The Maximum Modulus of a Trigonometric Trinomial
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Arxiv:1406.1948V2 [Math.GM] 18 Dec 2014 Hr = ∆ Where H Ouino 1 Is (1) of Solution the 1
Solution of Polynomial Equations with Nested Radicals Nikos Bagis Stenimahou 5 Edessa Pellas 58200, Greece [email protected] Abstract In this article we present solutions of arbitrary polynomial equations in nested periodic radicals Keywords: Nested Radicals; Quintic; Sextic; Septic; Equations; Polynomi- als; Solutions; Higher functions; 1 A general type of equations Consider the following general type of equations ax2µ + bxµ + c = xν . (1) Then (1) can be written in the form b 2 ∆2 a xµ + = xν , (2) 2a − 4a where ∆ = √b2 4ac. Hence − 2 µ b ∆ 1 ν x = − + 2 + x (3) 2a r4a a Set now √d x = x1/d, d Q 0 , then ∈ + −{ } 2 µ b ∆ 1 x = − + + xν (4) s 2a 4a2 a arXiv:1406.1948v2 [math.GM] 18 Dec 2014 r hence µ/ν 2 ν b ∆ 1 ν x = − + 2 + x (5) s 2a r4a a Theorem 1. The solution of (1) is µ v 2 µ/ν 2 2 u b v ∆ 1 b ∆ 1 µ/ν b ∆ x = u− + u + v− + v + − + + ... (6) u 2a u4a2 a u 2a u4a2 a s 2a 4a2 u u u u r u u u t t t t 1 Proof. Use relation (4) and repeat it infinite times. Corollary 1. The equation ax6 + bx5 + cx4 + dx3 + ex2 + fx + g = 0 (7) is always solvable with nested radicals. Proof. We know (see [1]) that all sextic equations, of the most general form (7) are equivalent by means of a Tchirnhausen transform y = kx4 + lx3 + mx2 + nx + s (8) to the form 6 2 y + e1y + f1y + g1 = 0 (9) But the last equation is of the form (1) with µ = 1 and ν = 6 and have solution 2 1/6 2 2 f v ∆ 1 f ∆ 1 1/6 f ∆ y = 1 + u 1 v 1 + 1 1 + 1 + .. -
ALGEBRAIC GEOMETRY (1) Compute the Points of Intersection
ALGEBRAIC GEOMETRY HOMEWORK 5 (1) Compute the points of intersection of the circle x2 +y2 +x−y = 0 with the lemniscate (x2 +y2)2 = x2 −y2 using resultants (can you compute the affine points of intersections directly?), and compute the multiplicities. Explain which coordinate system you choose, how the equations look like, what the resultant is, and what its factors are. (2) Here you will learn how to solve cubics using resultants. Assume you want to solve the cubic equation x3 + ax2 + bx + c = 0. (a) Show that the substitution y = x + a/3 transforms the cubic into y3 + By + C = 0. (b) Now assume that we have to solve x3 + bx + c = 0. Using linear re- lations y = rx ∗ b will not make the linear term disappear (without bringing back the quadratic term). Thus we try to put y = x2 + cx + d and then eliminate x using resultants: type in p = polresultant(x^3+b*x+c,y-x^2-d*x-e,x) polcoeff(p,2,y) polcoeff(p,1,y) (you can find out what polcoeff is doing by typing ?polcoeff). Now we know that we can keep the quadratic term out of the equation by choosing e = 2b/3. With this value of e go back and recompute the resultant; this will now be a cubic in y without quadratic term. The coefficient of the linear term can be made to disappear by solving a quadratic equation (which is called the resolvent of the original cubic). (c) Thus you can solve the cubic by solving the resolvent, using the trans- formations above to turn the cubic into a pure cubic y3 + c, which in turn is easy to solve. -
Calcium: Computing in Exact Real and Complex Fields Fredrik Johansson
Calcium: computing in exact real and complex fields Fredrik Johansson To cite this version: Fredrik Johansson. Calcium: computing in exact real and complex fields. ISSAC ’21, Jul 2021, Virtual Event, Russia. 10.1145/3452143.3465513. hal-02986375v2 HAL Id: hal-02986375 https://hal.inria.fr/hal-02986375v2 Submitted on 15 May 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Calcium: computing in exact real and complex fields Fredrik Johansson [email protected] Inria Bordeaux and Institut Math. Bordeaux 33400 Talence, France ABSTRACT This paper presents Calcium,1 a C library for exact computa- Calcium is a C library for real and complex numbers in a form tion in R and C. Numbers are represented as elements of fields suitable for exact algebraic and symbolic computation. Numbers Q¹a1;:::; anº where the extension numbers ak are defined symbol- ically. The system constructs fields and discovers algebraic relations are represented as elements of fields Q¹a1;:::; anº where the exten- automatically, handling algebraic and transcendental number fields sion numbers ak may be algebraic or transcendental. The system combines efficient field operations with automatic discovery and in a unified way. -
Variable Planck's Constant
Variable Planck’s Constant: Treated As A Dynamical Field And Path Integral Rand Dannenberg Ventura College, Physics and Astronomy Department, Ventura CA [email protected] [email protected] January 28, 2021 Abstract. The constant ħ is elevated to a dynamical field, coupling to other fields, and itself, through the Lagrangian density derivative terms. The spatial and temporal dependence of ħ falls directly out of the field equations themselves. Three solutions are found: a free field with a tadpole term; a standing-wave non-propagating mode; a non-oscillating non-propagating mode. The first two could be quantized. The third corresponds to a zero-momentum classical field that naturally decays spatially to a constant with no ad-hoc terms added to the Lagrangian. An attempt is made to calibrate the constants in the third solution based on experimental data. The three fields are referred to as actons. It is tentatively concluded that the acton origin coincides with a massive body, or point of infinite density, though is not mass dependent. An expression for the positional dependence of Planck’s constant is derived from a field theory in this work that matches in functional form that of one derived from considerations of Local Position Invariance violation in GR in another paper by this author. Astrophysical and Cosmological interpretations are provided. A derivation is shown for how the integrand in the path integral exponent becomes Lc/ħ(r), where Lc is the classical action. The path that makes stationary the integral in the exponent is termed the “dominant” path, and deviates from the classical path systematically due to the position dependence of ħ. -
Semiclassical Unimodular Gravity
Preprint typeset in JHEP style - PAPER VERSION Semiclassical Unimodular Gravity Bartomeu Fiol and Jaume Garriga Departament de F´ısica Fonamental i Institut de Ci`encies del Cosmos, Universitat de Barcelona, Mart´ıi Franqu`es 1, 08028 Barcelona, Spain [email protected], [email protected] Abstract: Classically, unimodular gravity is known to be equivalent to General Rel- ativity (GR), except for the fact that the effective cosmological constant Λ has the status of an integration constant. Here, we explore various formulations of unimod- ular gravity beyond the classical limit. We first consider the non-generally covariant action formulation in which the determinant of the metric is held fixed to unity. We argue that the corresponding quantum theory is also equivalent to General Relativity for localized perturbative processes which take place in generic backgrounds of infinite volume (such as asymptotically flat spacetimes). Next, using the same action, we cal- culate semiclassical non-perturbative quantities, which we expect will be dominated by Euclidean instanton solutions. We derive the entropy/area ratio for cosmological and black hole horizons, finding agreement with GR for solutions in backgrounds of infinite volume, but disagreement for backgrounds with finite volume. In deriving the arXiv:0809.1371v3 [hep-th] 29 Jul 2010 above results, the path integral is taken over histories with fixed 4-volume. We point out that the results are different if we allow the 4-volume of the different histories to vary over a continuum range. In this ”generalized” version of unimodular gravity, one recovers the full set of Einstein’s equations in the classical limit, including the trace, so Λ is no longer an integration constant. -
On the Solution to Nonic Equations
On the Solution to Nonic Equations By Dr. Raghavendra G. Kulkarni Abstract. This paper presents a novel decomposition tech- nique in which a given nonic equation is decomposed into quartic and quintic polynomials as factors, eventually lead- ing to its solution in radicals. The conditions to be satisfied by the roots and the coefficients of such a solvable nonic equation are derived. Introduction It is well known that the general polynomial equations of degree five and above cannot be solved in radicals, and have to be solved algebraically using symbolic coefficients, such as the use of Bring radicals for solving the general quintic equation, and the use of Kampe de Feriet functions to solve the general sextic equation [1, 2]. There is hardly any literature on the analytical solution to the polynomial equations beyond sixth degree. The solution to certain solvable octic equations is described in a recent paper [4]. This paper presents a method of determining all nine roots of a nonic equation (ninth-degree polynomial equation) in radicals. First, the given nonic equation is decomposed into two factors in a novel fashion. One of these factors is a fourth-degree polynomial, while the other one is a fifth-degree polynomial. When the fourth- degree polynomial factor is equated to zero, the four roots of the given nonic equation are extracted by solving the resultant quar- tic equation using the well-known Ferrari method or by a method given in a recent paper [3]. However, when the fifth-degree polyno- mial factor is equated to zero, the resultant quintic equation is also required to be solved in radicals, since the aim of this paper is to solve the nonic equation completely in radicals. -
Monodromies and Functional Determinants in the CFT Driven Quantum Cosmology
Monodromies and functional determinants in the CFT driven quantum cosmology A.O.Barvinsky and D.V.Nesterov Theory Department, Lebedev Physics Institute, Leninsky Prospect 53, Moscow 119991, Russia Abstract We discuss the calculation of the reduced functional determinant of a special second order differential operator F = −d2/dτ 2 + g¨=g, g¨ ≡ d2g/dτ 2, with a generic function g(τ), subject to periodic boundary conditions. This implies the gauge-fixed path integral representation of this determinant and the monodromy method of its calculation. Motivations for this particular problem, coming from applications in quantum cosmology, are also briefly discussed. They include the problem of microcanonical initial conditions in cosmology driven by a conformal field theory, cosmological constant and cosmic microwave background problems. 1. Introduction Here we consider the class of problems involving the differential operator of the form d2 g¨ F = − + ; : (1.1) dτ 2 g where g = g(τ) is a rather generic function of its variable τ. From calculational viewpoint, the virtue of this operator is that g(τ) represents its explicit basis function { the solution of the homogeneous equation, F g(τ) = 0; (1.2) which immediately allows one to construct its second linearly independent solution τ dy Ψ(τ) = g(τ) (1.3) g2(y) τZ∗ and explicitly build the Green's function of F with appropriate boundary conditions. On the other hand, from physical viewpoint this operator is interesting because it describes long-wavelength per- turbations in early Universe, including the formation of observable CMB spectra [1, 2], statistical ensembles in quantum cosmology [3], etc. -
This Article Was Published in an Elsevier Journal. the Attached Copy
This article was published in an Elsevier journal. The attached copy is furnished to the author for non-commercial research and education use, including for instruction at the author’s institution, sharing with colleagues and providing to institution administration. Other uses, including reproduction and distribution, or selling or licensing copies, or posting to personal, institutional or third party websites are prohibited. In most cases authors are permitted to post their version of the article (e.g. in Word or Tex form) to their personal website or institutional repository. Authors requiring further information regarding Elsevier’s archiving and manuscript policies are encouraged to visit: http://www.elsevier.com/copyright Author's personal copy Theoretical Computer Science 394 (2008) 159–174 www.elsevier.com/locate/tcs Physical constraints on hypercomputation$ Paul Cockshotta,∗, Lewis Mackenziea, Greg Michaelsonb a Department of Computing Science, University of Glasgow, 17 Lilybank Gardens, Glasgow G12 8QQ, United Kingdom b School of Mathematical and Computer Sciences, Heriot-Watt University, Riccarton, Edinburgh EH14 4AS, United Kingdom Abstract Many attempts to transcend the fundamental limitations to computability implied by the Halting Problem for Turing Machines depend on the use of forms of hypercomputation that draw on notions of infinite or continuous, as opposed to bounded or discrete, computation. Thus, such schemes may include the deployment of actualised rather than potential infinities of physical resources, or of physical representations of real numbers to arbitrary precision. Here, we argue that such bases for hypercomputation are not materially realisable and so cannot constitute new forms of effective calculability. c 2007 Elsevier B.V. All rights reserved. -
04. Rukhin-Final5a-116-1.Qxd
Volume 116, Number 1, January-February 2011 Journal of Research of the National Institute of Standards and Technology [J. Res. Natl. Inst. Stand. Technol. 116, 539-556 (2011)] Maximum Likelihood and Restricted Likelihood Solutions in Multiple-Method Studies Volume 116 Number 1 January-February 2011 Andrew L. Rukhin A formulation of the problem of considered to be known an upper bound combining data from several sources is on the between-method variance is National Institute of Standards discussed in terms of random effects obtained. The relationship between and Technology, models. The unknown measurement likelihood equations and moment-type Gaithersburg, MD 20899-8980 precision is assumed not to be the same equations is also discussed. for all methods. We investigate maximum likelihood solutions in this model. By representing the likelihood equations as Key words: DerSimonian-Laird simultaneous polynomial equations, estimator; Groebner basis; [email protected] the exact form of the Groebner basis for heteroscedasticity; interlaboratory studies; their stationary points is derived when iteration scheme; Mandel-Paule algorithm; there are two methods. A parametrization meta-analysis; parametrized solutions; of these solutions which allows their polynomial equations; random effects comparison is suggested. A numerical model. method for solving likelihood equations is outlined, and an alternative to the maximum likelihood method, the restricted Accepted: August 20, 2010 maximum likelihood, is studied. In the situation when methods variances are Available online: http://www.nist.gov/jres 1. Introduction: Meta Analysis and difficult when the unknown measurement precision Interlaboratory Studies varies among methods whose summary results may not seem to conform to the same measured property. -
The Cosmological Constant Problem 1 Introduction
The Cosmological Constant Problem and (no) solutions to it by Wolfgang G. Hollik 7/11/2017 Talk given at the Workshop Seminar Series on Vacuum Energy @ DESY. “Physics thrives on crisis. [... ] Unfortunately, we have run short on crisis lately.” (Steven Weinberg, 1989 [1]) 1 Introduction: the Cosmological Constant Besides the fact, that we are still running short on severe crises in physics also about 30 years after Weinberg’s statement, there is still yet no solution to what is called the “Cosmological Constant problem”. Neither is there any clue what the Cosmological Constant (CC) is made of and if the problem is indeed an outstanding problem. Weinberg defines and proves in his review on the Cosmological Constant [1] a “no-go” theorem. This no-go theorem is actually not a theorem on the smallness of the CC in the sense of a Vacuum Energy,1 it is rather a theorem prohibiting any kind of adjustment mechanisms that lead effectively to a universe with a flat and static (i.e. Minkowski) space-time metric in the presence of a CC. In other words: with a CC there is no Minkowski universe possible. An old crisis When Einstein first formulated his field equations for General Relativity, he was neither aware of a possible Cosmological Constant nor of an expanding universe solution to them. Originally, the proposed equations are 1 R g R = 8πG T , (1) µν − 2 µν − µν using Weinberg’s ( + ++)-metric. The matter content is given by the energy-stress tensor − Tµν, where the geometry of space-time is encoded in the Ricci tensor Rµν and the scalar µν curvature R = g Rµν of the metric gµν. -
International Journal of Pure and Applied Mathematics ————————————————————————– Volume 18 No
International Journal of Pure and Applied Mathematics ————————————————————————– Volume 18 No. 2 2005, 213-222 NEW WAY FOR A TWO-PARAMETER CANONICAL FORM OF SEXTIC EQUATIONS AND ITS SOLVABLE CASES Yoshihiro Mochimaru Department of International Development Engineering Graduate School of Science and Engineering Tokyo Institute of Technology 2-12-1, O-okayama, Meguru-ku, Tokyo 152-8550, JAPAN e-mail: [email protected] Abstract: A new way for a two-parameter canonical form of sextic equations is given, through a Tschirnhausian transform by multiple steps, supplemented with some solvable cases at most in terms of hypergeometric functions. AMS Subject Classification: 11D41 Key Words: sextic equation, Tschirnhausian transform 1. Introduction 6 6 6−n Actually the general sextic equation x + anx = 0 can be solved in nX=1 terms of Kamp´ede F´eriet functions, and it can be reduced to a three-parameter Received: October 21, 2004 c 2005, Academic Publications Ltd. 214 Y. Mochimaru 6 4 2 resolvent of the form y + ay + by + cy + c = 0 by Joubert [3]. Such a type of the sextic equation was treated by Felix Klein and a part was given in [4]. Other contributions to treatment on sextic equations were given e.g. by Cole [2] and Coble [1]. In this paper, a new way leading to a two-parameter canonical form of sextic equations is given. 2. Analysis 2.1. General Let the original given sextic equation be expressed as 6 ∗ 5 ∗ 4 ∗ 3 ∗ 2 ∗ ∗ x + a x + b x + c x + d x + e x + f = 0. (1) 3 Here the quantity 5a∗ − 18a∗b∗ + 27c∗ corresponding to the polynomial of the left hand side of equation (1) is invariant with respect to the parallel shift x → x+constant. -
Analytic Solutions to Algebraic Equations
Analytic Solutions to Algebraic Equations Mathematics Tomas Johansson LiTH{MAT{Ex{98{13 Supervisor: Bengt Ove Turesson Examiner: Bengt Ove Turesson LinkÄoping 1998-06-12 CONTENTS 1 Contents 1 Introduction 3 2 Quadratic, cubic, and quartic equations 5 2.1 History . 5 2.2 Solving third and fourth degree equations . 6 2.3 Tschirnhaus transformations . 9 3 Solvability of algebraic equations 13 3.1 History of the quintic . 13 3.2 Galois theory . 16 3.3 Solvable groups . 20 3.4 Solvability by radicals . 22 4 Elliptic functions 25 4.1 General theory . 25 4.2 The Weierstrass } function . 29 4.3 Solving the quintic . 32 4.4 Theta functions . 35 4.5 History of elliptic functions . 37 5 Hermite's and Gordan's solutions to the quintic 39 5.1 Hermite's solution to the quintic . 39 5.2 Gordan's solutions to the quintic . 40 6 Kiepert's algorithm for the quintic 43 6.1 An algorithm for solving the quintic . 43 6.2 Commentary about Kiepert's algorithm . 49 7 Conclusion 51 7.1 Conclusion . 51 A Groups 53 B Permutation groups 54 C Rings 54 D Polynomials 55 References 57 2 CONTENTS 3 1 Introduction In this report, we study how one solves general polynomial equations using only the coef- ¯cients of the polynomial. Almost everyone who has taken some course in algebra knows that Galois proved that it is impossible to solve algebraic equations of degree ¯ve or higher, using only radicals. What is not so generally known is that it is possible to solve such equa- tions in another way, namely using techniques from the theory of elliptic functions.