Threshold aerogel Cherenkov counters of the KEDR detector

A.Yu. Barnyakov * , M.Yu. Barnyakov, V.S. Bobrovnikov, A.R.

Buzykaev, A.F. Daniluk, S.A. Kononov, E.A. Kravchenko, I.A.

Kuyanov, A.P. Onuchin, I.V. Ovtin, V.A. Rodiakin

OUTLINE: 1.

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ASHIPH method Cherenkov counters system of the KEDR detector Long term stability of ASHIPH counters Status of the system Summary

• • •

ASHIPH method

Development of aerogel counters in Novosibirsk was started in 1986 by collaboration of BINP and BIC for creation of threshold Cherenkov counters. Now this collaboration is working on the development of RICH detectors based on aerogel radiators( details on FARICH in oral presentation of S.

Kononov ) In 1988 first project of aerogel Cherenkov threshold counters for the KEDR detector with direct light collection was suggested Scientific, 1990, 208-213) (A. Onuchin et al., World ASHIPH (Aerogel SHifter PHotomultiplier) method of light collection was suggested in 1992. Cherenkov light from aerogel is collected by wavelength shifter (WLS) and transported by WLS like a lightguide to photomultiplier photocathode (A. Onuchin et al. NIM A315 (1992) 517-520) – This method permits to decrease photocathode area – This method permits to make very compact valuable PID system in HEP experiments (ex. Aerogel counters for SND detector, the system in two posters: K. Beloborodov and K. Martin ) more details on 26.02.14

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The system of ASHIPH counters for the KEDR detector

• • • • • • • INSTR14 160 counters arranged in 2 layers 96% of solid angel 1000 liters of aerogel with n=1.05

π/K- separation in momentum range 0.6 1.5GeV/c Light collection with help of WLS 160 MCP PMTs with photocathode ø18mm able to work in magnetic field up to 2T Thickness of the material is 12%X 0 3 26.02.14

0.08

0.1

K

Prototype testbeam results

P=1.2GeV/c Estimation for 2 layers system: p p 80% of particles from interaction point goes through aerogel in both layers

0.06

0.04

0.02

Counter with blocks with crumb 0 0

P, GeV/c 0.86

1

Pion supp. factor 900

2 3 Threshold, pe

Kaon reg. eff.

4 5

Separation 94% 4.7

 4.5

 26.02.14

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P, GeV/c

0.86

1.2

Pion supp. factor

8.1

 10 5 1.69

 10 6

Kaon reg. eff.

88% 81%

Separation

5.9σ 5.7σ 4

10 9 8 7

Long term stability

• • 80 counters (1 st layer of the system) were under operation in the KEDR detector from 2003 to 2011. Approximately 3.5 years of operation in magnetic field 0.6T.

17 counters were non operational due to drops of magnetic field. All barrel counters had efficiency worse than expected.

6 ATC efficiency in KEDR (BhaBha events) 5 4 1 10 3 2 1 P1 P2 P3 39.41 / 20 8.938

37.32

0.6468

0.8

9 8 0.6

7 0 0 20 40 60 80 100 120 Time, month

Prototype endcap ASHIPH counter are under operation since 2000. From time to time it is tested in Cosmic Ray Telescope (CRT) and its signal degradation now is stabilized at the level of 60% from initial value.

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0.4

6 5 0.2

4 3 0 2 0

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0 1 0 P1 10 P2 P3 20 20 30 8.938

37.32

0.6468

40 40 60 2004 2010 50 80 60 70 80 Number of counter 100 120 Time, month

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Reasons of degradation of ASHIPH counters

The main reasons of the signal degradation • Aerogel 0-45%. In average: – 22% for endcap – 34% for barrel • QE of PMT 0-50%. In average 18% • Magnetic field: – Tilt PMTs in endcap 4-6 ° ( up to 20% ) – Tilt PMTs in barrel 15-17 ° ( up to 30% ) – Broken optical contacts 0-54%. In average 9.5%

22.5

20 17.5

15 12.5

Entries Mean RMS 80 0.8213

0.1086

All counters of the 1 st layer were inspected for the reasons of degradation, repaired and upgraded during the stop of the KEDR experiment in 2011-2013 26.02.14

10 7.5

5 2.5

0 0.2

0.4

0.6

0.8

1 1.2

QE AFTER / QE BEFORE

Details on MCP PMT in oral presentation of M. Barnyakov in the evening session INSTR14 6

Aerogel degradation due to water adsorption

• • • Aerogel internal surface in 10 6 times greater than external. Adsorption of water is very fast process (1-2 hours).

Degradation of light absorption length is very slow process (1-2 months) after water absorption.

The time degradation and are level of depend the on impurities in aerogel from raw materials and production procedure (Fe, Mn, Cr, etc.).

Concentration of metals in aerogel, ppb Fe 500 Cu 56 Mn 7 Cr 26 Ni 26.02.14

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Aerogel light absorption length

Refractive index (n-1) and light scattering length depends on adsorbed water and are changed less than 10% after water adsorption of 2-4% of aerogel mass.

Light absorption length (L abs ) in different aerogel samples after baking is the same, but after water impregnation is very different It is possible to make aerogel selection impregnation after water One atom Fe is able to attract 6 molecules of water To achieve maximum degradation of L abs enough to adsorb 1ppm of water (NIM A598 (2009) 166-168) 26.02.14

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• • • • •

Status of ASHIPH system of the KEDR detector

N pe ( f ) In 2013 all 160 counters of the system were installed in the KEDR detector All counters were tested in the CRT before installation 16 14 12

1 st layer WLS

All software and DAQ system were adapted for 2 layer system 10 8 In the KEDR detector cosmic events with straight tracks were collected for relative alignment of the system and to complex check its operability In next few weeks the data taking with KEDR detector on VEPP-4M collider will started and the system is ready to work powerfully 6 4 2 0 1.1

2 nd layer

1.2

1.3

1.4

1.5

N pe ( q ) 1.6

1.7

f , rad 12

35 1 st layer Entries Mean RMS 160 7.944

0.9487

10

Endcap 30

8

25 Barrel 20

6

15

4

10 5

2 0

2 nd layer

0.5

1 1.5

2 2.5

3 Q , rad 9 26.02.14

0 0 2 4 6 8 10 12 Number of photoelectrons

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Some pictures of the system

The system inside the KEDR detector 26.02.14

INSTR14 The barrel part of the system in Lab 10

• • • • •

Some perspective to use in the KEDR experiment

Br(J/Ψ pp, K + K , π + π , …). Br(Ψ ’ pp, K + K , π + π , …).

Ψ(3770): – D-meson mass measurement. Identification of D-decay modes could be used to improve accuracy of mass measurement – … γγ-physics (at Υ-meson energy). More than 10% of events contains pions in momentum range from 0.44 to 1.5GeV/c. Their identification give 10-20% additional statistic for some processes … 26.02.14

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SUMMARY

• • • • In 2013 the system of ASHIPH counters of the KEDR detector was repair, upgraded and installed in the detector Now the system is launched in operation and ready to use In few next weeks we will have possibility to determine PID parameters of the system in real experimental conditions Since 2013 we have a valuable PID instrument in the KEDR experiment 26.02.14

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