Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 R&D Status of ATF2 IP Beam Size Monitor (Shintake Monitor) Taikan SUEHARA, H.Yoda, M.Oroku,

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Presentation transcript:

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 R&D Status of ATF2 IP Beam Size Monitor (Shintake Monitor) Taikan SUEHARA, H.Yoda, M.Oroku, T.Yamanaka (Univ. of Tokyo) T.Sanuki (Tohoku Univ.) T.Tauchi, Y.Honda, T.Kume (KEK)

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01Topics 1.Overview 2.Laser Fringe Phase Control 1.Phase Monitor 2.Phase Scanner 3.Stabilization Result 3.Collimator & Gamma Detector 1.Beam Tail Charge Distribution & Upstream Collimator 2.Gamma Detector Status 3.Effect of Gamma Collimator 4.Shintake Monitor for ILC 1.DUV laser & optics 2.Resolution for 5nm Beam Size 3.Background Source 5.Summary

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01Overview 70nm meas. in FFTB Shintake Optical Table Schematic

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 ATF & KEK ATF2 About 110 m 1.3 GeV Linac Dumping ring (ATF)

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Shintake Monitor for ATF2 Measure 35nm ATF2 beam, < 2nm error (about half of FFTB experience) Upgrades implemented & planned –Laser wavelength change (1064nm  532nm) –Laser fringe phase stabilization –Background subtraction by  detector –Background collimation (beam &  -ray) –etc.  detector Shintake table bend Beam dump Brief layout around IP

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Laser Fringe Phase Control

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Required Fringe Stability 3% modulation error  10nm phase stabilization. We need active stabilization system. 2nm beam size (required resolution)   3% modulation resolution.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Phase Monitor Phase magnification by microscope lens, captured by image sensor Phase detection sample Lens and image sensor The phase does not sensitive to vibration of lens & sensor. Fourier method suppresses sensitivity to optical noise.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Phase Scan & Control Delay line for phase scanning. Piezo stage of 0.2nm resolution is installed under right 2 mirrors. Control system. Control cycle is 10Hz, that is the repetition rate of the pulsed laser.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Stabilization Result (cw. Test Laser) Phase change of ref.ch Long time drift is suppressed. We use 2 image sensors. Stab.ch  stabilized Ref.ch  not stabilized Check correlation of 2 ch. to confirm beam (and IP) phase stabilization. Ref.ch phase data shows rad. (1.5nm) stability in 1min rad. (5.6nm) stability in 10min. which meets 10nm stability ATF2 goal.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Collimator & Gamma Detector

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Beam Tail & Collimator Tail estimation using ATF ext. background meas. Beam tail must be cut before FD. We need >40mm aperture for OC1,SF1,QF1,SD0,QD0 and additional quad after IP (before bend) Effect of tail cut must be checked by tracking simulation.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Gamma Detector Schematic of gamma detector. 4 forward layers will be used for background subtraction. Distribution of energy deposit. Deposit of signal is concentrated to forward region. Background subtraction will be done by comparing energy deposit of forward and background region. Conceptual design of  detector was finished. Detailed designing is ongoing. We will perform beam tests in ATF ext. by end of this year.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Effect of Gamma Collimator Compton signal is well focused while background has a relatively broad spacial distribution. We will put a cone-like collimator to select Compton signal. Simulation result. ~1.5mrad aperture (~2mm radius at top) accepts 80% of signal and ~0.1% of background from Final Q. ~2mrad (~3mm r) accepts 95% of signal and 1% of bg.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Shintake Monitor for ILC

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Lasers for 5nm Measurement F2 laser (157nm) –Shortest wavelength of commercial lasers –92.3% 5nm, % mod. / 1% BS –50mJ/20ns available, need special optics ArF excimer laser (193nm) –Shortest wavelength of excimer lasers –94.8% 5nm, 0.101% mod. / 1% BS –650mJ/25ns (enough) widely available excimer optics FEL ?? Sensitivity for ILC & ATF2 Coherent LPXPro series F2 and ArF eximer

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Resolution for 5nm Measurement Assuming 157nm F2 laser 3% modulation error (same as ATF2 goal)  20% beam size error (5 ± 1 nm) Stability of Laser Fringe Phase –Requirement is factor 3.38 harder (depend on laser wavelength, 532/157=3.38) –3nm stability required for same condition as ATF2 Signal photons –Compton cross section is around 1/10 of ATF2 (high energy suppression) –At least ~600 photons required for statistics (4%) We must raise laser power or decrease laser spot size

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Background ILC Signal photon energy is near beam energy Brems. background up to beam energy –Beam halo must be collimated upstream Synchrotron radiation up to O(100MeV) –Must be cut by thick shield just before detector (Pb:10~20cm) Signal energy spectrum of 500GeV ILC Most of 100 MeV  stopped by 20cm Pb shield

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01Summary Shintake monitor aims to measure ATF2 35nm beam size within 2nm error. Fringe phase stabilization system was established, 1.5nm (1min.) & 5.6nm (10min.) stabilization achieved using cw. test laser, that meets ATF2 goal stability (10nm). Background subtraction by  detector will be performed using difference about shower development. The detector is under detailed design. Collimator for  can reduce background from final Q to 1%~0.1% (but alignment is difficult because of narrow aperture of the collimator) For ILC, 5nm beam size measurement can be done using DUV F2 or ArF laser. 3nm phase stability and other errors same as ATF2 correspond to 5 ± 1 nm resolution.

Taikan SUEHARA et al., LCWS2007 & DESY, 2007/06/01 Thank you!!