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Moreover, an increase in the fitted mass transfer timescale of each of the single-rate models is coupled with an increase in the associated fraction of instantaneous sorption sites.
The correlation explains many of the variations in the mass transfer timescale encountered when single-rate sorption approaches were utilized to model solute transport in previous miscible displacement studies.
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Several driving mechanisms exist for stable mass transfer with their own characteristic mass transfer timescales.
If the timescale of the mass transfer is shorter than the thermal timescale of the accretor, the star will temporarily fall out of thermal equilibrium.
Whereas the duration of the CE-phase is likely of the order of (10^{3}~mbox{yr}) (i.e. the thermal timescale of the envelope), stable mass transfer occurs on much longer timescales.
Analysis on characteristic timescale of heat and mass transfer reveals that condensation of Cu on Al NPs occurs faster than the overall thermite reaction.
We assume mass transfer in the inner binary takes place on either the thermal or nuclear timescale of the donor star.
The mass transfer rate is estimated by (dot{m}_{mathrm{MT}} = m/tau _{mathrm{MT}}), where (tau_{mathrm{MT}}) is the timescale of mass transfer.
mass transfer coefficient.
Mass transfer coefficient (m/s).
Overall mass transfer coefficient (s−1).
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