Dilatonic Dark Matter: Experimental Detection of Dilaton and Extra Dimension

Total Page:16

File Type:pdf, Size:1020Kb

Dilatonic Dark Matter: Experimental Detection of Dilaton and Extra Dimension Dilatonic Dark Matter: Experimental Detection of Dilaton and Extra Dimension Young Min Cho Konkuk University, Seoul 143-701, Republic of Korea DOI: http://dx.doi.org/10.3204/DESY-PROC-2016-03/Cho Youngmin The Kaluza-Klein dilaton in higher-dimensional unified theory has important implications. First, as the gravitationally interacting massive particle (GIMP) it becomes an ideal can- didate of the dark matter of the universe. Second, as the massive scalar graviton (MSG) it generates the fifth force which modifies the Einstein’s gravity. Most importantly, it repre- sents the extra space itself, so that detecting the dilaton we can confirm the existence of the extra space. We present a simple way to detect the dilaton experimentally, detecting the two photon decay of the remnant dilaton. We show how the fifth force constraint and the dark matter constraint restrict the dilaton mass and the size of the extra space. Moreover, based on the fact that the dilaton mass comes from the curvature of the extra space, we propose the geometric mass generation mechanism that the curvature creates the mass as an alternative to the Higgs mechanism. All existing unified theories are based on the higher-dimensional space-time, which makes the experimental confirmation of the extra space an important issue. In this talk we discuss the physical consequence of the higher-dimensional unification, and present a simple way to detect the extra space experimentally. An unavoidable consequence of higher-dimensional unification is the appearance of gravi- tationally interacting massive particles (GIMPs) or massive scalar gravitons (MSGs) known as the Kaluza-Klein (KK) dilaton and internal gravitons, in 4-dimensional physics [1, 2]. They come in as the gravitons of the extra space, so that they actually represent the very extra space itself. This means that by detecting them we could confirm the existence of the extra space and justify the higher-dimensional unification. The dilaton plays very important roles in physics. First, as the GIMP it becomes an ideal candidate of the dark matter. Second, as the MSG it generates the fifth force which could violate the equivalence principle. Third, it realizes the Dirac’s large number hypothesis making the cosmological constant space-time dependent. Moreover, it could play the role of the quintessence in cosmology [4, 3]. Finally, it appears in all higher-dimensional unified theories, which strongly implies that the dilaton must exist. This makes the experimental detection of the dilaton very important. Unfortunately the dilaton (and the internal gravitons) so far have not been received the due attention, because the extra space has traditionally been assumed to be extremely small (of the Planck scale) [1, 5, 6]. A small extra space could make them very heavy and decay quickly, in which case they leave almost no trace in the present universe. And they cannot easily be produced because it will cost too much energy. In this case they become almost irrelevant. Patras 2016 1 PATRAS 2016 23 YOUNG MIN CHO But this is not entirely true. First, even a small extra space can make the dilaton massless [1, 2]. Moreover, there is the possibility that the extra space may not be so small, which could make the dilaton very light [2]. Indeed this is exactly the proposal made by Arkani-Hamed, Dimopoulos, and Dvali (ADD) to resolve the hierarchy problem [7]. The mass of the dilaton is very important for the following reasons. First, it determines the range of the fifth force [8, 9]. Moreover, it determines the energy density of the dark matter [4, 10]. And obviously we have to know the mass to detect the dilaton. So it is crucial for us to understand how the dilaton acquires the mass and to figure out what is the mass range. We show that the cosmological constraint on the dark matter rules out the dilaton mass between 160 MeV and 276 MeV, and argue that the size of the extra space may not be smaller 9 than 10− m. Moreover, we suggest to detect the dilaton detecting the two photon decay of the remnant dilatons in the universe. Finally, from the fact that the curvature of the extra space makes the dilaton massive, we propose a geometric mass generation mechanism that mass can be generated by curvatureas an alternative to the Higgs mechanism. To demonstrate these points, we consider the Kaluza-Klein theory, the protopype of all higher-dimensional unified theories. To obtain the 4-dimensional physics, we have to make the dimensional reduction. There are two contending dimensional reduction schemes, the popular zero mode approximation and the dimensional reduction by isometry. In the zero mode ap- proximation one treats the (4+n)-dimensional space as real and views the 4-dimensional physics as a low energy approximation [5, 6]. In the dimensional reduction by isometry, however, the isometry in the unified space makes the extra space invisible and determines the 4-dimensional physics [1, 11]. A sensitive issue in the zero mode approximation is how one can actually make the approx- imation. A simple way to do this is to impose a proper isometry as an approximate symmetry. In this case the zero mode approximation becomes very much like the dimensional reduction by isometry. In general, however, the two methods have totally different 4-dimensional physics. This is because the zero mode approximation produces an infinite tower of the KK excited modes in 4-dimension. To show how the dimensional reduction by isometry works, we suppose that the (4+n)- dimensional unified space has an n-dimensional isometry G and assume the unified space to be a principal fiber bundle P(M,G) made of the 4-dimensional space-time M and the n-dimensional group manifold G. Let γµν and φab be the metrics on M and G. In this setting the (4+n)- dimensional Einstein-Hilbert action becomes [1, 2] 1 IEH = √γ√φ RM (γµν ) −16πG0 n 1 (∂ φ)(∂ φ) Re2κ2 h − γµν µ ν + √n φ ρ γµαγνβF a F b − 4n φ2 4 ab µν αβ γµν 1 + (D ρab)(D ρ ) + Rˆ (ρ ) 4 µ ν ab κ2 √n φ G ab +Λ + λ( detρ 1) d4xdnθ, P | ab| − γ = det γ , φ = deti φ , | µν | | ab| 1/n ρ = φ− φ , ( det ρ = 1), ab ab | ab| 1 1 Rˆ (ρ ) = f df bρac + f mf nρacρbdρ . (1) G ab 2 ab cd 4 ab cd mn 2 Patras 2016 24 PATRAS 2016 DILATONIC DARK MATTER:EXPERIMENTAL DETECTION OF DILATON AND EXTRA ... Here G0 is the (4 + n)-dimensional gravitational constant, RM is the scalar curvature of M, e a is the coupling constant of the KK gauge field Fµν , κ is the scale of the extra space, Λ0 is the (4+n)-dimensional cosmological constant, and λ is a Lagrange multiplier. Notice that RˆG(ρab) is the normalized curvature of the fiber space G. To proceed, we introduce the Pauli metric (also called the Einstein metric in string theory) gµν and the Kaluza-Klein dilaton σ by [1, 4] n g = √φ γ , φ = φ exp 2 σ . (2) µν µν h i n + 2 r But, since κ is left arbitrary, we can always normalize φ = 1, (3) h i without loss of generality. With this understanding we have the following Lagrangian in the Pauli frame [1, 4] ˆ VG 1 2 1 ab µ = √g R + 2 (∂µσ) + (Dµρ )(D ρab) L −16πG0 4 h Rˆ n + 2 n + G exp σ + Λ exp σ κ2 − n P − n + 2 r r e2κ2 n + 2 + exp σ ρ F a F bµν , 4 n ab µν r i Vˆ = dnθ = κn. ( φ = 1) (4) G h i R This describes the well-known unification of gravitation with the gauge field, provided that [1, 2] κn 1 e2κ2 = , = 1, (5) 16πG0 16πG 16πG where G is Newton’s constant. To understand the meaning of (5), notice that by the first equality κ sets the strength of the higher-dimensional gravity l0, 1/(n+2) κ n/2(n+2) l0 = G0 = lp, (6) lp where lp = √G is the Planck scale. This is precisely what one has in the ADD proposal, which confirms that a large extra space can indeed make the higher-dimensional gravity strong [8, 7]. However, from the second equality κ is determined by the fine structure constant of the KK gauge boson αKK [1, 2], 2 2 4 2 e κ = lp. (αKK = ) . (7) αKK 4π This means that a large extra space makes αKK extremely small. In fact this tells that, for the 5 42 ADD proposal which favors κ 10− nm, we need αKK 10− for n = 6. (For n = we 32 ' ' ∞ have α 4 10− , which sets the upper limit of α .) KK ' × KK Patras 2016 3 PATRAS 2016 25 YOUNG MIN CHO To find the mass of the KK dilaton, we assume that (4) has the unique vacuum gµν = η , σ = 0, ρ = δ , A a = 0, and find the dilaton potential h i µν h i h abi ab h µ i 1 Rˆ n + 2 V (σ) = h Gi exp( σ) 16πG κ2 n −r h n +Λ exp( σ) + V , (8) 0 − n + 2 0 r i where RˆG = RˆG(δab) is the (dimensionless) vacuum curvature of the extra space and V0 is a constanth i introduced to assure that (8) has no non-vanishing 4-dimensional vacuum energy. Notice that Λ0 and V0 are completely fixed by the vacuum condition dV (0)/dσ = 0 and V (0) = 0. From (8) we find the mass of the KK dilaton µ (identifyingσ ˆ = σ/√16πG as the physical dilaton), 2 Rˆ 1 Rˆ µ2 = h Gi = h Gi α m2, (9) n κ2 2n KK p where mp is the Planck mass.
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 8. Compactification and T-Duality
    8. Compactification and T-Duality In this section, we will consider the simplest compactification of the bosonic string: a background spacetime of the form R1,24 S1 (8.1) ⇥ The circle is taken to have radius R, so that the coordinate on S1 has periodicity X25 X25 +2⇡R ⌘ We will initially be interested in the physics at length scales R where motion on the S1 can be ignored. Our goal is to understand what physics looks like to an observer living in the non-compact R1,24 Minkowski space. This general idea goes by the name of Kaluza-Klein compactification. We will view this compactification in two ways: firstly from the perspective of the spacetime low-energy e↵ective action and secondly from the perspective of the string worldsheet. 8.1 The View from Spacetime Let’s start with the low-energy e↵ective action. Looking at length scales R means that we will take all fields to be independent of X25: they are instead functions only on the non-compact R1,24. Consider the metric in Einstein frame. This decomposes into three di↵erent fields 1,24 on R :ametricG˜µ⌫,avectorAµ and a scalar σ which we package into the D =26 dimensional metric as 2 µ ⌫ 2σ 25 µ 2 ds = G˜µ⌫ dX dX + e dX + Aµ dX (8.2) Here all the indices run over the non-compact directions µ, ⌫ =0 ,...24 only. The vector field Aµ is an honest gauge field, with the gauge symmetry descend- ing from di↵eomorphisms in D =26dimensions.Toseethisrecallthatunderthe transformation δXµ = V µ(X), the metric transforms as δG = ⇤ + ⇤ µ⌫ rµ ⌫ r⌫ µ This means that di↵eomorphisms of the compact direction, δX25 =⇤(Xµ), turn into gauge transformations of Aµ, δAµ = @µ⇤ –197– We’d like to know how the fields Gµ⌫, Aµ and σ interact.
    [Show full text]
  • Dilaton and Off-Shell (Non-Critical String) Effects in Boltzmann Equation for Species Abundances AB Lahanas1, NE Mavromatos2 and DV Nanopoulos3,4,5
    Research article Open Access Dilaton and off-shell (non-critical string) effects in Boltzmann equation for species abundances AB Lahanas1, NE Mavromatos2 and DV Nanopoulos3,4,5 Address: 1University of Athens, Physics Department, Nuclear and Particle Physics Section, GR157 71, Athens, Greece., 2King's College London, University of London, Department of Physics, Strand WC2R 2LS, London, UK., 3George P. and Cynthia W. Mitchell Institute for Fundamental Physics, Texas A&M University, College Station, TX 77843, USA., 4Astroparticle Physics Group, Houston Advanced Research Center (HARC), Mitchell Campus, Woodlands, TX 77381, USA. and 5Academy of Athens, Division of Natural Sciences, 28 Panepistimiou Avenue, Athens 10679, Greece. Email: AB Lahanas - [email protected]; NE Mavromatos - [email protected]; DV Nanopoulos - [email protected] Published: 2 October 2007 Received: 3 June 2007 Accepted: 2 October 2007 PMC Physics A 2007, 1:2 doi:10.1186/1754-0410-1-2 This article is available from: http://www.physmathcentral.com/1754-0410/1/2 © 2007 Lahanas et al. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/ licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract In this work we derive the modifications to the Boltzmann equation governing the cosmic evolution of relic abundances induced by dilaton dissipative-source and non-critical-string terms in dilaton-driven non-equilibrium string Cosmologies. We also discuss briefly the most important phenomenological consequences, including modifications of the constraints on the available parameter space of cosmologically appealing particle physics models, imposed by recent precision data of astrophysical measurements.
    [Show full text]
  • 5D Kaluza-Klein Theories - a Brief Review
    5D Kaluza-Klein theories - a brief review Andr´eMorgado Patr´ıcio, no 67898 Departamento de F´ısica, Instituto Superior T´ecnico, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal (Dated: 21 de Novembro de 2013) We review Kaluza-Klein theory in five dimensions from the General Relativity side. Kaluza's original idea is examined and two distinct approaches to the subject are presented and contrasted: compactified and noncompactified theories. We also discuss some cosmological implications of the noncompactified theory at the end of this paper. ^ ^ 1 ^ I. INTRODUCTION where GAB ≡ RAB − 2 g^ABR is the Einstein tensor. Inspired by the ties between Minkowki's 4D space- For the metric, we identify the αβ-part ofg ^AB with time and Maxwell's EM unification, Nordstr¨om[3] in 1914 gαβ, the α4-part as the electromagnetic potential Aα and and Kaluza[4] in 1921 showed that 5D general relativ- g^44 with a scalar field φ, parametrizing it as follows: ity contains both Einstein's 4D gravity and Maxwell's g + κ2φ2A A κφ2A EM. However, they imposed an artificial restriction of no g^ (x; y) = αβ α β α ; (4) AB κφ2A φ2 dependence on the fifth coordinate (cylinder condition). β Klein[5], in 1926, suggested a physical basis to avoid this where κ is a multiplicative factor. If we identifyp it in problem in the compactification of the fifth dimension, terms of the 4D gravitational constant by κ = 4 πG, idea now used in higher-dimensional generalisations to then, using the metric4 and applying the cylinder con- include weak and strong interactions.
    [Show full text]
  • Supersymmetry and Stationary Solutions in Dilaton-Axion Gravity" (1994)
    University of Massachusetts Amherst ScholarWorks@UMass Amherst Physics Department Faculty Publication Series Physics 1994 Supersymmetry and stationary solutions in dilaton- axion gravity R Kallosh David Kastor University of Massachusetts - Amherst, [email protected] T Ortín T Torma Follow this and additional works at: https://scholarworks.umass.edu/physics_faculty_pubs Part of the Physical Sciences and Mathematics Commons Recommended Citation Kallosh, R; Kastor, David; Ortín, T; and Torma, T, "Supersymmetry and stationary solutions in dilaton-axion gravity" (1994). Physics Review D. 1219. Retrieved from https://scholarworks.umass.edu/physics_faculty_pubs/1219 This Article is brought to you for free and open access by the Physics at ScholarWorks@UMass Amherst. It has been accepted for inclusion in Physics Department Faculty Publication Series by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. SU-ITP-94-12 UMHEP-407 QMW-PH-94-12 hep-th/9406059 SUPERSYMMETRY AND STATIONARY SOLUTIONS IN DILATON-AXION GRAVITY Renata Kallosha1, David Kastorb2, Tom´as Ort´ınc3 and Tibor Tormab4 aPhysics Department, Stanford University, Stanford CA 94305, USA bDepartment of Physics and Astronomy, University of Massachusetts, Amherst MA 01003 cDepartment of Physics, Queen Mary and Westfield College, Mile End Road, London E1 4NS, U.K. ABSTRACT New stationary solutions of 4-dimensional dilaton-axion gravity are presented, which correspond to the charged Taub-NUT and Israel-Wilson-Perj´es (IWP) solu- tions of Einstein-Maxwell theory. The charged axion-dilaton Taub-NUT solutions are shown to have a number of interesting properties: i) manifest SL(2, R) sym- arXiv:hep-th/9406059v1 10 Jun 1994 metry, ii) an infinite throat in an extremal limit, iii) the throat limit coincides with an exact CFT construction.
    [Show full text]
  • Soft Theorems for the Gravity Dilaton and the Nambu-Goldstone Boson Dilaton
    Soft theorems for the Gravity Dilaton and the Nambu-Goldstone Boson Dilaton Raffaele Marotta INFN Naples GGI April 2019 Talk based on: . P. Di Vecchia, R. M., M. Mojaza, JHEP 1901 (2019) 038 + work in progress. P. Di Vecchia, R. M., M. Mojaza, JHEP 1710(2017)017 . P. Di Vecchia, R.M. , M. Mojaza, J. Nohle, Phys. Rev D93 (2016) n.8, 080515. Plan of the talk • Motivations • Soft theorems in spontaneously broken conformal field theories. • Soft theorems from tree level string amplitudes • Multiloop soft theorems in bosonic string theory • Conclusions. Motivations • It is well know that scattering amplitudes in the deep infrared region (or soft limit) satisfy interesting relations. Low’s theorem: Amplitudes with a soft photon are determined from the corresponding amplitude without the soft particle 푝1 푝1 푝 Soft-photon 2 푞 → 0 푛 = ෍ 퐼=1 푝푖 푝푛 Soft-photon polarization 푒푖 charge of the particle smooth in the soft limit Weinberg: Amplitudes involving gravitons and matter particles show and universal behavior when one graviton becomes soft. They were recognized to be a consequence of the gauge invariance Soft-Photon Soft-graviton Adler’s zero (Weiberg, The Quatum Theory of Fields Vol .II.) • Goldstone theorem: When a symmetry G is spontaneously broken to a sub-group H the spectrum of the theory contains as many Goldston bosons 휋푎, parametrizing the 퐺 coset space Τ퐻 . • 푇푖, 푋푎 are the unbroken and broken generators, 푖 푎 respectively. 퐽 휇, 퐽 휇 are the corresponding currents. 푎 • The matrix elements of the broken currents 퐽휇 are: • The matrix element of a broken current between arbitrary states I, j, has two contributions: 푎 푎 퐽 휇 퐽 휇 Goldstone pole No-pole contribution to F is the “decay constant” dominance the matrix element of for 푞2 → 0 the current.
    [Show full text]
  • Einstein and the Kaluza-Klein Particle
    ITFA-99-28 Einstein and the Kaluza-Klein particle Jeroen van Dongen1 Institute for Theoretical Physics, University of Amsterdam Valckeniersstraat 65 1018 XE Amsterdam and Joseph Henry Laboratories, Princeton University Princeton NJ 08544 Abstract In his search for a unified field theory that could undercut quantum mechanics, Einstein considered five dimensional classical Kaluza-Klein theory. He studied this theory most intensively during the years 1938-1943. One of his primary objectives was finding a non-singular particle solution. In the full theory this search got frustrated and in the x5-independent theory Einstein, together with Pauli, argued it would be impossible to find these structures. Keywords: Einstein; Unified Field Theory; Kaluza-Klein Theory; Quantization; Soli- tons 1 Introduction After having formulated general relativity Albert Einstein did not immediately focus on the unification of electromagnetism and gravity in a classical field theory - the issue that would characterize much of his later work. It was still an open question to him whether arXiv:gr-qc/0009087v1 26 Sep 2000 relativity and electrodynamics together would cast light on the problem of the structure of matter [18]. Rather, in a 1916 paper on gravitational waves he anticipated a different development: since the electron in its atomic orbit would radiate gravitationally, something that cannot “occur in reality”, he expected quantum theory would have to change not only the ”Maxwellian electrodynamics, but also the new theory of gravitation” [19]2. Einstein’s position, however, gradually changed. From about 1919 onwards, he took a strong interest in the unification programme3. In later years, after about 1926, he hoped that he would find a particular classical unified field theory that could undercut quantum theory.
    [Show full text]
  • Paolo Di Vecchia
    Soft Theorems for Massless Particles from Gauge Invariance Paolo Di Vecchia Niels Bohr Institute, Copenhagen and Nordita, Stockholm Brussels, 17.05.2018 Infrared Physics: Asymptotics & BMS symmetry, soft theorems, memory, information paradox and all that Brussels 16-18 May 2018 Paolo Di Vecchia (NBI+NO) Soft behavior Brussels, 17.05.2018 1 / 71 This talk is based on the work done together with I Zvi Bern, Scott Davies and Josh Nohle “Low-Energy Behavior of Gluons and Gravitons from Gauge Invariance", Phys. Rev. D 90 (2014) 084035, arXiv:1406:6987. I Raffaele Marotta, Matin Mojaza and Josh Nohle “The story of the two dilatons", Phys. Rev. D93 (2016) n.8,085015, arXiv:1512.03316. I Raffaele Marotta and Matin Mojaza “Soft theorem for the graviton, dilaton and the Kalb-Ramond field in the bosonic string”, JHEP 1512 (2015) 150, arXiv:1502.05258. “Subsubleading soft theorem for gravitons and dilatons in the bosonic string”, JHEP 1606 (2016) 054, arXiv:1604.03355. “Soft behavior of a closed massless state in superstring and universality in the soft behavior of the dilaton”, JHEP 1612 (2016) 020, arXiv:1610.03481. “The B-field soft theorem and its unification with the graviton and dilaton”, JHEP 1710 (2017) 017, arXiv:1706.02961. Paolo Di Vecchia (NBI+NO) Soft behavior Brussels, 17.05.2018 2 / 71 Plan of the talk 1 Introduction 2 Scattering of a photon and n scalar particles 3 Scattering of a graviton/dilaton and n scalar particles 4 Soft limit of gluon amplitudes 5 Soft limit of (n + 1)-graviton/dilaton amplitude 6 Soft behavior of the Kalb-Ramond Bµν 7 Soft theorems in string theory 8 Origin of string corrections 9 Soft behavior of graviton and dilaton at loop level 10 String dilaton versus field theory dilaton 11 Soft theorem from Ward Identities 12 Double-soft behavior 13 Conclusions and Outlook Paolo Di Vecchia (NBI+NO) Soft behavior Brussels, 17.05.2018 3 / 71 Introduction I In particle physics we deal with many kinds of symmetries.
    [Show full text]
  • Introduction to String Theory, Lecture Notes
    Introduction to String Theory Lecture Notes ETH Z¨urich, HS13 Prof. N. Beisert, Dr. J. Brodel¨ c 2014 Niklas Beisert, Johannes Br¨odel,ETH Zurich This document as well as its parts is protected by copyright. Reproduction of any part in any form without prior written consent of the author is permissible only for private, scientific and non-commercial use. Contents 0 Overview 6 0.1 Contents . .6 0.2 References . .6 1 Introduction 1.1 1.1 Definition . 1.1 1.2 Motivation . 1.1 1.3 Some Conventions . 1.5 2 Relativistic Point Particle 2.1 2.1 Non-Relativistic Actions . 2.1 2.2 Worldline Action . 2.2 2.3 Polynomial Action . 2.3 2.4 Various Gauges . 2.4 2.5 Quantisation . 2.4 2.6 Interactions . 2.5 2.7 Conclusions . 2.6 3 Classical Bosonic String 3.1 3.1 Nambu{Goto Action . 3.1 3.2 Polyakov Action . 3.2 3.3 Conformal Gauge . 3.3 3.4 Solution on the Light Cone . 3.4 3.5 Closed String Modes . 3.4 3.6 Hamiltonian Formalism . 3.7 4 String Quantisation 4.1 4.1 Canonical Quantisation . 4.1 4.2 Light Cone Quantisation . 4.2 4.3 String Spectrum . 4.3 4.4 Anomalies . 4.6 4.5 Covariant Quantisation . 4.7 5 Compactification and T-Duality 5.1 5.1 Kaluza{Klein Modes . 5.1 5.2 Winding Modes . 5.2 5.3 T-Duality . 5.3 5.4 General Compactifications . 5.5 6 Open Strings and D-Branes 6.1 6.1 Neumann Boundary Conditions .
    [Show full text]