Richter, Heiko and Pavlov, Sergei G. and Semenov, A. D. and Mahler, L. and Tredicucci, A. and Beere, H. E. and Ritchie, D. A. and Hübers, H.-W. (2010) Frequency stabilization of a THz quantum-cascade laser to a molecular absorption line. 21st International Symposium on Space Terahertz Technology, 23-25 Mar 2010, Oxford, UK.
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The terahertz (THz) portion of the electromagnetic spectrum bears an amazing scientific potential in astronomy. High resolution spectroscopy in particular heterodyne spectroscopy of molecular rotational lines and fine structure lines of atoms or ions is a powerful tool, which allows obtaining valuable information about the observed object such as temperature and dynamical processes as well as density and distribution of particular species. One example is the OI fine structure line at 4.7 THz. This is a main target to be observed with GREAT, the German Receiver for Astronomy at Terahertz Frequencies, which will be operated on board of SOFIA. A major challenge for a heterodyne receivers operating at this frequency is the local oscillator (LO). THz quantum-cascade lasers (QCLs) have the potential to replace the presently used gas laser LO. A major issue is the frequency stabilization of the QCL, because its free-running linewidth is several MHz. We report on the frequency stabilization of a THz QCL to the absorption line of methanol gas at a frequency of 2.55 THz. The QCL is mounted on the first stage of a pulse tube cooler and operates at a temperature of about 50 K. The stabilization method is based on frequency modulation of the laser emission across the absorption line. The resulting derivative-like signal is used as error signal for a control loop which keeps the laser frequency at maximum absorption. The unstabilized laser has frequency fluctuations of 15 MHz which are reduced to 300 kHz (full width at half maximum) with the control loop in action. The line shape of the locked signal is Gaussian. The achieved linewidth is already sufficient for many applications. For example the frequency resolution of a typical heterodyne receiver with an acousto-optical backend spectrometer is 1.5 MHz. With a 300 kHz linewidth of the LO this increases marginally to 1.53 MHz. In addition, the stabilization scheme is robust and versatile, because it requires only an additional detector and a small gas absorption cell, while being applicable even at the highest THz frequencies due to the rich absorption spectra of molecules such as CH3OH or H2O.
|Document Type:||Conference or Workshop Item (Poster)|
|Title:||Frequency stabilization of a THz quantum-cascade laser to a molecular absorption line|
|Date:||24 March 2010|
|Keywords:||THz, frequency stabilisation, quantum cascade laser|
|Event Title:||21st International Symposium on Space Terahertz Technology|
|Event Location:||Oxford, UK|
|Event Type:||international Conference|
|Event Dates:||23-25 Mar 2010|
|Organizer:||University of Oxford and STFC Rutherford Appleton Laboratory|
|HGF - Research field:||Aeronautics, Space and Transport (old)|
|HGF - Program:||Space (old)|
|HGF - Program Themes:||W EW - Erforschung des Weltraums|
|DLR - Research area:||Space|
|DLR - Program:||W EW - Erforschung des Weltraums|
|DLR - Research theme (Project):||W - Projekt SOFIA (old)|
|Institutes and Institutions:||Institute of Planetary Research > Terahertz and Infrared Sensors|
|Deposited By:||Dr.rer.nat. Heiko Richter|
|Deposited On:||05 Jan 2011 21:47|
|Last Modified:||11 Jan 2011 12:53|
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