Strain and grain size of TiO2 nanoparticles from TEM, Raman spectroscopy and XRD: The revisiting of the Williamson-Hall plot method
[Display omitted] •First revision of the Williamson-Hall βcosθ-sinθ plot to β2cos2θ-sinθ and βcos2θ-sinθ.•The β2cos2θ-sinθ overestimates crystallite size when compares to HRTEM sizes.•The new βcos2θ-sinθ plot improves strain approaching the Raman standard.•The new βcos2θ-sinθ plot is the same as the...
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Published in | Results in physics Vol. 9; pp. 628 - 635 |
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Main Authors | , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
01.06.2018
Elsevier |
Subjects | |
Online Access | Get full text |
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Abstract | [Display omitted]
•First revision of the Williamson-Hall βcosθ-sinθ plot to β2cos2θ-sinθ and βcos2θ-sinθ.•The β2cos2θ-sinθ overestimates crystallite size when compares to HRTEM sizes.•The new βcos2θ-sinθ plot improves strain approaching the Raman standard.•The new βcos2θ-sinθ plot is the same as the HRTEM on crystallite size.•The new βcos2θ-sinθ plot is better than W-H and Scherrer methods on crystallite size.
The Williamson-Hall (W-H) equation, which has been used to obtain relative crystallite sizes and strains between samples since 1962, is revisited. A modified W-H equation is derived which takes into account the Scherrer equation, first published in 1918, (which traditionally gives more absolute crystallite size prediction) and strain prediction from Raman spectra. It is found that W-H crystallite sizes are on average 2.11 ± 0.01 times smaller than the sizes from Scherrer equation. Furthermore the strain from the W-H plots when compared to strain obtained from Raman spectral red-shifts yield factors whose values depend on the phases in the materials – whether anatase, rutile or brookite. Two main phases are identified in the annealing temperatures (350 °C–700 °C) chosen herein – anatase and brookite. A transition temperature of 550 °C has been found for nano-TiO2 to irreversibly transform from brookite to anatase by plotting the Raman peak shifts against the annealing temperatures. The W-H underestimation on the strain in the brookite phase gives W-H/Raman factor of 3.10 ± 0.05 whereas for the anatase phase, one gets 2.46 ± 0.03. The new βtot2cos2θ-sinθ plot and when fitted with a polynomial yield less strain but much better matching with experimental TEM crystallite sizes and the agglomerates than both the traditional Williamson-Hall and the Scherrer methods. There is greater improvement in the model when linearized – that is the βtotcos2θ-sinθ plot rather than the βtot2cos2θ-sinθ plot. |
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AbstractList | The Williamson-Hall (W-H) equation, which has been used to obtain relative crystallite sizes and strains between samples since 1962, is revisited. A modified W-H equation is derived which takes into account the Scherrer equation, first published in 1918, (which traditionally gives more absolute crystallite size prediction) and strain prediction from Raman spectra. It is found that W-H crystallite sizes are on average 2.11 ± 0.01 times smaller than the sizes from Scherrer equation. Furthermore the strain from the W-H plots when compared to strain obtained from Raman spectral red-shifts yield factors whose values depend on the phases in the materials – whether anatase, rutile or brookite. Two main phases are identified in the annealing temperatures (350 °C–700 °C) chosen herein – anatase and brookite. A transition temperature of 550 °C has been found for nano-TiO2 to irreversibly transform from brookite to anatase by plotting the Raman peak shifts against the annealing temperatures. The W-H underestimation on the strain in the brookite phase gives W-H/Raman factor of 3.10 ± 0.05 whereas for the anatase phase, one gets 2.46 ± 0.03. The new βtot2cos2θ-sinθ plot and when fitted with a polynomial yield less strain but much better matching with experimental TEM crystallite sizes and the agglomerates than both the traditional Williamson-Hall and the Scherrer methods. There is greater improvement in the model when linearized – that is the βtotcos2θ-sinθ plot rather than the βtot2cos2θ-sinθ plot. Keywords: Williamson-Hall, Scherrer, Particle, Crystallite, Strain, Size [Display omitted] •First revision of the Williamson-Hall βcosθ-sinθ plot to β2cos2θ-sinθ and βcos2θ-sinθ.•The β2cos2θ-sinθ overestimates crystallite size when compares to HRTEM sizes.•The new βcos2θ-sinθ plot improves strain approaching the Raman standard.•The new βcos2θ-sinθ plot is the same as the HRTEM on crystallite size.•The new βcos2θ-sinθ plot is better than W-H and Scherrer methods on crystallite size. The Williamson-Hall (W-H) equation, which has been used to obtain relative crystallite sizes and strains between samples since 1962, is revisited. A modified W-H equation is derived which takes into account the Scherrer equation, first published in 1918, (which traditionally gives more absolute crystallite size prediction) and strain prediction from Raman spectra. It is found that W-H crystallite sizes are on average 2.11 ± 0.01 times smaller than the sizes from Scherrer equation. Furthermore the strain from the W-H plots when compared to strain obtained from Raman spectral red-shifts yield factors whose values depend on the phases in the materials – whether anatase, rutile or brookite. Two main phases are identified in the annealing temperatures (350 °C–700 °C) chosen herein – anatase and brookite. A transition temperature of 550 °C has been found for nano-TiO2 to irreversibly transform from brookite to anatase by plotting the Raman peak shifts against the annealing temperatures. The W-H underestimation on the strain in the brookite phase gives W-H/Raman factor of 3.10 ± 0.05 whereas for the anatase phase, one gets 2.46 ± 0.03. The new βtot2cos2θ-sinθ plot and when fitted with a polynomial yield less strain but much better matching with experimental TEM crystallite sizes and the agglomerates than both the traditional Williamson-Hall and the Scherrer methods. There is greater improvement in the model when linearized – that is the βtotcos2θ-sinθ plot rather than the βtot2cos2θ-sinθ plot. |
Author | Maaza, Malik Rayan, Diaa A. Rashad, Mohamed M. Mwakikunga, Bonex W. Dhlamini, Simon Liu, Chuan-Pu Kibasomba, Pierre M. |
Author_xml | – sequence: 1 givenname: Pierre M. surname: Kibasomba fullname: Kibasomba, Pierre M. organization: Department of Physics, Florida Research Centre, University of South Africa, Florida, South Africa – sequence: 2 givenname: Simon surname: Dhlamini fullname: Dhlamini, Simon organization: UNESCO-UNISA Africa Chair in Nanosciences/Nanotechnology, College of Graduate Studies, University of South Africa, Muckleneuk Ridge, P.O. Box 392, Pretoria, South Africa – sequence: 3 givenname: Malik surname: Maaza fullname: Maaza, Malik organization: Department of Physics, Florida Research Centre, University of South Africa, Florida, South Africa – sequence: 4 givenname: Chuan-Pu surname: Liu fullname: Liu, Chuan-Pu organization: Materials Science and Engineering, National Cheng Kung University, 1 University Rd, Tainan, Taiwan – sequence: 5 givenname: Mohamed M. surname: Rashad fullname: Rashad, Mohamed M. organization: Centre for Metallurgical Research and Development Institute, (CMRDI), P.O. Box 87, Helwan, Cairo 11421, Egypt – sequence: 6 givenname: Diaa A. surname: Rayan fullname: Rayan, Diaa A. organization: Centre for Metallurgical Research and Development Institute, (CMRDI), P.O. Box 87, Helwan, Cairo 11421, Egypt – sequence: 7 givenname: Bonex W. surname: Mwakikunga fullname: Mwakikunga, Bonex W. email: bmwakikunga@csir.co.za organization: DST/CSIR-National Centre for Nano-Structured Materials, PO Box 395 Pretoria, South Africa |
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•First revision of the Williamson-Hall βcosθ-sinθ plot to β2cos2θ-sinθ and βcos2θ-sinθ.•The β2cos2θ-sinθ overestimates crystallite size when... The Williamson-Hall (W-H) equation, which has been used to obtain relative crystallite sizes and strains between samples since 1962, is revisited. A modified... |
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Title | Strain and grain size of TiO2 nanoparticles from TEM, Raman spectroscopy and XRD: The revisiting of the Williamson-Hall plot method |
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