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New Frontiers in Modeling Planet-Disk Interactions: from Disk Thermodynamics to Multi-Planet Systems

Objective

Recent space missions such as CoRoT and Kepler have revolutionized exoplanetary science. Today, we know of thousands of systems with awide diversity of architectures, proving that our Solar System is not typical. Understanding how these systems form and evolve is currently one of the most active area of astrophysics. The processes that dictate the dynamics of planets play a fundamental role in shaping the architecture of the systems we observe. In the present paradigm, as planets accrete mass from the primordial disk, they are subject to interactions with it and with other planets. These interactions exert
torques, and make the planets migrate. Disk-planet interactions depend strongly on the physical processes governing the dynamics of the disk. I demonstrated a clear example of this in a recent paper in Nature, showing that the disk heating by an accreting embryo have a strong impact on the torques. This proposal has two objectives with the potential to produce a leap forward in our understanding of the long-term evolution of planetary systems. (i) I will produce the most advanced framework to date for investigating planetary migration in magnetohydrodynamic disk simulations, including ohmic, ambipolar and
Hall effects. I will do this self-consistently by considering the chemical evolution of the dusty gas. Calculating its ionization state and opacity, will moreover allow me to incorporate radiation more realistically. (ii) I will build on a new technique that I have developed, the use of 3D radially moving meshes. This groundbreaking technique enables to follow the migration of multiple planets allowing studying their long-range migration. I want to carry out this research program at The Niels Bohr Institute. The combined expertise of the groups in Copenhagen, together with their impressive computational resources, provide an unparalleled environment to achieve my research goals and develop myself as a leading international figure in this rapidly evolving field.

Fields of science (EuroSciVoc)

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Programme(s)

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Topic(s)

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Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

MSCA-IF-EF-ST - Standard EF

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) H2020-MSCA-IF-2016

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Coordinator

KOBENHAVNS UNIVERSITET
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 212 194,80
Address
NORREGADE 10
1165 KOBENHAVN
Denmark

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Region
Danmark Hovedstaden Byen København
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 212 194,80
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