BibTex format
@article{Duff:2006:10.1016/j.nuclphysb.2006.09.014,
author = {Duff, MJ and Kalkkinen, J},
doi = {10.1016/j.nuclphysb.2006.09.014},
journal = {Nuclear Physics B},
pages = {161--184},
title = {Signature reversal invariance},
url = {http://dx.doi.org/10.1016/j.nuclphysb.2006.09.014},
volume = {758},
year = {2006}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - 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 .
AU - Duff,MJ
AU - Kalkkinen,J
DO - 10.1016/j.nuclphysb.2006.09.014
EP - 184
PY - 2006///
SN - 0550-3213
SP - 161
TI - Signature reversal invariance
T2 - Nuclear Physics B
UR - http://dx.doi.org/10.1016/j.nuclphysb.2006.09.014
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000242495900007&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
VL - 758
ER -