NEUTRON EDM Philip Harris, on behalf of the CryoEDM collaboration: Rutherford Appleton Laboratory University of Oxford University of Sussex ILL University.

Slides:



Advertisements
Similar presentations
1 MICE Beamline: Plans for initial commissioning. Kevin Tilley, 16 th November. - 75days until commissioning Target, detectors, particle production Upstream.
Advertisements

Cryomodule Helium Volumes Tom Peterson, Fermilab AWLC14 13 May 2014.
IKON7, Instrument clip session, September 2014, ESS Headquarters and Medicon Village, Lund, Sweden A cold neutron beamline for Particle
Fermilab E906 Schedule Paul E. Reimer 20 June 2008.
1 Configuration Development for HIF Final Focus Superconducting Quadrupole Array HIF Final Focus Meeting July 2, 2002 Tom Brown Chang Jun Phil Heitzenroeder.
Philip Harris University of Sussex (for the EDM Collaboration) The Neutron EDM Experiments at the ILL.
1 MICE PM Report Installations to date Future installation work Preparations for Phase Two Target status MICE Video Conference, 22nd May, 2008.
The cryogenic neutron EDM experiment at ILL and the result of the room temperature experiment James Karamath University of Sussex.
Neutron background measurement at LNGS: present status Measurement carried out in collaboration between LNGS ILIAS-JRA1 and ICARUS groups.
Studies of radiation hardness of ECAL modules 1Yu. Guz 2013/05/28.
H IGH L UMINOSITY LHC WP1 - CERN S AFETY R EQUIREMENTS Stefan Roesler - Phillip Santos Silva – Ralf Trant EDMS# HSE Unit April 2011.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices iteratively to determine trace.
MICE TECHNICAL UPDATE & ISIS/RAL PLANS. Belgium Italy Japan The Netherlands Russian Federation Switzerland UK USA Acknowledge.
What happened to our shutter? and a brief description of our upstream beamline for those who were not around when it was built.
Fundamental Physics With Cold and Ultra-cold Neutrons Albert Young North Carolina State University.
Task 6: Short Period Nb 3 Sn Superconducting Helical Undulator Dr Owen Taylor Institutes Science and Technology Facilities Council (STFC) UK –Daresbury.
Neutron Beam Intensity for the Spallation Neutron Source Beamline 13: The NPDGamma Experiment Analysis and Results Jeremy Stewart University of Tennessee.
1 Flux concentrator for SuperKEKB Kamitani Takuya IWLC October.20.
G-2 accelerator and cryo needs Mary Convery Muon Campus Review 1/23/13.
1 Target Station Design Dan Wilcox High Power Targets Group, Rutherford Appleton Laboratory EuroNu Annual Meeting 2012.
CryoEDM at ILL Philip Harris.
Collab 4/15/04 #1 EDMEDM UIUC meeting 12/3/2004 Walter Sondheim, P-25, Los Alamos for presentation to The EDM Collaboration UIUC meeting, Urbana, IL UCN.
June 17, 2004 / Collab Meeting Strategy to reduce uncertainty on a  to < 0.25 ppm David Hertzog University of Illinois at Urbana-Champaign n Present data.
Plots from RCNP UCN Run (April 20-25, 2010). EDM Set-up Schematic H0H0 (RF) H 1 Spin Flipper RF Coil Spherical Coil Cell Valve EDM Cell Magnetized Foil.
1 Target Station Design for Neutrino Superbeams Dan Wilcox High Power Targets Group, Rutherford Appleton Laboratory NBI 2012, CERN.
Thomas Jefferson National Accelerator Facility G0 Collaboration Meeting, June 18-19, 2003 Updates G0 Tiger Laser High Polarization Photocathodes Mott polarimeter.
CryoEDM – A Cryogenic Neutron-EDM Experiment Collaboration: Sussex University, RAL, ILL, Kure University, Oxford University Hans Kraus … but before: some.
March 18, 2008 TJRMICE Beamline Status1 MICE Beamline Status (March 18, 2008) Tom Roberts Muons, Inc. Illinois Institute of Technology.
RSVP AGS Upgrade Projects MECO RSVP Preliminary Baseline Review Brookhaven National Lab April 6-8, 2005 D. Phillips.
1 How Can We Get More Neutrons? Upgrade Paths for the EDM Geoff Greene University of Tennessee /Oak Ridge National Laboratory Oct 2006.
RSVP AGS Upgrade Projects MECO RSVP Preliminary Baseline Review Brookhaven National Lab April 6-8, 2005 D. Phillips.
COMET. μ-e conversion search from muonic aluminium J-PARC pulsed proton beam to produce pulsed muon beam Forbidden in the Standard Model  clue to the.
Collab_NSAC 4/2/03 #1 EDMEDM Martin Cooper, Los Alamos Co-spokesperson for the EDM Project for presentation to EDM Collaboration Meeting Los Alamos, NM.
Electric dipole moment searches E.A. Hinds Birmingham 11 th July 2011 Centre for Cold Matter Imperial College London.
Triple GEM Beam Test within PHENIX DC Upgrades Meeting 4/14/04 B. Azmoun PHENIX Brookhaven National Lab.
LHC-CC Validity Requirements & Tests LHC Crab Cavity Mini Workshop at CERN; 21. August Remarks on using the LHC as a test bed for R&D equipment.
Commissioning of REX Jose Alberto Rodriguez, BE-OP-PSB (167538) on behalf of the ISOLDE operations team.
EDM Assembly and Commissioning – or – How to Cut Two Years from the Project P. Huffman and V. Cianciolo.
Philip Burrows MDI Panel Meeting 15/08/06 Philip Burrows John Adams Institute Oxford University SiD and IR/MDI Issues.
The cryogenic neutron EDM experiment at ILL Technical challenges and solutions James Karamath University of Sussex.
BASIC SKETCH OF ACTIVITIES FOR THE CERN LHCB-RICH TEAM (2012 – 2017) Team composition Present activities and consolidation plans RICH – CERN R&D and Upgrade.
SCU 3-Lab Review Meeting, Dec. 16, 2014 SCU Presentations Today Intro. & Performance Motivations (P. Emma, SLAC, 20+5) Conceptual Cryostat Design: Option-A.
A monochromatic neutrino beam for  13 and  J. Bernabeu U. de Valencia and IFIC NO-VE III International Workshop on: "NEUTRINO OSCILLATIONS IN VENICE"
A. Baldini PSI July 05 Overview of the experiment MEG is being built (Beam line, Magnet, LXe, DC, TC, Elect., Software) Delays in some items: O(months)
Cryogenic scheme, pipes and valves dimensions U.Wagner CERN TE-CRG.
Assembly 12/14/06 #1 Assembly and Commissioning Paul Huffman.
Neutron and electron EDMs PPAP meeting, Birmingham, 18 th September 2012 Mike Tarbutt Centre for Cold Matter, Imperial College London.
HEBT Design Considerations Jingyu Tang, Xiangqi Wang, Hao Hao, Jiajia Tian IHEP, USTC International Review Meeting on Accelerator Physics Design of C-ADS,
SOLEIL OPERATION AND ON-GOING PROJECTS C. Herbeaux On behalf of SOLEIL Groups C. Herbeaux, November ESLS23, 24-25, 2015, PSI1.
1. Baseline – from LMC  Presentation by F. Bordry at LHC Machine Committee 5.10 on LS1 Organisation: 1. Linac4 is not going to be connected.
Lucio Rossi The High Luminosity LHC Project Distinguished Lecturer 2013.
Yannis K. Semertzidis Brookhaven National Laboratory New opportunities at CERN CERN, 12 May 2009 Storage Ring EDM Experiments The storage ring method can.
June 2, 2008 Bill Wisniewski1 BaBar Disassembly and Disposal Overview.
Specifications for the Integrated Tests II Paul Huffman.
Operation Status of the RF Systems and Taiwan Photon Source
Latest results from the superfluid-helium UCN source SUN2 at ILL
CBM magnet overview of the BINP work
Requirements for Efficient CW SRF Cryomodules
Neutron and electron electric dipole moments
Introduction BaBar Components The Problem IFR Upgrade: 2004 & 2005
EDM Experiments: UK interests
Validating Magnets Using Beam
Muon Front End Status Chris Rogers,
Effect of Reduced Focus Coil Current on Step IV and Step VI
Status of FMS Refurbishment
K. Tilley, ISIS, Rutherford Appleton Laboratory, UK Introduction
Muon Collider Magnet Technologies/Challenges
cNPM pre-CDR Concluding Remarks
Review of Quench Limits
Presentation transcript:

NEUTRON EDM Philip Harris, on behalf of the CryoEDM collaboration: Rutherford Appleton Laboratory University of Oxford University of Sussex ILL University of Kure

Technology Neutrons in HV in

Sensitivity (NB sensitivity/day is actually closer to ) Successfully produced, transported, stored UCN, but need to reduce losses Successfully applied 10 kV/cm (same as previous expt); aiming for kV/cm Achieved 60% polarisation in source, but must improve RT-edm: 130 s. So far we have 62 s cell storage time.

Sensitivity in 2012 Room-temperature expt final sensitivity ~2E-25 ecm/day Took 12 years of incremental developments from known technology Systematics limited (geometric phase effect) We can come within factor 4-5 of this in 2012 by increasing detector area x10: technology now proved refurbishing damaged detector-valve: in hand applying ~70 kV (previously ~40 kV): should be straightforward opening beam aperture from 43 to 50 mm: depends on radiation levels retaining polarisation: superconducting material has been removed There may be additional improvements beyond this  peak above background (detector improvement) Polarisation to 60% (improved guide field) Increasing cell storage lifetime (insulator bakeout) (we will achieve these by 2014)

Shutdown and move to new beamline Mid-2013: Have to vacate current location. ILL will shut down for a year; we will move to new dedicated beamline. New beam 4x more intense; and dedicated Due to become operational mid-2014 Beam must then be characterised (9A flux, divergence, stability, polarisation) We will then have access to the area (late 2014) to move our apparatus into it. M&O uplift requested to fund move and infrastructure in new location.

Upgrade : Upcoming PPRP request Not yet fully costed Major upgrade to experiment: Cryogenics design changes: Pressurise the liquid helium: increase E field x 2-3 Upgrade from two-cell to four-cell system 2 x neutrons Cancellation of some systematic effects Installation of inner superconducting magnetic shield B-field stability improves x1000, for systematics Construction of non-magnetic SCV Improves depolarisation: better T 2 Overcome geometric-phase systematic error Net result: Order of magnitude improvement in sensitivity Commensurate improvement in systematics

Sensitivity timeline DateItem factorecm/year Comment 2002RT-edm 1.7E-26 Baseline 2010CryoEDM commission 1.7E Large-area detector E-25 Proven 2012HV to 70 kV E-25 OK to 50 kV, lab tests suggest should work at 70 kV 2012Repair detector valve E-25 Repair – should be fine 2012Polarisation 60% E-25 Seen in source. Should transfer ok to cells. 2012Aperture to 50 mm E-25 Will increase radiation levels slightly, but should be ok 2012Ramsey time to 60 s E-26 Almost certain – undergoing mag. scan now to confirm 2013See alpha peak E-26 Quite likely by 2012, but we do not count on it by then 2014New beam E-26 ILL produced this estimate 2014Recover missing input flux? E-26 Depends on geometry match to new beam. 2014Improve cell storage lifetime to 100 s E-27 Not guaranteed, but haven't yet tried most obvious solutions (e.g. bakeout), so improvement likely 2014Match aperture to beam E-27 Likely 2015HV to 135 kV E-27 Requires pressurisation. Lab tests show this is realistic. 2015Four-cell system E-27 Guaranteed part of upgrade 2015Polarisation to 90% E-27 No known reason why not Inner supercond. shield Lab tests on scale model shows factor Cryogenics Included in upgrade Non-magnetic SCV Included in upgrade

Sensitivity and systematics Without upgrade, we may reach factor ~3 better stats than RT- edm (possibly better if storage lifetime improves significantly). Systematics is a different matter. Back-to-back cells (4-cell system) provide important cancellations Completely non-mag SCV would eliminate most of geometric-phase systematic (which limited RT-edm). 1 nT/m very difficult otherwise. Magnetic shielding controls fluctuations, reduces broadening of Ramsey fringes Changes to cryogenics would increase reliability (reduce down-time), reduce manpower burden, reduce He consumption... With upgrade, should reach factor ~10 improvement in stat sensitivity, with commensurate improvement in systematics.