Skip to main content
Go to the home page of the European Commission (opens in new window)
English English
CORDIS - EU research results
CORDIS
Content archived on 2024-06-18

Mapping the Dark Web of the Cosmos

Objective

With this research project we propose a full morphological analysis of clusters of galaxies and the cosmic web itself, based on very high resolution maps of the dark matter distribution in these structures. Those maps will be derived by means of gravitational lensing and other tracers of the dark matter distribution like temperature maps of the Cosmic Microwave Background. This analysis will go far beyond the usual simplifications made in the characterisation and classification of structure, like azimuthally averaged, 1-dimensional functional forms of the density profile or the sole use of 2-point correlation functions in astrophysical data.
The cosmic web is the global, filamentary structure of the Universe with clusters of galaxies sitting at the intersects of this network. We will produce high-resolution maps of this web using wide-field galaxy redshift surveys and analyse its morphology, including its most prominent structures, clusters of galaxies, which are particularly interesting tracers of structure formation since they are the latest structures to form in the current paradigm of cosmological structure formation. All cluster mass components, the dominant dark matter, hot X-ray emitting intra-cluster gas and the small fraction of mass sitting in luminous stars are directly or indirectly observable through optical, X-ray, lensing or Sunyaev Zel'dovich observations. This morphological characterisation will be carried out with the techniques of mathematical morphology and include Minkowski functionals. By comparing to a large set of numerically simulated data, we aim to distinguish different models of dark matter including cold, warm and self-interacting dark matter. This is possible since the morphology of structure changes significantly in those different formation scenarios. Our analysis will use data from the cluster surveys CLASH and the Frontier Fields, from the wide-field surveys CFHTLenS and KiDS and will path the way for the Euclid mission.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.

You need to log in or register to use this function

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Call for proposal

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

FP7-PEOPLE-2013-IIF
See other projects for this call

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.

MC-IIF - International Incoming Fellowships (IIF)

Coordinator

THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD
EU contribution
€ 221 606,40
Address
WELLINGTON SQUARE UNIVERSITY OFFICES
OX1 2JD Oxford
United Kingdom

See on map

Region
South East (England) Berkshire, Buckinghamshire and Oxfordshire Oxfordshire
Activity type
Higher or Secondary Education Establishments
Links
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.

No data
My booklet 0 0