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“Dark” Z implications for parity violation, rare meson decays, and Higgs physics
General consequences of mass mixing between the ordinary Z boson and a relatively light Z sub(d) boson, the "dark" Z, arising from a U(1) sub(d) gauge symmetry, associated with a hidden sector such as dark matter, are examined. New effects beyond kinetic mixing are emphasized. Z-Z sub(d) m...
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Published in: | Physical review. D, Particles, fields, gravitation, and cosmology Particles, fields, gravitation, and cosmology, 2012-06, Vol.85 (11), Article 115019 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | General consequences of mass mixing between the ordinary Z boson and a relatively light Z sub(d) boson, the "dark" Z, arising from a U(1) sub(d) gauge symmetry, associated with a hidden sector such as dark matter, are examined. New effects beyond kinetic mixing are emphasized. Z-Z sub(d) mixing introduces a new source of low energy parity violation well explored by possible future atomic parity violation and planned polarized electron scattering experiments. Rare K(B) meson decays into [pi](K)l super(+)l super(-) (l =e, mu ) and [pi](K)vv are found to already place tight constraints on the size of Z-Z sub(d) mixing. Those sensitivities can be further improved with future dedicated searches at K and B factories as well as binned studies of existing data. Z-Z sub(d) mixing can also lead to the Higgs decay H arrow right ZZ sub(d), followed by Z arrow right l(ProQuest: Formulae and/or non-USASCII text omitted)l(ProQuest: Formulae and/or non-USASCII text omitted) and Z sub(d) arrow right l(ProQuest: Formulae and/or non-USASCII text omitted)l(ProQuest: Formulae and/or non-USASCII text omitted) or "missing energy," providing a potential hidden sector discovery channel at the Large Hadron Collider. An illustrative realization of these effects in a 2 Higgs doublet model is presented. |
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ISSN: | 1550-7998 1550-2368 |
DOI: | 10.1103/PhysRevD.85.115019 |