2003
DOI: 10.1002/pssa.200306502
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Positron annihilation and infrared spectroscopy studies of porous silicon

Abstract: Measurements of the angular correlation of annihilation radiation and infrared absorption spectra were conducted with porous silicon samples, containing capillary macropores with a diameter of about 1 µm. The set of data shows that a high proportion of Si -O bonds contribute to positron annihilation and IR absorption for porous silicon. Annihilation parameters and estimated values of the specific surface area point to the availability of a nanoporous system in the macroporous silicon. Most likely the macropore… Show more

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Cited by 6 publications
(2 citation statements)
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References 9 publications
(14 reference statements)
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“…Guessoum, Ramaty and Lingenfelter (1991) added spectral considerations to the positron-dust process but kept a simplified picture of the dust and showed that unless the abundance of dust in the annihilation regions is increased many times compared to "normal" quantities, grains change the spectrum of the line mostly in the hot phase. Astrophysical knowledge of grains has since increased considerably (see the reviews by Draine 2003, Li 2004, and Krugel 2003 and although a huge body of work exists on positron interactions with solids and solid surfaces (Nieminen & Oliva 1980;Huttunen et al 1990;Dannefaer et al 1996;Dupasquier & Mills 1995;Puska & Nieminen 1994;Weiss et al 1994;Suzuki et al 2003;Mills et al 1989;Mokrushin et al 2003;Pi et al 2003;Weber & Lynn 2000), experiments dealing with positrons and dust like materials remain scarce. We here summarize our best understanding of the relevant information we have collected on dust grains in our context.…”
Section: Grains and Positron Processesmentioning
confidence: 99%
“…Guessoum, Ramaty and Lingenfelter (1991) added spectral considerations to the positron-dust process but kept a simplified picture of the dust and showed that unless the abundance of dust in the annihilation regions is increased many times compared to "normal" quantities, grains change the spectrum of the line mostly in the hot phase. Astrophysical knowledge of grains has since increased considerably (see the reviews by Draine 2003, Li 2004, and Krugel 2003 and although a huge body of work exists on positron interactions with solids and solid surfaces (Nieminen & Oliva 1980;Huttunen et al 1990;Dannefaer et al 1996;Dupasquier & Mills 1995;Puska & Nieminen 1994;Weiss et al 1994;Suzuki et al 2003;Mills et al 1989;Mokrushin et al 2003;Pi et al 2003;Weber & Lynn 2000), experiments dealing with positrons and dust like materials remain scarce. We here summarize our best understanding of the relevant information we have collected on dust grains in our context.…”
Section: Grains and Positron Processesmentioning
confidence: 99%
“…13,14,19 A disadvantage of electrodes based on macroporous GPS with a porosity of 50-60% is the low specific surface area of the working surface. Despite the presence of nanoscale (1-2 nm) pores on the surface of the wall in a layer with a thickness of ∼100 nm, 21,22 no significant increase in the active surface area is observed. Efforts have been made to increase the specific surface area by depositing a layer of carbon nanotubes 20-50 nm in diameter on the inner surface of the pore walls.…”
Section: Experimental or Theoreticalmentioning
confidence: 93%