Gold-Hyperdoped Germanium with Room-Temperature Sub-Band-Gap Optoelectronic Response

Hemi H. Gandhi, David Pastor, Tuan T. Tran, S. Kalchmair, L.A. Smilie, Jonathan P. Mailoa, Ruggero Milazzo, Enrico Napolitani, Marco Loncar, James S. Williams, Michael J. Aziz, and Eric Mazur
Phys. Rev. Applied 14, 064051 – Published 16 December 2020
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Abstract

Short-wavelength-infrared (SWIR; 1.4–3.0 µm) photodetection is important for various applications. Inducing a low-cost silicon-compatible material, such as germanium, to detect SWIR light would be advantageous for SWIR applications compared with using conventional (III-V or II-VI) SWIR materials. Here, we present a scalable nonequilibrium method for hyperdoping germanium with gold for dopant-mediated SWIR photodetection. Using ion implantation followed by nanosecond pulsed laser melting, we obtain a single-crystal material with a peak gold concentration of 3 × 1019cm3 (103 times the solubility limit). This hyperdoped germanium has fundamentally different optoelectronic properties from those of intrinsic and conventionally doped germanium. This material exhibits sub-band-gap absorption of light up to wavelengths of at least 3 µm, with a sub-band-gap optical absorption coefficient comparable to that of commercial SWIR photodetection materials. We show that germanium hyperdoped with gold exhibits sub-band-gap SWIR photodetection at room temperature, in contrast with previous doped-germanium photodetector studies, which only show a low-temperature response. This material is a potential pathway to low-cost room-temperature silicon-compatible SWIR photodetection.

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  • Received 19 March 2020
  • Revised 27 August 2020
  • Accepted 9 October 2020

DOI:https://doi.org/10.1103/PhysRevApplied.14.064051

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Hemi H. Gandhi1,*,**,††, David Pastor1,2,†,**,††, Tuan T. Tran3,4, S. Kalchmair1, L.A. Smilie3, Jonathan P. Mailoa5, Ruggero Milazzo6, Enrico Napolitani6, Marco Loncar1, James S. Williams3, Michael J. Aziz1,‡,**, and Eric Mazur1,§,**

  • 1Harvard John A. Paulson School of Engineering and Applied Sciences, Cambridge, Massachusetts 02138, USA
  • 2Departamento de Estructura de la Materia, Física térmica y Electrónica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, Madrid 28040, Spain
  • 3Department of Electronic Materials Engineering, Research School of Physics and Engineering, Australian National University, Canberra, Australian Capital Territory 0200, Australia
  • 4Department of Physics and Astronomy, Ångström Laboratory, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
  • 5Robert Bosch LLC, Cambridge, Massachusetts 02138, USA
  • 6Dipartimento di Fisica e Astronomia, Università di Padova and CNR-IMM, Via Marzolo 8, I-35131 Padova, Italy

  • *hemi.gandhi@alumni.harvard.edu
  • dpastor@seas.harvard.edu and dpastor@fis.ucm.es
  • maziz@harvard.edu
  • §mazur@seas.harvard.edu
  • **To whom all correspondence (inquiry) should be addressed.
  • ††H.H.G. and D.P. are co-first authors and contributed equally to this work.

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Vol. 14, Iss. 6 — December 2020

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