Power Stabilization of the 35W Reference System

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Power Stabilization of the 35W Reference System Frank Seifert, Patrick Kwee, Benno Willke, Karsten Danzmann Max-Planck-Institute for Gravitational Physics (Albert-Einstein-Institute) University of Hannover LSC Caltech, March 19th, 2008 LIGO-G08xxxx-xx

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Power Stabilization of the 35W Reference System. Frank Seifert, Patrick Kwee, Benno Willke, Karsten Danzmann Max-Planck-Institute for Gravitational Physics (Albert-Einstein-Institute) University of Hannover LSC Caltech, March 19th, 2008 LIGO-G08xxxx-xx. 35W Laser Overview. - PowerPoint PPT Presentation

Transcript of Power Stabilization of the 35W Reference System

Page 1: Power Stabilization of the 35W Reference System

Power Stabilization of the 35W Reference System

Frank Seifert, Patrick Kwee, Benno Willke, Karsten Danzmann

Max-Planck-Institute for Gravitational Physics(Albert-Einstein-Institute)

University of Hannover

LSC Caltech, March 19th, 2008

LIGO-G08xxxx-xx

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35W Laser Overview

• More details see Saschas talk „ELIGO Laser„ wednesday afternoon

• Design & fabrication by LZH• 2W NPRO seed laser• 4-stage Nd:YVO amplifier• > 35 W output power• Assembled on breadboard in

single housing• AOM, EOM, isolator, and shutter

included• Running 24/7 @ AEI since 12/07

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35W Laser Performance

• More details (spatial profile etc.) see Saschas talk „ELIGO Laser„ wednesday afternoon

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Power Actuators I : AOM

• AOM: Crystal Technology 3080-194• Driver: Landwehr A274-18 (80MHz, 5W max)

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Power Actuators I : AOM (cont.)

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Power Actuators II: LD current

• „Digital modulation“ via Beckhoff @ diode control box• 2 inputs → 2 laser diodes each (in series)• Modulation index adjustable via touch panel• On/Off-control via touch panel• Low speed

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Reference System Setup

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Spatial filtering

• Classical PMC design (only reflectivities changed)

• F≈46 (p-pol) / F≈383 (s-pol)• Locked in s-pol most of the time

since 12/07• higher circulating power as for

the 200W laser system(factor 8.3 between s and p→ 33W x 8.3 = 275W)

• Curved mirror T=20ppm (for power stabilization in-loop PD)

• Small acoustic enclosure

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Reference System Setup (cont.)

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Free Running Noise

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First Results

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First Results (cont.)

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Work In Progress

• Further reduction of beam pointing → shorter beam pathes, beam tubes(?)

• Reduction of scattered light → superpolished mirrors, block ghost beams

• Increasing loop gain and bandwidth

• More in-loop power → (second) in-loop detector behind PMC

• Reduction of particle count → beam tubes (?)

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Other related work

• Photodiode characterization for >500mA detector:- breakdown voltage (dark current vs bias)- linearity- thermal impedance

• Resistor current noise:- 40 different types measured so far (100 Ohm)- higher values next couple of weeks

• New high current photodetector topologies:- lower input referred noise / higher photocurrent without decreasing effective gain

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spare slides

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Resistor Current Noise

10-9

10-8

10-7

10-6

100 101 102 103 104

frequency [Hz]

resistor current noise / 100 / SMD / P<1W / 10V voltage drop

Johnson noise 100, 300K1/ f

Welwyn PCF0805, 0.1%, 5ppmPhycomp TFx13 series, 0.1%, 25ppm

Vishay Beyschlag MMA 0204, 1%, 50ppmVishay SMM0204-MS1, 1%, 50ppm

Vitrom ZC 0204, 1%, 50ppmMira Electronic 1206, 1%, 100ppmMira Electronic 0805, 1%, 100ppm

Yageo RC 0805, 1%, 100ppmYageo RC 1206, 1%, 100ppm

10-9

10-8

10-7

100 101 102 103 104

frequency [Hz]

resistor current noise / 100 / leaded / P<1W / 10V voltage drop

Johnson noise 100, 300K1/ f

Arcol MRA 0207, 0.1%, 15ppmWelwyn RC55Y, 0.1%, 15ppm

Vishay Beyschlag MBB 0207, 0.1%, 25ppmYageo MF0207, 0.1%, 25ppm

Tyco LR1F, 1%, 50ppmVishay Beyschlag MBB 0207, 1%, 50ppm

Yageo MF0207, 1%, 50ppmRamtronics, 1%, ??ppm

Uni-Ohm CFR-25, carbon, 5%, 450ppmVishay S102K, 0.1%, 2ppm

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Power Stabilization Setup

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Results – DC & AC Coupled Loop

Shot noise level 2E-9

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Critical Factors

• very (!) sensitive to ground loops avoid any (!) ground loop, even at RF (capacitive coupling) independent supply of components battery powered devices

• beam pointing reduction by PMC (passive filtering) proper adjustment of photodiodes (minimize with impressed pointing) (PZT behind PMC)

• acoustics shielded environment proper mechanical design

• air currents vacuum

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Photodiode Non-uniformity & Pointing

pointing measurementspatial uniformity measurement

(when) does it limit the performance ?

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Pointing Sensitivity Measurement

EG&G C30642G

3 different methods very good agreement

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Power Fluctuations Due To Pointing

PMC: F=4100

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Low Frequency Noise in PD‘s

• pre-stabilized laser system below 1E-8 level• amplification after substraction of photocurrents• temperature stabilized photodiodes• vacuum tank

Balanced detection setup

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Balanced Detection Setup

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Balanced Detection – First Experiment

first test of balanced detection setup with large area Si photodiodeswithout temperature stabilization:

nearly shot noise limited

unknown noise source

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Balanced Detection – Results (1)

bias voltage dependence:

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Balanced Detection – Results (2)

temperature dependence:

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Balanced Detection – Results (3)

power dependence:

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Low Frequency Limit

:PD low frequency noise limiting ?:

different photodiodes !!

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Photodiode Temperature Measurements

• ∆T only ≈ 10K• real chip temperature ?

P = 0 mW P = 65 mW

P = 130 mWP = 105 mW

PD EG&G C30642Gwithout window