Huygens' principle for the Klein-Gordon equation in the de Sitter spacetime

被引:27
|
作者
Yagdjian, Karen [1 ]
机构
[1] Univ Texas Pan Amer, Dept Math, Edinburg, TX 78539 USA
关键词
OPERATORS;
D O I
10.1063/1.4821115
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this article we prove that the Klein-Gordon equation in the de Sitter spacetime obeys the Huygens' principle only if the physical mass m of the scalar field and the dimension n >= 2 of the spatial variable are tied by the equation m(2) = (n(2) - 1)/4. Moreover, we define the incomplete Huygens' principle, which is the Huygens' principle restricted to the vanishing second initial datum, and then reveals that the massless scalar field in the de Sitter spacetime obeys the incomplete Huygens' principle and does not obey the Huygens' principle, for the dimensions n = 1, 3, only. Thus, in the de Sitter spacetime the existence of two different scalar fields (in fact, with m = 0 and m(2) = (n(2) - 1)/4), which obey incomplete Huygens' principle, is equivalent to the condition n = 3, the spatial dimension of the physical world. In fact, Paul Ehrenfest in 1917 addressed the question: "Why has our space just three dimensions?". For n = 3 these two values of the mass are the endpoints of the so-called in quantum field theory the Higuchi bound. The value m(2) = (n(2) - 1)/4 of the physical mass allows us also to obtain complete asymptotic expansion of the solution for the large time. (C) 2013 AIP Publishing LLC.
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页数:18
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