「space-times」の共起表現(1語右で並び替え) - Weblio英語共起表現検索


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Weblio 辞書 > 英和辞典・和英辞典 > space-timesに関連した共起表現

「space-times」の共起表現一覧(1語右で並び替え)

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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
                                                                                                   


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