论文信息 - Laser frequency stabilization by locking to a LISA arm

Laser frequency stabilization by locking to a LISA arm

We analyze a technique for suppressing laser frequency noise for the laser interferometer space antenna (LISA) gravitational wave detector. We demonstrate that the laser frequency can be stabilized to a LISA arm by high gain feedback. It is shown that the feedback bandwidth is not limited by the 33 second round-trip propagation time and example frequency controller designs are presented.

[1] N. Mavalvala,et al. Readout and control of a power-recycled interferometric gravitational-wave antenna. , 2001, Applied optics.

[2] Daniel A. Shaddock,et al. Data Combinations Accounting for LISA Spacecraft Motion , 2003, gr-qc/0307080.

[3] Daniel A. Shaddock,et al. Implementation of time-delay interferometry for LISA , 2003, gr-qc/0303013.

[4] John W. Armstrong,et al. Cancellation of laser noise in an unequal-arm interferometer detector of gravitational radiation , 1999 .

[5] Jun Ye,et al. Absolute frequency atlas of molecular I2 lines at 532 nm , 1999, IEEE Trans. Instrum. Meas..

[6] Robin T. Stebbins,et al. Demonstration of the LISA phase measurement principle , 2001 .

[7] F. Bondu,et al. Ultrahigh-spectral-purity laser for the VIRGO experiment. , 1996, Optics letters.

[8] M. Zucker,et al. Improved multistage wide band laser frequency stabilization , 1997 .

[9] N. Cornish,et al. The effects of orbital motion on LISA time delay interferometry , 2003, gr-qc/0306096.