Assessing the effect of a liquid water layer on the adsorption of hydrate anti-agglomerants using molecular simulations

Author:

Mohr Stephan12ORCID,Pétuya Rémi1ORCID,Sarria Juan3,Purkayastha Nirupam3,Bodnar Scot4,Wylde Jonathan45,Tsimpanogiannis Ioannis N.6ORCID

Affiliation:

1. Nextmol (Bytelab Solutions SL), Barcelona, Spain

2. Barcelona Supercomputing Center (BSC), Barcelona, Spain

3. Clariant Produkte (Deutschland) GmbH, Frankfurt, Germany

4. Clariant Oil Services, Clariant Corporation, Houston, Texas 77258, USA

5. Heriot Watt University, Edinburgh, Scotland, United Kingdom

6. Centre for Research and Technology Hellas (CERTH), Chemical Process and Energy Resources Institute (CPERI), 57001 Thermi-Thessaloniki, Greece

Abstract

We have performed molecular dynamics simulations to study the adsorption of ten hydrate anti-agglomerants onto a mixed methane–propane sII hydrate surface covered by layers of liquid water of various thickness. As a general trend, we found that the more liquid water that is present on the hydrate surface, the less favorable the adsorption becomes even though there are considerable differences between the individual molecules, indicating that the presence and thickness of this liquid water layer are crucial parameters for anti-agglomerant adsorption studies. Additionally, we found that there exists an optimal thickness of the liquid water layer favoring hydrate growth due to the presence of both liquid water and hydrate-forming guest molecules. For all other cases of liquid water layer thickness, hydrate growth is slower due to the limited availability of hydrate-forming guests close to the hydrate formation front. Finally, we investigated the connection between the thickness of the liquid water layer and the degree of subcooling and found a very good agreement between our molecular dynamics simulations and theoretical predictions.

Funder

Partnership for Advanced Computing in Europe AISBL

Publisher

AIP Publishing

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy

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