\(D^{+}\longrightarrow K^{-}K^{+}K^{+}\)
CERN Summer Student Programme
Sebastian Ordoñez
jsordonezs@unal.edu.co
Supervisor: Alberto C. dos Reis
9th of July 2021
For those models the knowledge of branching fractions and resonant structures are key inputs!
Current status within the LHCb collaboration (as far as I know)
Mainly summarized in two papers:
The amplitude analysis is performed using two models: the traditional isobar model and the most interesting one, the Multi-Meson Model alias Triple-M.
Big picture of a three-body decay as described by the Triple-M:
\(c\) quark decay
Formation of the mesons
Final State Interactions
Three-body decays of \(D\) mesons into kaons \(K\) and pions \(\pi\) are interesting laboratories for light-meson spectroscopy.
It is neccesary to isolate the physics of two-body systems from the rich dynamics of three-body decays!
It is required:
The most important variables used for selecting candidates are:
\(\phi(1020)\)
Fake background!
A closer look
Background!
Zoom
Background coming from the wrong reconstruction of a couple of kaons as just one. This is due to the fact that the angle between the assocciated tracks is quite small and then the identification fails.
In order to reject fake background it was used the angle between the kaons, i.e.
p3_ProbNNp>0.9
p3_ProbNNp>0.95
p3_ProbNNp>0.99
p3_ProbNNp>0.995
p3_ProbNNp>0.999
2255\(<m_{KKp}<\)2320
p3_ProbNNp>0.9
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
p3_ProbNNp>0.95
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
2255\(<m_{KKp}<\)2320
p3_ProbNNp>0.99
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
2255\(<m_{KKp}<\)2320
p3_ProbNNp>0.995
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
2255\(<m_{KKp}<\)2320
p3_ProbNNp>0.999
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
2255\(<m_{KKp}<\)2320
0.8<p3_ProbNNp<0.9
0.8<p3_ProbNNp<0.9
2255\(<m_{KKp}<\)2320
2265\(<m_{KKp}<\)2310
2275\(<m_{KKp}<\)2300
0.85<p3_ProbNNp<0.95
0.85<p3_ProbNNp<0.95
2265\(<m_{KKp}<\)2310
2255\(<m_{KKp}<\)2320
2275\(<m_{KKp}<\)2300
p3_ProbNNp<0.8
p3_ProbNNp<0.9
p3_ProbNNp<0.95
p3_ProbNNp<0.99
p3_ProbNNp<0.995
p3_ProbNNp<0.999
0.6<p3_ProbNNp<0.7
0.6<p3_ProbNNp<0.65