contains a region with naked closed time-like curves. The centre of the space-time is a conically singular pseudo- horizon that repels geodesics, otherwise known as a repulson. The region exterior to the closed time-like curves is outwardly geodesically complete and possesses an asymptotic region free of pathologies provided the angular momentum is chosen appropriately. -
Homogeneous Spherically Symmetric Bodies with a Nonminimal Coupling
Gen. Rel. Grav. manuscript No. (will be inserted by the editor) Homogeneous spherically symmetric bodies with a non-minimal coupling between curvature and matter The choice of the Lagrangian density for matter Orfeu Bertolami · Jorge Páramos Received: September 20, 2021/ Accepted: Abstract In this work we study how a non-minimal coupling between matter and gravity can modify the structure of a homogeneous spherical body. The physical rele- vance of the adopted Lagrangian density is ascertained, with results obtained for two different choices of the latter. Keywords Nonminimal Coupling · Lagrangean Density · Interior Solution PACS 04.20.Fy · 04.80.Cc · 11.10.Ef 1 Introduction Despite its great experimental success (see e.g. Refs. [1,2]), General Relativity (GR) is not the most encompassing way to couple matter with curvature. Indeed, matter and curvature can be coupled, for instance, in a non-minimal way [3], extending the well-known class of f (R) theories [4–6]. This nonminimal coupling can have a bearing on the dark matter [3,7,8] and dark energy [9–12] problems, impact the well-known energy conditions [13], affect the Yukawa potential addition prompted by f (R) theories in Solar System tests of gravity [14, 15], modify the Layzer-Irvine equation of virial equilibrium [16] and can give rise to wormhole and time machines [17]. In Ref. [18], several phenomenological aspects of the dynamics of perfect fluids non-minimally coupled to curvature were addressed — in particular, the scenario of an axisymmetric dust distribution with constant