Note that the Gowdy metric corresponding to ,
and
is the flat
Kasner metric. Consequently, the curvature tensor is in that case identically zero. For this solution,
. In particular, if
, the Kretschmann scalar need not necessarily be unbounded along
a causal curve ending at
.
http://www.livingreviews.org/lrr-2010-2 |
Living Rev. Relativity 13, (2010), 2
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