1,713 research outputs found

    Gyrations: The Missing Link Between Classical Mechanics with its Underlying Euclidean Geometry and Relativistic Mechanics with its Underlying Hyperbolic Geometry

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    Being neither commutative nor associative, Einstein velocity addition of relativistically admissible velocities gives rise to gyrations. Gyrations, in turn, measure the extent to which Einstein addition deviates from commutativity and from associativity. Gyrations are geometric automorphisms abstracted from the relativistic mechanical effect known as Thomas precession

    On algebraic endomorphisms of the Einstein gyrogroup

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    We describe the structure of all continuous algebraic endomorphisms of the open unit ball B\mathbf{B} of R3\mathbb{R}^3 equipped with the Einstein velocity addition. We show that any nonzero such transformation originates from an orthogonal linear transformation on R3\mathbb{R}^3

    Harmonic analysis on the Möbius gyrogroup

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    In this paper we propose to develop harmonic analysis on the Poincaré ball BtnB_t^n, a model of the n-dimensional real hyperbolic space. The Poincaré ball BtnB_t^n is the open ball of the Euclidean n-space RnR^n with radius t>0t>0, centered at the origin of RnR^n and equipped with Möbius addition, thus forming a Möbius gyrogroup where Möbius addition in the ball plays the role of vector addition in Rn\mathbb{R}^n. For any t>0t>0 and an arbitrary parameter σR\sigma \in R we study the (σ,t)(\sigma,t)-translation, the (σ,t)( \sigma,t)-convolution, the eigenfunctions of the (σ,t)(\sigma,t)-Laplace-Beltrami operator, the (σ,t)(\sigma,t)-Helgason Fourier transform, its inverse transform and the associated Plancherel's Theorem, which represent counterparts of standard tools, thus, enabling an effective theory of hyperbolic harmonic analysis. Moreover, when t+t \rightarrow +\infty the resulting hyperbolic harmonic analysis on BtnB_t^n tends to the standard Euclidean harmonic analysis on RnR^n, thus unifying hyperbolic and Euclidean harmonic analysis. As an application we construct diffusive wavelets on BtnB_t^n

    Anterior Dental Microwear Texture Analysis of the Krapina Neandertals

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    Some Neandertal anterior teeth show unusual and excessive gross wear, commonly explained by non-dietary anterior tooth use, or using the anterior dentition as a tool, clamp, or third hand. This alternate use is inferred from aboriginal arctic populations, who used their front teeth in this manner. Here we examine anterior dental microwear textures of the Krapina Neandertals to test this hypothesis and further analyze tooth use in these hominins. Microwear textures from 17 Krapina Dental People were collected by white-light confocal profilometry using a 100x objective lens. Four adjacent scans were generated, totaling an area of 204x276 μm, and were analyzed using Toothfrax and SFrax SSFA software packages. The Neandertals were compared to six bioarchaeological/ethnographic samples with reported variation in diet, abrasive load, and non-dietary anterior tooth use. Results indicate that Krapina anterior teeth lack extreme microwear textures expected of hominins exposed to heavy abrasives or those that regularly generated high stresses associated with intense use of the front teeth as tools. Krapina hominins have microwear attributes in common with Coast Tsimshian, Aleut, and Puye Pueblo samples. Collectively, this suggests that the Krapina Neandertals faced moderate abrasive loads and only periodically used their anterior teeth as tools for non-diet related behaviors

    Spacecraft Crew Cabin Condensation Control

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    A report discusses a new technique to prevent condensation on the cabin walls of manned spacecraft exposed to the cold environment of space, as such condensation could lead to free water in the cabin. This could facilitate the growth of mold and bacteria, and could lead to oxidation and weakening of the cabin wall. This condensation control technique employs a passive method that uses spacecraft waste heat as the primary wallheating mechanism. A network of heat pipes is bonded to the crew cabin pressure vessel, as well as the pipes to each other, in order to provide for efficient heat transfer to the cabin walls and from one heat pipe to another. When properly sized, the heat-pipe network can maintain the crew cabin walls at a nearly uniform temperature. It can also accept and distribute spacecraft waste heat to maintain the pressure vessel above dew point
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