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2015, arXiv (Cornell University)
We achieve compositions rules for the geometric parameters of the composed rotations, which is in a certain sense analogous to the well known Rodrigues formula. We also obtain a necessary and sufficient condition for a composition of two simple rotations in E 4 to be a simple rotation.
Journal of Geometry and Symmetry in Physics, 2015
We achieve compositions rules for the geometric parameters of the composed rotations, which is in a certain sense analogous to the well known Rodrigues formula. We also obtain a necessary and sufficient condition for a composition of two simple rotations in E 4 to be a simple rotation.
2013
Here we consider new decompositions of the special orthogonal transformations in R 3 into products of two rotations, one of them has a fixed scalar parameter, and the other -a fixed axis. The obtained analytic solutions constitute an alternative parametrization of the group SO(3) with charts in S 2 × S 1 . As it should be expected, from topological point of view, this map has singularities -the number of images varies between zero, one, two and infinitely many. The corresponding formulae become particularly simple in the cases involving quarter turns and half turns, although in the latter additional geometric criteria appear. Transferring the same construction to the universal cover SU(2) ∼ = S 3 via quaternion parametrization eliminates the problem with infinite scalar parameters. The so obtained map can also be seen as a realization of the Hopf fibration S 1 → S 3 → S 2 .
Computational Methods and Function Theory, 2022
In both the Euclidean plane $${\mathbb {R}}^2$$ R 2 and the hyperbolic plane $${\mathbb {H}}^2$$ H 2 , a non-trivial group of rotations has a unique fixed point. We compare groups of rotations of the three-dimensional spaces $${\mathbb {R}}^3$$ R 3 and $${\mathbb {H}}^3$$ H 3 , and in each case we discuss the existence of a (possibly non-unique) common fixed point of the elements in such a group.
IEEE Computer Graphics and Applications, 2000
The connection between three-by-three orthogonal matrices and the rotations of space that they describe is quite misleading when trying to describe a rotation of space by angles of rotation about the three coordinate axes. If the relation between the linear algebra and the geometry is properly established, not only do obscurities vanish but less computation is required to obtain the matrix describing a specified rotation. This article will describe all three-by-three orthogonal matrices, what they do geometrically, and how to obtain directly a matrix having prescribed geometric properties. The arguments leading to the formulas are included for completeness, but the goals are the statements that connect these formulas with the geometry. Rotations This discussion is restricted to rigid motions of space that fix at least one point: rotations; a fixed point is chosen to be the origin. Such a rigid motion is then given by a three-by-three matrix A: The row vector x is sent to xA. Since angles are preserved, (xA) (yA) T always equals Xy T, where T denotes transpose, so xAA TyT=xyT. That is, AA T = I iS the identity; A is an orthogonal matrix. Conversely, orthogonal matrices yield rotations.
Journal of Modern Dynamics, 2015
We investigate the notion of complex rotation number which was introduced by V. I. Arnold in 1978. Let f : R/Z → R/Z be an orientation preserving circle diffeomorphism and let ω ∈ C/Z be a parameter with positive imaginary part. Construct a complex torus by glueing the two boundary components of the annulus { z ∈ C/Z | 0 < Im(z) < Im(ω) } via the map f + ω. This complex torus is isomorphic to C/(Z + τ Z) for some appropriate τ ∈ C/Z. According to Moldavskis [6], if the ordinary rotation number rot(f + ω 0) is Diophantine and if ω tends to ω 0 non tangentially to the real axis, then τ tends to rot(f + ω 0). We show that the Diophantine and non tangential assumptions are unnecessary: if rot(f + ω 0) is irrational then τ tends to rot(f + ω 0) as ω tends to ω 0. This, together with results of N.Goncharuk [4], motivates us to introduce a new fractal set ("bubbles"), given by the limit values of τ as ω tends to the real axis. For the rational values of rot(f + ω 0), these limits do not necessarily coincide with rot(f + ω 0) and form a countable number of analytic loops in the upper half-plane. Notation: • H = H + is the set of complex numbers with positive imaginary part. • H − is the set of complex numbers with negative imaginary part. • If p/q is a rational number, then p and q are assumed to be coprime. • If x and y are distinct points in R/Z, then (x, y) denotes the set of points z ∈ R/Z − { x, y } such that the three points x, z, y are in increasing order and [x, y]:=(x, y) ∪ { x, y }. • rot(f) ∈ R/Z is a rotation number of an orientation-preserving circle diffeomorphism f .
Transactions of A. Razmadze Mathematical Institute, 2016
It is studied the following problem: for a given function f what kind of may be a set of all rotations γ for which f is not differentiable with respect to γ-rotation of a given basis B? In particular, for translation invariant bases on the plane it is found the topological structure of possible sets of singular rotations.
Annales de l’institut Fourier, 1984
Computer Methods in Applied Mechanics and Engineering, 1997
In this work we discuss some aspects of the three-dimensional finite rotations pertinent to the formulation and computational treatment of the geometrically exact structural theories. Among various possibilities to parameterize the finite rotations, special attention is dedicated to a choice featuring an incremental rotation vector. Some computational aspects pertinent to the implementation of the Newton iterative scheme and the Newmark time-stepping algorithm applied to solving these problems are examined. Representative numerical simulations are presented in order to illustrate the performance of the proposed formulation. 0. Dedication Current strong interest in nonlinear analysis of physics phenomena, nourished by ever-growing computational resources, has long been anticipated by J. Tinsley Oden. In the early 1970s he published a book (see [l]), which served as a road-map for many developments which followed. In this and later works, Dr. Oden recognized that the proper setting for these developments is placed at the crossroads between nonlinear mechanics theories and numerical analysis, helping to establish an independent identity of the scientific discipline of Computational Mechanics. In particular, I have always appreciated a distinct style and mathematical rigor of Tinsley's works, which I believe is the only way to make headway in nonlinear problems. I personally benefited from many works of Tinsley Oden, starting from my PhD thesis at UC Berkeley in the late 1980s where the contact model proposed by Oden and Martins [2] proved very useful for structure-foundation interaction problems I was studying at the time. I am also pleased that my contribution selected for this occasion, regarding some computational aspects in structural theories with finite rotations, appears to be related to a very recent work of Tinsley (see [3]) with an ambitious goal of placing these structural theories in a proper harmony with classical continuum theories and delegating some of the traditional engineer's responsibilities to an adaptive modeling procedure.
Topology and its Applications, 2006
This paper is a study of invariant sets that have "geometric" rotation numbers, which we call rotational sets, for the angle-tripling map σ 3 : T → T, and more generally, the angle-d-tupling map σ d : T → T for d 2. The precise number and location of rotational sets for σ d is determined by d − 1, 1 d -length open intervals, called holes, that govern, with some specifiable flexibility, the number and location of root gaps (complementary intervals of the rotational set of length 1 d ). In contrast to σ 2 , the proliferation of rotational sets with the same rotation number for σ d , d > 2, is elucidated by the existence of canonical operations allowing one to reduce σ d to σ d−1 and construct σ d+1 from σ d by, respectively, removing or inserting "wraps" of the covering map that, respectively, destroy or create/enlarge root gaps.
Bulletin Polish Acad. Sci. Math., 2016
Consider an o-minimal structure on the real field R and two definable subsets A, B of the Euclidean space R n , of the unit sphere S n or of the hyperbolic space H n , n ≥ 2, which are of dimensions k, l ≤ n − 1, respectively. We prove that the dimension of the intersection σ(A) ∩ B is less than min{k, l} for a generic rotation σ of the ambient space; here we set dim ∅ = −1.
2021
In this paper, some physical expressions as the specific energy and the specific angular momentum on these surfaces of rotation are investigated using conditions being geodesic on rotational surfaces with the help of Clairaut’s theorem.
Relying on previously derived set of explicit solutions for the generalized Euler decomposition with respect to three arbitrary axes here we obtain the corresponding expressions in the case of infinitesimal (pseudo-)rotations. Possible generalizations, e.g., to higher dimensional groups and physical applications are briefly discussed as well.
2013
We use a vector parameter technique to obtain the generalized Euler decompositions with respect to arbitrarily chosen axes for the three-dimensional special orthogonal group SO(3) and the three-dimensional Lorentz group SO(2, 1). Our approach, based on projecting a quaternion (respectively split quaternion) from the corresponding spin cover, has proven quite effective in various problems of geometry and physics [1, 2, 3]. In particular, we obtain explicit (generally double-valued) expressions for the three parameters in the decomposition and discuss separately the degenerate and divergent solutions, as well as decompositions with respect to two axes. There are some straightforward applications of this method in special relativity and quantum mechanics which are discussed elsewhere (see [4]).
Results in Mathematics, 2012
In the present study we consider generalized rotation surfaces imbedded in an Euclidean space of four dimensions. We also give some special examples of these surfaces in E 4. Further, the curvature properties of these surfaces are investigated. We give necessary and sufficient conditions for generalized rotation surfaces to become pseudo-umbilical. We also show that every general rotation surface is Chen surface in E 4. Finally we give some examples of generalized rotation surfaces in E 4 .
Several explanations of complex numbers, rotations, and their interpretations in information theory are given in the appendix.
2020
We give a new formula for the rotation number (or Whitney index) of a smooth closed plane curve. This formula is obtained from the winding numbers associated with the regions and the crossing points of the curve. One difference with the classic Whitney formula is that ours does not need a base point.
A general class of matrices, covering, for instance, an important set of proper rotations, is considered. Several characteristics of the class are established, which deal with such notions and properties as determinant, eigenspaces, eigenvalues, idempotency, Moore-Penrose inverse, or orthogonality.
2021
In the present study we consider generalized rotational surfaces in Euclidean 4-space E. Further, we obtain some curvature properties of these surfaces. We also introduce some kind of generalized rotational surfaces in E with the choice of meridian curve. Finally, we give some examples.
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