Additional Z gauge bosons are predicted by a wide variety of extensions of the standard model (SM). Possibilities include TeV-scale bosons with electroweak coupling, very light bosons which nearly decouple from the standard model particles, and bosons which communicate with a quasi-hidden sector. A broad survey is given of the theoretical possibilities and of the physics implications for particle physics and cosmology. Several novel examples, including light Z s suggested by PAMELA, Stueckelberg Z s, and Z s associated with the mediation of supersymmetry breaking, are described.
MOTIVATIONSAn additional Z gauge boson is one of the best motivated extensions of the standard model or MSSM. String and grand unified theories often involve large underlying groups, or (in the case of Type IIa constructions) promote SU(n) groups to U(n). In many cases, it is more difficult to break the U(1) generators than the non-abelian ones, implying that extra Z s may survive to low energies as accidental remnants of the symmetry breaking. Also, many supersymmetric U(1) models provide a natural solution to the µ problem. In that case both the SU(2) ×U(1) and U(1) breaking scales are set by SUSY breaking scale (unless the breaking is associated with a flat direction), so one naturally expects the Z mass to be comparable to the electroweak scale, up to an order of magnitude or so. Similarly, alternative electroweak models (such as leftright symmetry) or alternatives to the elementary Higgs mechanisms, e.g., dynamical symmetry breaking or Little Higgs models, involve new TeV scale physics and extended gauge groups that often lead to new TeV-scale Z s. Models in which the standard model gauge bosons can propagate in large and/or warped extra dimensions involve Kaluza-Klein excitations, with M ∼ R −1 ∼ 2 TeV×(10 −17 cm/R) in the large dimension case. Another aspect is that Z s may provide a weak coupling between the ordinary sector of matter and other sectors associated with dark matter or with supersymmetry breaking. Finally, the existence of an extra Z , especially at the TeV scale, would have extensive implications for collider physics and cosmology. In this talk I will describe selected recent developments. More general treatments may be found in several recent reviews [1, 2, 3]. arXiv:0909.3260v2 [hep-ph]