Published May 21, 2005 | Version v1
Journal article

Laser frequency noise suppression by arm-locking in LISA: progress towards a bench-top demonstration

  • 1. Centre for Gravitational Physics, Department of Physics, Faculty of Science, Australian National University, Canberra ACT 0200 (Australia)
  • 2. Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA 91109 (United States)

Description

Overcoming laser frequency noise is a significant technical challenge for achieving the design sensitivity of the Laser Interferometer Space Antenna (LISA) gravitational wave detector. Arm-locking is a recently proposed technique for suppressing frequency noise in LISA and can be used in addition to the established techniques of pre-stabilization and time-delay interferometry. Incorporation of arm-locking into LISA could provide many benefits, however experimental verification and testing is needed. We present the progress of an experimental test of arm-locking which uses 10 km of optical fibre to generate a large propagation time delay, analogous to the propagation delay in LISA

Availability note (English)

Available online at http://stacks.iop.org/0264-9381/22/S221/cqg5_10_013.pdf or at the Web site for the journal Classical and Quantum Gravity (ISSN 1361-6382) http://www.iop.org/

Additional details

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
22
Journal Issue
10
Journal Page Range
p. S221-S226
ISSN
0264-9381
CODEN
CQGRDG

Conference

Title
5. international LISA symposium; 38. ESLAB symposium
Dates
12-15 Jul 2004
Place
Noordwijk (Netherlands)

INIS