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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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volume scattering function (VSF) The ratio<br />

of the scattered intensity [W sr −1 ] to the incident<br />

irradiance [W m −2 ] per unit volume [m 3 ],<br />

given in [m −1 sr −1 ]; the integral of the volume<br />

scattering function over all directions <strong>and</strong> all<br />

final wavelengths is the scattering coefficient;<br />

the VSF can be written as the product of the<br />

phase function [sr −1 ] <strong>and</strong> the scattering coefficient<br />

[m −1 ].<br />

volumetric water content (or simply water<br />

content) (θ) The ratio of liquid water volume to<br />

the total soil or rock volume: θ =Vw/Vs, where<br />

Vw is the volume of water in the sample, <strong>and</strong> Vs<br />

is the total volume of soil or rock in the sample.<br />

The theoretical range of the volumetric water<br />

content is from 0 (completely dry) to saturation<br />

(porosity or φ), but the range in natural systems<br />

is generally much less than this.<br />

von Mises criterion The condition by which<br />

a polycrystal can deform coherently to large<br />

strains by dislocation slip. von Mises criterion<br />

points out that five independent slip systems<br />

are needed in order to deform a polycrystalline<br />

material by crystallographic slip. This is<br />

because arbitrary shape change must be possible<br />

to satisfy the displacement compatibility at<br />

grain boundaries.<br />

vortex defect of the vacuum See cosmic<br />

string.<br />

vortex street The series of vortices shed systematically<br />

downstream from a body in a rapid<br />

fluid flow (sufficiently high Reynolds number).<br />

For a cylindrically symmetrical body, a pair of<br />

symmetrically placed opposite vortices (with a<br />

sign which can be deduced from the streamflow)<br />

form behind the body on either side of the down-<br />

© 2001 by CRC Press LLC<br />

vorton<br />

stream direction. Small disturbances then lead<br />

to a shedding of one of the two vortices, <strong>and</strong><br />

subsequently alternate shedding of vortices of<br />

opposite sign. The trail of vortices behind the<br />

body is the vortex street.<br />

vorticity A vector measure, ω, of local rotation<br />

in a fluid flow:<br />

ω = ∇ × v .<br />

vorton Equilibrium configurations of conducting<br />

cosmic string loops, where the string<br />

tension, tending to make the loop collapse, is<br />

balanced by the centrifugal repulsion due to rotation.<br />

Symmetry reasons (Lorentz invariance<br />

along the string world sheet) forbid rotating configurations<br />

for Goto–Nambu strings <strong>and</strong>, therefore,<br />

vortons can only arise in theories where<br />

cosmic strings have a microscopic internal structure,<br />

like currents flowing along the core.<br />

The existence of vorton equilibrium configurations<br />

would prevent the loops from decaying<br />

away in the form of radiation. They would then<br />

evolve like ordinary (eventually charged) nonrelativistic<br />

matter very early on in the history of<br />

the universe, eventually disrupting some of the<br />

predictions of st<strong>and</strong>ard cosmology.<br />

This possible incompatibility is known as the<br />

vorton excess problem. Many mechanisms aiming<br />

at diluting vorton overdensity are currently<br />

being studied. If successful, vortons could stop<br />

being a problem <strong>and</strong> would become one more<br />

interesting c<strong>and</strong>idate for the non-baryonic dark<br />

matter that combined observations <strong>and</strong> theoretical<br />

models tend to require. See CHUMP,<br />

conducting string, cosmic string, Goto–Nambu<br />

string.<br />

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