A Curvature Principle for the Interaction Between Universes
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Jhep01(2020)007
Published for SISSA by Springer Received: March 27, 2019 Revised: November 15, 2019 Accepted: December 9, 2019 Published: January 2, 2020 Deformed graded Poisson structures, generalized geometry and supergravity JHEP01(2020)007 Eugenia Boffo and Peter Schupp Jacobs University Bremen, Campus Ring 1, 28759 Bremen, Germany E-mail: [email protected], [email protected] Abstract: In recent years, a close connection between supergravity, string effective ac- tions and generalized geometry has been discovered that typically involves a doubling of geometric structures. We investigate this relation from the point of view of graded ge- ometry, introducing an approach based on deformations of graded Poisson structures and derive the corresponding gravity actions. We consider in particular natural deformations of the 2-graded symplectic manifold T ∗[2]T [1]M that are based on a metric g, a closed Neveu-Schwarz 3-form H (locally expressed in terms of a Kalb-Ramond 2-form B) and a scalar dilaton φ. The derived bracket formalism relates this structure to the generalized differential geometry of a Courant algebroid, which has the appropriate stringy symme- tries, and yields a connection with non-trivial curvature and torsion on the generalized “doubled” tangent bundle E =∼ TM ⊕ T ∗M. Projecting onto TM with the help of a natural non-isotropic splitting of E, we obtain a connection and curvature invariants that reproduce the NS-NS sector of supergravity in 10 dimensions. Further results include a fully generalized Dorfman bracket, a generalized Lie bracket and new formulas for torsion and curvature tensors associated to generalized tangent bundles. -
Geometric Horizons ∗ Alan A
Physics Letters B 771 (2017) 131–135 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Geometric horizons ∗ Alan A. Coley a, David D. McNutt b, , Andrey A. Shoom c a Department of Mathematics and Statistics, Dalhousie University, Halifax, Nova Scotia, B3H 3J5, Canada b Faculty of Science and Technology, University of Stavanger, N-4036 Stavanger, Norway c Department of Mathematics and Statistics, Memorial University, St. John’s, Newfoundland and Labrador, A1C 5S7, Canada a r t i c l e i n f o a b s t r a c t Article history: We discuss black hole spacetimes with a geometrically defined quasi-local horizon on which the Received 21 February 2017 curvature tensor is algebraically special relative to the alignment classification. Based on many examples Accepted 2 May 2017 and analytical results, we conjecture that a spacetime horizon is always more algebraically special (in Available online 19 May 2017 all of the orders of specialization) than other regions of spacetime. Using recent results in invariant Editor: M. Trodden theory, such geometric black hole horizons can be identified by the alignment type II or D discriminant conditions in terms of scalar curvature invariants, which are not dependent on spacetime foliations. The above conjecture is, in fact, a suite of conjectures (isolated vs dynamical horizon; four vs higher dimensions; zeroth order invariants vs higher order differential invariants). However, we are particularly interested in applications in four dimensions and especially the location of a black hole in numerical computations. © 2017 The Author(s). Published by Elsevier B.V. -
WHAT IS Q-CURVATURE? 1. Introduction Throughout His Distinguished Research Career, Tom Branson Was Fascinated by Con- Formal
WHAT IS Q-CURVATURE? S.-Y. ALICE CHANG, MICHAEL EASTWOOD, BENT ØRSTED, AND PAUL C. YANG In memory of Thomas P. Branson (1953–2006). Abstract. Branson’s Q-curvature is now recognized as a fundamental quantity in conformal geometry. We outline its construction and present its basic properties. 1. Introduction Throughout his distinguished research career, Tom Branson was fascinated by con- formal differential geometry and made several substantial contributions to this field. There is no doubt, however, that his favorite was the notion of Q-curvature. In this article we outline the construction and basic properties of Branson’s Q-curvature. As a Riemannian invariant, defined on even-dimensional manifolds, there is apparently nothing special about Q. On a surface Q is essentially the Gaussian curvature. In 4 dimensions there is a simple but unrevealing formula (4.1) for Q. In 6 dimensions an explicit formula is already quite difficult. What is truly remarkable, however, is how Q interacts with conformal, i.e. angle-preserving, transformations. We shall suppose that the reader is familiar with the basics of Riemannian differ- ential geometry but a few remarks on notation are in order. Sometimes, we shall write gab for a metric and ∇a for the corresponding connection. Let us write Rab and R for the Ricci and scalar curvatures, respectively. We shall use the metric to ‘raise and lower’ indices in the usual fashion and adopt the summation convention whereby one implicitly sums over repeated indices. Using these conventions, the Laplacian is ab a the differential operator ∆ ≡ g ∇a∇b = ∇ ∇a. A conformal structure on a smooth manifold is a metric defined only up to smoothly varying scale. -
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. -
Bounding Curvature by Modifying General Relativity
Bounding Curvature by Modifying General Relativity David R. Fiske Department of Physics, University of Maryland, College Park, MD 20742-4111 and Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Greenbelt, MD 20771 The existence of singularities is one the most surprising predictions of Einstein's general relativity. I review some work that tries to eliminate singularities in the theory by forcibly bounding curvature scalars. Although the authors of the original papers sought a possible effective theory in high curvature regions that might help develop either quantum gravity or string theory, the technical difficulties of calculating field equations within the modified theories is quite formidable and likely makes it impossible to gain any analytic insights. I also briefly discuss possible applications of these methods to numerical relativity. I. INTRODUCTION General relativity admits solutions that include essential, physical singularities. Although these singularities likely indicate a break down of the classical theory, the \next" theory has not yet been fully developed. Given the lack of a non-perturbative theory describing regions of high curvature, some authors have been motivated to examine corrections to general relativity that bound certain curvature invariants to values less than appropriate powers of the Planck length, both in the context of cosmologies [1, 2] and in the context of low-dimensional black holes [3]. This work was motivated by the hope that some features of the more fundamental theory can be found by such considerations and by the hope that predictions of this ad hoc theory might help in the formulation of the fundamental theory. The problem of singular solutions is also of interest from a less fundamental point of view. -
M-Eigenvalues of the Riemann Curvature Tensor at That Point Are All Positive
M-eigenvalues of The Riemann Curvature Tensor ∗ Hua Xianga† Liqun Qib‡ Yimin Weic§ a School of Mathematics and Statistics, Wuhan University, Wuhan, 430072, P.R. China b Department of Applied Mathematics, The Hong Kong Polytechnic University, Hong Kong c School of Mathematical Sciences and Shanghai Key Laboratory of Contemporary Applied Mathematics, Fudan University, Shanghai, 200433, P. R. of China August 31, 2018 Abstract The Riemann curvature tensor is a central mathematical tool in Ein- stein’s theory of general relativity. Its related eigenproblem plays an im- portant role in mathematics and physics. We extend M-eigenvalues for the elasticity tensor to the Riemann curvature tensor. The definition of M-eigenproblem of the Riemann curvature tensor is introduced from the minimization of an associated function. The M-eigenvalues of the Rie- mann curvature tensor always exist and are real. They are invariants of the Riemann curvature tensor. The associated function of the Rie- mann curvature tensor is always positive at a point if and only if the M-eigenvalues of the Riemann curvature tensor are all positive at that point. We investigate the M-eigenvalues for the simple cases, such as the 2D case, the 3D case, the constant curvature and the Schwarzschild so- lution, and all the calculated M-eigenvalues are related to the curvature invariants. Keywords. Eigenproblem, M-eigenvalue, Curvature tensor, Riemann ten- sor, Ricci tensor, Elasticity tensor, Schwarzschild solution, Invariant. 1 Introduction arXiv:1802.10248v6 [math.DG] 30 Aug 2018 The eigenproblem of tensor is an very important topic theoretically and practi- cally. In [9, 10, 18, 24], the elasticity tensor is investigated, including the strong ellipticity, the positive definiteness, the M-eigenvalues, etc. -
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. -
The Riemann Curvature Tensor
The Riemann Curvature Tensor Jennifer Cox May 6, 2019 Project Advisor: Dr. Jonathan Walters Abstract A tensor is a mathematical object that has applications in areas including physics, psychology, and artificial intelligence. The Riemann curvature tensor is a tool used to describe the curvature of n-dimensional spaces such as Riemannian manifolds in the field of differential geometry. The Riemann tensor plays an important role in the theories of general relativity and gravity as well as the curvature of spacetime. This paper will provide an overview of tensors and tensor operations. In particular, properties of the Riemann tensor will be examined. Calculations of the Riemann tensor for several two and three dimensional surfaces such as that of the sphere and torus will be demonstrated. The relationship between the Riemann tensor for the 2-sphere and 3-sphere will be studied, and it will be shown that these tensors satisfy the general equation of the Riemann tensor for an n-dimensional sphere. The connection between the Gaussian curvature and the Riemann curvature tensor will also be shown using Gauss's Theorem Egregium. Keywords: tensor, tensors, Riemann tensor, Riemann curvature tensor, curvature 1 Introduction Coordinate systems are the basis of analytic geometry and are necessary to solve geomet- ric problems using algebraic methods. The introduction of coordinate systems allowed for the blending of algebraic and geometric methods that eventually led to the development of calculus. Reliance on coordinate systems, however, can result in a loss of geometric insight and an unnecessary increase in the complexity of relevant expressions. Tensor calculus is an effective framework that will avoid the cons of relying on coordinate systems. -
THE CURVATURE INVARIANT of a HILBERT MODULE OVER C[Z 1
THE CURVATURE INVARIANT OF A HILBERT MODULE OVER C[z1; : : : ; zd] William Arveson Department of Mathematics University of California Berkeley CA 94720, USA Abstract. A notion of curvature is introduced in multivariable operator theory, that is, for commuting d tuples of operators acting on a common Hilbert space whose \rank" is finite in an appropriate sense. The curvature invariant is a real number in the interval [0; r] where r is the rank, and for good reason it is desireable to know its value. For example, there are significant and concrete consequences when it assumes either of the two extreme values 0 or r. In the few simple cases where it can be calculated directly, it turns out to be an integer. This paper addresses the general problem of computing this invariant. Our main result is an operator-theoretic version of the Gauss-Bonnet-Chern for- mula of Riemannian geometry. The proof is based on an asymptotic formula which expresses the curvature of a Hilbert module as the trace of a certain self-adjoint operator. The Euler characteristic of a Hilbert module is defined in terms of the algebraic structure of an associated finitely generated module over the algebra of complex polynomials C[z1; : : : ; zd], and the result is that these two numbers are the same for graded Hilbert modules. Thus the curvature of such a Hilbert module is an integer; and since there are standard tools for computing the Euler characteristic of finitely generated modules over polynomial rings, the problem of computing the curvature can be considered solved in these cases. -
Differential Geometry Lecture 18: Curvature
Differential geometry Lecture 18: Curvature David Lindemann University of Hamburg Department of Mathematics Analysis and Differential Geometry & RTG 1670 14. July 2020 David Lindemann DG lecture 18 14. July 2020 1 / 31 1 Riemann curvature tensor 2 Sectional curvature 3 Ricci curvature 4 Scalar curvature David Lindemann DG lecture 18 14. July 2020 2 / 31 Recap of lecture 17: defined geodesics in pseudo-Riemannian manifolds as curves with parallel velocity viewed geodesics as projections of integral curves of a vector field G 2 X(TM) with local flow called geodesic flow obtained uniqueness and existence properties of geodesics constructed the exponential map exp : V ! M, V neighbourhood of the zero-section in TM ! M showed that geodesics with compact domain are precisely the critical points of the energy functional used the exponential map to construct Riemannian normal coordinates, studied local forms of the metric and the Christoffel symbols in such coordinates discussed the Hopf-Rinow Theorem erratum: codomain of (x; v) as local integral curve of G is d'(TU), not TM David Lindemann DG lecture 18 14. July 2020 3 / 31 Riemann curvature tensor Intuitively, a meaningful definition of the term \curvature" for 3 a smooth surface in R , written locally as a graph of a smooth 2 function f : U ⊂ R ! R, should involve the second partial derivatives of f at each point. How can we find a coordinate- 3 free definition of curvature not just for surfaces in R , which are automatically Riemannian manifolds by restricting h·; ·i, but for all pseudo-Riemannian manifolds? Definition Let (M; g) be a pseudo-Riemannian manifold with Levi-Civita connection r. -
Symbols 1-Form, 10 4-Acceleration, 184 4-Force, 115 4-Momentum, 116
Index Symbols B 1-form, 10 Betti number, 589 4-acceleration, 184 Bianchi type-I models, 448 4-force, 115 Bianchi’s differential identities, 60 4-momentum, 116 complex valued, 532–533 total, 122 consequences of in Newman-Penrose 4-velocity, 114 formalism, 549–551 first contracted, 63 second contracted, 63 A bicharacteristic curves, 620 acceleration big crunch, 441 4-acceleration, 184 big-bang cosmological model, 438, 449 Newtonian, 74 Birkhoff’s theorem, 271 action function or functional bivector space, 486 (see also Lagrangian), 594, 598 black hole, 364–433 ADM action, 606 Bondi-Metzner-Sachs group, 240 affine parameter, 77, 79 boost, 110 alternating operation, antisymmetriza- Born-Infeld (or tachyonic) scalar field, tion, 27 467–471 angle field, 44 Boyer-Lindquist coordinate chart, 334, anisotropic fluid, 218–220, 276 399 collapse, 424–431 Brinkman-Robinson-Trautman met- ric, 514 anti-de Sitter space-time, 195, 644, Buchdahl inequality, 262 663–664 bugle, 69 anti-self-dual, 671 antisymmetric oriented tensor, 49 C antisymmetric tensor, 28 canonical energy-momentum-stress ten- antisymmetrization, 27 sor, 119 arc length parameter, 81 canonical or normal forms, 510 arc separation function, 85 Cartesian chart, 44, 68 arc separation parameter, 77 Casimir effect, 638 Arnowitt-Deser-Misner action integral, Cauchy horizon, 403, 416 606 Cauchy problem, 207 atlas, 3 Cauchy-Kowalewski theorem, 207 complete, 3 causal cone, 108 maximal, 3 causal space-time, 663 698 Index 699 causality violation, 663 contravariant index, 51 characteristic hypersurface, 623 contravariant -
CURVATURE INVARIANTS, KILLING VECTOR FIELDS, CONNECTIONS and COHOMOGENEITY a Classical Result of IM Singer
PROCEEDINGS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 137, Number 3, March 2009, Pages 1069–1072 S 0002-9939(08)09669-X Article electronically published on October 2, 2008 CURVATURE INVARIANTS, KILLING VECTOR FIELDS, CONNECTIONS AND COHOMOGENEITY SERGIO CONSOLE AND CARLOS OLMOS (Communicated by Jon G. Wolfson) Abstract. A direct, bundle-theoretic method for defining and extending local isometries out of curvature data is developed. As a by-product, conceptual direct proofs of a classical result of Singer and a recent result of the authors are derived. A classical result of I. M. Singer [11] states that a Riemannian manifold is locally homogeneous if and only if its Riemannian curvature tensor together with its co- variant derivatives up to some index k + 1 are independent of the point (the integer k is called the Singer invariant). More precisely, Theorem 1 (Singer [11]). Let M be a Riemannian manifold. Then M is a locally homogeneous if and only if for any p, q ∈ M there is a linear isometry F : TpM → TqM such that ∗ s s F ∇ Rq = ∇ Rp, for any s ≤ k +1. An alternate proof with a more direct approach was given in [8]. Out of the curvature tensor and its covariant derivatives one can construct scalar invariants, like for instance the scalar curvature. In general, any polynomial func- tion in the components of the curvature tensor and its covariant derivatives which does not depend on the choice of the orthonormal basis at the tangent space of each point is a scalar Weyl invariant or a scalar curvature invariant.BytheWeyl theory of invariants, a scalar Weyl invariant is a linear combination of complete m m 0 traces of tensors ∇ 1 R, ...∇ R, (m1,...ms ≥ 0, ∇ R = R).