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19932002
most citedHydrodynamic theory for dissipative hard spheres with multi-particle interactions

2 citations · 2 across the 1 of their papers we have counts for

collaborators

6 papers

cond-mat.stat-mech20022 cited

Hydrodynamic theory for dissipative hard spheres with multi-particle interactions

Stefan Luding, Alexander Goldshtein

Extensions to kinetic theory and hydrodynamic models are proposed that account for the existence of multi-particle contacts. In the presence of multi-particle contacts (involving e…

physics.flu-dyn2000

Threshold amplitudes for transition to turbulence in a pipe

Lloyd N. Trefethen, S. J. Chapman, Dan S. Henningson +3

Although flow in a circular pipe is stable to infinitesimal perturbations, it can be excited to turbulence by finite perturbations whose minimal amplitude shrinks as R goes to infi…

astro-ph1999

Surface photometry of bulge dominated low surface brightness galaxies

M. Beijersbergen, W. J. G. de Blok, J. M. van der Hulst

We present results of broad band {BVRI} observations of a sample of galaxies with a low surface brightness (LSB) disk and a bulge. These galaxies are well described as exponential…

astro-ph1999

Photomeson production in astrophysical sources

A. Muecke, J. P. Rachen, R. Engel +2

Photomeson production is the main energy loss for relativistic nucleons in dense radiation fields like the cosmic microwave background and the radiation fields in Gamma Ray Bursts…

astro-ph1998

Star formation and the interstellar medium in low surface brightness galaxies. II. Deep CO observations of low surface brightness disk galaxies

W. J. G. de Blok, J. M. van der Hulst

We present deep, pointed CO() observations of three late-type LSB galaxies. The beam-size was small enough that we could probe different environments (\HI maximum, \H…

astro-ph1993

Cosmic Rays, III. The CR spectrum between 1 GeV and 10^4 GeV and the radio emission from supernova remnants

Peter L. Biermann, Richard G. Strom

We develop a theory to account for the cosmic ray spectrum between 1 GeV and 10^4 GeV following the earlier papers of this series. We use the basic concept that the cosmic ray part…