Приказ основних података о документу

dc.creatorPopović, Marko
dc.date.accessioned2023-05-10T20:34:34Z
dc.date.available2023-05-10T20:34:34Z
dc.date.issued2010
dc.identifier.issn0354-9836
dc.identifier.urihttps://cer.ihtm.bg.ac.rs/handle/123456789/6116
dc.description.abstractMost people would face a problem if there is a need to calculate the mole fraction of a substance A in a gaseous solution (a thermodynamic system containing two or more ideal gases) knowing its molarity at a given temperature and pressure. For most it would take a lot of time and calculations to find the answer, especially because the quantities of other substances in the system aren’t given. An even greater problem arises when we try to understand how special relativity affects gaseous systems, especially solutions and systems in equilibrium. In this paper formulas are suggested that greatly shorten the process of conversion from molarity to mole fraction and give us a better insight into the relativistic effects on a gaseous system.sr
dc.language.isoensr
dc.publisherSociety of Thermal Engineers of Serbiasr
dc.rightsopenAccesssr
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.sourceThermal Sciencesr
dc.subjectmol fractionsr
dc.subjectmolaritysr
dc.subjectideal gassr
dc.subjectequation of statesr
dc.subjectspecial relativitysr
dc.titleEquation of state in form which relates mol fraction and molarity of two (or more) component thermodynamic system consisted of ideal gases, and it's applications.sr
dc.typearticlesr
dc.rights.licenseBY-NC-NDsr
dc.rights.holderSociety of Thermal Engineers of Serbiasr
dc.citation.volume14
dc.citation.issue3
dc.citation.spage859
dc.citation.epage863
dc.citation.rankM23
dc.identifier.doi10.2298/TSCI100325009P
dc.identifier.fulltexthttp://cer.ihtm.bg.ac.rs/bitstream/id/25237/bitstream_25237.pdf
dc.identifier.scopus2-s2.0-78649932615
dc.identifier.wos000283410400027
dc.type.versionpublishedVersionsr


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Приказ основних података о документу