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Summary: Workshop on CMS Beam Conditions, Radiation Monitoring and Luminosity Systems Oliver Stein, May 2013, CERN.

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Presentation on theme: "Summary: Workshop on CMS Beam Conditions, Radiation Monitoring and Luminosity Systems Oliver Stein, May 2013, CERN."— Presentation transcript:

1 Summary: Workshop on CMS Beam Conditions, Radiation Monitoring and Luminosity Systems
Oliver Stein, May 2013, CERN

2 Overview Workshop on CMS Beam Conditions 22. April – 24.April.2013
DESY Zeuthen, Germany 45 talks 32 participants All talks and slides:

3 Overview CVD Diamonds BRM Beam Radiation Monitor Others BCM
Beam Condition Monitor BCM1F (fast ~ ns) BCM1L (slow 40 µs ) BCM2 (slow 40 µs ) PLT Pixel Luminosity Telescope BSC Beam Scintillation Monitor BPTX Beam Pick-up time for Experiments CVD Diamonds

4 Overview CVD Diamonds BRM Beam Radiation Monitor Others BCM
Beam Condition Monitor BCM1F (fast ~ ns) BCM1L (slow 40 µs ) BCM2 (slow 40 µs ) PLT Pixel Luminosity Telescope BSC Beam Scintillation Monitor BPTX Beam Pick-up time for Experiments PLT z=175m BPTX CVD Diamonds

5 BCM Setup before LS1 BCM1F 8 sCVD diamond detectors
detection of fast beam losses (halo and collisions)

6 BCM Setup before LS1 BCM1F 8 sCVD diamond detectors
detection of fast beam losses (halo and collisions) BCM1L 8 pCVD diamond detectors leakage current monitor integrated in beam abort system BCM1F and BCML share mount carriage

7 BCM Setup before LS1 BCM1F 8 sCVD diamond detectors
detection of fast beam losses (halo and collisions) BCM1L 8 pCVD diamond detectors leakage current monitor integrated in beam abort system BCM1F and BCML share mount carriage Run 2011 & 2012 high reliability very stable (4 faults causing dumps) redundancy for lumi calc. system

8 BCM Results from run 2011 & 2012 use of BCM1F as luminometer is feasible backup as online luminosity monitors

9 BCM Results from run 2011 & 2012 BCMS signal decreases due to radiation efficiency decrease is correlated with neutron flux With CASTOR Without CASTOR

10 BCM >> CVD Diamonds
Radiation induced damage causes polarisation efficiency decrease

11 BCM >> CVD Diamonds
Radiation induced damage causes polarisation efficiency decrease Compensation increase HV Reactive Ion Etching (RIE) change of HV polarisation red light

12 BCM upgrade Increase of BCM1F channels to 48
bisected BCM1F sensors. Less susceptible to pulse pile up greater geometric acceptance for background monitoring greater pre-amplifier gain better SNR faster pre-amp shaper

13 BCM >> PLT installation of PLT during LS1
dedicated stand-alone luminosity monitor for CMS Pixel Luminosity Telescope consists of 3 layers of 8 single-crystal diamond pixel sensor measure bunch-by-bunch 3-fold coincidence rate pixel readout for tracking and diagnostics

14 BCM >> Data readout
Work during LS1 maintenance of existing front and backend electronics installation and change of hardware move of readout electronics to the service cavern installation of additional cables adaption of the readout electronics to the new setups development and implementation of new software codes

15 Conclusion many interesting talks large variety of different topics
presentation of hardware, data read out and software issues upgrade and optimization plans for LS1 All talks and slides:

16 Thank you for your attention!
Conclusion many interesting talks large variety of different topics presentation of hardware, data read out and software issues upgrade and optimization plans for LS1 All talks and slides: Thank you for your attention!

17 BCM >> CVD Diamonds
Radiation induced damage causes polarisation efficiency decrease

18 BCM upgrade Increase of BCM1F channels to 48
bisected BCM1F sensors. Less susceptible to pulse pile up greater geometric acceptance for background monitoring greater pre-amplifier gain better SNR faster pre-amp shaper


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