G.R.White: 1.6.2001 F.O.N. T. From Ground Motion studies by A.Seryi et al. (SLAC) ‘Fast’ motion (> few Hz) dominated by cultural noise Concern for structures.

Slides:



Advertisements
Similar presentations
ATF2: Status Update Glenn Christian (on behalf of FONT group) 10 th ATF Project Meeting.
Advertisements

K. Buesser & N. Walker TF Studies: A very first look.
1 MULTI-BUNCH INTEGRATED ILC SIMULATIONS Glen White, SLAC/QMUL Snowmass 2005.
GUINEA-PIG: A tool for beam-beam effect study C. Rimbault, LAL Orsay Daresbury, April 2006.
CESR-c Status CESR Layout - Pretzel, Wigglers, solenoid compensation Performance to date Design parameters Our understanding of shortfall Plans for remediation.
Pair backgrounds for different crossing angles Machine-Detector Interface at the ILC SLAC 6th January 2005 Karsten Büßer.
ATF2 FB/FF layout Javier Resta Lopez (JAI, Oxford University) for the FONT project group FONT meeting January 11, 2007.
NLC - The Next Linear Collider Project  IR background issues and plans for Snowmass Jeff Gronberg/LLNL Linear Collider Workshop October 25, 2000.
CESR Beam-Beam Effects at CESR Mark A. Palmer Cornell University July 14, 2001.
P.N. Burrows BDS/MDI, LCWS08 Chicago, 17/11/081 Beam-based feedback for LC ILC luminosity goal 10**34 / cm**2 / s 3000 or 6000 bunches, spacing ns.
EM background tests of IP feedback hardware Christine Clarke Oxford University 24 th September 2007 Oxford (P. Burrows, C. Perry, G. Christian, T. Hartin,
Progress towards nanometre-level beam stabilisation at ATF2 N. Blaskovic, D. R. Bett, P. N. Burrows, G. B. Christian, C. Perry John Adams Institute, University.
The Detector and Interaction Region for a Photon Collider at TESLA
M. Woods (SLAC) Beam Diagnostics for test facilities of i)  ii) polarized e+ source January 9 –11, 2002.
NLC - The Next Linear Collider Project NLC Backgrounds What’s New? Tom Markiewicz LC’99, Frascati, Italy October 1999.
A fast RF kicker for the MEIC electron cooler Andrew Kimber Amy Sy 31 st March 2015 Thomas Jefferson National Accelerator Facility is managed by Jefferson.
An Introduction to the Physics and Technology of e+e- Linear Colliders Lecture 7: Beam-Beam Effects Nick Walker (DESY) DESY Summer Student Lecture 31 st.
August 2005Snowmass Workshop IP Instrumentation Wolfgang Lohmann, DESY Measurement of: Luminosity (precise and fast) Energy Polarisation.
Ground Motion + Vibration Transfer Function for Final QD0/SD0 Cryomodule System at ILC Glen White, SLAC ALCPG11, Eugene March 21, 2011.
Karsten Büßer Beam Induced Backgrounds at TESLA for Different Mask Geometries with and w/o a 2*10 mrad Crossing Angle HH-Zeuthen-LC-Meeting Zeuthen September.
ATF2 Javier Resta Lopez (JAI, Oxford University) for the FONT project group 5th ATF2 project meeting, KEK December 19-21, 2007.
Feedback on Nanosecond Timescales (FONT) - Review of Feedback Prototype Tests at ATF(KEK) Glenn Christian John Adams Institute, Oxford for FONT collaboration.
Philip Burrows ECFA LC Workshop, Warsaw, 10 June Philip Burrows John Adams Institute Oxford University G. Christian, C. Clarke, B. Constance, H.
NLC Intra-Pulse Fast Feedback Simon Jolly Oxford University NLC Beam Delivery Meeting July 2001.
Feedback On Nano-second Timescales: An IP Feedback System for the Future Linear Collider Requirement for a fast IP beam-based feedback system Simulation.
Karsten Büßer Beam Induced Backgrounds at TESLA for Different Mask Geometries with and w/o a 2*10 mrad Crossing Angle LCWS 2004 Paris April 19 th 2004.
FAST KICKER STATUS Fabio Marcellini On behalf of LNF fast kickers study group* * D. Alesini, F. Marcellini P. Raimondi, S. Guiducci.
Analysis of Beamstrahlung Pairs ECFA Workshop Vienna, November 14-17, 2005 Christian Grah.
Synchrotron radiation at eRHIC Yichao Jing, Oleg Chubar, Vladimir N. Litvinenko.
Feedback On Nanosecond Timescales (FONT): Robert Apsimon, Philip Burrows, Neven Blaskovic, Douglas Bett, Glenn Christian, Michael Davis, Davide Gamba,
P.N. Burrows ECFA/GDE Meeting, BDIR session, Valencia, 9/11/06 Philip Burrows John Adams Institute Oxford University FONT4 tests at KEK/ATF EM background.
Magnet Motion Produces Luminosity Loss. NLC Feedback Operation Kicker Gain Bunch Charge Measure deflected bunches with BPM and kick other beam to eliminate.
Development of a Low-latency, High-precision, Intra-train Beam Feedback System Based on Cavity Beam Position Monitors N. Blaskovic Kraljevic, D. R. Bett,
Simulation of Beam-Beam Background at CLIC André Sailer (CERN-PH-LCD, HU Berlin) LCWS2010: BDS+MDI Joint Session 29 March, 2010, Beijing 1.
LCWS2004 Paris 1 Beam background study for GLC Tsukasa Aso, Toyama College of Maritime Technology and GLC Vertex Group H.Aihara, K.Tanabe, Tokyo Univ.
Beam-Beam Background and the Forward Region at a CLIC Detector André Sailer (CERN PH-LCD) LC Physics School, Ambleside 22st August, 2009.
1 FONT R&D status Philip Burrows Douglas Bett, Neven Blaskovic, Glenn Christian, Michael Davis, Young Im Kim, Colin Perry John Adams Institute Oxford University.
Philip Burrows ALCPG11, Eugene 21/03/111 Performance of FONT at ATF2 Philip Burrows John Adams Institute Oxford University.
1 FONT IP Feedback System Implications of increase of L* Philip Burrows John Adams Institute Oxford University.
1 Muon Collider Backgrounds Steve Geer Fermilab Steve Geer MC Detector & Physics DOE June 24, 2009.
1 Feedback On Nanosecond Timescales (FONT): Philip Burrows Neven Blaskovic, Douglas Bett, Glenn Christian, Michael Davis, Young Im Kim, Colin Perry John.
1 DR -> IP Beam Transport Simulations with Intra-Train Feedback Glen White, SLAC Jan 19 th 2006.
SLAC SD0/QD0 Cryomodule Jitter Tolerance Glen White SLAC March 27 th 2007.
Dec 2004 Low Energy backgrounds in the TESLA IR Impact on feedback BPMs FONT collaboration  QMUL: P Burrows, G Christian, C Clarke, G White, S Molloy.
Dec 2004 Simulation of Low Energy backgrounds in the TESLA IR Impact on feedback BPMs FONT collaboration  QMUL: P Burrows, G Christian, C Clarke, G White,
Design of ATF2 feedback/feed-forward systems Javier Resta Lopez (JAI, Oxford University) for the FONT project group LC-ABD meeting Birmingham, 17-18th.
February 5, 2005D. Rubin - Cornell1 CESR-c Status -Operations/Luminosity -Machine studies -Simulation and modeling -4.1GeV.
Beam Dynamics IR Stability Issues Glen White / SLAC September IRENG07 Vibration tolerances for final doublet cryomodules Settlement of detector.
1 Feedback On Nanosecond Timescales (FONT): Philip Burrows Neven Blaskovic, Douglas Bett, Glenn Christian, Michael Davis, Young Im Kim, Colin Perry John.
Feb 7, 2006S. Kahn -- Muon Collider Detector Backgrounds 1 Detector Backgrounds in a Muon Collider Steve Kahn Muons Inc. LEMC Workshop.
NLC - The Next Linear Collider Project Keeping Nanometer Beams Colliding Vibration Stabilization of the Final Doublet Tom Himel SLAC NLC MAC review October.
IoP HEPP/APP annual meeting 2010 Feedback on Nanosecond Timescales: maintaining luminosity at future linear colliders Ben Constance John Adams Institute,
NLC - The Next Linear Collider Project Intra-Pulse Feedback at the NLC Interaction Point Steve Smith SLAC Snowmass 2001.
Beam dynamics in crab collision K. Ohmi (KEK) IR2005, 3-4, Oct FNAL Thanks to K. Akai, K. Hosoyama, K. Oide, T. Sen, F. Zimmermann.
Simulation of feedback BPM signals in an intense background environment A Hartin, P Burrows, G Christian, C Clarke, B Constance, H Khah, C Perry, C Swinson.
Feedback On Nanosecond Timescales (FONT) Philip Burrows Neven Blaskovic, Talitha Bromwich, Glenn Christian, Colin Perry, Rebecca Ramjiawan John Adams Institute,
Fast Beam Collision Feedbacks for luminosity optimisation at next-generation lepton colliders Philip Burrows John Adams Institute Oxford University.
Dither Luminosity feedback versus Fast IP feedback
In collaboration with P. N. Burrows, A. Latina and D. Schulte
For Discussion Possible Beam Dynamics Issues in ILC downstream of Damping Ring LCWS2015 K. Kubo.
F.Marcellini, D.Alesini, A.Ghigo
SD0/QD0 Cryomodule Jitter Tolerance
Intra-Pulse Beam-Beam Scans at the NLC IP
Hongbo Zhu (IHEP, Beijing) On behalf of the CEPC Study Group
Study of e+ e- background due to beamstrahlung for different ILC parameter sets Stephan Gronenborn.
MULTI-BUNCH SIMULATIONS OF THE ILC FOR LUMINOSITY PERFORMANCE STUDIES
Feed forward orbit corrections for the CLIC RTML
Kicker specifications for Damping Rings
Status and plans for crab crossing studies at JLEIC
CLIC luminosity monitoring/re-tuning using beamstrahlung ?
Presentation transcript:

G.R.White: F.O.N. T. From Ground Motion studies by A.Seryi et al. (SLAC) ‘Fast’ motion (> few Hz) dominated by cultural noise Concern for structures with tolerances at nm level (Final Quads) Ground Motion

G.R.White: F.O.N. T. Luminosity Loss at IP Relative offsets in final Quads due to fast ground motion leads to beam offsets of several s y (2.7 nm for NLC-H 490 GeV). Correct using beam-based feedback system or by active mechanical stabilization of Quads or both.

G.R.White: F.O.N. T. LC Bunch Structure NLC-H 500 GeV TESLA 500 GeV CLIC 500 GeV Particles/Bunch x Bunches/train Bunch Sep (ns) s x / s y (nm) 245 / / / 2.5 Feedback system demonstrated for NLC-H 500 GeV Can be modified for use at TESLA and CLIC

G.R.White: F.O.N. T. Beam-Beam Interaction Beam-beam EM interactions at IP provide detectable signal Beam-beam interactions modelled with GUINEA-PIG Shown is the kick angle and percentage luminosity loss for different vertical beam offsets

G.R.White: F.O.N. T. Fast Feedback Operation Kicker Gain Bunch Charge Measure deflected bunches with BPM and kick other beam to eliminate vertical offsets at IP Feedback loop assesses intra-bunch performance and maintains correction signal to the kicker Minimise distance of components from IP to reduce latency

G.R.White: F.O.N. T. Feedback Components Stripline BPM Distance to IP Stripline radius Stripline Width Stripline length Stripline Impedance Roundtrip time 4.3 m 1 cm 4.4 mm 10 cm 50 W 0.7 ns Stripline Kicker Distance to IP Stripline radius Stripline length Stripline Impedance Roundtrip time Azimuthal coverage Drive voltage required Drive Power 100nm correction 4.3 m 6 mm 6 mm 75 cm 50 W 5 ns 120 degrees 250 mV/nm 12.5 W BPM response peak near 714 MHz bunch spacing frequency Kicker rise-time represents slowest component System Design by Steve Smith (SLAC)

G.R.White: F.O.N. T. Feedback Simulation Simulations performed using Simulink in Matlab

G.R.White: F.O.N. T. BPM Processor 3 ns rise- time

G.R.White: F.O.N. T. Feedback Performance Latency = 37.3 ns

G.R.White: F.O.N. T. Feedback Performance

G.R.White: F.O.N. T. Kicker Gain Optimisation Luminosity loss as function of gain input and beam offset

G.R.White: F.O.N. T. Luminosity Performance Lower gains gives better performance at smaller offsets, higher gains give better performance at higher offsets Vary gain dependent on observed beam conditions

G.R.White: F.O.N. T. Bunch Jitter Effects Introduction of random bunch-bunch jitter causes feedback system to exacerbate luminosity loss at larger gains Shown is the effect of randomly offsetting the bunches in a train about a zero offset, assuming a gaussian noise distribution

G.R.White: F.O.N. T. Effect of Angle Offset Beams get small additional kick if incoming with non- compensated crossing angle, also additional lumi loss Effect not addressed with this feedback system- if significant angle offset present, additional feedback system further up- stream of IP required s y’ = 27 m rad

G.R.White: F.O.N. T. IR Layout With FB System

G.R.White: F.O.N. T. IR Pair Backgrounds e + e - Pairs and g ’s produced in Beam-Beam field at IP Interactions with material in the IR produces secondary e + e -, g, and neutron radiation Study background encountered in Vertex and tracking detectors with and without FB system and background in FB system itself Use GEANT3 for EM radiation and Fluka99 for neutrons

G.R.White: F.O.N. T. EM Backgrounds at BPM Absorption of secondary emission in BPM striplines source of noise in Feedback system System sensitive at level of about 3 pm per electron knocked off striplines Hence, significant noise introduced if imbalanced intercepted spray at the level of 10 5 particles per bunch exists GEANT simulations suggest this level of imbalance does not exist at the BPM location z=4.3m for secondary spray originating from pair background

G.R.White: F.O.N. T. Detector EM Backgrounds Insertion of feedback system at z=4.3 m has no impact on secondary detector backgrounds arising from pair background Past studies suggest backgrounds adversely effected only when feedback system installed forward of z=3 m

G.R.White: F.O.N. T. Detector n Backgrounds Default IR: 6.6 ± 1.5 × 10 9 IR with FB: 8.6 ± 2.6 × 10 9 (neutrons/cm 2 /1 MeV n equiv./yr) No significant increase in neutron flux in vertex detector area seen arising from pair background More statistics being generated VTD Layer Hits/cm 2 /1 MeV n equiv./yr

G.R.White: F.O.N. T. Summary Ground motion moving final Quads major source of luminosity loss at a future linear collider Fast IP feedback system simulations shows considerable luminosity recovery even beyond linear kick region Backgrounds do not seem to be an issue for detector components or the FB system itself in suggested BPM and kicker installation positions Hardware tests commencing at SLAC (Simon Jolly) Simulations to be extended to include TESLA and CLIC