Signature reversal invariance
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Published version
Accepted version
Author(s)
Duff, MJ
Kalkkinen, J
Type
Journal Article
Abstract
We consider the signature reversing transformation of the metric tensor induced by the chiral transformation of the curved space gamma matrices in spacetimes with signature , which also induces a spacetime orientation reversal. We conclude: (1) It is a symmetry only for chiral theories with , with k integer. (2) Yang–Mills theories require dimensions with T even for which even rank antisymmetric tensor field strengths and mass terms are also allowed. For example, super-Yang–Mills is ruled out. (3) Gravitational theories require dimensions with T odd, for which the symmetry is preserved by coupling to odd rank field strengths. In , for example, it is a symmetry of and type IIB supergravity but not type IIA. A cosmological term and also mass terms are forbidden but non-minimal coupling is permitted. (4) Spontaneous compactification from leads to interesting but different symmetries in lower dimensions such as , so Yang–Mills terms, Kaluza–Klein masses and a cosmological constant may then appear. As a well-known example, IIB permits .
Date Issued
2006-12-04
Date Acceptance
2006-09-22
Citation
Nuclear Physics B, 2006, 758 (1-2), pp.161-184
ISSN
0550-3213
Publisher
Elsevier
Start Page
161
End Page
184
Journal / Book Title
Nuclear Physics B
Volume
758
Issue
1-2
Copyright Statement
© 2006 Published by Elsevier B.V.
Identifier
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000242495900007&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
Subjects
Science & Technology
Physical Sciences
Physics, Particles & Fields
Physics
COSMOLOGICAL CONSTANT PROBLEM
SUPERGRAVITY
Publication Status
Published
Date Publish Online
2006-10-16