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相关论文: Standing waves in the Universe

200 篇论文

Galaxies represent the visible fabric of the Universe and there has been considerable progress recently in both observational and theoretical studies. The underlying goal is to understand the present-day diversity of galaxy forms, masses…

天体物理学 · 物理学 2007-05-23 Richard S Ellis

In a large scale view of the universe, galaxies are the basic unit of structure. A typical bright galaxy may contain 100 billion stars and span tens of thousands of light years, but the empty expanses between the galaxies are much larger…

天体物理学 · 物理学 2007-05-23 David H. Weinberg

Dark energy is the candidate that can produce effective negative pressure and make the galaxies and galaxy clusters move away from each other in an accelerated way. The structures of the Universe have evolved from some initial primordial…

宇宙学与河外天体物理 · 物理学 2021-10-07 Srijita Sinha

A hydrophilic floating sphere that is denser than water drifts to an amplitude maximum (antinode) of a surface standing wave. A few identical floaters therefore organize into antinode clusters. However, beyond a transitional value of the…

流体动力学 · 物理学 2015-05-15 Ceyda Sanlı , Detlef Lohse , Devaraj van der Meer

Our universe may have formed via bubble nucleation in an eternally-inflating background. Furthermore, the background may have a compact dimension---the modulus of which tunnels out of a metastable minimum during bubble nucleation---which…

高能物理 - 理论 · 物理学 2014-11-21 Michael P. Salem

In the multi-scale view of the star formation process the material flows from large molecular clouds down to clumps and cores. In this paradigm it is still unclear if it is gravity or turbulence that drives the observed supersonic…

星系天体物理 · 物理学 2022-09-21 A. Traficante , G. A. Fuller , A. Duarte-Cabral , D. Elia , M. H. Heyer , S. Molinari , N. Peretto , E. Schisano

Star complexes are the largest globular regions of star formation in galaxies. If there is a spiral density wave, nuclear ring, tidal arm, or other well-defined stellar structure, then gravitational instabilities in the gaseous component…

天体物理学 · 物理学 2007-05-23 Bruce G. Elmegreen

The theory of cosmological perturbations has become a cornerstone of modern quantitative cosmology since it is the framework which provides the link between the models of the very early Universe such as the inflationary Universe scenario…

高能物理 - 理论 · 物理学 2017-08-23 Robert H. Brandenberger

Astrophysical disks that are sufficiently cold and dense are linearly unstable to the formation of axisymmetric rings as a result of the disk's gravity. In practice, spiral structures are formed, which may in turn produce bound fragments.…

地球与行星天体物理 · 物理学 2022-08-17 Hongping Deng , Gordon I. Ogilvie

This is a short note on the spatiotemporal complexity of the dynamical state(s) of the universe at subhorizon scales (up to 300 Mpc). There are reasons, based mainly on infrared radiative divergences, to believe that one can encounter a…

天体物理学 · 物理学 2009-10-22 H. C. Rosu

In this contribution I summarize our current knowledge of the nature and significance of starburst-driven galactic superwinds. These flows are driven primarily by the kinetic energy supplied by supernovae. Superwinds are complex, multiphase…

天体物理学 · 物理学 2007-05-23 Timothy M. Heckman

We introduce a new class of self-sustained states, which may exist as single solitons or form multisoliton clusters, in driven passive cylindrical microresonators. Remarkably, such states are stabilized by the radiation they emit, which…

This paper contains a discussion on the quantum cosmic models, starting with the interpretation that all of the accelerating effects in the current universe are originated from the existence of a nonzero entropy of entanglement. In such a…

广义相对论与量子宇宙学 · 物理学 2010-01-22 Pedro F. Gonzalez-Diaz , Alberto Rozas-Fernandez

The distance contraction, as observed in electrical soundings over horizontally stratified earth (static system), is identified as a counterpart of Doppler shift in dynamical systems. Identification of Doppler-like effect in a stock-still…

天体物理学 · 物理学 2007-05-23 Edward Szaraniec

The tangled nodal lines (wave vortices) in random, three-dimensional wavefields are studied as an exemplar of a fractal loop soup. Their statistics are a three-dimensional counterpart to the characteristic random behaviour of nodal domains…

计算物理 · 物理学 2018-02-14 Alexander J. Taylor

Based on the proposed unifying theory of dark matter and quintessence, a novel nonlinear structure formation scenario is suggested. This top-down singular and turbulent scenario results in a bottom-up hierarchical clustering and is…

综合物理 · 物理学 2007-05-23 Reza Dastvan

The evolution of globular cluster systems in some galaxies can be cause of merging of globulars in the very central regions. This high stellar density favours the growth of a central nucleus via swallowing of surrounding stars. The infall…

天体物理学 · 物理学 2016-08-30 Roberto Capuzzo-Dolcetta , Paolo Miocchi

The universe is found to have undergone several phases in which the gravitational constant had different behaviors. During some epochs the energy density of the universe remained constant and the universe remained static. In the radiation…

天体物理学 · 物理学 2007-05-23 Arbab I. Arbab

Superconductivity, superfluidity, condensation, cluster formation, etc. are phenomena that might occur in many-particle systems. These are due to residual interactions between the particles. To explain these phenomena consistently in a…

核理论 · 物理学 2007-05-23 Michael Beyer

Evidence for wave-like corrugations are well established in the Milky Way and in nearby disc galaxies. These were originally detected as a displacement of the interstellar medium about the midplane, either in terms of vertical distance or…

星系天体物理 · 物理学 2022-07-28 Thor Tepper-Garcia , Joss Bland-Hawthorn , Ken Freeman