Monte Carlo simulation of star/linear and star/star blends with chemically identical monomers
| dc.contributor.author | Theodorakis, P. E. | en |
| dc.contributor.author | Avgeropoulos, A. | en |
| dc.contributor.author | Freire, J. J. | en |
| dc.contributor.author | Kosmas, M. | en |
| dc.contributor.author | Vlahos, C. | en |
| dc.date.accessioned | 2015-11-24T16:42:17Z | |
| dc.date.available | 2015-11-24T16:42:17Z | |
| dc.identifier.issn | 0953-8984 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/8530 | |
| dc.rights | Default Licence | - |
| dc.subject | thermodynamic interaction parameter | en |
| dc.subject | bond-fluctuation model | en |
| dc.subject | polymer mixtures | en |
| dc.subject | star | en |
| dc.subject | chain | en |
| dc.subject | polybutadiene | en |
| dc.subject | homopolymers | en |
| dc.subject | architecture | en |
| dc.subject | miscibility | en |
| dc.subject | dimensions | en |
| dc.title | Monte Carlo simulation of star/linear and star/star blends with chemically identical monomers | en |
| heal.abstract | The effects of chain size and architectural asymmetry on the miscibility of blends with chemically identical monomers, differing only in their molecular weight and architecture, are studied via Monte Carlo simulation by using the bond fluctuation model. Namely, we consider blends composed of linear/linear, star/linear and star/star chains. We found that linear/linear blends are more miscible than the corresponding star/star mixtures. In star/linear blends, the increase in the volume fraction of the star chains increases the miscibility. For both star/linear and star/star blends, the miscibility decreases with the increase in star functionality. When we increase the molecular weight of linear chains of star/linear mixtures the miscibility decreases. Our findings are compared with recent analytical and experimental results. | en |
| heal.access | campus | - |
| heal.fullTextAvailability | TRUE | - |
| heal.identifier.primary | Doi 10.1088/0953-8984/19/46/466111 | - |
| heal.identifier.secondary | <Go to ISI>://000250689100013 | - |
| heal.identifier.secondary | http://iopscience.iop.org/0953-8984/19/46/466111/pdf/0953-8984_19_46_466111.pdf | - |
| heal.journalName | Journal of Physics-Condensed Matter | en |
| heal.journalType | peer reviewed | - |
| heal.language | en | - |
| heal.publicationDate | 2007 | - |
| heal.publisher | Institute of Physics | en |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Θετικών Επιστημών. Τμήμα Χημείας | el |
| heal.type | journalArticle | - |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.type.en | Journal article | en |
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