Investigation of effects associated with electrical charging of fused silica test mass V. Mitrofanov, L. Prokhorov, K. Tokmakov Moscow State University.

Slides:



Advertisements
Similar presentations
Moisture effect on the dielectric response and space charge behavior of mineral oil impregnated paper insulation Jian Hao1, 2, George Chen2, Ruijin.
Advertisements

1 LSC/VIRGO Meeting, Caltech, March 18, 2008 Overview of Charging Research Valery Mitrofanov Moscow State University On behalf of charging subgroup LIGO-G Z.
COSMIC RAY MUON DETECTION USING SCINTILLATION COUNTER AND WAVELENGTH SHIFTING FIBERS ARUNODAYA BHATTACHARYA VSRP-2009,TIFR,MUMBAI 6/7/09.
One Arm Cavity M0 L1 L2 TM M0 L1 L2 TRIPLE QUAD 16m R = 20m, T=1% R = ∞, T=1%  Optimally coupled cavity (no mode matched light reflected back)  Finesse.
Shantanu Menon Thomas Irons Michael Jacoutot. Cosmic Rays  High energy particles (mainly protons) from outer space.  Have up to 10 million times more.
Chapter 24 Capacitance, dielectrics and electric energy storage
Electrical Techniques MSN506 notes. Electrical characterization Electronic properties of materials are closely related to the structure of the material.
Lecture 8 Capacitance and capacitors
Nonstationary electrical charge distribution on the fused silica bifilar pendulum and its effect on the mechanical Q-factor V.P. Mitrofanov, L.G. Prokhorov,
MAGNETIC MONOPOLES Andrey Shmakov Physics 129 Fall 2010 UC Berkeley.
Rydberg physics with cold strontium James Millen Durham University – Atomic & Molecular Physics group.
Measurement of the Charge of a Particle in a Dusty Plasma Jerome Fung, Swarthmore College July 30, 2004.
Timing Properties of T0 Detectors At PHOBOS Saba Zuberi, Erik Johnson, Nazim Khan, Frank Wolfs, Wojtek Skulski University of Rochester.
Forward Detectors and Measurement of Proton-Antiproton Collision Rates by Zachary Einzig, Mentor Michele Gallinaro INTRODUCTION THE DETECTORS EXPERIMENTAL.
Performance of the DZero Layer 0 Detector Marvin Johnson For the DZero Silicon Group.
LIGO-G Z D. Ugolini, LSC March Progress Report on Charging Measurements at Trinity University Dennis Ugolini, Robert McKinney, Mark Girard.
LIGO-G Z D. Ugolini, Charging Workshop July UV Illumination Studies at Trinity University Dennis Ugolini, Mark Girard 2007 Workshop on.
Recent Developments toward Sub-Quantum-Noise-Limited Gravitational-wave Interferometers Nergis Mavalvala Aspen January 2005 LIGO-G R.
CPD and other imaging technics for gas sensor Mizsei, János 18-28/05/2006 Ustron Budapest University of Technology and Economics, Department of Electron.
GWADW, May 2012, Hawaii D. Friedrich ICRR, The University of Tokyo K. Agatsuma, S. Sakata, T. Mori, S. Kawamura QRPN Experiment with Suspended 20mg Mirrors.
Foundations of Physics
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
LIGO-G Z D. Ugolini, LSC March Developing a Kelvin Probe for Measuring Surface Charge on LIGO Optics Dennis Ugolini, Robert McKinney Trinity.
Overview of Research in the Optics Working Group Gregory Harry, on behalf of the OWG Massachusetts Institute of Technology July 25, 2007 LSC Meeting –
ILIAS GW Meeting Mallorca - October 23-24, 2005Luca Taffarello Status of the commissioning of the AURIGA detector Luca Taffarello (INFN Sezione di Padova)
Trinity Charging Experiment Gregg Harry, MIT On behalf of Dennis Ugolini, Trinity LIGO-G R.
STREGA WP1/M1 mirror substrates GEO LIGO ISA Scientific motivation: Mechanical dissipation from dielectric mirror coatings is predicted to be a significant.
Conceptual Design for Advanced LIGO Suspensions Norna A Robertson University of Glasgow and Stanford University for the GEO suspension team +contribution.
Z B Zhou, Y Z Bai, L Liu, D Y Tan, H Yin Center for Gravitational Experiments, School of Physics, Huazhong University of Science.
G O D D A R D S P A C E F L I G H T C E N T E R Surface Potential Measurements with the LISA Kelvin Probe Jordan Camp LIGO/LISA Charging Workshop July.
NEW COMMENTS TO ILC BEAM ENERGY MEASUREMENTS BASED ON SYNCHROTRON RADIATION FROM MAGNETIC SPECTROMETER E.Syresin, B. Zalikhanov-DLNP, JINR R. Makarov-MSU.
The investigation of thermal and non- thermal noises in fused silica fibers for Advanced LIGO suspension Moscow State University Bilenko I.A. Lyaskovskaya.
Y Z Bai, H Yin, L Liu, D Y Tan, Z B Zhou Center for Gravitational Experiments, School of Physics, Huazhong Univ. of Science &
LRT2004 Sudbury, December 2004Igor G. Irastorza, CEA Saclay NOSTOS: a spherical TPC to detect low energy neutrinos Igor G. Irastorza CEA/Saclay NOSTOS.
Test mass charge relaxation V.P.Mitrofanov, P.E.Khramchenkov, L.G.Prokhorov Moscow State University LIGO/VIRGO LSC Meeting, Baton Rouge, March 2007 G Z.
G R LIGO R&D1 Wireless optical controls of LIGO static suspensions actuators Maria Paola Clarizia University of Sannio Mentor: Riccardo De Salvo.
PeTeR: a hardware simulator for LISA PF TM-GRS system 23/05/ th LISA Symposium May 2012, BnF Paris L. Marconi and R. Stanga Università degli.
Parametric Instabilities and Control Li Ju ( 鞠莉), Chunnnong Zhao, David Blair Jiayi Qin, Qi Fang, Carl Blair, Jian Liu University of Western Australia.
LIGO- G D Proposal to the NSF: Low Noise Suspensions and Readout Systems for Future LIGO Interferometers Stan Whitcomb LIGO Program Advisory Committee.
Mechanics Electricity & Magnetism Thermal & Modern.
LCGT Technical Review Suspension Point Interferometer for Parasitic Noise Reduction and an Additional IFO S.Miyoki (ICRR, Univ. of TOKYO)
Test mass charge relaxation V.P.Mitrofanov, P.E.Khramchenkov, L.G.Prokhorov Moscow State University.
Cold damping of fused silica suspension violin modes V.P.Mitrofanov, K.V.Tokmakov Moscow State University G Z.
LIGO-G Z Mirror Q’s and thermal noise in the TNI with ring dampers Akira Villar LIGO Seminar April 20, 2006 Eric D. Black, Kenneth G. Libbrecht.
Effect of Charging on Thermal Noise Gregory Harry Massachusetts Institute of Technology - Core Optics and Suspensions Working Groups - March 19, 2004 –
D. Ugolini, Joint APS-AAPT Meeting at UT-Arlington, October 2006 Developing a Capacitive Probe for Measuring Charging Effects on In-Vacuum Optics Dennis.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
Thermal Noise performance of advanced gravitational wave detector suspensions Alan Cumming, on behalf of the University of Glasgow Suspension Team 5 th.
Parametric Instabilities In Advanced Laser Interferometer Gravitational Wave Detectors Li Ju Chunnong Zhao Jerome Degallaix Slavomir Gras David Blair.
Thermoelastic dissipation in inhomogeneous media: loss measurements and thermal noise in coated test masses Sheila Rowan, Marty Fejer and LSC Coating collaboration.
16722 We: noise51+1 noise We: noise51+2 noise: signal you don’t want technical noise: sources we can control.
QuarkNet and Cosmic Ray Muon Flux Experiments Florida Academy of Sciences Spring Conference 2009 Alfred Menendez and Michael Abercrombie with Dr. Marcus.
J.Vaitkus IWORID6, Glasgow,
Thermal Noise in Thin Silicon Structures
1 Kazuhiro Yamamoto Institute for Cosmic Ray Research (ICRR) the University of Tokyo KAGRA face to face meeting University of Toyama, Toyama, Japan 3 August.
Mechanical Mode Damping for Parametric Instability Control
Optical Spring Experiments With The Glasgow 10m Prototype Interferometer Matt Edgar.
LIGO-G Z Silicon as a low thermal noise test mass material S. Rowan, R. Route, M.M. Fejer, R.L. Byer Stanford University P. Sneddon, D. Crooks,
Study of repulsive nature of optical potential for high energy 12 C+ 12 C elastic scattering (Effect of the tensor and three-body interactions) Gaolong.
Measurement of coating mechanical loss Junko Katayama, K.Craig, K.Yamamoto, M.Ohashi ICRR 0.
Day 93, Monday, 1 February, 2016 Capacitance Electric Fields Electric Potential Coulombs Millikan's Oil Drop Experiment Capacitors Coulomb’s Law.
XI Workshop on Resistive Plate Chambers and Related Detectors, INFN, 5-10 February, Aging test of high rate MRPC Wang Yi Department of Engineering.
LIGO-G Z Bilenko I.A. Gromova E.S. 1 Recent Results on the Measurement of Transmission and Scattering Structure on Doped and Non-doped Mirrors.
PES 1000 – Physics in Everyday Life
Nergis Mavalvala Aspen January 2005
S. Rowan, M. Fejer, E. Gustafson, R. Route, G. Zeltzer
Ponderomotive Squeezing Quantum Measurement Group
General Physics (PHY 2140) Lecture 6 Electrostatics
FIGURE 12-1 A Leyden jar can be used to store an electrical charge.
FIGURE 12-1 A Leyden jar can be used to store an electrical charge.
Presentation transcript:

Investigation of effects associated with electrical charging of fused silica test mass V. Mitrofanov, L. Prokhorov, K. Tokmakov Moscow State University P. Willems LIGO Project, California Institute of Technology LIGO-G Z

2 Introduction Fused silica mirrors — dielectric bodies suspended in high vacuum They can trap and store electrical charges These charges interact through electrostatic coupling with the environment and electrostatic actuators in particular Result of this interaction may be:  additional loss  degradation of mechanical Q  additional thermal noise  accidental variation of electrical charge  q  variation of Coulomb force  additional noise

3 Mechanical loss in fused silica oscillators due to electrical charges or electric field A number of experiments which have demonstrated the effects of electrical charge on mechanical loss: Univ. of Glasgow (Class. Quantum Grav., 14 (1997) 1537 Moscow State Univ. (Phys. Lett. A., 278 (2000) 25 MIT (Rev. Sci. Instrum., 74 (2003) 4840 The mechanism of loss is not clear (only hypotheses were proposed) Nevertheless it is likely that the additional thermal noise associated with charges is not dangerous for Adv. LIGO if the electrical charge on mirrors is not unduly large

4 Experimental setup Vacuum p < Torr All fused silica bifilar pendulum: Mass M = 0.5 kg, Fibers: L = 25 cm, d =200  m, Torsion mode f  1.14 Hz, Quality factor Q  8  10 7, Relaxation time  *  2.2  10 7 sec, Initial amplitude A  0.07 rad Multistrip capacitive probe (two sets of gold strips sputter-deposited on fused silica plate) connected with high impedance amplifier. Probe voltage U = k  q  A q – electrical charge on the pendulum (distribution of charge is unknown)

5 Long-term measurements of probe signal in process of free decay of the cylinder oscillation About 2 years of observation a lot of runs ( each run is about 30 days )  Averaged rate of charge variation:  10 4 e/cm 2 day (assuming uniform distribution of charge on the end face of the cylinder)  Charge variation corresponds to negative charging of the cylinder  Resolution in measurement of charge is limited by seismic noise and parasitic effects

6 - Why we continue to study behavior of electrical charges on fused silica test masses? 1) 2) mass - q+  q d Conductive plate q=10 8 e  q= 10 4 e D=3 mm mass High energy particle Surface layer Surface charge Generation of mobile charges within surface layer of the material Their separation in electric field of surface charges

7 Rare big jumps of signal from the probe synchronous with fast decrease of the cylinder amplitude 4 events in 12 runs of measurements multistep structure of jump  Initial charge density: of order of e/cm 2  After the jump: of order 10 8 e/cm 2 (assuming uniform surface free charge density) Change of amplitude in the process of jump corresponds to damping Q -1 of order of Resolution of details is determined by averaging time – 70 sec

8 Behavior of the system after the first jump After the first jump: Repeated increase of torsion amplitude by means of electrostatic excitation results in a new cascade of jumps of amplitude and voltage from the probe (spoiled state of the system “fused silica pendulum  nearby electrodes”) With time elapsed from the first jump fast changes of the probe’s voltage decrease. Spoiled state transfers to the original state within relaxation time of order of one month

9 Possibility that the pendulum modes of the cylinder causes it to touch the electrode A contact electrification can take place if the pendulum is swinging far enough to touch the electrode plate due to seismic excitation Only torsional amplitude is well measured by the optical sensor The electrometer signal on the pendulum frequencies give information about pendulum amplitudes with large uncertainty So we can not control the touching or close approach of the pendulum to the electrode plate in this set up

10 Changes of torsional amplitude and probe signal in the case of provoked touching For the provoked touching behavior of the system is much the same as it is in the case of our “jumps”: decrease of amplitude and increase of probe signal as well as transfer to the “spoiled” state There are at least two distinctive property of provoked touching: In the case of provoked touching change of amplitude and probe signal is fast (within the time resolution)

11 Changes of torsional amplitude and probe signal in the case of provoked touching Admission of small portion of air into the chamber results in significant drop of probe signal (supposedly due to gas breakdown). After the “jump” the probe signal can be reduced only by electrical discharge in rough vacuum These facts can not be the evidence for the absence of touching in our experiments. It is worth further investigation Change of probe signal after admission of air

12 Search for correlation between signals from the probe and cosmic ray detectors Cosmic ray detector system 11 particle detectors (plastic scintillator paddles 180  18  0.8 cm 3 ) supplied by photomultipliers were installed around the vacuum chamber with the pendulum Selection of events with maximum summarized voltage from all paddles Vacuum chamber Scintillation detectors ADC Threshold setting Computer Peak detectors Wall

13 Result of measurements We have not found statistically significant time coincidences between large signals from detectors and jumps of charge and amplitude in the “spoiled” state of the test mass But we can not exclude correlation with: low energy particles passing locally through the surface layer of the test mass

14 Conclusion We have a number of empirical facts but we can not unambiguously interpret these facts yet We suppose that the electronic properties of the surface of dielectric mirror can play the important role but they are poorly studied till now We do not yet ready to say that electrical charges are not dangerous for LIGO