Energy transfer in small nano-sized systems can be very different from that in their
macroscopic counterparts due to reduced dimensionality, interaction with surfaces, disorder …

Prompted by the relevant problem of temperature inversion (ie gradient of density anti-
correlated to the gradient of temperature) in astrophysics, we introduce a novel method to …

The temperature of the solar atmosphere increases from thousands to millions of degrees
moving from the lower layer (chromosphere) to the outermost one (corona), while the density …

Dimensions and molecular structures play pivotal roles in the principle of heat conduction.
The dimensional characteristics of a solution within nanoscale systems depend on the …

Size dependence of energy transport and the effects of reduced dimensionality on transport
coefficients are of key importance for understanding nonequilibrium properties of matter on …

Prompted by the relevant problem of temperature inversion (ie gradient of density anti-
correlated to the gradient of temperature) in solar physics, we introduce a novel method to …

Many physical and chemical processes involve energy change with rates that depend
sensitively on local temperature. Important examples include heterogeneously catalyzed …

We summarize a series of numerical experiments of collisional dynamics in dense stellar
systems such as globular clusters (GCs) and in weakly collisional plasmas using a novel …