scholarly journals Erratum: High‐density amorphous ice. IV. Raman spectrum of the uncoupled O–H and O–D oscillators [J. Chem. Phys. 86, 5323 (1987)]

1987 ◽  
Vol 87 (10) ◽  
pp. 6212-6212 ◽  
Author(s):  
D. D. Klug ◽  
Edward Whalley ◽  
Osamu Mishima
Physica B+C ◽  
1986 ◽  
Vol 139-140 ◽  
pp. 475-478 ◽  
Author(s):  
D.D. Klug ◽  
Osamu Mishima ◽  
E. Whalley

1987 ◽  
Vol 86 (10) ◽  
pp. 5323-5328 ◽  
Author(s):  
D. D. Klug ◽  
Osamu Mishima ◽  
Edward Whalley

2013 ◽  
Vol 88 (17) ◽  
Author(s):  
Markus Seidl ◽  
Katrin Amann-Winkel ◽  
Philip H. Handle ◽  
Gerhard Zifferer ◽  
Thomas Loerting

2011 ◽  
Vol 115 (14) ◽  
pp. 3756-3760 ◽  
Author(s):  
Yukihiro Yoshimura ◽  
Sarah T. Stewart ◽  
Maddury Somayazulu ◽  
Ho Kwang Mao ◽  
Russell J. Hemley
Keyword(s):  

Author(s):  
Daniel Mariedahl ◽  
Fivos Perakis ◽  
Alexander Späh ◽  
Harshad Pathak ◽  
Kyung Hwan Kim ◽  
...  

Here we report about the structural evolution during the conversion from high-density amorphous ices at ambient pressure to the low-density state. Using high-energy X-ray diffraction, we have monitored the transformation by following in reciprocal space the structure factor S OO ( Q ) and derived in real space the pair distribution function g OO ( r ). Heating equilibrated high-density amorphous ice (eHDA) at a fast rate (4 K min –1 ), the transition to the low-density form occurs very rapidly, while domains of both high- and low-density coexist. On the other hand, the transition in the case of unannealed HDA (uHDA) and very-high-density amorphous ice is more complex and of continuous nature. The direct comparison of eHDA and uHDA indicates that the molecular structure of uHDA contains a larger amount of tetrahedral motives. The different crystallization behaviour of the derived low-density amorphous states is interpreted as emanating from increased tetrahedral coordination present in uHDA. This article is part of the theme issue ‘The physics and chemistry of ice: scaffolding across scales, from the viability of life to the formation of planets'.


1989 ◽  
Vol 91 (11) ◽  
pp. 7187-7192 ◽  
Author(s):  
M. A. Floriano ◽  
Y. P. Handa ◽  
D. D. Klug ◽  
Edward Whalley

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