Inner Perturbations in Noncommutative Geometry

Total Page:16

File Type:pdf, Size:1020Kb

Inner Perturbations in Noncommutative Geometry Inner perturbations in noncommutative geometry Walter D. van Suijlekom (joint with Ali Chamseddine and Alain Connes) January 17, 2014 Overview Spectral triples as noncommutative manifolds Gauge group, semi-group of inner perturbations Relation to Morita equivalence Examples: Yang{Mills, almost-commutative manifolds, SM Noncommutative manifolds Basic device: a spectral triple (A; H; D): algebra A of bounded operators on a Hilbert space H, a self-adjoint operator D in H with compact resolvent and such that the commutator [D; a] is bounded for all a 2 A. Key example: Riemannian spin geometry Let M be an compact m-dimensional Riemannian spin manifold. A = C 1(M) H = L2(S), square integrable spinors D = @= , Dirac operator Then D has compact resolvent because @= elliptic self-adjoint. Also[ D; f ] bounded for f 2 C 1(M). Real spectral triples (A; H; D) Extend to a real spectral triple: J : H!H real structure (anti-unitary) such that J2 = ±1; JD = ±DJ Action of Aop on H: aop = Ja∗J−1 such that aopbop = Ja∗J−1Jb∗J−1 = J(ba)∗J−1 = (ba)op We demand [aop; b] = 0; a; b 2 A D is said to satisfy the first-order condition if [[D; a]; bop] = 0 Spectral invariants 1 Tr f (D=Λ)+ hJ ; D i 2 Invariant under unitaries u 2 U(A) acting as D 7! UDU∗; U = uJuJ−1 Gauge group: G(A) := fuJuJ−1 : u 2 U(A)g Compute rhs: D 7! D + u[D; u∗] +u ^[D; u^∗] +^u[u[D; u∗]; u^∗] withu ^ = JuJ−1 and blue term vanishes if D satisfies first-order condition Semi-group of inner perturbations 8 9 P <X op op j aj bj = 1 = Pert(A) := aj ⊗ bj 2 A ⊗ A P op P ∗ ∗op aj ⊗ b = b ⊗ a : j j j j j j ; with semi-group law inherited from product in A ⊗ Aop. U(A) maps to Pert(A) by sending u 7! u ⊗ u∗op. Pert(A) acts on D: X D 7! aj Dbj j For real spectral triples we use the map Pert(A) ! Pert(A ⊗ A^) sending T 7! T ⊗ T^ so that X D 7! ai ^aj Dbi b^j i;j and this extends the action of the gauge group G(A). Morita equivalence Suppose A ∼M B. Can we construct a spectral triple on B from (A; H; D)? Let B' EndA(E) with E finitely generated projective. Define 0 H = E ⊗A H Then B acts as bounded operators on H0. The self-adjoint operator (1 ⊗r D)(η ⊗ ) := rD (η) + η ⊗ D requires a universal connection on E: 1 r : E ! E ⊗A Ω (A) 1 where rD indicates that aδ(b) 2 Ω (A) is represented as a[D; b]. 0 Then( B; H ; 1 ⊗r D) is a spectral triple [Connes, 1996]. Morita equivalence with real structure Again, suppose A ∼M B. If there is a real structure J on (A; H; D), then we define 0 H := (E ⊗A H) ⊗A E with the conjugate (left A-) module E and define analogously the 0 operator (1 ⊗r D) ⊗r 1 on H , where 1 r : E! Ω (A) ⊗A E; and we also define J0 : H0 !H0; η ⊗ ⊗ ρ 7! ρ ⊗ J ⊗ η Proposition (Chamseddine{Connes{vS, 2013) We have (1 ⊗r D) ⊗r 1 = 1 ⊗r (D ⊗r 1) and the tuple 0 0 (B; H ; (1 ⊗r D) ⊗r 1; J ) is a real spectral triple. Morita self-equivalence 0 0 If B = A (i.e. E = A) we have H = E ⊗A H ⊗A E'H and J ≡ J. 0 The operator D is perturbed to D ≡ D + A(1) + Ae(1) + A(2) where X X ^ −1 A(1) := aj [D; bj ]; Ae(1) := ^aj [D; bj ] = ±JA(1)J ; j j X ^ X ^ A(2):= ^aj [A(1); bj ] = ^aj ak [[D; bk ]; bj ] j j;k and blue terms vanish if D satisfies first-order condition Gauge transformations D0 7! UD0U∗ implemented by ∗ ∗ A(1) 7! uA(1)u + u[D; u ] −1 ∗ −1 −1 ∗ ∗ −1 A(2) 7! JuJ A(2)Ju J + JuJ [u[D; u ]; Ju J ] Perturbation semi-group and Morita self-equivalences Proposition (Chamseddine{Connes{vS, 2013) The linear map η : Pert(A) ! Ω1(A), η(a ⊗ bop) = aδ(b) is surjective. P op If j aj ⊗ bj 2 Pert(A) then the perturbed operator X X aj Dbj = D + aj [D; bj ] ≡ D + A(1) j j and, for real spectral triples: X ^ ai ^aj Dbi bj = D + A(1) + Ae(1) + A(2) i;j Examples: Pert(A) for matrix algebras (joint with Niels Neumann) 8 9 P <X op op j aj bj = 1 = Pert(A) := aj ⊗ bj 2 A ⊗ A P op P ∗ ∗op aj ⊗ b = b ⊗ a : j j j j j j ; N N If A = C , then in terms of basis vectors fei g of C : 8 9 N <X N2 Cii = 1 = N(N−1)=2 Pert(C ) ' Cij ei ⊗ ej 2 C ' C Cij = Cji : i;j ; Examples: Pert(A) for matrix algebras (joint with Niels Neumann) 8 9 P <X op op j aj bj = 1 = Pert(A) := aj ⊗ bj 2 A ⊗ A P op P ∗ ∗op aj ⊗ b = b ⊗ a : j j j j j j ; op If A = MN (C) 'A , then in terms of basis vectors feij g of MN (C): 8 9 P <X j Cij;jk = δik = Pert(MN (C)) ' Cij;kl eij ⊗ ekl 2 MN2 (C) Cij;kl = Clk;ji : i;j ; Ce1 = e1 ' C 2 MN2 (C) CΩ = ΩC 1 0 where Ω = N(N+1)=2 . 0 −1N(N−1)=2 Examples: Pert(A) for function algebras 8 9 P <X op op j aj bj = 1 = Pert(A) := aj ⊗ bj 2 A ⊗ A P op P ∗ ∗op aj ⊗ b = b ⊗ a : j j j j j j ; If A = C 1(M) then 1 1 f (x; x) = 1 8x 2 M Pert(C (M)) ' f 2 C (M × M) f (x; y) = f (y; x) 8x; y 2 M 1 µ Action of Pert(C (M)) on D = @= = iγ rµ is given by X µ µ aj @= bj = @= + iγ r @ f (x; y)jx=y =: @= + iγ Aµ @yµ j 1 with Aµ 2 C (M; u(1)) Non-abelian Yang{Mills theory On a 4-dimensional background: 1 A = C (M) ⊗ Mn(C) 2 H = L (S) ⊗ Mn(C) D = @= ⊗ 1 J = C ⊗ (:)∗. Proposition (Chamseddine-Connes, 1996) Tr f (D): pure gravity µ The perturbations A(1) + Ae(1) with A(1) = γ Aµ describes an su(n)-gauge field on M. Gauge group G(A) ' C 1(M; SU(n)) The spectral action of the perturbed Dirac operator is given by ! Z D + A(1) + Ae(1) f (0) µν −1 Tr f ∼ (··· ) + 2 Tr FµνF + O(Λ ) Λ 24π M Almost-commutative geometries A class of examples 1 2 (C (M) ⊗ AF ; L (S) ⊗ HF ; @= ⊗ 1 + γ5 ⊗ DF ) with real structure J = JM ⊗ JF . 1 1 Gauge group G(C (M) ⊗ AF ) = C (M; G(AF )) Inner perturbations: 0 µ D 7! D = @= ⊗ 1 + γ ⊗ adAµ + γ5 ⊗ Φ −1 with adAµ a g(AF )-gauge potential and Φ = DF + φ + JF φJF a map HF !HF Explicitly, X X Aµ = −i aj @µ(bj ); φ = aj [DF ; bj ] j j As G(AF )-representations: ∗ ∗ ∗ Aµ 7! uAµu − iu@µu ; Φ 7! UΦU Almost-commutative geometries Spectral action Proposition (Van den Dungen{vS, 2012) In the above setting, D0 f (0) 2f Λ2 f (0) Tr f ∼ (··· ) + Tr (F F µν) − 2 Tr (Φ2) + Tr (Φ4) Λ 24π2 µν 4π2 8π2 f (0) f (0) + sTr (Φ2) + Tr (D Φ)(DµΦ) + O(Λ−1): 48π2 8π2 µ with f2 the first moment of f . The noncommutative Standard Model 1 2 (C (M) ⊗ (C ⊕ H ⊕ M3(C)); L (S) ⊗ HF ; @= ⊗ 1 + γ5 ⊗ DF ) Fermions are given by: ⊕3 HF := Hl ⊕ Hl ⊕ Hq ⊕ Hq : Algebra acts as: 0λ 0 0 0 1 0λ 0 0 0 1 Hl B 0 λ 0 0 C Hq B 0 λ 0 0 C (λ, q; m) −! B C ; (λ, q; m) −−! B C ⊗ 13; @ 0 0 α β A @ 0 0 α β A 0 0 −β α 0 0 −β α Hl Hq (λ, q; m) −! λ14; (λ, q; m) −−! 14 ⊗ m Real structure JF interchanges fermions and anti-fermions. The noncommutative Standard Model The finite Dirac operator ST ∗ D := F T S The operator S is given by 0 1 0 1 0 0 Yν 0 0 0 Yu 0 0 0 0 Y 0 0 0 Y S := Sj = B e C ; S ⊗ 1 := Sj = B d C ⊗ 1 ; l Hl B ∗ C q 3 Hq B ∗ C 3 @Yν 0 0 0 A @Yu 0 0 0 A ∗ ∗ 0 Ye 0 0 0 Yd 0 0 where Yν, Ye , Yu and Yd are 3 × 3 mass matrices acting on the three generations. The symmetric operator T only acts on the right-handed (anti)neutrinos, T νR = YR νR for a 3 × 3 symmetric Majorana mass matrix YR , and Tf = 0 for all other fermions f 6= νR . The noncommutative Standard Model The spectral action Proposition (Chamseddine{Connes{Marcolli, 2007) In the above setting, The unimodular gauge group SG(C ⊕ H ⊕ M3(C)) = U(1) × SU(2) × SU(3) The inner perturbations of @= ⊗ 1 + γ5 ⊗ DF are parametrized by U(1); SU(2) and SU(3) gauge fields Λµ; Qµ; Vµ and a Higgs doublet H The spectral action is given by D0 f (0)10 Tr f ∼ (··· ) + Λ Λµν + Tr (Q Qµν) + Tr (V V µν) Λ π2 3 µν µν µν bf (0) −2af Λ2 + ef (0) af (0) + jHj4 + 2 jHj2 + jD Hj2 + O(Λ−1): 2π2 π2 2π2 µ Example beyond first-order [Chamseddine{Connes{vS, 2013] 0 AF = CR ⊕ CL ⊕ M2(C); 2 ◦ 2 ◦ ◦ HF = (CR ⊕ CL) ⊗ (C ) ⊕ C ⊗ (CR ⊕ CL); 0 1 J = ◦ C (C : complex conjugation); F 1 0 0 1 0 k ⊗ 1 ky 0 0 x 2 0 0 Bkx ⊗ 12 0 0 C DF = B C B ky 0 C @ 0 0 0 0 12 ⊗ kx A 0 0 12 ⊗ kx 0 The algebra action of (λR ; λL; m) 2 A on H is given explicitly by t ! λR 12 m op mt π(λ ; λ ; m) = λL12 ; π (λ ; λ ; m) = : R L m R L λR 12 m λL12 Proposition 0 The largest (even) subalgebra AF ⊂ AF ≡ CR ⊕ CL ⊕ M2(C) for which the first-order condition holds (for the above HF ; DF and JF ) is given by λ 0 A = λ ; λ ; R :(λ ; λ ; µ) 2 ⊕ ⊕ F R L 0 µ R L CR CL C Proposition The inner perturbed Dirac operatorD 0 is parametrized by three complex scalar fields φ, σ1; σ2 entering in A(1) and A(2): t 0 0 kx (1+φ)⊗12 ky vv 0 1 ^ kx (1+φ)⊗12 0 0 DF + A(1) + A(1) + A(2) = @ t A ky v v 0 0 12⊗kx (1+φ) 0 0 12⊗kx (1+φ) 0 1 + σ with v = 1 .
Recommended publications
  • Full Program, with Speakers
    Frontiers of Fundamental Physics 14 Marseille, July 15–18, 2014 Program and Speakers Updated on January 8, 2015 1 Program, July, 15 08h00 – 08h45 Conference Registration, Room “Salle de Conférences” 08h45 – 10h30 Plenary session Plenary Session (broadcast) Chairman: Eric Kajfasz Amphi “Sciences Naturelles” 08h45 – 09h00 Roland Triay (CPT) Opening 09h00 – 09h30 Gabriele Veneziano (CdF) Personal reflections on two success stories 09h30 – 10h00 Paraskevas Sphicas (CERN and Athens) Status of HEP after the LHC Run 1 10h00 – 10h30 Subir Sarkar (UOXF & NBI) Program Discovering dark matter 10h30 – 11h00 Coffee break July, 15 11h00 – 12h30 Morning parallel plenary sessions Plenary Session 1 The visible universe (broadcast) Chairman: François Bouchet Amphi “Sciences Naturelles” 11h00 – 11h30 Enrique Gaztañaga (ICE, IEEC-CSIC) LSS with angular cross-correlations: Combining Spectroscopic and Photometric Surveys 11h30 – 12h00 Adi Nusser (IIT) Dynamics of the Cosmic Web 12h00 – 12h30 Pierre Astier (LPNHE) Distances to supernovae: an efficient probe of dark energy Plenary Session 2 New Geometries for Physics Chairman: Fedele Lizzi Amphi “Massiani” 11h00 – 11h45 Ali Chamseddine (AUB and IHES) Geometric Unification 11h45 – 12h30 Pierre Bieliavsky (UCLouvain) Geometrical aspects of deformation quantization Plenary Session 3 Gravitation and the Quantum Chairman: Jerzy Lewandowski Amphi “Charve” 11h00 – 11h45 Walter Greiner (FIAS) There are no black holes: Pseudo-Complex General Relativity From Einstein to Zweistein 11h45 – 12h30 Eugenio Bianchi (Penn State)
    [Show full text]
  • Coll055-Endmatter.Pdf
    http://dx.doi.org/10.1090/coll/055 America n Mathematica l Societ y Colloquiu m Publication s Volum e 55 Noncommutativ e Geometry , Quantu m Field s an d Motive s Alai n Conne s Matild e Marcoll i »AMS AMERICAN MATHEMATICA L SOCIET Y öUöi HINDUSTA N SJU BOOKAGENC Y Editorial Boar d Paul J . Sally , Jr., Chai r Yuri Mani n Peter Sarna k 2000 Mathematics Subject Classification. Primar y 58B34 , 11G35 , 11M06 , 11M26 , 11G09 , 81T15, 14G35 , 14F42 , 34M50 , 81V25 . This editio n i s published b y th e America n Mathematica l Societ y under licens e fro m Hindusta n Boo k Agency . For additiona l informatio n an d Update s o n thi s book , visi t www.ams.org/bookpages/coll-55 Library o f Congres s Cataloging-in-Publicatio n Dat a Connes, Alain . Noncommutative geometry , quantu m fields an d motive s / Alai n Connes , Matild e Marcolli , p. cm . — (Colloquiu m publication s (America n Mathematica l Society) , ISS N 0065-925 8 ; v. 55 ) Includes bibliographica l reference s an d index . ISBN 978-0-8218-4210- 2 (alk . paper ) 1. Noncommutativ e differentia l geometry . 2 . Quantu m field theory , I . Marcolli , Matilde . IL Title . QC20.7.D52C66 200 7 512/.55—dc22 200706084 3 Copying an d reprinting . Individua l reader s o f thi s publication , an d nonprofi t librarie s acting fo r them , ar e permitted t o mak e fai r us e o f the material , suc h a s to cop y a chapte r fo r us e in teachin g o r research .
    [Show full text]
  • Noncommutative Geometry Models for Particle Physics and Cosmology, Lecture I
    Noncommutative Geometry models for Particle Physics and Cosmology, Lecture I Matilde Marcolli Villa de Leyva school, July 2011 Matilde Marcolli NCG models for particles and cosmology, I Plan of lectures 1 Noncommutative geometry approach to elementary particle physics; Noncommutative Riemannian geometry; finite noncommutative geometries; moduli spaces; the finite geometry of the Standard Model 2 The product geometry; the spectral action functional and its asymptotic expansion; bosons and fermions; the Standard Model Lagrangian; renormalization group flow, geometric constraints and low energy limits 3 Parameters: relations at unification and running; running of the gravitational terms; the RGE flow with right handed neutrinos; cosmological timeline and the inflation epoch; effective gravitational and cosmological constants and models of inflation 4 The spectral action and the problem of cosmic topology; cosmic topology and the CMB; slow-roll inflation; Poisson summation formula and the nonperturbative spectral action; spherical and flat space forms Matilde Marcolli NCG models for particles and cosmology, I Geometrization of physics Kaluza-Klein theory: electromagnetism described by circle bundle over spacetime manifold, connection = EM potential; Yang{Mills gauge theories: bundle geometry over spacetime, connections = gauge potentials, sections = fermions; String theory: 6 extra dimensions (Calabi-Yau) over spacetime, strings vibrations = types of particles NCG models: extra dimensions are NC spaces, pure gravity on product space becomes gravity
    [Show full text]
  • Dirac Operators: Yesterday and Today
    Dirac Operators: Yesterday and Today Dirac Operators: Yesterday and Today Proceedings of the Summer School & Workshop Center for Advanced Mathematical Sciences American University of Beirut, Lebanon August 27 to September 7, 2001 edited by Jean-Pierre Bourguignon Thomas Branson Ali Chamseddine Oussama Hijazi Robert J. Stanton International Press www.intlpress.com Dirac Operators: Yesterday and Today Editors: Jean-Pierre Bourguignon Thomas Branson Ali Chamseddine Oussama Hijazi Robert J. Stanton Copyright © 2005, 2010 by International Press Somerville, Massachusetts, U.S.A. All rights reserved. Individual readers of this publication, and non-profit libraries acting for them, are permitted to make fair use of the material, such as to copy a chapter for use in teaching or research. Permission is granted to quote brief passages from this publication in reviews, provided the customary acknowledgement of the source is given. Republication, systematic copying, or mass reproduction of any material in this publication is permitted only under license from International Press. ISBN 978-1-57146-184-1 Paperback reissue 2010. Previously published in 2005 under ISBN 1-57146-175-2 (clothbound). Typeset using the LaTeX system. v Preface The Summer School ”Dirac Operators: Yesterday and Today” was an ambitious endeavour to show to a public of advanced students a tableau of modern mathematics. The idea was to make available a topic, of considerable importance for mathematics itself because of its deep impact on many mathematical questions, but also for its interactions with one of mathematics historic partners, physics. The Dirac operator was undoubtedly created by Paul Adrien Maurice Dirac to deal with an important physical question.
    [Show full text]
  • Foundations of Mathematics and Physics One Century After Hilbert: New Perspectives Edited by Joseph Kouneiher
    FOUNDATIONS OF MATHEMATICS AND PHYSICS ONE CENTURY AFTER HILBERT: NEW PERSPECTIVES EDITED BY JOSEPH KOUNEIHER JOHN C. BAEZ The title of this book recalls Hilbert's attempts to provide foundations for mathe- matics and physics, and raises the question of how far we have come since then|and what we should do now. This is a good time to think about those questions. The foundations of mathematics are growing happily. Higher category the- ory and homotopy type theory are boldly expanding the scope of traditional set- theoretic foundations. The connection between logic and computation is growing ever deeper, and significant proofs are starting to be fully formalized using software. There is a lot of ferment, but there are clear payoffs in sight and a clear strategy to achieve them, so the mood is optimistic. This volume, however, focuses mainly on the foundations of physics. In recent decades fundamental physics has entered a winter of discontent. The great triumphs of the 20th century|general relativity and the Standard Model of particle physics| continue to fit almost all data from terrestrial experiments, except perhaps some anomalies here and there. On the other hand, nobody knows how to reconcile these theories, nor do we know if the Standard Model is mathematically consistent. Worse, these theories are insufficient to explain what we see in the heavens: for example, we need something new to account for the formation and structure of galaxies. But the problem is not that physics is unfinished: it has always been that way. The problem is that progress, extremely rapid during most of the 20th century, has greatly slowed since the 1970s.
    [Show full text]
  • JHEP08(2020)001 Springer July 7, 2020 May 29, 2020
    Published for SISSA by Springer Received: March 10, 2019 Revised: May 29, 2020 Accepted: July 7, 2020 Published: August 4, 2020 Four-dimensional gravity on a covariant noncommutative space JHEP08(2020)001 G. Manolakos,a P. Manousselisa and G. Zoupanosa;b;c;d aPhysics Department, National Technical University, Zografou Campus 9, Iroon Polytechniou str, GR-15780 Athens, Greece bInstitute of Theoretical Physics, D-69120 Heidelberg, Germany cMax-Planck Institut f¨urPhysik, Fohringer Ring 6, D-80805 Munich, Germany dLaboratoire d' Annecy de Physique Theorique, Annecy, France E-mail: [email protected], [email protected], [email protected] Abstract: We formulate a model of noncommutative four-dimensional gravity on a co- variant fuzzy space based on SO(1,4), that is the fuzzy version of the dS4. The latter requires the employment of a wider symmetry group, the SO(1,5), for reasons of covari- ance. Addressing along the lines of formulating four-dimensional gravity as a gauge theory of the Poincar´egroup, spontaneously broken to the Lorentz, we attempt to construct a four-dimensional gravitational model on the fuzzy de Sitter spacetime. In turn, first we consider the SO(1,4) subgroup of the SO(1,5) algebra, in which we were led to, as we want to gauge the isometry part of the full symmetry. Then, the construction of a gauge theory on such a noncommutative space directs us to use an extension of the gauge group, the SO(1,5)×U(1), and fix its representation. Moreover, a 2-form dynamic gauge field is included in the theory for reasons of covariance of the transformation of the field strength tensor.
    [Show full text]
  • Mimetic Gravity
    Mimetic Gravity Ali Chamseddine American University of Beirut, Lebanon & Radboud University Excellence Professor Modern Trends in Particle Physics, Nathfest 80, May 17 2019, Northeastern University, Boston, MA. Modified Gravity • Modifications of gravity in most cases involve adding new fields. • Modifications of GR or adding new fields are needs to solve well known problems in cosmology, such as adding an inflaton, curvaton, quintessence, or F( R) gravity (equivalent to φR+ f(φ) ) or as in Hordinski model using scalar with higher safe derivatives. • In some modified theories utilize breaking diffeomorphism invariance such as in unimodular gravity, or Horava‐Lifschitz gravity Dark Matter • Various new particles and interactions are proposed to account for the missing mostly non‐baryonic matter in the universe. • Examples: Supersymmetric neutralino, axions, WIMP, dilaton, • Lack of direct evidence for dark matter made some physicists to propose modification of GR at large scales. • Most modifications of GR are made to solve one problem at a time, and do not address solving the problems simultaneously. Scale factor for metric • GR is not invariant under scale transformations of the metric • Newton constant will be redefined. If we take Ω(x) then it will get kinetic term. It is related to determinant of metric. • Unimodular gravity assumes |det(g)|=1 breaking diffeomorphism Invariance. Scale factor • In string theory the metric is accompanied by a dilaton and axionin the form of antisymmetric tensor. New degrees of freedom. • How can one isolate physics of scaling factor? • Let Then it is scale invariant under This imply Mimetic gravity (with S. Mukhanov) • The system ( has 11 components subject to the constraint leaving 10 degrees, same as GR.
    [Show full text]
  • Non-Commutative Geometry, Non-Associative Geometry and the Standard Model of Particle Physics
    Non-commutative geometry, non-associative geometry and the standard model of particle physics Latham Boyle and Shane Farnsworth Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada Received 1 October 2014 Accepted for publication 28 October 2014 Published 10 December 2014 New Journal of Physics 16 (2014) 123027 doi:10.1088/1367-2630/16/12/123027 Abstract Connes’ notion of non-commutative geometry (NCG) generalizes Riemannian geometry and yields a striking reinterepretation of the standard model of particle physics, coupled to Einstein gravity. We suggest a simple reformulation with two key mathematical advantages: (i) it unifies many of the traditional NCG axioms into a single one; and (ii) it immediately generalizes from non-com- mutative to non-associative geometry. Remarkably, it also resolves a long- standing problem plaguing the NCG construction of the standard model, by precisely eliminating from the action the collection of seven unwanted terms that previously had to be removed by an extra, non-geometric, assumption. With this problem solved, the NCG algorithm for constructing the standard model action is tighter and more explanatory than the traditional one based on effective field theory. Keywords: non-commutative geometry, non-associative geometry, standard model of particle physics Introduction Since the early 1980s, Connes and others have been developing the subject of non-commutative geometry (NCG) [1, 2]. Its mathematical interest stems from the fact that it provides a natural generalization of Riemannian geometry (much as Riemannian geometry, in turn, provides a natural generalization of Euclidean geometry). Its physical interest stems from the fact that it Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence.
    [Show full text]
  • Unification of Gauge and Gravity Chern-Simons Theories in 3
    Unification of Gauge and Gravity Chern-Simons Theories in 3-D Space time Chireen A. Saghir, Laurence W. Shamseddine Physics Department, American University of Beirut, Lebanon Abstract Chamseddine and Mukhanov showed that gravity and gauge theories could be unified in one geometric construction provided that a metricity condition is imposed on the vielbein. In this paper we are going to show that by enlarging the gauge group we are able to unify Chern-Simons gauge theory and Chern-Simons gravity in 3-D space-time. Such unification leads to the quantization of the coefficients for both Chern-Simons terms for compact groups but not for non-compact groups. Moreover, it leads to a topological invariant quantity of the 3 dimensional space-time manifold on which they are defined. arXiv:1703.08237v3 [hep-th] 2 Jul 2017 1 Introduction Topological Field Theories (TFTs) are metric independent theories that de- fine topological invariants of the manifold M. In general, we can distinguish between a topological field theory of Schwarz type and of Witten or cohomo- logical type. In Schwarz type theories the action is explicitly independent on the metric δS =0 (1) δgµν Examples of such theories are Chern-Simons theories and BF theories. The other type is Witten type topological field theories like the Donaldson-Witten theory which was formulated by Witten in 1988 [1] and is used to compute Donaldson invariant. In a ground breaking paper [2], Witten (1989) showed that Chern-Simon gauge theories provide a physical description of a wide class of invariants of 3-manifolds and of knots and links in this manifold.
    [Show full text]
  • Mimetic Horava Gravity and Surface Terms
    Mimetic Horava Gravity and Surface terms O. Malaeb, C. Saghir Physics Department, American University of Beirut, Lebanon Abstract We consider mimetic Horava gravity, where the scalar field of mimetic gravity was used in the construction of diffeomorphism in- variant models reducing to Horava gravity in the synchronous gauge. It will be shown that the surface terms resulting from the variation of the action constructed will cancel out; therefore, there is no need for the addition of GibbonsHawkingYork boundary term. The result- ing surface terms contain higher order space derivatives and no higher order time derivatives. arXiv:2005.02469v1 [hep-th] 5 May 2020 1 General relativity GR is a classical theory describing gravity through Ein- stein field equation. It has proven success through several phenomena: the perihelion of mercury, prediction of black holes, gravitational waves... Al- though of the huge success that GR has achieved, still it is unable to explain some points: dark matter, singularities like the big bang and the black holes... This issue has pushed physicists to modify GR in several ways. Some mod- ified theories of gravity have aimed to quantize GR as a way to explain Big bang singularities or the black holes. Approaches to quantum gravity can be classified into two groups [1].The first group starts from the classical theory of gravity and then applies the quantization steps. The covariant quantum gravity is a good example, where one starts from the path integral of the GR action and then applies the perturbation procedures for the metric around a background one. The resulting theory has been a non renormalizable one upon extending it to higher energies.
    [Show full text]
  • Noncommutative Gauge Theories and Gravity
    Noncommutative Gauge Theories and Gravity G. Manolakos∗ Physics Department, National Technical University, GR-15780 Athens, Greece E-mail: [email protected] P. Manousselis Physics Department, National Technical University, GR-15780 Athens, Greece E-mail: [email protected] G. Zoupanos Physics Department, National Technical University, GR-15780 Athens, Greece Institute of Theoretical Physics, D-69120 Heidelberg, Germany Max-Planck Institut für Physik, Fohringer Ring 6, D-80805 Munchen, Germany Laboratoire d’ Annecy de Physique Theorique, Annecy, France E-mail: [email protected] First, we briefly review the description of gravity theories as gauge theories in three and four dimensions. Specifically, we recall the procedure in which the results of General Relativity in three and four dimensions are recovered in a gauge-theoretic approach. Also, the procedure is applied for the case of the Weyl gravity, too. Then, after reminding briefly the formulation of gauge theories on noncommutative spaces, we review our most recent works in which gravity models are constructed as gauge theories on noncommutative spaces. arXiv:1907.06280v1 [hep-th] 14 Jul 2019 Corfu Summer Institute 2018 "School and Workshops on Elementary Particle Physics and Gravity" (CORFU2018) 31 August - 28 September, 2018 Corfu, Greece ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). https://pos.sissa.it/ Noncommutatve gravity G. Manolakos 1. Introduction Three out of four interactions of nature are grouped together under a common description by the Standard Model in which they are described by gauge theories.
    [Show full text]
  • Reminiscences of My Work with Richard Lewis Arnowitt
    Reminiscences of my work with Richard Lewis Arnowitt Pran Nath∗ Department of Physics, Northeastern University, Boston, MA 02115, USA This article contains reminiscences of the collaborative work that Richard Arnowitt and I did together which stretched over many years and encompasses several areas of particle theory. The article is an extended version of my talk at the Memorial Symposium in honor of Richard Arnowitt at Texas A&M, College Station, Texas, September 19-20, 2014. My collaboration with Richard Arnowitt (1928-2014)1 to constrain the parameters of the effective Lagrangian. started soon after I arrived at Northeastern University in The effective Lagrangian was a deduction from the fol- 1966 and continued for many years. In this brief article lowing set of conditions: (i) single particle saturation in on the reminiscences of my work with Dick I review some computation of T-products of currents, (ii) Lorentz in- of the more salient parts of our collaborative work which variance, (iii) “spectator” approximation, and (iv) local- includes effective Lagrangians, current algebra, scale in- ity which implies a smoothness assumption on the ver- variance and its breakdown, the U(1) problem, formu- tices. The above assumptions lead us to the conclusion lation of the first local supersymmetry and the develop- that the simplest way to achieve these constraints is via ment of supergravity grand unification in collaboration an effective Lagrangian which for T-products of three of Ali Chamseddine, and its applications to the search currents requires writing cubic interactions involving π,ρ for supersymmetry. and A1 fields and allowing for no derivatives in the first -order formalism and up to one-derivative in the second order formalism.
    [Show full text]