| ET cut | Efficiency 1 tag jet (%) | Efficiency 2 tag jets (%) | ||||
| (GeV) | H | t |
jW | H | t |
jW |
| 15 | 85.1 |
35.8 |
29.0 |
36.4 |
4.0 |
2.4 |
| 20 | 81.3 |
30.2 |
23.8 |
31.6 |
2.8 |
1.6 |
| 30 | 71.4 |
21.2 |
16.1 |
21.0 |
1.3 |
0.7 |
| 50 | 49.9 |
12.1 |
8.8 |
8.5 |
0.4 |
0.2 |
Rejecting background through a requirement of tag jets in the forward
region sensitive to the pile-up creating both real and fake jets in
the forward regions. With a full GEANT simulation of the
Higgs events and pile-up at high luminosity is was in [77]
shown that the rate of jets originating from the pile-up with a
transverse energy above 30 GeV is below 2% in one hemisphere. This
means that a background event with no tag jets has a 4% probability
(two hemispheres) to pick up a tag jet from the pile-up while a
background event with one tag jet has a 2% probability to pick up a
second jet from the pile-up (pile-up jet has to be in the opposite
hemisphere of the real tag jet). With the numbers for the t
and
jW background from table 8.5 with a cut on the
transverse energy of 30 GeV it can be seen that this seriously affects
the rejection using two tag jets; the t
efficiency rise from
1.3% to 1.8% and the jW efficiency rise from 0.7% to 1.1%.
In principle a clean discovery within one year at high luminosity
should be possible with the rejection achieved against the reducible
background, but the signal to background ratio is a problem. The
background cannot be accurately calibrated as the signal is not a
clear peak on top of a flat background. With the above numbers an
uncertainty in the background level of 30% will be able to fake a
discovery. Some calibration can be done by specifically looking at the
events not surviving the cut confining the jet mass to the W mass. For
the Higgs signal and the t
and jW backgrounds the mass
spectrums for the central jet with the highest ET are shown in
fig. 8.7. All other central identification cuts and the
requirement on two tag jets have been applied. It can be seen that
both the t
and the JW backgrounds are peaked as the signal
around the W mass and hence a calibration looking at the side-bands to
the W mass peak will have a limited value.
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