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In this paper we establish a relationship between geodesic nets and critical points of the distance function. We bound the number of balanced points for certain minimizing geodesic nets on manifolds homeomorphic to the $n$-sphere. We also…

Differential Geometry · Mathematics 2020-04-22 Ian M Adelstein

We investigate the geodesics in the entire class of nonexpanding impulsive gravitational waves propagating in an (anti-)de Sitter universe using the distributional form of the metric. Employing a 5-dimensional embedding formalism and a…

General Relativity and Quantum Cosmology · Physics 2016-05-03 Clemens Sämann , Roland Steinbauer , Alexander Lecke , Jiří Podolský

The large-scale structure of the Universe is well approximated by the Friedmann equations, parametrized by several energy densities which can be observationally inferred. A natural question to ask is: How different would the Universe be if…

General Relativity and Quantum Cosmology · Physics 2025-01-20 Arthur G. Suvorov

We present Jordan-Brans-Dicke and general scalar-tensor gravitational theory in extra dimensions in an asymptotically flat or anti de Sitter spacetime. We consider a special gravitating, boson field configuration, a $q$-star, in 3, 4, 5 and…

High Energy Physics - Theory · Physics 2015-06-26 Athanasios Prikas

A metric space $(X,d)$ is called a $subline$ if every 3-element subset $T$ of $X$ can be written as $T=\{x,y,z\}$ for some points $x,y,z$ such that $d(x,z)=d(x,y)+d(y,z)$. By a classical result of Menger, every subline of cardinality $\ne…

Metric Geometry · Mathematics 2023-05-16 Iryna Banakh , Taras Banakh , Maria Kolinko , Alex Ravsky

We show that there exists a geodesic spanner with almost linear number of edges.

Computational Geometry · Computer Science 2015-11-06 Mohammad Ali Abam , Mark de Berg , Mohammad Javad Rezaei Seraji

A new solution to the coupled gravitational and scalar field equations for a condensed boson field is found in Newtonian approximation. The solution is axially symmetric, but not spherically symmetric. For N particles the mass of the object…

Astrophysics · Physics 2009-10-28 B. Schupp , J. J. van der Bij

We study deviations from geodesic motions in a Topological Star spacetime for either massive, charged and spinning particles, elucidating different behaviours with the Schwarzschild spacetime. We also consider the deviations for the motion…

General Relativity and Quantum Cosmology · Physics 2025-05-20 Donato Bini , Giorgio Di Russo

We study the geometry of Outer Space $CV_n$ in regard of the asymmetric Lipschitz metric via envelopes, that is the set of all geodesics between two points. In the simplicial structure of $CV_n$ the envelopes are polytopes. We construct a…

Geometric Topology · Mathematics 2019-07-16 Christian Steinhart

The generalized Busemann-Petty problem asks whether centrally-symmetric convex bodies having larger volume of all m-dimensional sections necessarily have larger volume. When m>3 this is known to be false, but the cases m=2,3 are still open.…

Functional Analysis · Mathematics 2007-05-23 Emanuel Milman

Stars are not perfectly spherically symmetric. They are deformed by rotation and magnetic fields. Until now, the study of stellar shapes has only been possible with optical interferometry for a few of the fastest-rotating nearby stars. We…

We describe a novel class of geometrical models of relativistic stars. Our approach to the static spherically symmetric solutions of Einstein equations is based on a careful physical analysis of radial gauge conditions. It brings us to a…

Astrophysics · Physics 2007-05-23 P. P. Fiziev

By a geodesic subspace of a metric space $X$ we mean a subset $A$ of $X$ such that any two points in $A$ can be connected by a geodesic in $A$. It is easy to check that a geodesic metric space $X$ is an $\mathbb{R}$-tree (that is, a…

Metric Geometry · Mathematics 2017-01-04 Thomas Weighill

Let $m$ be a positive integer, $q$ be a prime power, and $\mathrm{PG}(2,q)$ be the projective plane over the finite field $\mathbb F_q$. Finding complete $m$-arcs in $\mathrm{PG}(2,q)$ of size less than $q$ is a classical problem in finite…

Combinatorics · Mathematics 2020-07-03 Daniele Bartoli , Giacomo Micheli

What one obtains when the min-max methods for the distance function are applied on the space of pairs of points of a Riemannian two-sphere? This question is studied in details in the present article. We show that the associated min-max…

Differential Geometry · Mathematics 2025-03-18 Rafael Montezuma , Idalina Ribeiro

We study q-stars with global and local U(1) symmetry in extra dimensions in asymptotically anti de Sitter or flat spacetime. The behavior of the mass, radius and particle number of the star is quite different in 3 dimensions, but in 5, 6, 8…

High Energy Physics - Theory · Physics 2009-11-10 Athanasios Prikas

We discuss whether it is possible to reconstruct a metric by its unparameterized geodesics, and how to do it effectively. We explain why this problem is interesting for general relativity. We show how to understand whether all curves from a…

Differential Geometry · Mathematics 2013-01-14 Vladimir S. Matveev

We provide an alternative, constructive proof that the collection $\mathcal{M}$ of isometry classes of compact metric spaces endowed with the Gromov-Hausdorff distance is a geodesic space. The core of our proof is a construction of explicit…

Metric Geometry · Mathematics 2018-03-21 Samir Chowdhury , Facundo Mémoli

In this paper we explore the idea that Teichm\"uller space is hyperbolic "on average." Our approach focuses on studying the geometry of geodesics which spend a definite proportion of time in some thick part of Teichm\"uller space. We…

Geometric Topology · Mathematics 2013-11-27 Spencer Dowdall , Moon Duchin , Howard Masur

We define the notion of geodesic completeness for semi-Riemannian metrics of low regularity in the framework of the geometric theory of generalized functions. We then show completeness of a wide class of impulsive gravitational wave…

Differential Geometry · Mathematics 2015-01-30 Clemens Sämann , Roland Steinbauer
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