| ID | 34169 |
| FullText URL | |
| Author |
Tsuno, S
Nakano, I
Tanaka, R
|
| Abstract | We present a quantitative study on sensitivities to the top-decay anomalous couplings, taking into account realistic experimental conditions expected at Tevatron and LHC. A double angular distribution of W and charged lepton in the top-decay is analyzed, using t<(t)<($)over bar> events in the leptons+jets channel. In order to improve sensitivities to the anomalous couplings, we apply two techniques: (i) We use a likelihood fitting method for full kinematical reconstruction of each top event. (ii) We develop a new effective spin reconstruction method for leptonically-decayed top quarks; this method does not require spin information of the antitop side. For simplicity, we neglect couplings of right-handed bottom quark as well as CP violating couplings. The 95% C.L. estimated bound on a ratio of anomalous couplings reads -0.81 < f(2)/f(1)<-0.70, -0.12 < f(2)/f(1)< 0.14 using 1000 reconstructed top events at Tevatron, while -0.74 < f(2)/f(1)<-0.72, -0.01 < f(2)/f(1)< 0.01 is expected with 100 k reconstructed top events at LHC, where only statistical errors are taken into account. A two-fold ambiguity in the allowed range remains when the number of events exceeds a few hundred. |
| Keywords | quark pair production
order qcd correction
spin correlations
linear
colliders
charged leptons
width
thvatron
collisions
threshold
|
| Note | Digital Object Identifer:10.1103/PhysRevD.73.054011
Published with permission from the copyright holder. This is the institute's copy, as published in Physical Review D, March 2006, Volume 73, Issue 5, Pages 12. Publisher URL:http://dx.doi.org/10.1103/PhysRevD.73.054011 Direct access to Thomson Web of Science record Copyright © 2006 The American Physical Society. All rights reserved. |
| Published Date | 2006-3
|
| Publication Title |
Physical Review D
|
| Volume | volume73
|
| Issue | issue5
|
| Content Type |
Journal Article
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| language |
English
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| Refereed |
True
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| DOI | |
| Web of Science KeyUT | |
| Submission Path | astronomy_general/2
|