arXiv Analytics

Sign in

arXiv:1703.07124 [astro-ph.EP]AbstractReferencesReviewsResources

Growing into and out of the bouncing barrier in planetesimal formation

Maximilian Kruss, Jens Teiser, Gerhard Wurm

Published 2017-03-21Version 1

In recent laboratory studies the robustness of a bouncing barrier in planetesimal formation was studied with an ensemble of preformed compact mm-sized aggregates. Here we show that a bouncing barrier indeed evolves self-consistently by hit-and-stick from an ensemble of smaller dust aggregates. In addition, we feed small aggregates to an ensemble of larger bouncing aggregates. The stickiness temporarily increases, but the final number of aggregates still bouncing remains the same. However, feeding on the small particle supply, the size of the bouncing aggregates increases. This suggests that in the presence of a dust reservoir aggregates grow into but also out of a bouncing barrier at larger size.

Related articles: Most relevant | Search more
arXiv:1609.00501 [astro-ph.EP] (Published 2016-09-02)
Failed Growth at the Bouncing Barrier in Planetesimal Formation
arXiv:1201.4282 [astro-ph.EP] (Published 2012-01-20)
Planetesimal formation by sweep-up: How the bouncing barrier can be beneficial to growth
arXiv:1609.07052 [astro-ph.EP] (Published 2016-09-22)
The role of pebble fragmentation in planetesimal formation II. Numerical simulations