Denis Anielski 02.04.2009 1 Detector systems to find HFS of 209 Bi ESR Emission characteristics Counting rates at existing mirror section Straight.

Slides:



Advertisements
Similar presentations
NDVCS measurement with BoNuS RTPC M. Osipenko December 2, 2009, CLAS12 Central Detector Collaboration meeting.
Advertisements

Monte Carlo Studies of the HERMES RICH in SBS—progress report Andrew Puckett 11/10/2010.
USE OF GEANT4 FOR LHCB RICH SIMULATION S. Easo, RAL, LHCB AND ITS RICH DETECTORS. TESTBEAM DATA FOR LHCB-RICH. OVERVIEW OF GEANT4 SIMULATION.
Interference and Diffraction
Chapter 33 - Light and Illumination
The Nature or Light and Matter Chapter 4 Survey of Astronomy astro1010-lee.com.
Quartz Plate Calorimeter Prototype Ugur Akgun The University of Iowa APS April 2006 Meeting Dallas, Texas.
DHC 101 Introduction to scintillation detectors. How many PE/MIP should we expect? Scintillation & Fluorescence WSFWSF PMTPEs  (MIP)
End of 2007 SPECTRAP’ is being built in London to trap Ca+ ions with real imaging capabilities Early RF operation expected Jan 2008 Penning operation Feb/Mar.
Measures of Source Intensity 1. Radiant Flux, Φ Rate of transfer of energy Φ = δQ/δt (W)
S. Bricola, A. Menegolli, M. Prata, M.C. Prata, G.L. Raselli, M. Rossella, C. Vignoli INFN and University of Pavia - Via Bassi, 6 – Pavia – Italy.
Status of the Tagger Hall Background Simulation Simulation A. Somov, Jefferson Lab Hall-D Collaboration Meeting, University of Regina September
KEK beam test H. Sakamoto. Purpose To optimize a concentration of the second dopant for scintillating fibers KEK beam test to study light yields for various.
Pair backgrounds for different crossing angles Machine-Detector Interface at the ILC SLAC 6th January 2005 Karsten Büßer.
Simulation of a Ring Imaging Cerenkov detector to identify relativistic heavy ions. M.Fernández-Ordóñez, J.Benlliure, E.Casarejos, J.Pereira Universidad.
Could CKOV1 become RICH? 1. Simulations 2. Sensitive area of the detection plane 3. Example of a workable solution 4. Geometrical efficiency of the photon.
Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC)
Spontaneous Radiation at LCLS Sven Reiche UCLA - 09/22/04 Sven Reiche UCLA - 09/22/04.
E-  identification 1. Reminder from previous presentations, questions, remarks 2. Čerenkov option 3. Study of several optical configurations 4. Conclusions.
Backgrounds and Forward Region Backgrounds and Forward Region FCAL Collaboration Workshop TAU, September 18-19, 2005 Christian Grah.
Zoran Andjelkovic Johannes Gutenberg – Mainz University GSI Darmstadt Laser Spectroscopy of Highly Charged Ions and Exotic Radioactive Nuclei (Helmholtz.
4-1 Chap. 7 (Optical Instruments), Chap. 8 (Optical Atomic Spectroscopy) General design of optical instruments Sources of radiation Selection of wavelength.
Characterization of CF 4 primary scintillation Andrey Morozov.
Optics and magnetic field calculation for the Hall D Tagger Guangliang Yang Glasgow University.
SPECTROSCOPIC DIAGNOSTIC COMPLEX FOR STUDYING PULSED TOKAMAK PLASMA Yu. Golubovskii, Yu. Ionikh, A. Mestchanov, V. Milenin, I. Porokhova, N. Timofeev Saint-Petersburg.
A Reconstruction Algorithm for a RICH detector for CLAS12 Ahmed El Alaoui RICH Workchop, Jefferson Lab, newport News, VA November th 2011.
Liquid scintillator for an off-axis neutrino detector? (The Minnesota group) We are actively investigating a liquid scintillator option for the off-axis.
Measurement of 'intrinsic' properties of scintillating fibers H. Sakamoto Osaka University, Japan A.Sato M. Yoshida Y. Kuno Osaka Univ. K. Yoshimura KEK.
1 Fast Timing via Cerenkov Radiation‏ Earle Wilson, Advisor: Hans Wenzel Fermilab CMS/ATLAS Fast Timing Simulation Meeting July 17,
1 Brilliant Pattern Problem Problem Suspend a water drop at the lower end of a vertical pipe. Illuminate the drop using a laser pointer and observe the.
Optical Engineering Lecture 1.  17 th Century, Sir Isaac Newton said that rays of light are streams of very small particles emitted from a light source.
Laser Stripping and H 0 monitor systems 10/18/2011B.Cheymol, E. Bravin, U. Raich, F. Roncarolo BE/BI1.
Zoran Andjelkovic Johannes Gutenberg Universität Mainz GSI Darmstadt Laser Spectroscopy of Highly Charged Ions and Exotic Radioactive Nuclei (Helmholtz.
THE FORWARD PROTON DETECTOR AT DZERO Gilvan Alves Lafex/CBPF 1) MOTIVATION 2) DETECTOR OPTIONS 3) FPD R&D 4) OUTLOOK Lishep 98 Lafex/CBPF Feb 17, 1998.
Single atom manipulations Benoît Darquié, Silvia Bergamini, Junxiang Zhang, Antoine Browaeys and Philippe Grangier Laboratoire Charles Fabry de l'Institut.
Cherenkov Counters for SoLID Z.-E. Meziani on behalf of Simona Malace & Haiyan Gao (Duke University) Eric Fuchey (Temple University) SoLID Dry Run Review,
RICH SIMULATION USING GEANT4 S.EASO, RAL OBJECTIVES OF THE SIMULATION. CURRENT STATUS AND PLANS. INTEGRATION WITH LHCb SOFTWARE. SUMMARY.
work for PID in Novosibirsk E.A.Kravchenko Budker INP, Novosibirsk.
PID for super Belle (design consideration) K. Inami (Nagoya-u) - Barrel (TOP counter) - Possible configuration - Geometry - Endcap (Aerogel RICH) - Photo.
Timing properties of MCP-PMT K.Inami (Nagoya university, Japan) - Time resolution - Lifetime - Rate dependence Photon Detector Workshop at Kobe,
1 Brilliant Pattern Problem Problem Suspend a water drop at the lower end of a vertical pipe. Illuminate the drop using a laser pointer and observe the.
HBD Gas and QE Monitoring Craig Woody BNL HBD Working Group Meeting October 19, 2005.
A. Bondarevskaya Highly charged ion beam polarization and its application to the search for the parity nonconservation effects in ions
T. Suehara, H. Yoda, T. Sanuki, Univ. of Tokyo, T. Kume, Y. Honda, T. Tauchi, High Energy Accelerator Research Organization (KEK) ATF2-IN2P3-KEK kick-off.
Status Report particle identification with the RICH detector Claudia Höhne - GSI Darmstadt, Germany general overview focus on ring radius/ Cherenkov angle.
Elemental Analysis using Atomic Absorption and Emission Spectroscopy Bodhisatwa Das.
October,05 HCAL Meeting 10/15/05 Quartz Plate Simulation Studies Quartz Plate Simulation Status F. Duru, U. Akgun, A.S. Ayan, J. Olson, Y. Onel The University.
1.1 What’s electromagnetic radiation
X-ray SNR in 3 steps. I ∆I. X-ray transmission SNR Review Let N = average number of transmitted x-rays N = N 0 exp [ - ∫  dz ] Emission and transmission.
SL/BI 16/05/1999DIPAC’99 -- JJ Gras -- CERN SL/BI -- Adaptive Optics for the LEP 2 SR Monitors G. Burtin, R.J. Colchester, G. Ferioli, J.J. Gras, R. Jung,
TORCH IOP meeting Manchester March 31, 2015 TORCH Maarten van Dijk On behalf of the TORCH collaboration (CERN, University of Oxford,
Aerogel detector revisited Sokolov Oleksiy, UNAM, progress report, 20 Sept 2006 E int = M – wall reflectivity є – PMT relative area Belle geometry (traditional):
Progress on new electron cloud monitors in the PS Christina Yin Vallgren, TE-VSC P. Chiggiato, S. Gilardoni, J. A. Ferreira Somoza G. Iadarola, H. Neupert,
Study of the cryogenic THGEM-GPM for the readout of scintillation light from liquid argon Xie Wenqing( 谢文庆 ), Fu Yidong( 付逸冬 ), Li Yulan( 李玉兰 ) Department.
ODR Diagnostics for Hadron Colliders Tanaji Sen APC.
Prism Pairs for Elliptical Beams
B. Meadows University of Cincinnati
Central detector for CLAS12: CTOF and Neutron detector
KM2A Electron Detector Optimization
Really Basic Optics Instrument Sample Sample Prep Instrument Out put
Mass Spectronomer.
Particle Identification in LHCb
RICH simulation for CLAS12
Proposals of new electron cloud monitor in the PS
Multianode Photo Multipliers for Ring Imaging Cherenkov Detectors
Deng Ziyan Jan 10-12, 2006 BESIII Collaboration Meeting
MC simulation of the DIRC prototype
Beam size diagnostics using diffraction radiation
Development of microchannel plate phototubes in Novosibirsk
Beam Halo Considerations for Back Angle Running
Presentation transcript:

Denis Anielski Detector systems to find HFS of 209 Bi ESR Emission characteristics Counting rates at existing mirror section Straight on detector option Parabolic mirror system Outlook Denis Anielski, Volker Hannen, Raphael Jöhren, Christian Weinheimer Westfälische Wilhelms-Universität Münster

Denis Anielski Relativistic Doppler Effect λ = λ´γ(1- βcos(θ))θ= 0° → 640nm λ´ = 1555nm θ= 40° → 1000nm Observed angle Boost Relativistic Doppler Effect and Boost (β = 0.71)

Denis Anielski Simulation of Boost Polar angles in the comoving system Polar angles in the lab system (Isotropic light source) A(0°,10°) = 4% A(10°;30°) = 25% A(10°;50°) = 52% →Most photons not in straight forward direction, because of sin(θ) in solid angle!

Denis Anielski Ideas For Detector Systems

Denis Anielski General Assumptions Number of excited ions: 2 e5 Lifetime in lab system: 82 ms [1] Lifetime in comoving system: 116 ms QE = 10% Circumference of ESR: 108 m β = 0.71 [1] V. M. Shabaev, PHYSICAL REVIEW A, JAN 1998

Denis Anielski Mirror System 10 elliptical mirrors on a 65cm section Original simulation software not available First order estimate: geometric count rate estimate Realistic simulations using GEANT4 under progress

Denis Anielski Estimated counting rate Counting rate is proportional to  Emitted photons per second N Ph = N/tau = 1,72 e6  Ratio of totally emitted photonsA = 0.38 (646 nm – 950 nm; 5°-37° )  Loss by reflexion and transmission R*T = 1/3 (R=0.35!!!)  Quantum efficencyQE = 0,1  Relevant beam sectionb = 0.065m/ 108m  Geometry of mirror systemg = 2/3  Number of windows(dia: 7cm)# = 3 →f = N Ph · A · g · RT · QE · b · # = 26 Hz

Denis Anielski Straight on option Diameter of window: 60mm Straight beam section: 17 m Distance – beam – detector: 3,5 m All Photons are focused on detector by a lense Transmission of lense: 0.9 →0,36 Hz(simulation c++)

Denis Anielski Parabolic mirror Detects forward emission → short wavelengths

Denis Anielski Parabolic mirror Assumptions Reflectivity coefficient: 0.8 Hole in mirror with diameter of 2cm for the beam GEANT4 model

Denis Anielski flange option Diameter of flange for mirror: 10 cm Diameter of flange for detector: 3.8 cm Distance: Beam - Detektor: 30 cm Straight section before mirror: 5 m Radius of mirror: 5 cm Lightguide as interface from window to detector GEANT4 simulation (Volker Hannen) →15 Hz

Denis Anielski flange option

Denis Anielski flange option – C++ Simulation Diameter of flange: 20 cm Distance: Beam - Detektor: 25 cm Straight section before mirror: 5 m / 10 m Radius of mirror: 7.5 cm Radius of detector/ focussing system: 3 cm Counting rate is multiplied by 0.9 because of slit →45 Hz / 60 Hz (Flange is just in front of mirror system!) Possible improvement with recessed exit window (distance beam – exit window = 15cm):154 Hz

Denis Anielski CPM beam tests Two setups have been installed at ESR yesterday Investigations of background photons and behaviour of CPM next to dipole magnet Positions: – 2-flange option – Straight on option Detectors: Channel-Photomultiplier – Easy to handle – Low dark count rate – Only 2% QE around 650nm – Suitable for 244nm transition at SPECTRAP (QE= 18%)

Denis Anielski Conclusions Mirror system:  26 Hz, but dark counts of three detectors, broad wavelength range  Reflexion of mirror?  Not all three windows present  ??? Straight on  very low rate ( < 1Hz)  ??? Parabolic mirror  System with highest counting rate on a SINGLE detector  Small wavelengths (640 – 680nm)  !!!

Denis Anielski Outlook Test of Hamamatsu R PMT (suitable detector for parabolic mirror system) Detailed GEANT4 simulation of existing mirror system and search for best parameters of parabolic mirror system