Laser systems for LISA and its precursor mission LISA ... · Seed lasers for LISA AEI Hannover...

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GWADW / Elba 23.05.2011

Laser systems for LISA

and its precursor mission LISA Pathfinder

Michael Tröbs

Max-Planck-Institut für Gravitationsphysik und Universität Hannover

1

GWADW / Elba 23.05.2011

Lasers for LISA Pathfinder

AEI Hannover

2

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LISA Pathfinder optical metrology system

AEI Hannover

3

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LISA Pathfinder interferometry concept

AEI Hannover

4

Heinzel et al. CQG vol. 20 pp. S153 (2003)

GWADW / Elba 23.05.2011

LISA Pathfinder interferometry concept

AEI Hannover

stableunstable

GWADW / Elba 23.05.2011

LISA Pathfinder Interferometry concept

AEI Hannover

6

reference

interferometer

measurement

interferometer

Wand et al. CQG vol. 23 pp. S159 (2006)

GWADW / Elba 23.05.2011

LISA Pathfinder hardware implementation

AEI Hannover

7

stable

Laser Laser modulator Optical bench

unstable

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LISA Pathfinder optical bench PFM

AEI Hannover

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LISA Pathfinder optical bench PFM

AEI Hannover

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Laser system for LISA Pathfinder

AEI Hannover

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Reference laser unit FM free-running noise

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Frequency noise Relative power noise

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Laser frequency stabilization

AEI Hannover

12

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Laser power stabilisation

AEI Hannover

13

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Optical pathlength difference stabilisation

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14

reference

interferometer

measurement

interferometer

Pathlength

changes

common-mode

in reference and

measurement

interferometers

Common-mode noise suppression only works down to nm/√Hz

GWADW / Elba 23.05.2011

Optial pathlength difference stabilisation

AEI Hannover

15

Wand et al. CQG

vol. 23 pp. S159 (2006)

GWADW / Elba 23.05.2011

Optical pathlength difference stabilisation

AEI Hannover

16Wand et al. CQG vol. 23 pp. S159 (2006)

GWADW / Elba 23.05.2011

AEI Hannover

17

GWADW / Elba 23.05.2011

LISA laser

AEI Hannover

18

GWADW / Elba 23.05.2011

LISA laser system components

AEI Hannover

19

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Seed lasers for LISA

AEI Hannover

20Tröbs et al. JOSAB 26 pp. 1137 (2009)

GWADW / Elba 23.05.2011

Ultra Stable Oscillator (USO) phase noise

Phase noise of on-board

clocks (USOs) is too high!

Therefore low noise in

clock tone transfer chain required

Baseline design concept: measure

phase noise for later cancellation.

GWADW / Elba 23.05.2011

USO clock tone transfer chain

2 GHz

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USO phase noise measurement

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Requirements

Phase read-out:

Ancillary Modulation Error:

LISA frequency band:

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EOM phase fidelity

AEI Hannover

25

Barke et al. Appl Phys B (2010) 98: 33–39

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Phase characteristics of optical amplifiers

Potential sources of differential phase noise in amplifiers

Lc

fEOM2

• nonlinear dispersion and

laser frequency changes

• first measurements show

tiny effect

• should be negligible in LISA

GWADW / Elba 23.05.2011

Phase characteristics of optical amplifiers

Optical amplifiers under test

Core-pumped amplifier

Two identical stages

Pumping directly the core of a

single-mode fiber

2 x 0.4 m active fiber

1 W output power

Cladding-pumped amplifier

Single stage

Pumping in the multi-mode

cladding

3 m active fiber

1 W output power

Amplifiers supplied by Laser Zentrum Hannover e. V.

GWADW / Elba 23.05.2011

Phase characteristics of optical amplifiers

Optical amplifiers under test

Core-pumped amplifier

Two identical stages

Pumping directly the core of a

single-mode fiber

2 x 0.4 m active fiber

1 W output power

Cladding-pumped amplifier

Single stage

Pumping in the multi-mode

cladding

3 m active fiber

1 W output power

Amplifiers supplied by Laser Zentrum Hannover e. V.

GWADW / Elba 23.05.2011

Phase characteristics of optical amplifiers

Measurement setup

GWADW / Elba 23.05.2011

Phase characteristics of optical amplifiers

Differential phase noise of amplifiers

1 W output power

Within LISA requirement 2 GHz sideband frequency

Tröbs et al. JPCS (2010) 208: 012042

GWADW / Elba 23.05.2011

Summary

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31

GWADW / Elba 23.05.2011

Thank you

AEI Hannover

32LISA Pathfinder in acoustic test chamber at ESA

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