Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2004-08-10
Phys.Rev.D70:106004,2004; Erratum-ibid.D71:029901,2005
Physics
High Energy Physics
High Energy Physics - Theory
39 pages, 1 figure
Scientific paper
10.1103/PhysRevD.70.106004
We consider a picture in which the transition from a big crunch to a big bang corresponds to the collision of two empty orbifold planes approaching each other at a constant non-relativistic speed in a locally flat background space-time, a situation relevant to recently proposed cosmological models. We show that $p$-brane states which wind around the extra dimension propagate smoothly and unambiguously across the orbifold plane collision. In particular we calculate the quantum mechanical production of winding M2-branes extending from one orbifold to the other. We find that the resulting density is finite and that the resulting gravitational back-reaction is small. These winding states, which include the string theory graviton, can be propagated smoothly across the transition using a perturbative expansion in the membrane tension, an expansion which from the point of view of string theory is an expansion in {\it inverse} powers of $\alpha'$. We argue that interactions should be well-behaved because the string coupling tends to zero at the crunch. The production of massive Kaluza-Klein states should also be exponentially suppressed for small collision speeds. We contrast this good behavior with that found in previous studies of strings in Lorentzian orbifolds.
Perry Malcolm
Steinhardt Paul J.
Turok Neil
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