The Classification of Three-Dimensional Lie Algebras Allegra Fowler-Wright Mathematics Institute
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University of Groningen the Bianchi Classification of Maximal D = 8 Gauged Supergravities Bergshoeff, Eric; Gran, Ulf; Linares
University of Groningen The Bianchi classification of maximal D = 8 gauged supergravities Bergshoeff, Eric; Gran, Ulf; Linares, Román; Nielsen, Mikkel; Ortín, Tomás; Roest, Diederik Published in: Classical and Quantum Gravity IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2003 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Bergshoeff, E., Gran, U., Linares, R., Nielsen, M., Ortín, T., & Roest, D. (2003). The Bianchi classification of maximal D = 8 gauged supergravities. Classical and Quantum Gravity, 20, 3997-4014. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 24-09-2021 INSTITUTE OF PHYSICS PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum Grav. 20 (2003) 3997–4014 -
Anisotropic, Nonsingular Early Universe Model Leading to a Realistic Cosmology
This is a repository copy of Anisotropic, nonsingular early universe model leading to a realistic cosmology. White Rose Research Online URL for this paper: https://eprints.whiterose.ac.uk/85582/ Version: Accepted Version Article: Dechant, Pierre-Philippe orcid.org/0000-0002-4694-4010, Lasenby, Anthony and Hobson, Michael (2009) Anisotropic, nonsingular early universe model leading to a realistic cosmology. Physical Review D. 043524. ISSN 1550-2368 https://doi.org/10.1103/PhysRevD.79.043524 Reuse Items deposited in White Rose Research Online are protected by copyright, with all rights reserved unless indicated otherwise. They may be downloaded and/or printed for private study, or other acts as permitted by national copyright laws. The publisher or other rights holders may allow further reproduction and re-use of the full text version. This is indicated by the licence information on the White Rose Research Online record for the item. Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ An anisotropic, non-singular early universe model leading to a realistic cosmology † ‡ Pierre-Philippe Dechant,∗ Anthony N. Lasenby, and Michael P. Hobson Astrophysics Group, Cavendish Laboratory, J J Thomson Avenue, University of Cambridge, CB3 0HE, UK (Dated: February 18, 2013) Abstract We present a novel cosmological model in which scalar field matter in a biaxial Bianchi IX geometry leads to a non-singular ‘pancaking’ solution: the hypersurface volume goes to zero instantaneously at the ‘Big Bang’, but all physical quantities, such as curvature invariants and the matter energy density remain finite, and continue smoothly through the Big Bang. -
Ring (Mathematics) 1 Ring (Mathematics)
Ring (mathematics) 1 Ring (mathematics) In mathematics, a ring is an algebraic structure consisting of a set together with two binary operations usually called addition and multiplication, where the set is an abelian group under addition (called the additive group of the ring) and a monoid under multiplication such that multiplication distributes over addition.a[›] In other words the ring axioms require that addition is commutative, addition and multiplication are associative, multiplication distributes over addition, each element in the set has an additive inverse, and there exists an additive identity. One of the most common examples of a ring is the set of integers endowed with its natural operations of addition and multiplication. Certain variations of the definition of a ring are sometimes employed, and these are outlined later in the article. Polynomials, represented here by curves, form a ring under addition The branch of mathematics that studies rings is known and multiplication. as ring theory. Ring theorists study properties common to both familiar mathematical structures such as integers and polynomials, and to the many less well-known mathematical structures that also satisfy the axioms of ring theory. The ubiquity of rings makes them a central organizing principle of contemporary mathematics.[1] Ring theory may be used to understand fundamental physical laws, such as those underlying special relativity and symmetry phenomena in molecular chemistry. The concept of a ring first arose from attempts to prove Fermat's last theorem, starting with Richard Dedekind in the 1880s. After contributions from other fields, mainly number theory, the ring notion was generalized and firmly established during the 1920s by Emmy Noether and Wolfgang Krull.[2] Modern ring theory—a very active mathematical discipline—studies rings in their own right. -
Classification of Six-Dimensional Leibniz Algebras ${\Mathcal E} 3
Classification of six-dimensional Leibniz algebras E3 Ladislav Hlavatý∗ Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Czech Republic May 11, 2020 Abstract Leibniz algebras En were introduced as algebraic structure under- lying U-duality. Algebras E3 derived from Bianchi three-dimensional Lie algebras are classified here. Two types of algebras are obtained: Six-dimensional Lie algebras that can be considered extension of semi- Abelian four-dimensional Drinfel’d double and unique extensions of non-Abelian Bianchi algebras. For all of the algebras explicit forms of generalized frame fields are given. 1 Introduction arXiv:2003.06164v4 [hep-th] 8 May 2020 Extensions of Poisson–Lie T-dualities to non-perturbative symmetries of string theories are so called U-dualities (for review see e.g.[1]). Algebraic structures underlying U-duality were suggested in [2] and [3] as Leibniz algebras En obtained as extensions of n-dimensional Lie algebra defining non-symmetric product ◦ in [n + n(n − 1)/2]-dimensional vector space1 that satisfies Leibniz identity X ◦ (Y ◦ Z))=(X ◦ Y ) ◦ Z + Y ◦ (X ◦ Z). (1) ∗hlavaty@fjfi.cvut.cz 1for n ≤ 4 1 In those papers examples of these Leibniz algebras derived from two-dimensional and four-dimensional Lie algebras are given. Goal of the present note is to write down all algebras that can be derived from three dimensional Lie alge- bras whose classification given by Bianchi is well known. a1a2 a2a1 a1a2 Namely, let (Ta, T ), a, a1, a2 ∈ 1,...,n, T = −T is a basis of [n + n(n − 1)/2]-dimensional vector space. -
The Bianchi Classification in the Schü
P1: FLT General Relativity and Gravitation (GERG) PP736-GERG-459711 February 7, 2003 18:36 Style file version May 27, 2002 General Relativity and Gravitation, Vol. 35, No. 3, March 2003 (C 2003) The Bianchi Classification in the Sch¨ucking-Behr Approach1 A. Krasi´nski,2 Christoph G. Behr,3 Engelbert Sch¨ucking,4 Frank B. Estabrook,5 Hugo D. Wahlquist,6 George F. R. Ellis,7 Robert Jantzen,8 and Wolfgang Kundt9 Received July 15, 2002 The historical development of the Bianchi classification of homogeneous cosmological models is described with special emphasis on the contributions by Sch¨ucking and Behr. KEY WORDS: Bianchi models; Lie algebra; cosmology.3 1. INTRODUCTION Today, the Bianchi classification of 3-dimensional Lie algebras is no longer pre- sented by the original Bianchi method [4]. The now-common approach is usually credited to C. G. Behr, but one never sees any reference to a paper by him. Tracing the references back in time one is most often led either to the paper by Ellis and 1 Written collectively as “Golden Oldie XXX; each author is signed under his segment. 2 Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland; e-mail: [email protected] 3 Eduard-Steinle-Strae 19, 70 619 Stuttgart, Germany. 4 29 Washington Square West, New York, NY 10011, USA; e-mail: [email protected] 5 Jet Propulsion Laboratory, Mail Stop 169-327, 4800 Oak Grove Drive, Pasadena, California 91109, USA 6 Jet Propulsion Laboratory, Mail Stop 169-327, 4800 Oak Grove Drive, Pasadena, California 91109, USA; e-mail: [email protected] 7 Mathematics -
Dynamics of Bianchi Spacetimes
Dynamics of Bianchi spacetimes Fran¸coisB´eguin Universit´eParis-Sud 11 & ENS´ Febuary 9th, 2012 Raisons d'^etre: I natural finite dimensional class of spacetimes ; I BKL conjecture : generic spacetimes \behave like" spatially homogeneous spacetimes close to their initial singularity. Bianchi cosmological models : presentation Bianchi spacetimes are spatially homogeneous (not isotropic) cosmological models. Bianchi cosmological models : presentation Bianchi spacetimes are spatially homogeneous (not isotropic) cosmological models. Raisons d'^etre: I natural finite dimensional class of spacetimes ; I BKL conjecture : generic spacetimes \behave like" spatially homogeneous spacetimes close to their initial singularity. I A Bianchi spacetime is a spacetime (M; g) with 2 M ' I × G g = −dt + ht where I = (t−; t+) ⊂ R, G is 3-dimensional Lie group, ht is a left-invariant riemannian metric on G. I A Bianchi spacetime amounts to a one-parameter family of left-invariant metrics (ht )t2I on a 3-dimensional Lie group G. Bianchi cosmological models : definitions I A Bianchi spacetime is a globally hyperbolic spatially homogeneous (but not isotropic) spacetime. I A Bianchi spacetime amounts to a one-parameter family of left-invariant metrics (ht )t2I on a 3-dimensional Lie group G. Bianchi cosmological models : definitions I A Bianchi spacetime is a globally hyperbolic spatially homogeneous (but not isotropic) spacetime. I A Bianchi spacetime is a spacetime (M; g) with 2 M ' I × G g = −dt + ht where I = (t−; t+) ⊂ R, G is 3-dimensional Lie group, ht is a left-invariant riemannian metric on G. Bianchi cosmological models : definitions I A Bianchi spacetime is a globally hyperbolic spatially homogeneous (but not isotropic) spacetime. -
On the Energy of Homogeneous Cosmologies
On the energy of homogeneous cosmologies James M. Nester Department of Physics, National Central University, Chungli 32054, Taiwan Department of Physics and Institute of Astronomy, National Central University, Chungli 32054, Taiwan. [email protected] Lau Loi So1 Department of Physics, National Central University, Chungli 32054, Taiwan [email protected] T. Vargas2 Instituto de Fisica Teorica, Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 Sao Paulo SP, Brazil. [email protected] Received ; accepted 1present address:Department of physics, Tamkang University, Tamsui 251, Taiwan. 2present address:Department of Physics, National Central University, Chungli 32054, Tai- wan. – 2 – ABSTRACT We investigate the quasi-local energy of all the homogeneous cosmological models. More specifically using the standard natural prescription we find the quasi-local energy-momentum for a large class of gravity theories with a tetrad description for all 9 Bianchi types with general gravitational sources. Using ideas related to a Hamiltonian approach we find that, with homogeneous boundary conditions, the quasi-local energy vanishes for all regions in all Bianchi class A models, and it does not vanish for any class B model. This is so not only for Einstein’s general relativity but, moreover, for the whole 3-parameter class of tetrad-teleparallel theories. For the physically favored one parameter subclass, which includes the teleparallel equivalent of Einstein’s theory as an important special case, the quasi-local energy for all class B models is positive. PACS 04.20.Cv, 04.20.Fy, 98.80.Jk 2006-12-19jmn 1. Introduction Energy has been one of the most useful physical concepts, no less so in gravitating systems—one need only recall its utility in the Newtonian Kepler problem. -
Rotating Dust Solutions of Einstein's Equations with 3-Dimensional Symmetry Groups. I. Two Killing Fields Spanned on U and W
Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on ua and wa Andrzej Krasin´ski N. Copernicus Astronomical Center and College of Science, Polish Academy of Sciences, Bartycka 18, 00 716 Warszawa, Poland ~Received 14 May 1997; accepted for publication 7 July 1997! For a rotating dust with a 3-dimensional symmetry group all possible metric forms can be classified and, within each class, explicitly written out. This is made possible by the formalism of Pleban´ski based on the Darboux theorem. In the resulting coordinates, the Killing vector fields ~if any exist! assume a special form. Each Killing vector field may be either spanned on the fields of velocity and rotation or linearly independent of them. By considering all such cases one arrives at the classification. With respect to the structures of the groups, this is just the Bianchi classification, but with all possible orientations of the orbits taken into account. In this paper, which is part 1 of a 3-part series, all solutions are considered for which two Killing fields are spanned on velocity and rotation. The solutions of Lanczos and Go¨del are identified as special cases, and their new invariant definitions are provided. In addition, a new invariant definition is given of the Ozsvath class III solution. © 1998 American Institute of Physics. @S0022-2488~97!03112-5# I. INTRODUCTION AND SUMMARY The theorem of Darboux presented in Sec. II allows one to introduce invariantly defined coordinates in which the velocity field of a fluid ~not assumed to be perfect! acquires a ‘‘canoni- cal’’ form. -
Zaneville Testimonial Excerpts and Reminisces
Greetings Dean & Mrs. “Jim” Fonseca, Barbara & Abe Osofsky, Surender Jain, Pramod Kanwar, Sergio López-Permouth, Dinh Van Huynh& other members of the Ohio Ring “Gang,” conference speakers & guests, Molly & I are deeply grateful you for your warm and hospitable welcome. Flying out of Newark New Jersey is always an iffy proposition due to the heavy air traffic--predictably we were detained there for several hours, and arrived late. Probably not coincidently, Barbara & Abe Osofsky, Christian Clomp, and José Luis Gómez Pardo were on the same plane! So we were happy to see Nguyen Viet Dung, Dinh Van Huynh, and Pramod Kanwar at the Columbus airport. Pramod drove us to the Comfort Inn in Zanesville, while Dinh drove Barbara and Abe, and José Luis & Christian went with Nguyen. We were hungry when we arrived in Zanesville at the Comfort Inn, Surender and Dinh pointed to nearby restaurants So, accompanied by Barbara & Abe Osofsky and Peter Vámos, we had an eleventh hour snack at Steak and Shake. (Since Jose Luis had to speak first at the conference, he wouldn’t join us.) Molly & I were so pleased Steak and Shake’s 50’s décor and music that we returned the next morning for breakfast. I remember hearing“You Are So Beautiful,” “Isn’t this Romantic,” and other nostalgia-inducing songs. Rashly, I tried to sing a line from those two at the Banquet, but fell way short of Joe Cocker’s rendition of the former. (Cocker’s is free to hear on You Tube on the Web.) Zanesville We also enjoyed other aspects of Zanesville and its long history. -
Scientific Workplace· • Mathematical Word Processing • LATEX Typesetting Scientific Word· • Computer Algebra
Scientific WorkPlace· • Mathematical Word Processing • LATEX Typesetting Scientific Word· • Computer Algebra (-l +lr,:znt:,-1 + 2r) ,..,_' '"""""Ke~r~UrN- r o~ r PooiliorK 1.931'J1 Po6'lf ·1.:1l26!.1 Pod:iDnZ 3.881()2 UfW'IICI(JI)( -2.801~ ""'"""U!NecteoZ l!l!iS'11 v~ 0.7815399 Animated plots ln spherical coordln1tes > To make an anlm.ted plot In spherical coordinates 1. Type an expression In thr.. variables . 2 WMh the Insertion poilt In the expression, choose Plot 3D The next exampfe shows a sphere that grows ftom radius 1 to .. Plot 3D Animated + Spherical The Gold Standard for Mathematical Publishing Scientific WorkPlace and Scientific Word Version 5.5 make writing, sharing, and doing mathematics easier. You compose and edit your documents directly on the screen, without having to think in a programming language. A click of a button allows you to typeset your documents in LAT£X. You choose to print with or without LATEX typesetting, or publish on the web. Scientific WorkPlace and Scientific Word enable both professionals and support staff to produce stunning books and articles. Also, the integrated computer algebra system in Scientific WorkPlace enables you to solve and plot equations, animate 20 and 30 plots, rotate, move, and fly through 3D plots, create 3D implicit plots, and more. MuPAD' Pro MuPAD Pro is an integrated and open mathematical problem solving environment for symbolic and numeric computing. Visit our website for details. cK.ichan SOFTWARE , I NC. Visit our website for free trial versions of all our products. www.mackichan.com/notices • Email: info@mac kichan.com • Toll free: 877-724-9673 It@\ A I M S \W ELEGRONIC EDITORIAL BOARD http://www.math.psu.edu/era/ Managing Editors: This electronic-only journal publishes research announcements (up to about 10 Keith Burns journal pages) of significant advances in all branches of mathematics. -
Joseph Wedderburn
Joseph Wedderburn Joseph Wedderburn Maclagan Henry (1882-1948) 02 februarie 1882 Născut Forfar , Angus , Scoţia 09 octombrie 1948 (cu vârsta 66) Decedat Princeton, New Jersey , Statele Unite ale Americii Reşedinţă Statele Unite ale Americii Cetăţenie American Naţionalitate Scoţian Domenii Matematician Instituţii Universitatea Princeton Alma Mater Universitatea din Edinburgh De doctorat George Chrystal Merrill Flood Doctoranzi Nathan Jacobson Ernst Snapper Cunoscut pentru Artin-Wedderburn teorema premii MacDougall-Brisbane Medalia de aur notabile Joseph Henry Maclagan Wedderburn (02 februarie 1882 Forfar, Angus , Scoţia - 9 octombrie 1948, Princeton, New Jersey ) a fost un matematician scoţian, care a predat la Universitatea Princeton pentru cea mai mare din cariera sa. Algebrist de prestigiu , el a dovedit că orice corp finit este comutativ , şi o parte a teoremei Artin-Wedderburn referitoare la algebre. De asemenea, el a lucrat in teoria grupurilor si algebra matricilor . Viaţa si opera Joseph Wedderburn a fost al zecelea din cei 14 copii ai medicului Alexander Wedderburn şi ai Ogilvie Anne. În 1898, el a intrat la Universitatea din Edinburgh . In 1903, el a publicat primele trei lucrari, a lucrat ca asistent la Laboratorul de Fizică a Universităţii, şi a obţinut o diplomă MA cu onoruri deosebite în matematică. A studiat apoi timp scurt la Universitatea din Leipzig şi Universitatea din Berlin, unde s-a întâlnit cu algebriştii Frobenius şi Schur. O Bursa Carnegie i-a permis să-şi petreacă anul universitar 1904-1905 la Universitatea din Chicago, unde a lucrat cu Oswald Veblen , EH Moore , şi cel mai important, Leonard Dickson , care avea să devină cel mai important algebrist american al acelor timpuri. -
University of Groningen the Bianchi Classification of Maximal D
CORE Metadata, citation and similar papers at core.ac.uk Provided by University of Groningen University of Groningen The Bianchi classification of maximal D = 8 gauged supergravities Bergshoeff, Eric; Gran, Ulf; Linares, Román; Nielsen, Mikkel; Ortín, Tomás; Roest, Diederik Published in: Classical and Quantum Gravity IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2003 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Bergshoeff, E., Gran, U., Linares, R., Nielsen, M., Ortín, T., & Roest, D. (2003). The Bianchi classification of maximal D = 8 gauged supergravities. Classical and Quantum Gravity, 20, 3997-4014. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 12-11-2019 INSTITUTE