Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2004-06-22
Gen.Rel.Grav. 37 (2005) 1823-1831
Physics
High Energy Physics
High Energy Physics - Theory
5pages, 4figures, to be published in GRG
Scientific paper
10.1007/s10714-005-0162-4
We consider five dimensional deSitter spacetimes with a deficit angle due to the presence of a closed 2-brane and identify one dimension as an extra dimension. From the four dimensional viewpoint we can see that the spacetime has a structure similar to a Kaluza-Klein bubble of nothing, that is, four dimensional spacetime ends at the 2-brane. Since a spatial section of the full deSitter spacetime has the topology of a sphere, the boundary surface surrounds the remaining four dimensional spacetime, and can be considered as the celestial sphere. After the spacetime is created from nothing via an instanton which we describe, some four dimensional observers in it see the celestial sphere falling down, and will be in contact with a 2-brane attached on it.
Mukohyama Shinji
Shiromizu Tetsuya
Tomizawa Shinya
Uchida Yuki
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