An international team of researchers led by SRON and TU Delft have successfully demonstrated a superconducting heterodyne receiver with an unprecedented high sensitivity at 4,7 THz in frequency or 63 micrometers in wavelength. The so called super-terahertz heterodyne receiver - about 85 times more sensitive than its predecessor, operating near the quantum noise limit - is able to operate at the exact frequency that is needed to enable the detection of the astrophysically important neutral atomic oxygen (OI) line. This is very good news for astronomers who need to study the oxygen lines from different astronomic sources to trace star formation and galactic evolution. It is also an important milestone in the development of the technology for the candidate balloon mission GUSSTO (NASA). The research results appeared this month in Applied Physics Letters.A heterodyne receiver can convert a (high-frequency) signal from space into a lower frequency without losing any information. Similar to FM radio, this mixing of frequencies makes the reception clearer and the signal from space can be amplified better. The heterodyne receiver can offer line detection with a nearly quantum noise limited sensitivity and an unparalleled high spectral resolution. The new superconducting heterodyne receiver is based on a novel solid-state terahertz quantum cascade laser to generate the local signal that is to be mixed with the signal from space (local oscillator, operating at 4,7 THz). A superconducting hot electron bolometer is used as a mixing detector..
A terahertz quantum cascade laser (QCL) is actually a tiny semiconductor chip that is based on a repeated stack of semiconductor multiple quantum well heterostructures, where laser emission is achieved through the use of intersubband transitions. Although a QCL has been demonstrated as a local oscillator in the lab before, it is the first time that the QCL is applied at 4,7 THz with an exact targeting frequency. The new QCL is based on a so-called third-order distributed feedback grating design. The grating has a double purpose in realizing both controllable single-frequency emission and a good output beam. The laser used was developed by a research group at the MIT in USA.
The detector used is a hot electron bolometer that consists in essence of a superconducting Niobium-Nitride nanobridge and an on-chip planar antenna. Such a detector was developed by SRON in a close collaboration with the Kavli Institute of Nanoscience at the TU Delft.
The observations of key astronomic cooling lines allow astronomers to trace star formation and galactic evolution. The fine-structure line of electrically neutral atomic oxygen (OI) at 4.7 THz is the dominant cooling line of warm, dense, and neutral atomic gas. In strongly UV irradiated photodissociation regions (PDRs), the OI line flux is generally larger than that of the carbon CII line, making it an ideal diagnostic for probing the physical conditions in regions of massive star formation and galactic centers. The spectrally resolved OI line is necessary to untangle the complexities of the interstellar medium.
The key results were obtained at SRON by a group of young scientists: Darren Hayton (SRON), Jenna Kloosterman (University of Arizona), Ren Yuan (TU Delft and Purple Mountain Observatory), and