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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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ing the gravitational field outside a rotating axisymmetric,<br />

electrically charged source. When<br />

the electric charge is zero, the metric becomes<br />

the Kerr metric.<br />

The line element in Boyer–Lindquist coordinates(t,r,θ,φ)is<br />

ds 2 =−ρ<br />

+ 2<br />

ρ 2<br />

2 <br />

dt2<br />

2<br />

<br />

<br />

dφ 2 − 2aMr<br />

2 dt<br />

+ ρ2<br />

dr2 +ρ 2 dθ 2 ,<br />

2<br />

whereρ 2 =r 2 +a 2 cos 2 θ,=(r −r+)(r −<br />

r−), <strong>and</strong> 2 =(r 2 +a 2 ) 2 −a 2 sin 2 θ. The<br />

quantityM is the ADM mass of the source,a≡<br />

J/M its angular momentum per unit mass, <strong>and</strong><br />

Q its electric charge. WhenQ= 0 one also has<br />

an electromagnetic field given by<br />

Frt = Q r2 −a 2 cos 2 θ<br />

ρ 4<br />

Fφr = a sin 2 θFrt<br />

Ftθ = Q a2 r sin 2θ<br />

ρ 4<br />

Fθφ = r2 +a 2<br />

a<br />

Ftθ .<br />

For M 2 < a 2 +Q 2 the metric describes<br />

a naked singularity at r = 0 <strong>and</strong> θ = π/2.<br />

For M 2 ≥ a 2 +Q 2 the metric describes<br />

a charged, spinning black hole. See also<br />

Reissner–Nordström metric, black hole, naked<br />

singularity.<br />

Kerr–Schild space-times The collection of<br />

metrics<br />

ds 2 = λℓaℓbdx a dx b + ds 2 0<br />

where λ is the parameter <strong>and</strong> ds2 0 is the “seed”<br />

metric, often assumed to be the Minkowski metric.<br />

The vector ℓ is null with respect to all metrics<br />

of the collection. Many space-times, e.g.,<br />

the Kerr metric <strong>and</strong> the plane-fronted gravitational<br />

waves, are in the Kerr–Schild class.<br />

Keulegan–Carpenter Number A dimensionless<br />

parameter used in the study of waveinduced<br />

forces on structures. The Keulegan–<br />

Carpenter Number is defined as ūmaxT/D,<br />

© 2001 by CRC Press LLC<br />

Killing horizon<br />

where ūmax is the maximum wave-induced velocity,<br />

averaged over the water depth, T is wave<br />

period, <strong>and</strong> D is structure diameter.<br />

K-function Diffuse attenuation coefficient.<br />

Kibble mechanism Process by which defects<br />

(strings, monopoles, domain walls) are<br />

produced in phase transitions occurring in the<br />

matter. In the simplest cases there is a field<br />

φ (called the Higgs field) whose lowest-energy<br />

state evolves smoothly from an expected value<br />

of zero at high temperatures to some nonzero<br />

φ at low temperatures which gives minimum<br />

energies, but there is more than one such minimum<br />

energy (vacuum) configuration. Both thermal<br />

<strong>and</strong> quantum fluctuations influence the new<br />

value taken by φ, leading to the existence of domains<br />

wherein φ is coherent <strong>and</strong> regions where it<br />

is not. The coherent regions have typical size ξ,<br />

the coherence length. Thus, points separated by<br />

r ≫ ξ will belong to domains with, in principle,<br />

arbitrarily different orientations of the field. It is<br />

the interfaces of these different regions (sheets,<br />

strings, points) which become the topological<br />

defects. In cosmology, this is viewed as occurring<br />

in the early universe. Because of the finite<br />

speed of light, ξ is bounded by the distance light<br />

can travel in one Hubble time: ξ ∼

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