About: Non-linear structure formation in cosmologies with early dark energy

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About: Non-linear structure formation in cosmologies with early dark energy Goto Sponge NotDistinct Permalink

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scientific article published in Astronomy and Astrophysics

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в липні 2006 (uk) im Juli 2006 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astronomy and Astrophysics (fr) scientific article published in Astronomy and Astrophysics (en)
publication date	wds:Q56937410-47B02D7E-1D6B-4A20-8920-86E78C3C9200
publication date	2006-07-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56937410-7791C3F2-3881-494A-B6A4-4CE63F16B329
language of work or name	English
cites work	wds:Q56937410-0152A668-492E-4AED-A764-6BADEB1B9080 wds:Q56937410-0B1D11C2-6515-49F4-AB75-6D53D2BFC3BE wds:Q56937410-116264B2-19E7-4348-AED5-DA87CFE40312 wds:Q56937410-3922EDBE-42F2-4BBF-815A-7F6AF1234819 wds:Q56937410-49884BDC-28EA-47F4-9511-722581BE5B27 wds:Q56937410-4FD7689E-2B1A-4947-8BB6-9EB2C68B27F2 wds:Q56937410-5268CEB6-9E10-48D8-96CE-4924CAC7FC8B wds:Q56937410-5C27F001-E682-4189-847F-A8DBD5F8F4CE wds:Q56937410-658FDF3A-C317-48B7-9073-3D2E9DC88BAF wds:Q56937410-66D0A0EB-84AE-4FAE-A44D-98C7A435A7AE wds:Q56937410-67062A9B-8AC4-4D60-A5E2-E4A879B61028 wds:Q56937410-87FA0BF9-E2A2-4CF8-A684-1C32AC51B9DD wds:Q56937410-8C10107D-2EF7-43A6-8581-8635582139E7 wds:Q56937410-8D355F6E-2ADC-4732-A8D7-1A5F91961A0A wds:Q56937410-8F472635-61CF-4F2E-A461-C241A4498F76 wds:Q56937410-935CA102-0BDD-44F7-BF3F-996B0098E9AE wds:Q56937410-9D21DA3F-1910-4458-8FD2-242CEA537C2F wds:Q56937410-A3BC5884-CFCF-4054-AEDF-6EAC37524AC0 wds:Q56937410-B93AE52E-24F8-4563-B017-A0FF3338FE04 wds:Q56937410-BB741E43-14A0-4AE5-9636-A0F2FF161DC5 wds:Q56937410-C9E3D88A-0F1A-4FAF-A432-2B69866D0A0F wds:Q56937410-D60896A9-0871-4345-87E8-866C055ADB68 wds:Q56937410-DC970512-F732-4971-A5E0-91E6B742E8D6 wds:Q56937410-F6D05D36-F535-4989-9991-265B536BAA56
cites work	Cosmological parameters from SDSS and WMAP Cosmological consequences of a rolling homogeneous scalar field Cosmology and the fate of dilatation symmetry First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters A Universal Density Profile from Hierarchical Clustering Weak gravitational lensing Cosmological Imprint of an Energy Component with General Equation of State Cosmology with a primordial scaling field A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state Phenomenological parameterization of quintessence The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe On the spherical collapse model in dark energy cosmologies The ROSAT Brightest Cluster Sample -- I. The compilation of the sample and the cluster log N--log S distribution The inner structure of CDM haloes -- I. A numerical convergence study Merger rates in hierarchical models of galaxy formation Cosmological parameter estimation using Very Small Array data out to ℓ= 1500 Excursion set mass functions for hierarchical Gaussian fluctuations Quintessence and the Separation of Cosmic Microwave Background Peaks The Mass Power Spectrum in Quintessence Cosmological Models Merger rates in hierarchical models of galaxy formation – II. Comparison with N-body simulations On determining the cluster abundance normalization Early Quintessence in Light of theWilkinson Microwave Anisotropy Probe Estimates of Cosmological Parameters Using the Cosmic Microwave Background Angular Power Spectrum of ACBAR TheROSAT‐ESO Flux‐limited X‐Ray (REFLEX) Galaxy Cluster Survey. IV. The X‐Ray Luminosity Function
author name string	wds:Q56937410-115E554C-65B8-4588-82CD-A13FF7992610
author name string	M. Doran
rdfs:label	Non-linear structure formation in cosmologies with early dark energy (en) Non-linear structure formation in cosmologies with early dark energy (nl)
skos:prefLabel	Non-linear structure formation in cosmologies with early dark energy (en) Non-linear structure formation in cosmologies with early dark energy (nl)
name	Non-linear structure formation in cosmologies with early dark energy (en) Non-linear structure formation in cosmologies with early dark energy (nl)
author	wds:Q56937410-07CADFB1-7A4F-4341-BD61-9C1BE4E095B8 wds:Q56937410-389AD0CA-4F2A-4F70-9F4E-59BCE21007F1
author	Christof Wetterich Matthias Bartelmann
title	wds:Q56937410-20832E32-0730-4CCC-943A-F2F52AEBD251
title	Non-linear structure formation in cosmologies with early dark energy (en)
page(s)	wds:Q56937410-225C0397-4D85-4922-8909-D8B1249CE5C1
page(s)	27–36
instance of	wds:Q56937410-60E4264D-BEB6-47C2-B998-AF8735937B1D
instance of	scholarly article
published in	wds:Q56937410-1324091A-E7BE-410E-AE9B-8C70C75C8187
published in	Astronomy and Astrophysics
issue	wds:Q56937410-4CF64C74-1B23-4D3F-9E92-6AD3373BD4DE
volume	wds:Q56937410-3C5A14E7-FFAB-4956-AAFE-0FC1F4719AE4
issue	1
volume	454
DOI	wds:Q56937410-E47EB72A-A61C-444C-AC65-337CC1D1B7F5
DOI	http://dx.doi.org/10.1051/0004-6361:20053922
DOI	10.1051/0004-6361:20053922
maintained by WikiProject	wds:Q56937410-2E71E776-A4CA-445B-8D99-35FDD7CEA73D
maintained by WikiProject	WikiProject Mathematics
zbMATH Open document ID	wds:Q56937410-8D12A575-6519-4446-8826-41EAAB54BE1E
zbMATH Open document ID	1134.85309
arXiv ID	wds:Q56937410-A419BE46-083E-46B0-9562-2BF89E4A0A87
arXiv ID	astro-ph/0507257
ADS bibcode	wds:Q56937410-3C763C5F-D97E-4C2C-BBE5-5E010C51DD5B
ADS bibcode	2006A&A...454...27B
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56937410
is cites work of	Relativistic virialization in the spherical collapse model for Einstein-de Sitter andΛCDMcosmologies Statistics of gravitational potential perturbations: A novel approach to deriving the X-ray temperature function Quintessence cosmologies with a growing matter component Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies A comparison of structure formation in minimally and non-minimally coupled quintessence models

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