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20022026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 33.2k across the 388 of their papers we have counts for

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Showing 2012Show all

6 papers · 1 filter

astro-ph.CO2012★ 3 cited

Less is more: How cosmic voids can shed light on dark energy

E. G. Patrick Bos, Rien van de Weygaert, Jarno Ruwen +2

We showed how the shape of cosmic voids can be used to distinguish between different models of dark energy using galaxy positions.

astro-ph.CO2012★ 83 cited

Constraints on coupled dark energy using CMB data from WMAP and SPT

Valeria Pettorino, Luca Amendola, Carlo Baccigalupi +1

We consider the case of a coupling in the dark cosmological sector, where a dark energy scalar field modifies the gravitational attraction between dark matter particles. We find th…

astro-ph.CO2012★ 164 cited

The darkness that shaped the void: dark energy and cosmic voids

E. G. Patrick Bos, Rien van de Weygaert, Klaus Dolag +1

Aims: We assess the sensitivity of void shapes to the nature of dark energy that was pointed out in recent studies. We investigate whether or not void shapes are useable as an obse…

astro-ph.CO2012★ 905 cited

Cosmology and fundamental physics with the Euclid satellite

Luca Amendola, Stephen Appleby, David Bacon +60

Euclid is a European Space Agency medium class mission selected for launch in 2019 within the Cosmic Vision 2015-2025 programme. The main goal of Euclid is to understand the origin…

astro-ph.CO2012★ 50 cited

Hydrodynamical simulations of galaxy clusters in dark energy cosmologies: II. c-M relation

Cristiano De Boni, Stefano Ettori, Klaus Dolag +1

We use hydrodynamical simulations of different dark energy cosmologies to investigate the concentration-mass (c-M) relation in galaxy clusters. In particular, we consider a referen…

astro-ph.CO2012★ 35 cited

Non-minimally coupled dark matter: effective pressure and structure formation

Dario Bettoni, Valeria Pettorino, Stefano Liberati +1

We propose a phenomenological model in which a non-minimal coupling between gravity and dark matter is present in order to address some of the apparent small scales issues of \lcdm…