k 0 s reconstruction in alice giuseppe lo re infn, sezione di catania, and dipartimento di fisica e...
DESCRIPTION
Introduction Sec. vertex Dpn Dpn = distance of closest approach V0 position = middle point between the two tracks at the distance of closest approach Primary vertex Radial distanceTRANSCRIPT
![Page 1: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/1.jpg)
K0s reconstruction in
ALICE
Giuseppe Lo Re
INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia,
Università di Catania, Italy,
March 2002
![Page 2: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/2.jpg)
Summary
• Introduction• Simulation• Optimization of cuts• Results• Conclusions
![Page 3: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/3.jpg)
Introduction
Sec. vertex
Dpn
Dpn = distance of closest approach
V0 position = middle point between the two tracks at the distance of closest approach
Primary vertex
Radial distance
![Page 4: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/4.jpg)
Simulation• B = 0.2 T
• Aliroot v 3.06
• Event generator: HIJING (full)
- generated 31 events with b = 3 fm
• “Slow” simulation of the ITS
• Tracking V1 in the ITS (with 6 points)
- step 1: with vertex constraint
- rejection of the “primary tracks”
- step 2: without vertex constraint
• Straight line approximation from the beam pipe backwards to the primary vertex
• Combination of + and - tracks and application of the cuts
- search of K0S within a fiducial region (R=0.5-2.5 cm)
![Page 5: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/5.jpg)
• Cut 1: product of the radial impact parameter (Dr- Dr+)
• Cut 2: distance of closest approach (Dpn)
• Cut 3: angle between the K0s position vector and
the K0s momentum ()
• Cut 4: impact parameter of the daughters (D)
•Cut 5: 2 of the daughters
List of the cuts used
![Page 6: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/6.jpg)
-
+
Dr-
Dr+
Primary vertex
Sec. vertex
Cut 1: product of the radial impact parameter
Dr- Dr+ < 0
![Page 7: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/7.jpg)
Cut 2: distance of closest approach (Dpn)
Dpn < 0.14 cm
![Page 8: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/8.jpg)
Primary vertex
Sec. vertex
Cut 3: angle between the K0s position vector (R) and
the K0s momentum (PK)
Cos > 0.9985
R
PK
![Page 9: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/9.jpg)
Effect of cuts
Mass (GeV/c2)
Without any cut Dr- Dr+ < 0
Cos > 0.9985 Dpn < 0.14 cm
![Page 10: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/10.jpg)
N. found K0
S 2.5 per event
Results
![Page 11: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/11.jpg)
x, y and z resolution of secondary vertices
![Page 12: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/12.jpg)
, and Pt resolution
= 5 mrad = 3 mrad
![Page 13: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/13.jpg)
Efficiency of algorithm and cuts
Eff = no. of found K0s / no. of findable K0
s after the TPC-ITS tracking
Found Eff. = 32 %
Fake Prob. = 11 %
![Page 14: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/14.jpg)
Total found efficiency
Eff = no. of found K0s / no. of generated K0
s
Found Eff. = 0.37 %
Fake Prob. = 0.12 %
![Page 15: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/15.jpg)
Reconstructed Pt spectrum
Generated spectrumReconstructed spectrum
![Page 16: K 0 s reconstruction in ALICE Giuseppe Lo Re INFN, Sezione di Catania, and Dipartimento di Fisica e Astronomia, Università di Catania, Italy, March 2002](https://reader036.vdocuments.mx/reader036/viewer/2022082510/5a4d1b637f8b9ab0599ae57a/html5/thumbnails/16.jpg)
Conclusions and future work
• The problem of reconstructing K0S in ALICE is under
investigation in a realistic simulation framework
• An algorithm for Aliroot has been written and its resolution and efficiency have been evaluated
• Evaluation of the effect of a different choice of the fiducial region
• Simulations with a magnetic field of 0.4 T
• Studies for reconstructing the s are already started