Please use this identifier to cite or link to this item:
https://olympias.lib.uoi.gr/jspui/handle/123456789/8530Full metadata record
| DC Field | Value | Language |
|---|---|---|
| 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.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| 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.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Θετικών Επιστημών. Τμήμα Χημείας | el |
| heal.publicationDate | 2007 | - |
| 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.publisher | Institute of Physics | en |
| heal.journalName | Journal of Physics-Condensed Matter | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά). ΧΗΜ | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Theodorakis-2007-Monte Carlo simulati.pdf | 341.34 kB | Adobe PDF | View/Open Request a copy |
This item is licensed under a Creative Commons License
