Non-degenerate-pump four-wave mixing kinetic inductance travelling-wave parametric amplifiers

被引:3
|
作者
Longden, J. C. [1 ]
Tan, B-K [1 ]
机构
[1] Univ Oxford, Dept Phys Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
来源
ENGINEERING RESEARCH EXPRESS | 2024年 / 6卷 / 01期
基金
英国科学技术设施理事会; 欧洲研究理事会;
关键词
parametric amplifier; travelling-wave; kinetic inductance; Superconducting thin films; wave mixing; BAND;
D O I
10.1088/2631-8695/ad213c
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Kinetic inductance travelling-wave parametric amplifiers (KITWPAs) have been demonstrated to achieve high gain over broad bandwidths whilst achieving near quantum-limited noise performance, properties which are extremely important for many ultra-sensitive experiments. In early KITWPA designs, the requirement for phase-matching lead to the creation of a large zero-gain gap in the centre of the gain profile where the peak gain is, which also slightly narrows down the operational bandwidth of the device. This has been mitigated in more recent designs by introducing a DC bias to the KITWPA device, which allows the gap to be tuned away from the amplification band. However, the added DC biasing requires a more complicated experimental setup and potentially leads to unwanted heat leak in the cryogenic environment. Additionally, operation with a DC bias also become challenging at higher frequencies beyond the microwave regime. In this paper, we present the concept of a KITWPA operating in a non-degenerate-pump four-wave mixing (NP-4WM) regime, whereby the injection of two pump tones along with a weak signal results in a broad, flat gain profile that removes the zero-gain gap as well as eliminates the need for a DC bias and the complexities associated with it. We demonstrate how a NP-4WM KITWPA is feasible to achieve broadband amplification at a range of frequencies, first in the microwave range where most KITWPAs reported to-date have been successfully experimentally characterised. We then extend the designs to several millimetre (mm) bands to illustrate how we can use this technique to design a broadband front-end pre-amplifier that covers several Atacama Large Millimetre/sub-millimetre Array (ALMA) Bands.
引用
收藏
页数:16
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