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相关论文: Planck-Kerr Turbulence

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General Relativity is extended into the quantum domain. A thought experiment is explored to derive a specific topological build-up for Planckian space-time. The presented arguments are inspired by Feynman's path integral for superposition…

综合物理 · 物理学 2013-07-18 Marco Spaans

It is shown that if kinetics of quantum transitions takes account of energy uncertainty of intermediate states, then it creates non-decaying correlations and non-averagable (flicker) fluctuations in the energy as well as in rates of…

统计力学 · 物理学 2018-12-21 Yuriy E. Kuzovlev

The understanding of turbulent flows is one of the biggest current challenges in physics, as no first-principles theory exists to explain their observed spatio-temporal intermittency. Turbulent flows may be regarded as an intricate…

流体动力学 · 物理学 2021-12-08 Juan Ignacio Polanco , Nicolás P. Müller , Giorgio Krstulovic

An evolution of a spherical region, subjected to uniform buoyancy force, is investigated. Incompressibility and axial symmetry are assumed, together with a buoyancy discontinuity at the boundary. The boundary turns into a vortex sheet and…

流体动力学 · 物理学 2023-05-12 Paweł Jędrejko , Jun-Ichi Yano , Marta Wacławczyk

We study the interplay between turbulent heating, mixing, and radiative cooling in an idealized model of cool cluster cores. Active galactic nuclei (AGN) jets are expected to drive turbulence and heat cluster cores. Cooling of the…

星系天体物理 · 物理学 2015-06-19 Nilanjan Banerjee , Prateek Sharma

The Black Hole Uncertainty Principle correspondence proposes a connection between the Uncertainty Principle on microscopic scales and black holes on macroscopic scales. This is manifested in a unified expression for the Compton wavelength…

广义相对论与量子宇宙学 · 物理学 2014-02-07 B. J. Carr

We analyze the spectrum of gravitational waves generated by the induced spectrum of tensor fluctuation during warm natural inflation. In our previous work it has been demonstrated that an epoch of warm natural inflation can lead to…

宇宙学与河外天体物理 · 物理学 2023-06-19 Miguel Correa , Mayukh R. Gangopadhyay , Nur Jaman , Grant J. Mathews

We consider classically scale-invariant theories with non-minimally coupled scalar fields, where the Planck mass and the hierarchy of physical scales are dynamically generated. The classical theories possess a fixed point, where scale…

高能物理 - 唯象学 · 物理学 2017-05-03 K. Kannike , M. Raidal , C. Spethmann , H. Veermäe

A study of the high angular momentum particles 'atmosphere' near the Schwarzschild black hole horizon suggested that strong gravitational interactions occur at invariant distance of the order of $\sqrt[3]{M}$ (A. Casher et. al). We present…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Kirill Tuchin

The internal interactions of fluids occur at all scales therefore the resulting force fields have no reason to be smooth and differentiable. The release of the differentiability hypothesis has important mathematical consequences, like scale…

综合物理 · 物理学 2013-03-15 Louis de Montera

The wavelet regression detrended fluctuations of the reconstructed temperature for the past three ice ages: approximately 340000 years (Antarctic ice cores isotopic data), exhibit clear evidences of the galactic turbulence modulation up to…

星系天体物理 · 物理学 2010-07-12 A. Bershadskii

It is possible that black holes hide a core of Planckian density, sustained by quantum-gravitational pressure. As a black hole evaporates, the core remembers the initial mass and the final explosion occurs at macroscopic scale. We…

广义相对论与量子宇宙学 · 物理学 2015-06-19 Aurelien Barrau , Carlo Rovelli

If you fall into a real astronomical black hole (choosing a supermassive black hole, to make sure that the tidal forces don't get you first), then you will probably meet your fate not at a central singularity, but rather in the…

广义相对论与量子宇宙学 · 物理学 2015-03-13 Andrew J. S. Hamilton , Pedro P. Avelino

A nonlinear two dimensional fluid model of whistler turbulence is developed that nonlinearly couples wave magnetic field with electron density perturbations. This coupling leads essentially to finite compressibility effects in whistler…

空间物理 · 物理学 2015-05-18 Dastgeer Shaikh

We numerically solve Einstein's equations coupled to a scalar field in the interior of Kerr black holes. We find shock waves form near the inner horizon. The shocks grow exponentially in amplitude and need not be axisymmetric. Observers who…

广义相对论与量子宇宙学 · 物理学 2019-04-24 Paul M. Chesler , Erik Curiel , Ramesh Narayan

Since the idea of quantum turbulence was first proposed by Feynman, and later realized in experiments of superfluid helium and Bose-Einstein condensates, much emphasis has been put in finding signatures that distinguish quantum turbulence…

量子气体 · 物理学 2025-04-24 Julian Amette Estrada , Marc E. Brachet , Pablo D. Mininni

The quantum gravity vacuum must contain virtual fluctuations of black hole microstates. These extended-size fluctuations get `crushed' when a closed trapped surface forms, and turn into on-shell `fuzzball' states that resolve the…

高能物理 - 理论 · 物理学 2022-01-26 Samir D. Mathur

Nondifferentiable fluctuations in space-time on a Planck scale introduce stochastic terms into the equations for quantum states, resulting in a proposed new foundation for an existing alternative quantum theory, primary state diffusion…

量子物理 · 物理学 2015-06-26 I. C. Percival

Matter entanglement is a common chaotic structure in both quantum and classical systems. Turbulence can be pictured as a tangle of vortex filaments in superfluids and viscous vortices in classical fluids. However, it is hard to explain how…

流体动力学 · 物理学 2024-08-21 Weiyu Shen , Jie Yao , Yue Yang

The scattering process of two particles at Planck energies or beyond is calculated using the gravitational shock wave metric for a massive black hole. Then, the scattering between a heavy mass particle and a small mass one is deal with. The…

高能物理 - 理论 · 物理学 2007-05-23 Koichi HAYASHI , Toshiharu SAMURA