Soft Theorems for the Gravity Dilaton and the Nambu-Goldstone Boson Dilaton
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Report of the Supersymmetry Theory Subgroup
Report of the Supersymmetry Theory Subgroup J. Amundson (Wisconsin), G. Anderson (FNAL), H. Baer (FSU), J. Bagger (Johns Hopkins), R.M. Barnett (LBNL), C.H. Chen (UC Davis), G. Cleaver (OSU), B. Dobrescu (BU), M. Drees (Wisconsin), J.F. Gunion (UC Davis), G.L. Kane (Michigan), B. Kayser (NSF), C. Kolda (IAS), J. Lykken (FNAL), S.P. Martin (Michigan), T. Moroi (LBNL), S. Mrenna (Argonne), M. Nojiri (KEK), D. Pierce (SLAC), X. Tata (Hawaii), S. Thomas (SLAC), J.D. Wells (SLAC), B. Wright (North Carolina), Y. Yamada (Wisconsin) ABSTRACT Spacetime supersymmetry appears to be a fundamental in- gredient of superstring theory. We provide a mini-guide to some of the possible manifesta- tions of weak-scale supersymmetry. For each of six scenarios These motivations say nothing about the scale at which nature we provide might be supersymmetric. Indeed, there are additional motiva- tions for weak-scale supersymmetry. a brief description of the theoretical underpinnings, Incorporation of supersymmetry into the SM leads to a so- the adjustable parameters, lution of the gauge hierarchy problem. Namely, quadratic divergences in loop corrections to the Higgs boson mass a qualitative description of the associated phenomenology at future colliders, will cancel between fermionic and bosonic loops. This mechanism works only if the superpartner particle masses comments on how to simulate each scenario with existing are roughly of order or less than the weak scale. event generators. There exists an experimental hint: the three gauge cou- plings can unify at the Grand Uni®cation scale if there ex- I. INTRODUCTION ist weak-scale supersymmetric particles, with a desert be- The Standard Model (SM) is a theory of spin- 1 matter tween the weak scale and the GUT scale. -
Spectra of Conformal Sigma Models
Spectra of Conformal Sigma Models Dissertation zur Erlangung des Doktorgrades an der Fakultät für Mathematik, Informatik und Naturwissenschaften Fachbereich Physik der Universität Hamburg vorgelegt von Václav Tlapák aus Berlin Hamburg 2014 Tag der Disputation: 30. Januar 2015 Folgende Gutachter empfehlen die Annahme der Dissertation: Prof. Dr. Volker Schomerus Prof. Dr. Gleb Arutyunov Zusammenfassung Die vorliegende Arbeit beschäftigt sich mit den Spektren von konformen Sigma Modellen, die auf (verallgemeinerten) symmetrischen Räumen defi- niert sind. Die Räume, auf denen Sigma Modelle ohne Wess-Zumino-Term konform sind, sind Supermannigfaltigkeiten, also Mannigfaltigkeiten, die fermionische Richtungen aufweisen. Wir stellen die Konstruktion von Ver- tex Operatoren vor, gefolgt von der Hintergrundfeld-Entwicklung. Für semi- symmetrische Räume berechnen wir anschließend die diagonalen Terme der anomalen Dimensionen dieser Operatoren in führender Ordnung. Das Resul- tat stimmt mit dem für symmetrische Räume überein, jedoch treten nicht- diagonale Terme auf, die hier nicht weiter betrachtet werden. Anschließend präsentieren wir eine detaillierte Analyse des Spectrums des Supersphären S3j2 Sigma Modells. Dies ist eins der einfachsten Beispie- le für konforme Sigma Modelle auf symmetrischen Räumen und dient als Illustration für die Mächtigkeit der vorgestellten Methoden. Wir verwenden die erhaltenen Daten, um eine Dualität mit dem OSP(4j2) Gross-Neveu Modell zu untersuchen, die von Candu und Saleur vorgeschlagen wurde. Wir verwenden dazu ein Resultat, welches die anomalen Dimensionen von 1 2 BPS Operatoren zu allen Ordnungen berechnet. Wir finden das gesamte Grundzustandsspektrum des Sigma Modells. Darüber hinaus legen wir dar, dass sowohl die Zwangsbedingungen als auch die Bewegungsgleichungen des Sigma Modells korrekt vom Gross-Neveu Modell implementiert werden. Die Dualität wird weiterhin durch ein neues exaktes Resultat für die anomalen Dimensionen der Grundzustände unterstützt. -
Durham Research Online
Durham Research Online Deposited in DRO: 30 January 2017 Version of attached le: Published Version Peer-review status of attached le: Peer-reviewed Citation for published item: Bhattacharya, Jyotirmoy and Lipstein, Arthur E. (2016) '6d dual conformal symmetry and minimal volumes in AdS.', Journal of high energy physics., 2016 (12). p. 105. Further information on publisher's website: https://doi.org/10.1007/JHEP12(2016)105 Publisher's copyright statement: Open Access, c The Authors. Article funded by SCOAP3. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Additional information: 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 DRO • 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 DRO policy for further details. Durham University Library, Stockton Road, Durham DH1 3LY, United Kingdom Tel : +44 (0)191 334 3042 | Fax : +44 (0)191 334 2971 https://dro.dur.ac.uk Published for SISSA by Springer Received: November 16, 2016 Revised: December 8, 2016 Accepted: December 12, 2016 Published: December 20, 2016 6d dual conformal symmetry and minimal volumes JHEP12(2016)105 in AdS Jyotirmoy Bhattacharya and Arthur E. -
Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
Conformal Symmetry in Field Theory and in Quantum Gravity
universe Review Conformal Symmetry in Field Theory and in Quantum Gravity Lesław Rachwał Instituto de Física, Universidade de Brasília, Brasília DF 70910-900, Brazil; [email protected] Received: 29 August 2018; Accepted: 9 November 2018; Published: 15 November 2018 Abstract: Conformal symmetry always played an important role in field theory (both quantum and classical) and in gravity. We present construction of quantum conformal gravity and discuss its features regarding scattering amplitudes and quantum effective action. First, the long and complicated story of UV-divergences is recalled. With the development of UV-finite higher derivative (or non-local) gravitational theory, all problems with infinities and spacetime singularities might be completely solved. Moreover, the non-local quantum conformal theory reveals itself to be ghost-free, so the unitarity of the theory should be safe. After the construction of UV-finite theory, we focused on making it manifestly conformally invariant using the dilaton trick. We also argue that in this class of theories conformal anomaly can be taken to vanish by fine-tuning the couplings. As applications of this theory, the constraints of the conformal symmetry on the form of the effective action and on the scattering amplitudes are shown. We also remark about the preservation of the unitarity bound for scattering. Finally, the old model of conformal supergravity by Fradkin and Tseytlin is briefly presented. Keywords: quantum gravity; conformal gravity; quantum field theory; non-local gravity; super- renormalizable gravity; UV-finite gravity; conformal anomaly; scattering amplitudes; conformal symmetry; conformal supergravity 1. Introduction From the beginning of research on theories enjoying invariance under local spacetime-dependent transformations, conformal symmetry played a pivotal role—first introduced by Weyl related changes of meters to measure distances (and also due to relativity changes of periods of clocks to measure time intervals). -
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. -
UV Behavior of Half-Maximal Supergravity Theories
UV behavior of half-maximal supergravity theories. Piotr Tourkine, Quantum Gravity in Paris 2013, LPT Orsay In collaboration with Pierre Vanhove, based on 1202.3692, 1208.1255 Understand the pertubative structure of supergravity theories. ● Supergravities are theories of gravity with local supersymmetry. ● Those theories naturally arise in the low energy limit of superstring theory. ● String theory is then a UV completion for those and thus provides a good framework to study their UV behavior. → Maximal and half-maximal supergravities. Maximal supergravity ● Maximally extended supergravity: – Low energy limit of type IIA/B theory, – 32 real supercharges, unique (ungauged) – N=8 in d=4 ● Long standing problem to determine if maximal supergravity can be a consistent theory of quantum gravity in d=4. ● Current consensus on the subject : it is not UV finite, the first divergence could occur at the 7-loop order. ● Impressive progresses made during last 5 years in the field of scattering amplitudes computations. [Bern, Carrasco, Dixon, Dunbar, Johansson, Kosower, Perelstein, Rozowsky etc.] Half-maximal supergravity ● Half-maximal supergravity: – Heterotic string, but also type II strings on orbifolds – 16 real supercharges, – N=4 in d=4 ● Richer structure, and still a lot of SUSY so explicit computations are still possible. ● There are UV divergences in d=4, [Fischler 1979] at one loop for external matter states ● UV divergence in gravity amplitudes ? As we will see the divergence is expected to arise at the four loop order. String models that give half-maximal supergravity “(4,0)” susy “(0,4)” susy ● Type IIA/B string = Superstring ⊗ Superstring Torus compactification : preserves full (4,4) supersymmetry. -
Conformal Theory of Everything (CTOE)
Conformal theory of everything F. F. Faria ∗ Centro de Ciˆencias da Natureza, Universidade Estadual do Piau´ı, 64002-150 Teresina, PI, Brazil Abstract By using conformal symmetry we unify the standard model of par- ticle physics with gravity in a consistent quantum field theory which describes all the fundamental particles and forces of nature. arXiv:1903.04893v3 [hep-ph] 26 Feb 2020 PACS numbers: 104.60.-m, 98.80.-k, 04.50.+h * [email protected] 1 Introduction It is well know that the standard model (SM) of particle physics is consistent with the experiments performed so far on particle accelerators such as the large hadron collider (LHC). However, the theory presents some problems such as the hierarchy and the Landau pole problems. Several modifications of the SM at scales between the electroweak and Planck scales, such as GUT [1, 2, 3, 4] or SUSY [5, 6, 7, 8, 9, 10, 11, 12, 13], have been proposed to solve such problems. However, it is likely that there is no new physics beyond the SM all the way up to the Planck scale [14]. This leads us to suppose that the SM is a low energy limit of a fundamental theory defined at the Planck scale. Since gravitational effects are expected to be important around the Planck scale, it is natural to conjecture that this fundamental theory includes quantum gravity. One of the most straightforward ways to extend and unify physical the- ories is to change the symmetry of their actions. A strong candidate to be incorporated in the unification of the SM with gravity is the (local) conformal symmetry, which performs a multiplicative rescaling of all fields according to Φ=Ω(˜ x)−∆Φ Φ, (1) where Ω(x) is an arbitrary function of the spacetime coordinates, and ∆Φ is the scaling dimension of the field Φ, whose values are 2 for the metric field, 0 for gauge bosons, 1 for scalar fields, and 3/2 for fermions.− The consideration of the conformal symmetry as one of the fundamen- tal symmetries of physics is justified for several reasons. -
Conformally Invariant Equations for Graviton 50 5.1 the Conformally Invariant System of Conformal Degree 1
Conformally Invariant Equations for Graviton Mohsen Fathi Department of Physics, Tehran Central Branch Islamic Azad Univeristy arXiv:1210.3436v3 [physics.gen-ph] 12 Nov 2012 A thesis submitted for the Master degree Master of Science in Physics Tehran, Winter 2010 I am grateful to my supervisor Dr. Mohammad Reza Tanhayi for the helps, supports and scientific training, during this work and thereafter. Abstract Recent astrophysical data indicate that our universe might currently be in a de Sitter (dS) phase. The importance of dS space has been primarily ignited by the study of the inflationary model of the universe and the quantum gravity. As we know Einstein’s theory of gravitation (with a nonzero cosmological constant) can be interpreted as a theory of a metric field; that is, a symmetric tensor field of rank-2 on a fixed de Sitter back- ground. It has been shown the massless spin-2 Fierz-Pauli wave equation (or the linearized Einstein equation) is not conformally invariant. This result is in contrary with what we used to expect for massless theories. In this thesis we obtain conformally invariant wave equation for the massless spin-2 in the dS space. This study is motivated by the belief that confor- mal invariance may be the key to a future theory of quantum gravity. Contents Introduction 1 1 The Lorentz and the conformal groups, and the concept of invari- ance 3 1.1 Grouptheory ............................... 3 1.1.1 Orthogonalgroups ........................ 4 1.1.2 Rotationgroups.......................... 5 1.2 Invarianceunderagroupaction . 7 1.2.1 Invarianceofthelawsofphysics. 7 1.3 TheLorentzgroup ............................ 8 1.4 Theconformalgroup .......................... -
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. -
S-Duality of D-Brane Action at Order $ O (\Alpha'^ 2) $
S-duality of D-brane action 2 at order O(α′ ) Mohammad R. Garousi1 Department of Physics, Ferdowsi University of Mashhad P.O. Box 1436, Mashhad, Iran Abstract Using the compatibility of the DBI and the Chern-Simons actions with the T- duality transformations, the curvature corrections to these actions have been recently extended to include the quadratic B-field couplings at order O(α′2). In this paper, we use the compatibility of the couplings on D3-brane with the S-duality to find the nonlinear RR couplings at order O(α′2). We confirm the quadratic RR couplings in the DBI part with the disk-level scattering amplitude. Using the regularized non- holomorphic Eisenstein series E1, we then write the results in SL(2,Z) invariant form. arXiv:1103.3121v5 [hep-th] 25 Dec 2013 [email protected] 1 Introduction The low energy effective field theory of D-branes consists of the Dirac-Born-Infeld (DBI) [1] and the Chern-Simons (CS) actions [2]. The curvature corrections to the CS part can be found by requiring that the chiral anomaly on the world volume of intersecting D-branes (I-brane) cancels with the anomalous variation of the CS action. This action for a single ′2 Dp-brane at order O(α ) is given by [3, 4, 5], 2 ′2 π α Tp (p−3) SCS C tr(RT RT ) tr(RN RN ) (1) p+1 ⊃ − 24 ZM ∧ ∧ − ∧ p+1 where M represents the world volume of the Dp-brane. For totally-geodesic embeddings of world-volume in the ambient spacetime, RT,N are the pulled back curvature 2-forms of the tangent and normal bundles respectively (see the appendix in ref. -
Non-Critical String Theory Formulation of Microtubule Dynamics And
ACT-09/95 CERN-TH.127/95 CTP-TAMU-24/95 ENSLAPP-A|-/95 hep-ph/9505401 Non-Critical String Theory Formulation of Microtubule Dynamics and Quantum Asp ects of Brain Function a; b;c N.E. Mavromatos and D.V. Nanop oulos a Lab oratoire de Physique Theorique ENSLAPP (URA 14-36 du CNRS, asso ciee a l' E.N.S de Lyon, et au LAPP (IN2P3-CNRS) d'Annecy-le-Vieux), Chemin de Bellevue, BP 110, F-74941 Annecy-le-Vieux Cedex, France. b Texas A & M University, College Station, TX 77843-424 2, USA and Astroparticle Physics Group, Houston Advanced Research Center (HARC), The Mitchell Campus, Wo o dlands, TX 77381, USA. c CERN, Theory Division, Geneva 23 Switzerland Abstract Microtubule (MT) networks, subneural paracrystalline cytosceletal structures, seem to play a fundamental role in the neurons. We cast here the complicated MT dynamics in processed by the SLAC/DESY Libraries on 30 May 1995. 〉 the form of a 1 + 1-dimensional non-critical string theory,thus enabling us to provide a consistent quantum treatment of MTs, including enviromental friction e ects. We suggest, thus, that the MTs are the microsites, in the brain, for the emergence of stable, macroscopic PostScript quantum coherent states, identi able with the preconscious states. Quantum space-time e ects, as describ ed by non-critical string theory, trigger then an organizedcol lapse of the coherent states down to a sp eci c or conscious state. The whole pro cess we estimate to take O (1 sec), in excellent agreement with a plethora of exp erimental/observational ndings.