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相关论文: Cosine formula for generalized O'Hara's energies

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O'Hara introduced several functionals as knot energies. One of them is the M\"{o}bius energy. We know its M\"{o}bius invariance from Doyle-Schramm's cosine formula. It is also known that the M\"{o}bius energy was decomposed into three…

微分几何 · 数学 2019-04-16 Aya Ishizeki , Takeyuki Nagasawa

We introduce a new discretization of O'Hara's M\"obius energy. In contrast to the known discretizations of Simon and Kim and Kusner it is invariant under M\"obius transformations of the surrounding space. The starting point for this new…

泛函分析 · 数学 2018-09-24 Simon Blatt , Aya Ishizeki , Takeyuki Nagasawa

The M\"{o}bius energy is one of the knot energies, and is named after its M\"{o}bius invariant property. It is known to have several different expressions. One is in terms of the cosine of conformal angle, and is called the cosine formula.…

微分几何 · 数学 2020-02-24 Aya Ishizeki , Takeyuki Nagasawa

We considered random discrete approximation of O'Hara energy. O'Hara energy is the energy defined for a knot, and O'Hara energy was introduced for defining the standard shape for each knot class (equivalence class by ambient isotopy) by…

经典分析与常微分方程 · 数学 2019-05-17 Jun Okamoto

O'Hara's energies, introduced by Jun O'Hara, were proposed to answer the question of what is the canonical shape in a given knot type, and were configured so that the less the energy value of a knot is, the "better" its shape is. The…

偏微分方程分析 · 数学 2019-09-02 Shoya Kawakami , Takeyuki Nagasawa

In the present paper we investigate generalizations of O'Hara's M\"obius energy on curves \cite{ohara_1991a}, to M\"obius-invariant energies on non-smooth subsets of $\R^n$ of arbitrary dimension and co-dimension. In particular, we show…

微分几何 · 数学 2021-02-17 Bastian Käfer , Heiko von der Mosel

We define a new class of knot energies (known as renormalization energies) and prove that a broad class of these energies are uniquely minimized by the round circle. Most of O'Hara's knot energies belong to this class. This proves two…

几何拓扑 · 数学 2007-05-23 Aaron Abrams , Jason Cantarella , Joseph H. G. Fu , Mohammad Ghomi , Ralph Howard

The O'Hara energies, introduced by Jun O'Hara in 1991, were proposed to answer the question of what is a "good" figure in a given knot type. A property of the O'Hara energies is that the "better" the figure of a knot is, the less the energy…

偏微分方程分析 · 数学 2019-09-02 Shoya Kawakami

In this paper, we propose a discrete version of O'Hara's knot energy defined on polygons embedded in the Euclid space. It is shown that values of the discrete energy of polygons inscribing the curve which has bounded O'Hara's energy…

数值分析 · 数学 2019-08-30 Shoya Kawakami

The M\"{o}bius energy, defined by O'Hara, is one of the knot energies, and named after the M\"{o}bius invariant property which was shown by Freedman-He-Wang. The energy can be decomposed into three parts, each of which is M\"{o}bius…

微分几何 · 数学 2019-04-16 Simon Blatt , Aya Ishizeki , Takeyuki Nagasawa

We investigate a discrete version of the M\"obius energy, that is of geometric interest in its own right and is defined on equilateral polygons with $n$ segments. We show that the $\Gamma$-limit regarding $L^{q}$ or $W^{1,q}$ convergence,…

几何拓扑 · 数学 2014-05-20 Sebastian Scholtes

We define and study a M\"obius invariant energy associated to planar domains, as well its generalization to space curves. This generalization is a M\"obius version of Banchoff-Pohl's notion of area enclosed by a space curve. A relation with…

微分几何 · 数学 2016-03-21 Jun O'Hara , Gil Solanes

We generalize the cosmic energy equation to the case when massive particles interact via a modified gravitational potential of the form phi(a, r), which is allowed to explicitly depend upon the cosmological time through the expansion factor…

宇宙学与河外天体物理 · 物理学 2010-12-23 Yuri Shtanov , Varun Sahni

A covariant formula for conserved currents of energy, momentum and angular-momentum is derived from a general form of Noethers theorem applied directly to the Einstein-Hilbert action of classical general relativity. Energy conservation in a…

广义相对论与量子宇宙学 · 物理学 2008-02-03 Philip E. Gibbs

We refine and extend a programme initiated by one of the current authors [Science 276 (1997) 88; Phys. Rev. D56 (1997) 7578] advocating the use of the classical energy conditions of general relativity in a cosmological setting to place very…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Celine Cattoen , Matt Visser

We consider a gas of N weakly interacting bosons in the ground state. Such gases exhibit Bose-Einstein condensation. The binding energy is defined as the energy it takes to remove one particle from the gas. In this article, we prove an…

数学物理 · 物理学 2024-05-09 Lea Boßmann , Nikolai Leopold , David Mitrouskas , Sören Petrat

The problem of a particle of mass m in the field of the inverse square potential is studied in quantum mechanics with a generalized uncertainty principle, characterized by the existence of a minimal length. Using the coordinate…

量子物理 · 物理学 2017-11-15 Djamil Bouaziz , Tolga Birkandan

The problem of defining the average kinetic energy of statistical systems is addressed. The conditions of applicability for the formula, relating the average kinetic energy with the mass derivative of the internal energy, are analysed. It…

统计力学 · 物理学 2015-06-25 V. I. Yukalov

Now that the properties of low temperature Bose gases at low density, $\rho$, can be examined experimentally it is appropriate to revisit some of the formulas deduced by many authors 4-5 decades ago. One of these is that the leading term in…

软凝聚态物质 · 物理学 2009-10-30 Elliott H. Lieb , Jakob Yngvason

It is shown here that if we assume that what is conserved in nature is not simply mass-energy, but rather mass-energy plus the energy uncertainty of the uncertainty principle, and if we also assume that position uncertainty is reduced by…

综合物理 · 物理学 2016-11-23 M. E. McCulloch
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