Explore the words cloud of the DiskTorqueOnPlanets project. It provides you a very rough idea of what is the project "DiskTorqueOnPlanets" about.
The following table provides information about the project.
|Coordinator Country||Denmark [DK]|
|Total cost||212˙194 €|
|EC max contribution||212˙194 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2017-09-01 to 2019-08-31|
Take a look of project's partnership.
|1||KOBENHAVNS UNIVERSITET||DK (KOBENHAVN)||coordinator||212˙194.00|
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.
|year||authors and title||journal||last update|
Philipp Weber, SebastiÃ¡n PÃ©rez, Pablo BenÃtez-Llambay, Oliver Gressel, Simon Casassus, Leonardo Krapp
Predicting the Observational Signature of Migrating Neptune-sized Planets in Low-viscosity Disks
published pages: 178, ISSN: 1538-4357, DOI: 10.3847/1538-4357/ab412f
|The Astrophysical Journal 884/2||2020-02-12|
Troels HaugbÃ¸lle, Philipp Weber, Daniel P. Wielandt, Pablo BenÃtez-Llambay, Martin Bizzarro, Oliver Gressel, Martin E. Pessah
Probing the Protosolar Disk Using Dust Filtering at Gaps in the Early Solar System
published pages: 55, ISSN: 1538-3881, DOI: 10.3847/1538-3881/ab1591
|The Astronomical Journal 158/2||2020-02-12|
Leonardo Krapp, Pablo BenÃtez-Llambay, Oliver Gressel, Martin E. Pessah
Streaming Instability for Particle-size Distributions
published pages: L30, ISSN: 2041-8213, DOI: 10.3847/2041-8213/ab2596
|The Astrophysical Journal 878/2||2020-02-12|
SebastiÃ¡n PÃ©rez, S Casassus, P BenÃtez-Llambay
Observability of planetâ€“disc interactions in CO kinematics
published pages: L12-L17, ISSN: 1745-3933, DOI: 10.1093/mnrasl/sly109
|Monthly Notices of the Royal Astronomical Society: Letters 480/1||2020-02-12|
Philipp Weber, Pablo BenÃtez-Llambay, Oliver Gressel, Leonardo Krapp, Martin E. Pessah
Characterizing the Variable Dust Permeability of Planet-induced Gaps
published pages: 153, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aaab63
|The Astrophysical Journal 854/2||2020-02-12|
Pablo BenÃtez-Llambay, Martin E. Pessah
Torques Induced by Scattered Pebble-flow in Protoplanetary Disks
published pages: L28, ISSN: 2041-8213, DOI: 10.3847/2041-8213/aab2ae
|The Astrophysical Journal 855/2||2020-02-12|
Pablo BenÃtez-Llambay, Leonardo Krapp, Martin E. Pessah
Asymptotically Stable Numerical Method for Multispecies Momentum Transfer: Gas and Multifluid Dust Test Suite and Implementation in FARGO3D
published pages: 25, ISSN: 1538-4365, DOI: 10.3847/1538-4365/ab0a0e
|The Astrophysical Journal Supplement Series 241/2||2020-02-12|
Colin P McNally, Richard P Nelson, Sijme-Jan Paardekooper, Pablo BenÃtez-Llambay
Migrating super-Earths in low-viscosity discs: unveiling the roles of feedback, vortices, and laminar accretion flows
published pages: 728-748, ISSN: 0035-8711, DOI: 10.1093/mnras/stz023
|Monthly Notices of the Royal Astronomical Society 484/1||2020-02-12|
Leonardo Krapp, Oliver Gressel, Pablo BenÃtez-Llambay, Turlough P. Downes, Gopakumar Mohandas, Martin E. Pessah
Dust Segregation in Hall-dominated Turbulent Protoplanetary Disks
published pages: 105, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aadcf0
|The Astrophysical Journal 865/2||2020-02-12|
Are you the coordinator (or a participant) of this project? Plaese send me more information about the "DISKTORQUEONPLANETS" project.
For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.
Send me an email (email@example.com) and I put them in your project's page as son as possible.
Thanks. And then put a link of this page into your project's website.
The information about "DISKTORQUEONPLANETS" are provided by the European Opendata Portal: CORDIS opendata.