Rare top quark decays [Formula presented] and [Formula presented]
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN: 1550-2368, Vol: 56, Issue: 1, Page: 458-466
1997
- 45Citations
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Citations45
- Citation Indexes45
- 45
- CrossRef28
Article Description
The large value of the top quark mass implies that the rare top quark decays [Formula presented], [Formula presented], and [Formula presented], and [Formula presented] and [Formula presented], are kinematically allowed so long as [Formula presented] or [Formula presented] respectively. The partial decay widths for these decay modes are calculated in the standard model. The partial widths depend sensitively on the precise value of the top quark mass. The branching ratio for [Formula presented] is as much as [Formula presented] for [Formula presented] GeV, and could be observable at the CERN Large Hadron Collider. The rare decay modes [Formula presented] and [Formula presented] are highly Glashow-Iliopoulos-Maiani (GIM) suppressed, and thus provide a means for testing the GIM mechanism for three generations of quarks in the [Formula presented], [Formula presented], [Formula presented] sector. © 1997 The American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=0000881173&origin=inward; http://dx.doi.org/10.1103/physrevd.56.458; https://link.aps.org/doi/10.1103/PhysRevD.56.458; http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.56.458/fulltext; http://link.aps.org/article/10.1103/PhysRevD.56.458
American Physical Society (APS)
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