2020
DOI: 10.1140/epjc/s10052-020-8292-0
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Cosmological analogies, Lagrangians, and symmetries for convective–radiative heat transfer

Abstract: A formal analogy between the Friedmann equation of relativistic cosmology and models of convective–radiative cooling/heating of a body (including Newton’s, Dulong–Petit’s, Newton–Stefan’s laws, and a generalization) is discussed. The analogy highlights Lagrangians, symmetries, and mathematical properties of the solutions of these cooling laws.

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Cited by 4 publications
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“…It is also well known that the solutions of Equation (1) present steep fronts and shocks, which need to be accurately resolved in applications and often cause severe numerical challenges. Lagrangian methods are among the numerical techniques used in the literature to handle these difficulties generated from the presence of convective terms in the governing equations, see for instance [9, 21]. The main shortcoming for these methods is the grid distortion drawback specially when characteristic curves are required to be computed for time‐dependent velocity fields.…”
Section: Introductionmentioning
confidence: 99%
“…It is also well known that the solutions of Equation (1) present steep fronts and shocks, which need to be accurately resolved in applications and often cause severe numerical challenges. Lagrangian methods are among the numerical techniques used in the literature to handle these difficulties generated from the presence of convective terms in the governing equations, see for instance [9, 21]. The main shortcoming for these methods is the grid distortion drawback specially when characteristic curves are required to be computed for time‐dependent velocity fields.…”
Section: Introductionmentioning
confidence: 99%
“…Moreover, numerical solutions need an accurate approximation in order to resolve possible steep fronts and shocks, see for instance [19,21,38,44]. To deal with the difficulties generated by the presence of convective terms in the governing equations, it is possible to opt for numerical techniques based on Lagrangian methods, see for example [13,26]. However, the main disadvantage of these methods is the grid distortion drawback specially when characteristic curves are required to be computed for time-dependent velocity fields.…”
Section: Introductionmentioning
confidence: 99%