例文 | 共起表現 |
「space-times」の共起表現一覧(1語右で並び替え)
該当件数 : 26件
Lorentzian manifolds, spherically symmetric | spacetimes admit a family of nested round spheres. |
the theorem to asymptotically anti-de Sitter | spacetimes and to Einstein-Maxwell theory. |
Press 2003 (Kundt | spacetimes are studied in Chapter 31) |
In mathematical physics, VSI | spacetimes are Lorentzian manifolds with all polynomial |
In mathematical physics, Kundt | spacetimes are Lorentzian manifolds admitting a geodesi |
In this reformulation, | spacetimes are sliced up into spatial hyperslices in a |
illing vector fields may be used to classify | spacetimes, as there is a limit to the number of global |
of curvature invariants fails to distinguish | spacetimes as well as they distinguish Riemannian manif |
For spherically symmetric | spacetimes, every point in the diagram corresponds to a |
e mathematically independent, as there exist | spacetimes for which the weak cosmic censorship is vali |
VSI | spacetimes however also contain some other four-dimensi |
Ricci-flat Kundt | spacetimes in arbitrary dimension are algebraically spe |
VSI | spacetimes in higher dimensions have similar properties |
"Time machines", i.e. initially nice | spacetimes in which at some stage of evolution closed c |
Various approaches to classifying | spacetimes, including using the Segre classification of |
The significance of M-H | spacetimes is that they allow for the implementation of |
ed quantity for motion in the Kerr family of | spacetimes may be referred to as "Carter's constant". |
r non-zero cosmological constants, on curved | spacetimes quantum fields lose their interpretation as |
For | spacetimes satisfying asymptotic flatness, it is often |
try group of axisymmetric, stationary vacuum | spacetimes that are solutions of Einstein's equations o |
ve should hold for spacelike submanifolds of | spacetimes that are not necessarily time-symmetric. |
In the case of dynamical | spacetimes, the problem may be divided into the initial |
momentum is not conserved for general curved | spacetimes, unless it happens to be asymptotically rota |
hysics, in the theory of general relativity, | spacetimes with at least a 1-parameter group of isometr |
view D., 1990, (in press), Cauchy Problem in | Spacetimes with Closed Timelike Curves. |
the string theory community that background | spacetimes with different asymptotics can represent dif |
例文 | 共起表現 |
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