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相关论文: Standing waves in the Universe

200 篇论文

In the standard theory of the large scale structure formation, matter accretes onto high density perturbations via gravitational instability. Collisionless dark matter forms caustics around such structures, while collisional baryonic matter…

天体物理学 · 物理学 2007-05-23 Dongsu Ryu , Hyesung Kang

The current observational evidences suggest there are about hundred billion galaxies in the observable universe and within each, on an average, about hundred billion stars. But no cosmological model indicates as to why there are these many…

综合物理 · 物理学 2012-02-08 C Sivaram , Kenath Arun

We study experimentally how waves affect distribution of particles that float on a water surface. We show that clustering of small particles in a standing wave is a nonlinear effect with the clustering time decreasing as the square of the…

混沌动力学 · 物理学 2007-05-23 P. Denissenko , G. Falkovich , S. Lukaschuk

Hydrodynamic waves propagate through stellar interiors, transporting energy and angular momentum. They can also advect fluid elements to produce mixing, but this effect has not been quantified from first principles. We derive the leading…

太阳与恒星天体物理 · 物理学 2022-09-20 Adam S. Jermyn

Turbulence is defined as an eddy-like state of fluid motion where the inertial-vortex forces of the eddies are larger than all the other forces that tend to damp the eddies out. Fossil turbulence is a perturbation produced by turbulence…

流体动力学 · 物理学 2012-04-30 Carl H. Gibson

We present a new perspective on the symmetries that govern the formation of large-scale structures across the Universe, particularly focusing on the transition from the seeds of galaxy clusters to the seeds of galaxies themselves. We…

宇宙学与河外天体物理 · 物理学 2024-03-28 Giovanni Montani , Nakia Carlevaro

Most cosmological structures in the universe spin. Although structures in the universe form on a wide variety of scales from small dwarf galaxies to large super clusters, the generation of angular momentum across these scales is poorly…

星系天体物理 · 物理学 2021-06-14 Peng Wang , Noam I. Libeskind , Elmo Tempel , Xi Kang , Quan Guo

We present two dimensional hydrodynamic calculations of free expanding supergalactic winds, taking into consideration strong radiative cooling. Our main premise is that supergalactic winds are powered by collections of superstar clusters.…

天体物理学 · 物理学 2009-11-10 G. Tenorio-Tagle , S. Silich , C. Munoz-Tunon

We generalize the big-bang model in a previous paper by extending the real vacuum scalar field to a complex vacuum scalar field, within the FLRW framework. The phase dynamics of the scalar field, which makes the universe a superfluid, is…

广义相对论与量子宇宙学 · 物理学 2012-10-11 Kerson Huang , Hwee-Boon Low , Roh-Suan Tung

Clusters of galaxies, the largest collapsed structures in the Universe, are located at the intersection of extended filaments of baryons and dark matter. Cosmological accretion onto clusters through large scale filaments adds material at…

The stars of the middle main sequence often have relatively quiescent outer layers and spot-like chemical structures may develope in their atmospheres. Recent observations show that abundance peculiarities can change as stars evolve on the…

太阳与恒星天体物理 · 物理学 2016-02-17 Vadim Urpin

The universe's large-scale structure forms a vast, interconnected network of filaments, sheets, and voids known as the cosmic web. For decades, astronomers have observed that the orientations of neighboring galaxy clusters within these…

宇宙学与河外天体物理 · 物理学 2025-06-25 Michael J. West , Roberto De Propris , Maret Einasto , Z. L. Wen , J. L. Han

The local Universe displays a rich hierarchical pattern of galaxy clusters and superclusters. The early Universe, however, was almost smooth, with only slight 'ripples' seen in the cosmic microwave background radiation. Models of the…

天体物理学 · 物理学 2009-10-31 Peter Coles , Lung-Yih Chiang

Research done during the previous century established our Standard Cosmological Model. There are many details still to be filled in, but few would seriously doubt the basic premise. Past surveys have revealed that the large-scale…

天体物理学 · 物理学 2008-11-26 Bernard J. T. Jones , Vicent J. Martinez , Enn Saar , Virginia Trimble

The kinetic approach to the formation of the filaments in the large-scale matter distribution in the Universe is considered within the Vlasov formalism. The structures arise due to the self-consistent dynamics, along with the repulsive term…

宇宙学与河外天体物理 · 物理学 2022-10-19 V. G. Gurzadyan , N. N. Fimin , V. M. Chechetkin

Clusters of galaxies are storage rooms of cosmic rays. They confine the hadronic component of cosmic rays over cosmological time scales due to diffusion, and the electron component due to energy losses. Hadronic cosmic rays can be…

天体物理学 · 物理学 2015-06-24 Pasquale Blasi

The large scale distribution of galaxies in the universe displays a complex pattern of clusters, super-clusters, filaments and voids with sizes limited only by the boundaries of the available samples. A quantitative statistical…

宇宙学与河外天体物理 · 物理学 2015-05-20 Francesco Sylos Labini , Luciano Pietronero

The class of non-stationary braneworld models generated by the coupled gravitational and scalar fields is reviewed. The model represents a brane in a space-time with single time and one large (infinite) and several small (compact)…

高能物理 - 理论 · 物理学 2016-05-19 Merab Gogberashvili , Irakli Mantidze , Otari Sakhelashvili , Tsotne Shengelia

(ABBREVIATED) Understanding the formation of stars in galaxies is central to much of modern astrophysics. In this review the relation between interstellar turbulence and star formation is discussed. Supersonic turbulence can provide support…

天体物理学 · 物理学 2009-09-29 Ralf S. Klessen

A new, very different physical model of the universe is proposed. Its virtues include unifying relativity and quantum mechanics, and particles with de Broglie waves. It also appears to provide a truly unified physical basis for…

综合物理 · 物理学 2008-02-03 Ben Kristoffen