Explore the words cloud of the COSMO_SIMS project. It provides you a very rough idea of what is the project "COSMO_SIMS" about.
The following table provides information about the project.
Coordinator |
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
Organization address contact info |
Coordinator Country | France [FR] |
Project website | https://cosmo.oca.eu |
Total cost | 1˙471˙382 € |
EC max contribution | 1˙471˙382 € (100%) |
Programme |
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC)) |
Code Call | ERC-2015-STG |
Funding Scheme | ERC-STG |
Starting year | 2016 |
Duration (year-month-day) | from 2016-09-01 to 2021-08-31 |
Take a look of project's partnership.
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1 | CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS | FR (PARIS) | coordinator | 1˙471˙382.00 |
The objective of this ambitious research proposal is to push forward the frontier of computational cosmology by significantly improving the precision of numerical models on par with the increasing richness and depth of surveys that aim to shed light on the nature of dark matter and dark energy.
Using new phase-space techniques for the simulation and analysis of dark matter, completely new insights into its dynamics are possible. They allow, for the first time, the accurate simulation of dark matter cosmologies with suppressed small-scale power without artificial fragmentation. Using such techniques, I will establish highly accurate predictions for the properties of dark matter and baryons on small scales and investigate the formation of the first galaxies in non-CDM cosmologies. Baryonic effects on cosmological observables are a severe limiting factor in interpreting cosmological measurements. I will investigate their impact by identifying the relevant astrophysical processes in relation to the multi-wavelength properties of galaxy clusters and the galaxies they host. This will be enabled by a statistical set of zoom simulations where it is possible to study how these properties correlate with one another, with the assembly history, and how we can derive better models for unresolved baryonic processes in cosmological simulations and thus, ultimately, how we can improve the power of cosmological surveys. Finally, I will develop a completely unified framework for precision cosmological initial conditions (ICs) that is scalable to both the largest simulations and the highest resolution zoom simulations. Bringing ICs into the ‘cloud’ will enable new statistical studies using zoom simulations and increase the reproducibility of simulations within the community.
My previous work in developing most of the underlying techniques puts me in an excellent position to lead a research group that is able to successfully approach such a wide-ranging and ambitious project.
year | authors and title | journal | last update |
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2018 |
Aseem Paranjape, Oliver Hahn, Ravi K Sheth The dependence of galaxy clustering on tidal environment in the Sloan Digital Sky Survey published pages: 5442-5452, ISSN: 0035-8711, DOI: 10.1093/mnras/sty633 |
Monthly Notices of the Royal Astronomical Society 476/4 | 2020-02-26 |
2017 |
Frank C van den Bosch, Go Ogiya, Oliver Hahn, Andreas Burkert Disruption of dark matter substructure: fact or fiction? published pages: 3043-3066, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2956 |
Monthly Notices of the Royal Astronomical Society 474/3 | 2020-02-26 |
2017 |
C. Uhlemann, S. Codis, O. Hahn, C. Pichon, F. Bernardeau Two is better than one: joint statistics of density and velocity in concentric spheres as a cosmological probe published pages: 2481-2497, ISSN: 0035-8711, DOI: 10.1093/mnras/stx969 |
Monthly Notices of the Royal Astronomical Society 469/2 | 2020-02-26 |
2017 |
Go Ogiya, Oliver Hahn What sets the central structure of dark matter haloes? published pages: 4339-4359, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2639 |
Monthly Notices of the Royal Astronomical Society 473/4 | 2020-02-26 |
2018 |
Frank C van den Bosch, Go Ogiya Dark matter substructure in numerical simulations: a tale of discreteness noise, runaway instabilities, and artificial disruption published pages: 4066-4087, ISSN: 0035-8711, DOI: 10.1093/mnras/sty084 |
Monthly Notices of the Royal Astronomical Society 475/3 | 2020-02-26 |
2017 |
Kohei Hayashi, Tomoaki Ishiyama, Go Ogiya, Masashi Chiba, Shigeki Inoue, Masao Mori Universal Dark Halo Scaling Relation for the Dwarf Spheroidal Satellites published pages: 97, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aa74d9 |
The Astrophysical Journal 843/2 | 2020-02-26 |
2018 |
Aseem Paranjape, Oliver Hahn, Ravi K Sheth Halo assembly bias and the tidal anisotropy of the local halo environment published pages: 3631-3647, ISSN: 0035-8711, DOI: 10.1093/mnras/sty496 |
Monthly Notices of the Royal Astronomical Society 476/3 | 2020-02-26 |
2018 |
Go Ogiya Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter published pages: L106-L110, ISSN: 1745-3933, DOI: 10.1093/mnrasl/sly138 |
Monthly Notices of the Royal Astronomical Society: Letters 480/1 | 2020-02-26 |
2019 |
Michael Buehlmann, Oliver Hahn Large-scale velocity dispersion and the cosmic web published pages: 228-245, ISSN: 0035-8711, DOI: 10.1093/mnras/stz1243 |
Monthly Notices of the Royal Astronomical Society 487/1 | 2020-02-26 |
2019 |
Cora Uhlemann, Cornelius Rampf, Mateja Gosenca, Oliver Hahn Semiclassical path to cosmic large-scale structure published pages: 83524, ISSN: 2470-0010, DOI: 10.1103/physrevd.99.083524 |
Physical Review D 99/8 | 2020-02-26 |
2018 |
R. Adam, O. Hahn, F. Ruppin, P. Ade, P. André, M. Arnaud, I. Bartalucci, A. Beelen, A. Benoît, A. Bideaud, N. Billot, O. Bourrion, M. Calvo, A. Catalano, G. Coiffard, B. Comis, A. D’Addabbo, F.-X. Désert, S. Doyle, C. Ferrari, J. Goupy, C. Kramer, G. Lagache, S. Leclercq, J.-F. Lestrade, J. F. MacÃas-Pérez, G. Martinez Aviles, D. Martizzi, S. Maurogordato, P. Mauskopf, F. Mayet, A. Monfardini, F. Pajot, E. Pascale, L. Perotto, G. Pisano, E. Pointecouteau, N. Ponthieu, G. W. Pratt, V. Revéret, M. Ricci, A. Ritacco, L. Rodriguez, C. Romero, H. Roussel, K. Schuster, A. Sievers, S. Triqueneaux, C. Tucker, H.-Y. Wu, R. Zylka Substructure and merger detection in resolved NIKA Sunyaev-Zel’dovich images of distant clusters published pages: A118, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731950 |
Astronomy & Astrophysics 614 | 2020-02-26 |
2019 |
Go Ogiya, Frank C van den Bosch, Oliver Hahn, Sheridan B Green, Tim B Miller, Andreas Burkert DASH: a library of dynamical subhalo evolution published pages: 189-202, ISSN: 0035-8711, DOI: 10.1093/mnras/stz375 |
Monthly Notices of the Royal Astronomical Society 485/1 | 2020-02-26 |
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