1. Experimental test of higher-order LG modes in the 10m Glasgow prototype interferometer B. Sorazu, P. Fulda, B. Barr, A. Bell, C. Bond, L. Carbone, A. Freise, S. Hild, S. Huttner, J. Macarthur, K. Strain LIGO-G1100752

2. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Introduction – Overview Motivation of the current work. Presenting Glasgow interferometric GW detector 10 m prototype. LG 33 mode generation on the prototype’s input laser bench. Preliminary results. Conclusions. 1

3. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Motivations Higher-order LG mode beams are being considered for implementation on future generations of GW interferometers. LG modes are expected to considerably reduce thermal noise (both mirror coating and substrate Brownian noise) in comparison with TEM 00 beams [1,2,3]. Results from simulation work and benchtop experiments [3,4] on higher order LG mode interferometry encourage us to take the next step; testing in an environment similar to an interferometric GW detector. [1] B. Mours et al. Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes, CQG 23, 5777, 2006 [2] J.-Y. Vinet On special optical modes and thermal issues in advanced gravitational wave interferometric detectors, Living Revs. Rel. 12(5), 2009 [3] S. Chelkowski et al. Prospects of higher-order Laguerre- Gauss modes in future gravitational wave detectors, Physical Review D 79,122002, 2009 [4] P. Fulda et al. Experimental demonstration of higher-order Laguerre-Gauss mode interferometry, Physical Review D 82, 012002, 2010 2

4. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 The Glasgow 10m Prototype Interferometer GEO-like infrastructure:  Similar vacuum systems  Triple stage GEO- suspensions  Same local control Ideal test bed for advanced interferometry concepts (e.g. Signal recycling, optical spring). Fast turn around for rapid, small-scale tests Timely validation of various innovative technologies (e.g. higher order LG modes, diffractive interferometry) Excellent training for students and Postdocs 3

5. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Maximise potential of the Glasgow prototype by carrying out several strands of experiments in parallel: Direct measurement of thermal noise 3-mirror coupled cavity systems: Control strategies  S.Huttner et al. Novel sensing and control schemes for a three-mirror coupled cavity, CQG 24, 3825, 2007.  B. Barr et al. Optical modulation techniques for length sensing and control of optical cavities, Appl. Opt. 46, 2007.  S. H. Huttner et al. Techniques in the optimization of length sensing and control systems for a three-mirror coupled cavity, CQG 25, 235003, 2008. Radiation pressure experiments  more at Monday poster session, poster 7: B. Barr Optical springs on a prototype scale Frequency reference for TN experiment The Glasgow 10m Prototype Interferometer Thermal Noise Reduction Cavity 4

6. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Thermal noise reduction cavity systems: Diffractive grating as cavity incoupler  M.Edgar et al. Experimental demonstration of a suspended diffractively coupled optical cavity, Opt. Lett. 34, pp. 3184-3186, 2009.  M.Edgar et al. Experimental demonstration of a suspended, diffractively coupled Fabry–Perot cavity, CQG 27, 084029, 2010.  B. Barr et al.Translational, rotational and vibrational coupling into phase in diffractively- coupled optical cavities, accepted for publication Optics Letters. Waveguide mirror (First realization of a waveguide suspended cavity with a finesse of 800)  D. Friedrich et al. Waveguide grating mirror in a fully suspended 10 m cavity, accepted for pub. Optics Exp. http://arxiv.org/abs/1104.2780 http://arxiv.org/abs/1104.2780 The Glasgow 10m Prototype Interferometer Thermal Noise Reduction Cavity 5 Waveguide Cavity

7. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Thermal noise reduction cavity systems: Diffractive grating as cavity incoupler  M.Edgar et al. Experimental demonstration of a suspended diffractively coupled optical cavity, Opt. Lett. 34, pp. 3184-3186, 2009.  M.Edgar et al. Experimental demonstration of a suspended, diffractively coupled Fabry–Perot cavity  CQG 27, 084029, 2010.  B. Barr et al.Translational, rotational and vibrational coupling into phase in diffractively- coupled optical cavities, accepted for publication Optics Letters. Waveguide mirror (First realization of a waveguide suspended cavity with a finesse of 800)  D. Friedrich et al. Waveguide grating mirror in a fully suspended 10 m cavity, accepted for pub. Optics Exp. http://arxiv.org/abs/1104.2780 http://arxiv.org/abs/1104.2780 Higher order LG modes The Glasgow 10m Prototype Interferometer Thermal Noise Reduction Cavity 6

8. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 LG 33 in the Glasgow 10m GW detector prototype Outcome of the successful ongoing collaboration with the University of Birmingham. Main aims of the experiment:  Gain some experience in how to handle high order LG modes in a prototype environment.  Study of interferometer control signals with high order LG modes.  Locking a single 10m cavity on high order LG modes.  Investigating effects from mode-degeneracy (see talk by C. Bond at 14:30 Monday in the Advanced det. Technologies session, R. Adhikari at GWADW 2010 at Kyoto) 7

9. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Some notes about mode - degeneracy Different mode orders are separated in cavities because the round trip Gouy phase for a mode = (order + 1) * Gouy phase Modes of the same order have the same round trip Gouy phase, therefore aren't separated in cavities. Coupling into other modes of the same order will lead, potentially, to different combinations of modes in the different arm cavities. Circulating Power PDH Error Signal Cavity tuning [deg] In real cavities the modes are not perfectly degenerated, they have slightly different resonant frequencies due to experiencing a different average mirror curvature or cavity length. This leads to error signals with multiple zero crossings making it difficult to lock stably to one of this ‘pseudo’ degenerated modes. Here we show an example of such ‘pseudo’ degeneracy on a 3 mirror mode cleaner with astigmatism. However, first simulations with mirror maps have shown that the expected range of the frequency splitting is much smaller than our 10m cavity line width. Therefore we do not expect to observe this phenomenon. 8

10. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 LG 33 generation – Input Laserbench 9

11. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 LG 33 generation – Input Laserbench 10

12. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 LG 33 generation – Input Laserbench LG 33 generation optics have four purposes:  Generation of a LG 33 mode from a laser emitted TEM 00 mode. This is done with a diffractive optical element (DOE).  Purification of the generated LG 33 mode. By means of a linear modecleaner (LMC); 23 cm long planoconcave cavity with a finesse of 172 and 714MHz FSR.  Adding phase modulation onto the beam for cavity lock. Through an EOM.  Ensuring a good alignment of the prototype’s 10m cavity for the LG 33 beam. For this we have a pick off path of the TEM 00 that avoids the DOE and passes the LMC. TEM 00 and LG 33 share same eigenmode inside the LMC. 11

13. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 After LMC LG 33 degradation through the Glasgow prototype Max. residual 0.18 Max. residual 0.33 Max. residual 0.30 Cavity misaligned End Mirror - transmission After 4 EOM crystals and FI After 1 st MM lens Max. residual 0.50 12

14. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Results – Locking onto high order LG modes 13 0 th order 1 st order Still see reasonable resonances but so far cavity power buildup is a factor 5 less. However, still the desired mode- order is dominant. Good cavity alignment as shown by the visibility of TEM00 mode resonance respect to higher order one.

15. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Examples of modes we were able to lock to 14

16. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Results – High order modes resonance freq. split 15 The resonance peak of the TEM 00 mode shows a single peak...as expected.

17. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Results – High order modes resonance freq. split 16 Scanning several FSR for LG 33 mode

18. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Control signals (errorsignal, feedback signal and transmitted power) and cavity mode shape when locked onto the highest peak. During the video we intentionally gave longitudinal kicks to the mirrors to lock to different modes within the peak. Results – High order modes resonance freq. split 17

19. B. SorazuAmaldi 9 & NRDA, July 2011B. SorazuAmaldi 9 & NRDA, July 2011 Conclusions Set up an experiment to test LG 33 mode in a suspended 10m cavity featuring a nominal finesse of 600 (close to Advanced Detector config). Found it relatively easy to lock to order 9 modes. After some preliminary experimental test it may seem that the same setup that was adequate for stable locking to the TEM 00 mode was not found to be adequate for the locking of the cavity to the LG 33 mode. Further measurements will be carried out to allow confirmation. => So far no quantitative statement can be made about the expected mode degeneracy and associated problems Observation of multiples peaks around the order-9 resonance. So far unexplained. Simulations with real mirror imperfections and further measurements in progress. Outlook: Different reflectivity mirrors are available to investigate how unexplained effects scale with different cavity finesse. 18