「Spherically」の共起表現一覧(1語右で並び替え)
該当件数 : 47件
| It comprises around 500 facets, which are | spherically arranged, and the whole eye is movable by u |
| The concept of a photon sphere in a static | spherically metric was generalized to a photon surface |
| The ball is made from eight | spherically molded panels and has a textured surface in |
| This means that a | spherically pulsating star cannot emit gravitational wa |
| n-luciferase system located in thousands of | spherically shaped organelles, or “microsources”, locat |
| For a general static | spherically symmetric metric |
| For a | spherically symmetric spacetime M, there are precisely |
| with the loop orbits which are observed in | spherically symmetric or axisymmetric systems. |
| In addition to the family of static | spherically symmetric perfect fluids, noteworthy rotati |
| In the theory of Lorentzian manifolds, | spherically symmetric spacetimes admit a family of nest |
| Within a | spherically symmetric mass distribution, it is possible |
| s give the same result for a general static | spherically symmetric metric. |
| Suppose we have a | spherically symmetric star of fixed mass which is exper |
| It states that any | spherically symmetric solution of the source-free Maxwe |
| In an isotropic chart (on a static | spherically symmetric spacetime), the line element take |
| For | spherically symmetric spacetimes, every point in the di |
| asional application in the theory of static | spherically symmetric perfect fluids. |
| his means that the exterior region around a | spherically symmetric gravitating object must be static |
| it was assumed that the metric was vacuum, | spherically symmetric and static. |
| ein equations for a general time-invariant, | spherically symmetric metric. |
| proof that black holes cannot form from the | spherically symmetric gravitational collapse of a star. |
| to an energy condition, a black hole in any | spherically symmetric spacetime must be surrounded by a |
| ectromagnetism, Birkhoff's theorem concerns | spherically symmetric static solutions of Maxwell's fie |
| where the problem assumes some number n of | spherically symmetric masses. |
| ies are then interpreted as rotations and a | spherically symmetric spacetime is often described as o |
| A | spherically symmetric spacetime can be characterised in |
| mportant special case is that of the static | spherically symmetric perfect fluid solutions. |
| ltrarelativistic encounter with an isolated | spherically symmetric object. |
| tion (which models the exterior of a static | spherically symmetric object endowed with a massless mi |
| uations reduce to the MOND equations in the | spherically symmetric case, although they differ somewh |
| ativity, Birkhoff's theorem states that any | spherically symmetric solution of the vacuum field equa |
| e Lie algebra of Killing vector fields of a | spherically symmetric static spacetime takes the same f |
| A | spherically symmetric spacetime is a spacetime whose is |
| ired, as Birkhoff's theorem states that any | spherically symmetric vacuum solution of Einstein's fie |
| detected that the X-ray halo has an almost | spherically symmetric appearance, except for two locali |
| d Instability of the Cauchy Horizon for the | Spherically Symmetric Einstein-Maxwell-Scalar Field Equ |
| TOV) equation constrains the structure of a | spherically symmetric body of isotropic material which |
| spherical coordinate chart on a static and | spherically symmetric spacetime, which is adapted to th |
| ystem; that is the CoM of the system in the | spherically symmetric One Body Case, or that of the com |
| In a | spherically symmetric star at dynamic equilibrium there |
| e (for example, in deriving an exact static | spherically symmetric solution of the Einstein field eq |
| For isolated | spherically symmetric solutions of the Einstein field e |
| well, e.g. about one of the branches of its | spherically symmetric solution found by Boulware and De |
| al solid solutions, these stress fields are | spherically symmetric, meaning they have no shear stres |
| it expands by nearly 5 nm and changes from | spherically symmetrical to icosahedrally symmetrical. |
| ving the conditions for fusion in imploding | spherically symmetrical fuel capsules. |
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