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High power single frequency solid state master oscillator power amplifier for gravitational wave detection.

Chandrajit Basu1, Peter Wessels, Jörg Neumann

  • 1Laser Zentrum Hannover e.V., Hollerithallee 8, D-30419 Hannover, Germany. c.basu@lzh.de

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|July 25, 2012
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Researchers developed a high-power, single-frequency laser for gravitational wave detectors. This solid-state master oscillator power amplifier (MOPA) system achieved 177 W of linearly polarized output power.

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Area of Science:

  • Optics and Photonics
  • Laser Physics
  • Gravitational Wave Astronomy Instrumentation

Background:

  • Interferometric gravitational wave detectors (GWDs) require high-power, single-frequency, single-mode, linearly polarized laser sources at the 1 μm wavelength.
  • Solid-state master oscillator power amplifier (MOPA) systems are a promising technology for meeting these demanding laser requirements.

Purpose of the Study:

  • To develop and demonstrate a robust single-frequency, solid-state MOPA system capable of delivering high output power suitable for GWD applications.
  • To characterize the output power, polarization, and beam quality of the developed MOPA system.

Main Methods:

  • Design and construction of a multistage, single-frequency, solid-state MOPA system.
  • Utilizing a master oscillator to generate the initial single-frequency seed laser.
  • Employing multiple amplifier stages to boost the laser power while maintaining single-frequency and single-mode characteristics.
  • Characterization of output power, polarization state, and beam quality (TEM(00) mode content).

Main Results:

  • The multistage MOPA system successfully delivered 177 W of continuous wave (CW) output power at 1 μm.
  • The output laser was single-frequency, single-mode, and linearly polarized.
  • The TEM(00) mode content of the output beam was measured to be 83.5%, indicating excellent beam quality.

Conclusions:

  • The presented single-frequency solid-state multistage MOPA system is a viable and robust solution for generating high-power laser output required by interferometric gravitational wave detectors.
  • The system's performance, including high power and excellent beam quality, demonstrates its potential for advancing gravitational wave detection sensitivity.