Literature DB >> 26598245

NH4(+) Resides Inside the Water 20-mer Cage As Opposed to H3O(+), Which Resides on the Surface: A First Principles Molecular Dynamics Simulation Study.

Soohaeng Yoo Willow1, N Jiten Singh1, Kwang S Kim1.   

Abstract

Experimental vibrational predissociation spectra of the magic NH4(+)(H2O)20 clusters are close to those of the magic H3O(+)(H2O)20 clusters. It has been assumed that the geometric features of NH4(+)(H2O)20 clusters might be close to those of H3O(+)(H2O)20 clusters, in which H3O(+) resides on the surface. Car-Parrinello molecular dynamics simulations in conjunction with density functional theory calculations are performed to generate the infrared spectra of the magic NH4(+)(H2O)20 clusters. In comparison with the experimental vibrational predissociation spectra of NH4(+)(H2O)20, we find that NH4(+) is inside the cage structure of NH4(+)(H2O)20 as opposed to on the surface structure. This shows a clear distinction between the structures of NH4(+)(H2O)20 and H3O(+)(H2O)20 as well as between the hydration phenomena of NH4(+) and H3O(+).

Entities:  

Year:  2011        PMID: 26598245     DOI: 10.1021/ct200486c

Source DB:  PubMed          Journal:  J Chem Theory Comput        ISSN: 1549-9618            Impact factor:   6.006


  1 in total

1.  Ammonia clathrate hydrates as new solid phases for Titan, Enceladus, and other planetary systems.

Authors:  Kyuchul Shin; Rajnish Kumar; Konstantin A Udachin; Saman Alavi; John A Ripmeester
Journal:  Proc Natl Acad Sci U S A       Date:  2012-08-20       Impact factor: 11.205

  1 in total

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