McGill.CA / Science / Department of Physics

CPM Seminar

Optical Spectroscopy in Highly Enriched 28Si: from Isotopic Fingerprints of (Supposedly) Well Known Defects to Applications in Quantum Information

Mike Thewalt

Department of Physics
Simon Fraser University

Natural Si (nSi), the basis of our electronic, communication and information technologies, contains ~92% 28Si, so it is not surprising that many of the properties of highly enriched 28Si are almost indistinguishable from those of nSi. We were therefore surprised to discover[1] that 28Si was remarkably different from nSi in a very important way the linewidths of many different optical transitions can be more than an order of magnitude narrower in 28Si than in nSi, even though those linewidths in nSi are already typically sharper than in other semiconductors.

This huge improvement in spectral resolution has revealed new phenomena and potential applications. Recently[2] we have found that the luminescence of many well known deep centers has resolved fine structure in 28Si which reveals an isotopic fingerprint of the defect constituents, leading to many surprises regarding the actual composition of what were thought to be well-understood defects. We have also resolved hyperfine components in the optical spectra of several centers, and in particular of the bound exciton associated with the shallow donor 31P [3]. Both the electronic and nuclear spins of 31P have been the basis of many proposed schemes for quantum computation in Si, which all suffer from the problem of reading out the spin state of a single impurity. The new ability to measure the 31P nuclear spin optically, and also to polarize it by dynamic pumping, and to selectively ionize donors in specific electronic and nuclear spin states opens up a number of promising new approaches for Si-based quantum computation.

[1] D. Karaskaij et al., Phys. Rev. Lett. 26, 6010 (2001).
[2] M. Steger et al., Phys. Rev. Lett. 100, 177402 (2008).
[3] A. Yang et al., Phys. Rev. Lett. 97, 227401 (2006).

Friday, June 13th 2008, 11:30
Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
Hosted by: G. Gervais.