Fabrication and characterization of heavily doped n-type GaAs for mid-infrared plasmonics

Author:

Duan Juanmei12ORCID,Liedke Maciej O.3ORCID,Dawidowski Wojciech4ORCID,Li Rang1ORCID,Butterling Maik3ORCID,Hirschmann Eric3ORCID,Wagner Andreas3ORCID,Wang Mao1ORCID,Young Lawrence Boyu5ORCID,Lin Yen-Hsun Glen5ORCID,Hong Minghwei5ORCID,Helm Manfred12ORCID,Zhou Shengqiang1ORCID,Prucnal Slawomir1ORCID

Affiliation:

1. Helmholtz-Zentrum Dresden-Rossendorf, Institute of Ion Beam Physics and Materials Research 1 , Bautzner Landstrasse 400, D-01328 Dresden, Germany

2. 2 TU Dresden, 01062 Dresden, Germany

3. Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics 3 , Bautzner Landstrasse 400, D-01328 Dresden, Germany

4. Wrocław University of Science and Technology, Faculty of Electronics, Photonics and Microsystems 4 , Janiszewskiego 11/17, 50-372 Wrocław, Poland

5. 5 Graduate Institute of Applied Physics and Department of Physics, National Taiwan University, Taipei 10617, Taiwan

Abstract

N-type doping in GaAs is a self-limited process, rarely exceeding a carrier concentration level of 1019 cm−3. Here, we investigated the effect of intense pulsed light melting on defect distribution and activation efficiency in chalcogenide-implanted GaAs by means of positron annihilation spectroscopy and electrochemical capacitance–voltage techniques. In chalcogenide-doped GaAs, donor–vacancy clusters are mainly responsible for donor deactivation. Using positrons as a probe of atomic scale open volumes and DFT calculations, we have shown that after nanosecond pulsed light melting the main defects in heavily doped GaAs are gallium vacancies decorated with chalcogenide atoms substituting As, like VGa–nTeAs or VGa–nSAs. The distribution of defects and carriers in annealed GaAs follows the depth distribution of implanted elements before annealing and depends on the change in the solidification velocity during recrystallization.

Funder

MOST-BMBF

MOST

NSTC

Wroclaw University Science and Technology

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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