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Title:
Grand Challenges in Protoplanetary Disc Modelling
Authors:
Haworth, Thomas J.; Ilee, John D.; Forgan, Duncan H.; Facchini, Stefano; Price, Daniel J.; Boneberg, Dominika M.; Booth, Richard A.; Clarke, Cathie J.; Gonzalez, Jean-François; Hutchison, Mark A.; Kamp, Inga; Laibe, Guillaume; Lyra, Wladimir; Meru, Farzana; Mohanty, Subhanjoy; Panic, Olja; Rice, Ken; Suzuki, Takeru; Teague, Richard; Walsh, Catherine; Woitke, Peter; Community authors
Affiliation:
AA(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK; Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK), AB(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK), AC(School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK), AD(Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany), AE(Monash Centre for Astrophysics and School of Physics and Astronomy, Monash University, Clayton, VIC 3800, Australia 0000-0002-4716-4235), AF(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK), AG(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK), AH(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK), AI(Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69230, Saint-Genis-Laval, France), AJ(Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia), AK(Kapteyn Astronomical Institute, Postbus 800, 9700 AV Groningen, The Netherlands), AL(School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews KY16 9SS, UK), AM(Department of Physics and Astronomy, California State University Northridge, 18111 Nordhoff St, Northridge, CA 91330, USA; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA), AN(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK), AO(Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK), AP(Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, UK; School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, UK), AQ(Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK), AR(School of Arts & Sciences, University of Tokyo 3-8-1, Komaba, Meguro, Tokyo, 153-8902, Japan; Department of Physics, Nagoya University, Furo-cho, Chikusa, Nagoya, Aichi, 464-8602, Japan), AS(Max-Planck-Institut fr Astronomie, Knigstuhl 17, 69117 Heidelberg, Germany), AT(Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA, Leiden, The Netherlands), AU(Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, UK)
Publication:
Publications of the Astronomical Society of Australia, Volume 33, id.e053 22 pp. (PASA Homepage)
Publication Date:
10/2016
Origin:
CUP
Astronomy Keywords:
astrochemistry, magnetohydrodynamics (MHD), hydrodynamics, planetary systems: formation, protoplanetary disks, radiative transfer
Abstract Copyright:
2016: Astronomical Society of Australia
DOI:
10.1017/pasa.2016.45
Bibliographic Code:
2016PASA...33...53H

Abstract

The Protoplanetary Discussions conference-held in Edinburgh, UK, from 2016 March 7th-11th-included several open sessions led by participants. This paper reports on the discussions collectively concerned with the multi-physics modelling of protoplanetary discs, including the self-consistent calculation of gas and dust dynamics, radiative transfer, and chemistry. After a short introduction to each of these disciplines in isolation, we identify a series of burning questions and grand challenges associated with their continuing development and integration. We then discuss potential pathways towards solving these challenges, grouped by strategical, technical, and collaborative developments. This paper is not intended to be a review, but rather to motivate and direct future research and collaboration across typically distinct fields based on community-driven input, to encourage further progress in our understanding of circumstellar and protoplanetary discs.
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