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Cosmo-Blow-Up SIGNED

Deflating the blow-up: controlling infinities in cosmic fluid descriptions

Total Cost €

EC-Contrib. €

Partnership

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Cosmo-Blow-Up project word cloud

Explore the words cloud of the Cosmo-Blow-Up project. It provides you a very rough idea of what is the project "Cosmo-Blow-Up" about.

model nobel experts descriptions thereby birth computations physics expertise exactly heart body numerical trajectories gap structure utterly shell complementing complementary times fluid space discovery interdisciplinary begin macrophysical crossing world pioneering either place marks vicinity approximative mathematical curie simulations outstanding tackled opposes houses detecting dark usually epic leads universe full exact standard rewarding ways nature certain equations trend instant prize fledged scales heavily critical instance ups shrouded intersect solutions models resolving cosmology precious mystery gained marie infinities close expansion collapse blow opposing point energy lagrange cosmological quite fellowship cluttered analytical until overlapping starting accelerated witnesses host battle

Project "Cosmo-Blow-Up" data sheet

The following table provides information about the project.

Coordinator	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS Organization address address: RUE MICHEL ANGE 3 city: PARIS postcode: 75794 website: www.cnrs.fr contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	France [FR]
Total cost	185˙076 €
EC max contribution	185˙076 € (100%)
Programme	1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
Code Call	H2020-MSCA-IF-2017
Funding Scheme	MSCA-IF-EF-ST
Starting year	2018
Duration (year-month-day)	from 2018-12-01 to 2020-11-30

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS Organization address address: RUE MICHEL ANGE 3 city: PARIS postcode: 75794 website: www.cnrs.fr contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	FR (PARIS)	coordinator	185˙076.00

Map

Project objective

'According to the standard model of cosmology, we are witnesses of an epic battle: While dark energy leads to an accelerated expansion, matter and particularly the dark matter, opposes this trend, leading to the observed large-scale structure of the Universe. Since the pioneering discovery of dark energy that lead to a Nobel Prize in Physics, the nature of dark matter is still shrouded in mystery. What we know is that matter can be described as a fluid on macrophysical scales, and that the fluid has, at early times, no overlapping matter trajectories. Yet, matter trajectories do eventually begin to intersect ('shell-crossing'), which marks the starting point of very complex computations in the phase-space on the one side, and the birth of our cluttered Universe on the other side. Understanding the collapse and shell-crossing is quite a challenge that is usually tackled by utterly opposing means, either by (approximative) analytical models or by cosmological N-body simulations. With this Marie-Curie fellowship, I will close this gap and get full control of the instant of shell-crossing in two complementary ways. I will develop full-fledged numerical simulations of the cosmological fluid equations and develop certain matter collapse models, that, at their heart, determine the matter trajectories by exact analytical descriptions until the instance of shell-crossing, where infinities become real and the solutions 'blow up'. Detecting blow-ups is one of the most challenging and rewarding problems in mathematical physics; by resolving them, precious information will be gained which we will use to improve (heavily used) N-body simulations at the critical vicinity of shell-crossing. The department Lagrange (host institute) is a unique place in Europe that houses both world experts in numerical cosmology and in mathematical analysis, thereby complementing exactly my expertise (exact analytical models). This allows us to solve outstanding problems in interdisciplinary fields.'

Publications

List of publications.
year	authors and title	journal	last update
2019	Cornelius Rampf Quasi-spherical collapse of matter in Î›CDM published pages: 5223-5235, ISSN: 0035-8711, DOI: 10.1093/mnras/stz372	Monthly Notices of the Royal Astronomical Society 484/4	2019-06-27
2019	Cora Uhlemann, Cornelius Rampf, Mateja Gosenca, Oliver Hahn Semiclassical path to cosmic large-scale structure published pages: , ISSN: 2470-0010, DOI: 10.1103/physrevd.99.083524	Physical Review D 99/8	2019-06-27

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