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We consider the binding energy of a two-body system with a repulsive Coulomb interaction in a finite periodic volume. We define the finite-volume Coulomb potential as the usual Coulomb potential, except that the distance is defined as the…

核理论 · 物理学 2023-12-01 Hang Yu , Sebastian König , Dean Lee

The holographic relation between quantum correlations and connectivity of spacetime is explored for single R-charged AdS$_5$ black holes and their half-BPS limits (superstars). In a two boundary set-up, the wormhole between both universes…

高能物理 - 理论 · 物理学 2018-11-14 Joan Simon

An analysis is given of the local phase space of gravity coupled to matter to second order in perturbation theory. Working in local regions with boundaries at finite distance, we identify matter, Coulomb, and additional boundary modes. The…

广义相对论与量子宇宙学 · 物理学 2024-02-09 Viktoria Kabel , Časlav Brukner , Wolfgang Wieland

We discuss the transition from quasi-circular inspiral to plunge of a system of two nonrotating black holes of masses $m_1$ and $m_2$ in the extreme mass ratio limit $m_1m_2\ll (m_1+m_2)^2$. In the spirit of the Effective One Body (EOB)…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Alessandro Nagar , Thibault Damour , Angelo Tartaglia

The bulk-boundary correspondence is an integral feature of topological analysis and the existence of boundary or interface modes offers direct insight into the topological structure of the Bloch wave function. While only the topology of the…

强关联电子 · 物理学 2022-11-28 Chang-geun Oh , Doohee Cho , Se Young Park , Jun-Won Rhim

The goal of this paper is to obtain an approximate solution of the restricted three-body problem in the case of small perturbations in the vicinity of, but not in exact resonance. In this paper, we study the restricted threebody problem…

地球与行星天体物理 · 物理学 2025-11-11 Alexey Rosaev , Eva Plavalova , Pavel Nesterov

Rotating black holes can produce superradiant clouds of ultralight bosons. When the black hole is part of a binary system, its cloud can undergo resonances and ionization. These processes leave a distinct signature on the gravitational…

广义相对论与量子宇宙学 · 物理学 2025-08-19 Giovanni Maria Tomaselli , Thomas F. M. Spieksma , Gianfranco Bertone

Axially symmetric, stationary solutions of the Einstein-Maxwell equations with disconnected event horizon are studied by developing a method of explicit integration of the corresponding boundary-value problem. This problem is reduced to…

广义相对论与量子宇宙学 · 物理学 2009-11-07 G. G. Varzugin , A. S. Chistyakov

The correspondence principle between strings and black holes is a general framework for matching black holes and massive states of fundamental strings at a point where their physical properties (such as mass, entropy and temperature)…

高能物理 - 理论 · 物理学 2023-12-05 Nejc Čeplak , Roberto Emparan , Andrea Puhm , Marija Tomašević

We present the results of 14 simulations of nonspinning black hole binaries with mass ratios $q=m_1/m_2$ in the range $1/100\leq q\leq1$. For each of these simulations we perform three runs at increasing resolution to assess the finite…

广义相对论与量子宇宙学 · 物理学 2017-07-26 James Healy , Carlos O. Lousto , Yosef Zlochower

We construct a fully analytic, general relativistic, nonspinning black hole binary spacetime that approximately solves the vacuum Einstein equations everywhere in space and time for black holes sufficiently well separated. The metric is…

广义相对论与量子宇宙学 · 物理学 2014-05-13 Bruno C. Mundim , Hiroyuki Nakano , Nicolás Yunes , Manuela Campanelli , Scott C. Noble , Yosef Zlochower

Recently, there is an interest in studying the bulk-edge correspondence for nonlinear eigenvalues problems in a two-dimensional topological system with spin-orbit coupling. By introducing auxiliary eigenvalues, the nonlinear bulk-edge…

无序系统与神经网络 · 物理学 2023-11-27 Shujie Cheng , Yonghua Jiang , Gao Xianlong

There are two powerful arguments against the possibility of extending quantum mechanics, the violation of Bell inequalities and the Kochen-Specker theorem, but the connection between the two remains confused. Following the distinctive…

量子物理 · 物理学 2025-01-08 Jianqi Sheng , Dongkai Zhang , Lixiang Chen

$N$-body non efimovian bound or quasi-bound states for particles with short range interactions are considered in arbitrary dimensions. The different resonance regimes near the threshold are depicted by using a generalization of the…

量子气体 · 物理学 2024-10-09 Ludovic Pricoupenko

Evidence has been mounting for the existence of black holes with masses from 10^2 to 10^4 M_Solar associated with stellar clusters. Such intermediate-mass black holes (IMBHs) will encounter other black holes in the dense cores of these…

天体物理学 · 物理学 2009-11-07 Kayhan Gultekin , M. Coleman Miller , Douglas P. Hamilton

We study black-hole binaries in the intermediate-mass-ratio regime 0.01 < q < 0.1 with a new technique that makes use of nonlinear numerical trajectories and efficient perturbative evolutions to compute waveforms at large radii for the…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Carlos O. Lousto , Hiroyuki Nakano , Yosef Zlochower , Manuela Campanelli

In this paper, we propose a new type of bulk-boundary correspondence as a generic approach to theoretically and experimentally detect fragile topological states. When the fragile phase can be written as a difference of a trivial atomic…

介观与纳米尺度物理 · 物理学 2020-03-18 Zhi-Da Song , Luis Elcoro , B. Andrei Bernevig

Quantum correlations represent a fundamental tool for studies ranging from basic science to quantum technologies. Different non-classical correlations have been identified and studied, as entanglement and discord. In this Paper we explore…

量子物理 · 物理学 2016-12-15 E. Moreva , M. Gramegna , M. A. Yurischev

We investigate the interaction between a non-rotating black hole and incoming gravitational waves using the characteristic formulation of the Einstein field equations, framed as a Bondi problem. By adopting retarded time as the null…

广义相对论与量子宇宙学 · 物理学 2025-05-16 H. P. de Oliveira

We analyze a new numerical relativity dataset of spinning but nonprecessing binary black holes on eccentric orbits, with eccentricities from approximately $0.1$ to $0.5$, with dimensionless spins up to $0.75$ included at mass ratios…