The growth of planets by pebble accretion in evolving protoplanetary discs

By B. Bitsch, Michiel Lambrechts, Anders Johansen. 2015

278 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/0a5095f6b1bc03327adb034f0d907e5d3d24751a

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In Astronomy and Astrophysics

Citations in the corpus

Chemical enrichment of giant planets and discs due to pebble drift (2017, methodology): “The formation and evolution of planets via pebble accretion has been studied in detail in previous studies (e.g Lambrechts et al. 2014; Bitsch et al. 2015), so we only discuss the essential features here.”
Planetesimal formation near the snowline: in or out? (2017, background): “After planetesimals of a certain size have formed, they can subsequently accrete pebbles and quickly grow to larger bodies (e.g., Ormel & Klahr 2010; Lambrechts & Johansen 2012, 2014; Bitsch et al. 2015; Visser & Ormel 2016).”
The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “From the simulations of Bitsch et al. (2015), migration inward to 3 AU is plausible.”
Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion (2017, methodology): “is the level of orbital energy loss via gas drag in the asteroid region. Motivated by observations (Andrews et al., 2009, 2010) and viscous disk theory (Lynden-Bell and Pringle, 1974; Chambers, 2006; Bitsch et al., 2015) we chose a simple power-law prole for the disk. New models that account for non”
Fossilized condensation lines in the Solar System protoplanetary disk (2015, background): “In the most sophisticated models, the aspect ratio of the disk is grossly independent of radius in the region where the viscous heating dominates, although bumps and dips exist (with the associated shadows) due to temperature-dependent transitions in the opacity law (Bitsch et al., 2014a, 2015a).”
Formation of planetary systems by pebble accretion and migration (2018, methodology): “(1) We thus have a flat aspect ratio with orbital distance (zero flaring), which is approximately realised in the inner disc, where viscous heating dominates over irradiation (Bitsch et al. 2015b; Ida et al. 2016).”
Pebble-isolation mass: Scaling law and implications for the formation of super-Earths and gas giants (2018, methodology): “The dominant particle size in the planet formation simulations of Bitsch et al. (2015b) with α = 0.0054 presented below is of the order of 0.1 (Fig.”