Young sub-Neptunes transition from core-powered bolometric escape to photoevaporative escape at smaller radii for lower-mass and more irradiated planets, with self-consistent simulations yielding combined mass-loss rates and analytic transition scalings.
Journal of Computational Physics , year = 2014, month = feb, volume =
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A new well-balanced high-order scheme for non-conservative hyperbolic systems with sources, verified on blood flow equations in arterial networks.
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Characterizing the bolometric-photoevaporative transition in young sub-Neptunes with radiation-hydrodynamic simulations
Young sub-Neptunes transition from core-powered bolometric escape to photoevaporative escape at smaller radii for lower-mass and more irradiated planets, with self-consistent simulations yielding combined mass-loss rates and analytic transition scalings.
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Well-balanced high-order method for non-conservative hyperbolic PDEs with source terms: application to one-dimensional blood flow equations with gravity
A new well-balanced high-order scheme for non-conservative hyperbolic systems with sources, verified on blood flow equations in arterial networks.