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- W2773518612 abstract "The aim of planet population synthesis is to incorporate all physical processes from planet formation theories to arrive at a synthetic population of planets that can be compared to observations. In this way, shortcomings in the theories can be shown. In particular, planet population synthesis has to incorporate theories and models regarding (1) core accretion, (2) gas accretion, (3) planet migration and (4) disk evolution . A general problem of the core accretion scenario is that the building time of a planetary core of a few Earth masses with just the accretion of planetesimals takes longer than the lifetime of the protoplanetary disk . This time-scale problem can be overcome when taking the accretion of pebbles into account. We will review here the differences of planetesimal and pebble accretion on the formation of planets that migrate through evolving protoplanetary disks ." @default.
- W2773518612 created "2017-12-22" @default.
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- W2773518612 date "2017-01-01" @default.
- W2773518612 modified "2023-09-26" @default.
- W2773518612 title "Planet Population Synthesis via Pebble Accretion" @default.
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- W2773518612 doi "https://doi.org/10.1007/978-3-319-60609-5_12" @default.
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