Surface density profile and surface tension of the one-component classical plasma

1983 ◽  
Vol 119 (1-2) ◽  
pp. 356-368 ◽  
Author(s):  
P. Ballone ◽  
G. Senatore ◽  
M.P. Tosi
Keyword(s):  
Surface Tension ◽  
Density Profile ◽  
Surface Density ◽  
Classical Plasma ◽  
The One

Surface density profile of the one-component plasma

1983 ◽  
Vol 16 (11) ◽  
pp. 2183-2195 ◽  
Author(s):  
J P Badiali ◽  
M L Rosinberg ◽  
D Levesque ◽  
J J Weis
Keyword(s):  
Density Profile ◽  
Surface Density ◽  
Component Plasma ◽  
The One

scholarly journals An Existence Theory for Gravity–Capillary Solitary Water Waves

Water Waves ◽  
2021 ◽  
Author(s):  
M. D. Groves
Keyword(s):  
Surface Tension ◽  
Water Waves ◽  
Applied Mathematics ◽  
Spatial Dynamics ◽  
Existence Theory ◽  
Water Wave Problem ◽  
Reduction Methods ◽  
Centre Manifold Reduction ◽  
Weak Surface ◽  
The One

AbstractIn the applied mathematics literature solitary gravity–capillary water waves are modelled by approximating the standard governing equations for water waves by a Korteweg-de Vries equation (for strong surface tension) or a nonlinear Schrödinger equation (for weak surface tension). These formal arguments have been justified by sophisticated techniques such as spatial dynamics and centre-manifold reduction methods on the one hand and variational methods on the other. This article presents a complete, self-contained account of an alternative, simpler approach in which one works directly with the Zakharov–Craig–Sulem formulation of the water-wave problem and uses only rudimentary fixed-point arguments and Fourier analysis.

The density profile and surface tension of a drop

1981 ◽  
Vol 16 ◽  
pp. 33 ◽  
Author(s):  
S. J. Hemingway ◽  
J. R. Henderson ◽  
J. S. Rowlinson
Keyword(s):  
Surface Tension ◽  
Density Profile

scholarly journals Exact and Asymptotic Features of the Edge Density Profile for the One Component Plasma in Two Dimensions

2014 ◽  
Vol 158 (5) ◽  
pp. 1147-1180 ◽  
Author(s):  
T. Can ◽  
P. J. Forrester ◽  
G. Téllez ◽  
P. Wiegmann
Keyword(s):  
Density Profile ◽  
Two Dimensions ◽  
Edge Density ◽  
Component Plasma ◽  
The One

scholarly journals A Halo Occupation Interpretation of Quasars at z ∼ 1.5 Using Very Small-Scale Clustering Information

2019 ◽  
Vol 486 (1) ◽  
pp. 274-282 ◽  
Author(s):  
S Eftekharzadeh ◽  
A D Myers ◽  
E Kourkchi
Keyword(s):  
Dark Matter ◽  
Density Profile ◽  
Small Scale ◽  
Minimum Mass ◽  
Concentration Parameter ◽  
Free Parameters ◽  
The One ◽  
Halo Occupation Distribution ◽  
Best Fit

Abstract We combine the most precise small-scale ($\lt 100\, \rm h^{-1}kpc$) quasar clustering constraints to date with recent measurements at large scales ($\gt 1\, \rm h^{-1}Mpc$) from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) to better constrain the satellite fraction of quasars at z ∼ 1.5 in the halo occupation formalism. We build our Halo Occupation Distribution (HOD) framework based on commonly used analytic forms for the one and two-halo terms with two free parameters: the minimum halo mass that hosts a central quasar and the fraction of satellite quasars that are within one halo. Inspired by recent studies that propose a steeper density profile for the dark matter haloes that host quasars, we explore HOD models at kiloparsec scales and best-fit parameters for models with 10 × higher concentration parameter. We find that an HOD model with a satellite fraction of $f_{\rm sat} = 0.071_{-0.004}^{+0.009}$ and minimum mass of $\rm M_{m} = 2.31_{-0.38}^{+0.41} \times 10^{12}\, \, \rm h^{-1} M_{\odot }$ for the host dark matter haloes best describes quasar clustering (on all scales) at z ∼ 1.5. Our results are marginally inconsistent with earlier work that studied brighter quasars, hinting at a luminosity-dependence to the one-halo term.

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