29.03.2013 Views

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

tension head (ψ)<br />

is the energy-momentum tensor computed from<br />

the microscopic field configuration, in the particular<br />

case of a straight string. For an ordinary<br />

relativistic string we haveT tt +T zz = 0; hence<br />

we recover the equation of state for a structureless<br />

Goto–Nambu string, where U (the energy<br />

per unit length) <strong>and</strong> T are constant <strong>and</strong> equal<br />

to each other. For more general vortex-forming<br />

field theories, the corresponding cosmic string<br />

model will be characterized by variable tension<br />

<strong>and</strong> energy per unit length which, in a generic<br />

state, will be related by an inequality of the form<br />

T ≤ U. See duality in elastic string models, energy<br />

per unit length (cosmic string), equation of<br />

state (cosmic string), Goto–Nambu string.<br />

tension head (ψ) There is tension on pore<br />

water in the unsaturated zone because water is<br />

held to the mineral grains by surface-tension<br />

forces. It is conventional to measure pressure<br />

(p) relative to atmospheric pressure, thus in the<br />

unsaturated zone p0. Negative<br />

pressure is often called suction or tension, <strong>and</strong><br />

ψ is called tension head when p

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!