4.4 Article

Towards quantum-limited coherent detection of terahertz waves in charge-neutral graphene

期刊

NATURE ASTRONOMY
卷 3, 期 11, 页码 983-988

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NATURE PUBLISHING GROUP
DOI: 10.1038/s41550-019-0843-7

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资金

  1. Swedish Foundation for Strategic Research (SSF) [IS14-0053, GMT14-0077, RMA15-0024]
  2. Knut and Alice Wallenberg Foundation
  3. Chalmers Area of Advance NANO
  4. Swedish Research Council (VR) [2015-03758, 2016-04828]
  5. Swedish-Korean Basic Research Cooperative Program of the NRF [NRF-2017R1A2A1A18070721]
  6. European Union's Horizon 2020 research and innovation programme [766714/HiTIMe]
  7. Swedish Research Council [2015-03758, 2016-04828] Funding Source: Swedish Research Council
  8. Swedish Foundation for Strategic Research (SSF) [IS14-0053] Funding Source: Swedish Foundation for Strategic Research (SSF)
  9. Vinnova [2015-03758] Funding Source: Vinnova

向作者/读者索取更多资源

Spectacular advances in heterodyne astronomy(1,2) have been largely due to breakthroughs in detector technology(3). To exploit the full capacity of future terahertz (similar to 300 GHz-5 THz) telescope space missions(4), new concepts of terahertz coherent receivers are needed, providing larger bandwidths and imaging capabilities with multipixel focal plane heterodyne arrays(5). Here we show that graphene uniformly doped to the Dirac point, with material resistance dominated by quantum localization and thermal relaxation governed by electron diffusion, enables highly sensitive and wideband coherent detection of signals from 90 to 700 GHz and, prospectively, across the entire terahertz range. We measure on proof-of-concept graphene bolometric mixers an electron diffusion-limited gain bandwidth of 8 GHz (corresponding to a Doppler shift of 480 km s(-1) at 5 THz) and intrinsic mixer noise temperature of 475 K (which would be equivalent to similar to 2 hf/k(B) at f = 5 THz, where h is Planck's constant, f is the frequency and k(B) is the Boltzmann constant), limited by the residual thermal background in our setup. An optimized device will result in a mixer noise temperature as low as 36 K, with the gain bandwidth exceeding 20 GHz, and a local oscillator power of <100 pW. In conjunction with the emerging quantum-limited amplifiers at the intermediate frequency(6,7), our approach promises quantum-limited sensing in the terahertz domain, potentially surpassing superconducting technologies, particularly for large heterodyne arrays.

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