- Page 1 and 2: CERN/SPSC 2000-028 SPSC/P318 LNGS P
- Page 3 and 4: N. Bruski, S. Buontempo, F. Carbona
- Page 5 and 6: Contents 1 Introduction 5 1.1 Physi
- Page 7 and 8: 6.7.1 Multiple scattering analysis
- Page 9 and 10: 1 Introduction In this document we
- Page 11 and 12: eactor experiments (KAMLAND [22], B
- Page 13 and 14: difference being the nature of the
- Page 15 and 16: The total energy of electrons and
- Page 17 and 18: through the decay topology and its
- Page 19 and 20: Figure 6: Simulated ν τ event wit
- Page 21 and 22: particles above 10 MeV . One can se
- Page 23 and 24: vertex position as predicted by the
- Page 25 and 26: • stability and maintenance: no p
- Page 27 and 28: Figure 11: Illustration of the vari
- Page 29 and 30: Table 3: Expected numbers of τ and
- Page 31 and 32: 3 The CNGS neutrino beam 3.1 The be
- Page 33 and 34: per year of operation because the S
- Page 35 and 36: ν µ at GS (p.o.t. GeV m 2 ) -1 10
- Page 37 and 38: Figure 19: Generated (continuous li
- Page 39: Emulsion Film + 56 (Lead + Emulsion
- Page 43 and 44: Figure 24: Film thickness distribut
- Page 45 and 46: contact at different temperature an
- Page 47 and 48: Figure 27: Photograph of a minimum
- Page 49 and 50: entry : 85 RMS: 0.060 15 10 5 0 0 d
- Page 51 and 52: [micron] 2 1 0 -1 -2 [micron] 2 1 0
- Page 53 and 54: een searching for old emulsion plat
- Page 55 and 56: Figure 33: Thickness distribution f
- Page 57 and 58: Figure 35: RMS distribution of 472
- Page 59 and 60: Figure 37: Wall support structure.
- Page 61 and 62: ensures a well defined brick positi
- Page 63 and 64: Figure 41: Detail of the brick mani
- Page 65 and 66: The strips are 6.7 m long, 2.6 cm w
- Page 67 and 68: the effective maximal length (for p
- Page 69 and 70: Table 7: Characteristics of the 64-
- Page 71 and 72: photomultiplier to be tested diaphr
- Page 73 and 74: modate from 512 up to 5180 fibres.
- Page 75 and 76: The fast shaper has a high gain in
- Page 77 and 78: The Ethernet capable device provide
- Page 79 and 80: R&D already performed by the MINOS
- Page 81 and 82: Figure 54: Isometric view of the di
- Page 83 and 84: Figure 56: Magnetic field distribut
- Page 85 and 86: RPC layout 8.00 m 8.75 m Figure 58:
- Page 87 and 88: formance, it is presently foreseen
- Page 89 and 90: Figure 61: Drift plane arrangement
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Figure 63: Schematic view of a XPC
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Figure 64: Acceleration spectrum fo
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Figure 65: The OPERA detector shown
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Table 9: Number of electronic chann
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Adjustable gain Channel 0 Sample &
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Trigger OUT IN Discri. Time Ref. PP
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Super Module 1 Super Module 2 Super
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5 Analysis of the electronic detect
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Track segments on both the emulsion
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5.5 Brick finding efficiency The se
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Wall finding efficiency 1 0.95 0.9
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The worst case leading to the lowes
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electromagnetic showering events an
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Studies on the strategies have star
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which may enter in such a compariso
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Figure 84: The total brick finding
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Figure 86: Charge determination of
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Figure 89: Muon momentum resolution
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Figure 91: Muon momentum resolution
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Reconstructed Pion Energy N Analog
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Figure 98: The difference between r
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By using the above running modes of
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µm EXP.: DONUT 3039/01910 MOD.:ECC
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emulsion film plastic foils and edg
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200micron base 50micron emulsion la
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Figure 106: Tracking efficiency of
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a base track on film 2 a penetratin
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Long decays, defined as a decay top
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more than 60 views/s recognising al
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Table 12: Basic numbers used to des
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an area that one S-UTS can process
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unit cell L=1300micron Pb plate ( 1
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We recall that the intrinsic positi
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Figure 116: The top histograms show
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The error on θ S due to both the s
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Figure 120: Fraction of pions which
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#1 #2 #3 #4 #5 γ γ ∆θ 4= |θ 5
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Figure 124: Energy resolution for e
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Figure 126: Efficiency for γ’s t
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7 Physics performance 7.1 Electron
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7.2 Muon identification efficiency
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Table 13: Muon identification effic
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Table 14: Brick finding efficiency
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The second result is obtained from
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Figure 134: Brick-to-brick connecti
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Figure 136: Distribution of τ deca
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For long decays the overall efficie
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The φ angle is expected to peak at
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Table 19: Summary of the kinematica
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known. Because of these uncertainti
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Table 21: Expected charm background
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π− e+ γ e- e+ e- γ π− Figur
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Table 24: Estimates of the rate of
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Table 27: Expected numbers of τ an
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Table 28: Sensitivity at the 90% CL
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7.6 Determination of the oscillatio
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measurement of the ratio between ν
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Table 30: Neural network recognitio
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(mrad) 0.04 0.02 0 -0.02 -0.04 10 2
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Table 31: Radioactivity measurement
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ick. There is approximately a facto
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Figure 152: A typical PMT response
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1m π, µ 15 GeV/c mini-walls 1.6 m
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Electrons 1GeV/c 20mm Pb Number of
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tube. An Image Intensifier (II) by
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1 0 0 l = 1 1 .8 m N, p.e. 1 0 1 0
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HPD’s pixels (Fig. 162). The cook
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A complete system has been designed
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The acquisition system (VA-DAQ) use
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The upstream tracker T 1-3 between
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Figure 168: Distributions of the ap
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Figure 169: Example of a large-angl
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multiple scattering, given the smal
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9.1.3 Wall support structures An al
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Nevertheless, the possibility to us
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Figure 174: (a) 3D view of the spec
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9 p.e. and 6.9 p.e. at a distance f
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Figure 176: Neutrino induced charm
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A test programme for emulsion brick
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The space requirements in the exper
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advance. The sets of scintillator s
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Task Name Start Finish Study of mai
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11 Experimental infrastructure 11.1
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After the exposure to cosmic rays,
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on the size of these stations. A co
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Table 38: Expected contributions to
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the developed emulsions and to stan
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As the sensitivity is not limited b
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[26] M. Apollonio et al., Phys. Let
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[89] http : //tosca.web.cern.ch/T O