spherically's Usage Examples:

Tolman–Oppenheimer–Volkoff (TOV) equation constrains the structure of a spherically symmetric body of isotropic material which is in static gravitational.

Isotropy Rotational symmetry Particle in a spherically symmetric potential Gauss's theorem Weisstein, Eric W.

In general relativity, Birkhoff's theorem states that any spherically symmetric solution of the vacuum field equations must be static and asymptotically.

In order to convert a spherically expanding wavefront into a spherically converging one using only a single boundary between.

The gravitational force outside a spherically symmetric body is the same as if its entire mass were concentrated in.

fields are conservative or spherically symmetric.

However, a central force is conservative if and only if it is spherically symmetric or rotationally invariant.

In the theory of Lorentzian manifolds, spherically symmetric spacetimes admit a family of nested round spheres.

They contrast with the loop orbits that are observed in spherically symmetric or axisymmetric systems.

down by Sean Hayward as the minimal model which is regular, static, spherically symmetric and asymptotically flat.

In mathematics, a field K with an absolute value is called spherically complete if the intersection of every decreasing sequence of balls (in the sense.

An important problem in quantum mechanics is that of a particle in a spherically symmetric potential, i.

NSTX studies the physics principles of spherically shaped plasmas—hot ionized gases in which nuclear fusion will occur under.

describes spacetime under the influence of a massive, non-rotating, spherically symmetric object.

In mathematical physics, the Lemaître–Tolman metric is the spherically symmetric dust solution of Einstein's field equations.

Early models of Mira stars assumed that the star remained spherically symmetric during this process (largely to keep the computer modelling.

In physics, spherically symmetric spacetimes are commonly used to obtain analytic and numerical solutions to Einstein's field equations in the presence.

class of this galaxy is E0, indicating it is an elliptical galaxy with a spherically symmetric form.

gravitational simplifications that can be applied to objects inside or outside a spherically symmetrical body.

approximation lies in the potential in which the potential is assumed to be spherically symmetric in the muffin-tin region and constant in the interstitial region.