About: Homogeneous cosmological models and new inflation

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

scientific article published on 01 October 1986

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована в жовтні 1986 (uk) article scientifique publié en 1986 (fr) im Oktober 1986 veröffentlichter wissenschaftlicher Artikel (de) artículu científicu espublizáu n'ochobre de 1986 (ast) scientific article published on 01 October 1986 (en)
publication date	wds:Q74475006-1DF6563D-0EED-4748-B3A5-56C11ECAF968
publication date	1986-10-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q74475006-5A46A1CE-9BC3-45B4-B4FD-8F5C533807A8
language of work or name	English
cites work	wds:Q74475006-12FB81A5-849E-42DB-96D8-77E018DBD7C3 wds:Q74475006-3A81553A-6F6F-485F-97DC-98EF3C01984A wds:Q74475006-7C5AF991-9C00-4C08-95F0-C52C9B7B43D3 wds:Q74475006-855E923C-BF83-4856-9664-DCDEFFE351A4 wds:Q74475006-91B67426-92C3-4905-9B15-496E7AF6B1BB wds:Q74475006-9E5D2E9F-4D8A-4004-9648-332B56A7701B wds:Q74475006-D2B741B0-20B0-45F0-8E4E-9FDDDBCF1E94 wds:Q74475006-D9D1E5C2-F645-47D7-9366-4506865FF0B2 wds:Q74475006-ED53EA58-515D-45EF-9DE6-E1B341510222
cites work	Inflationary universe: A possible solution to the horizon and flatness problems Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking Spontaneous creation of almost scale-free density perturbations in an inflationary universe Wave function of the Universe A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems A class of homogeneous cosmological models Effect of inflation on anisotropic cosmologies Why is the Universe Isotropic? Expansion isotropization during the inflationary era
author name string	wds:Q74475006-2FC52EB9-94DB-4648-BCE3-3C40BCC7FEBB wds:Q74475006-455FF58E-A46C-437E-AD60-BF2FE3E43496
author name string	Turner MS Widrow LM
rdfs:label	Homogeneous cosmological models and new inflation (en) Homogeneous cosmological models and new inflation (nl)
skos:prefLabel	Homogeneous cosmological models and new inflation (en) Homogeneous cosmological models and new inflation (nl)
name	Homogeneous cosmological models and new inflation (en) Homogeneous cosmological models and new inflation (nl)
title	wds:Q74475006-A368699F-C7A0-470B-B0EF-9863F3195B11
title	Homogeneous cosmological models and new inflation (en)
page(s)	wds:Q74475006-5485AF6C-545A-46B6-B8F9-B8D86087553C
page(s)	2237
instance of	wds:Q74475006-E4E92CFC-F28F-43F1-9F82-286728785175
instance of	scholarly article
PubMed ID	wds:Q74475006-10A99BF2-5A77-4D85-8D2C-667F8DA1890F
PubMed ID	http://rdf.ncbi.nlm.nih.gov/pubchem/reference/10033671
PubMed ID	10033671
published in	wds:Q74475006-59429DFF-5433-43F3-A271-B647617A3376
published in	Physical Review Letters
issue	wds:Q74475006-4BC9FF46-4D6D-42B6-8F04-BAEF0FBB11E5
volume	wds:Q74475006-412582D9-9380-4D98-9C12-E70218F5C1B2
issue	17
volume	57
DOI	wds:Q74475006-AC630BD8-A2CA-46F4-95DA-F43D32730F9F
DOI	http://dx.doi.org/10.1103/PHYSREVLETT.57.2237
DOI	10.1103/PHYSREVLETT.57.2237
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q74475006
is cites work of	How Anisotropic is Our Universe? Kantowski-Sachs universes and the cosmic no-hair conjecture. Anisotropy dissipation in brane-world inflation Old inflation and anisotropy Inhomogeneous initial conditions for inflation Szekeres universes with homogeneous scalar fields
is cites work of	wds:Q57221994-FA211F7F-F463-42D1-AC63-049E753891A4 wds:Q52396021-9A524441-604D-4F55-BC29-D1FDBB227C29 wds:Q63390688-B053B988-D5D9-4290-AA85-9317C85A8B33 wds:Q58968777-0B1378BD-EB97-4486-98F7-0E513D9CF321 wds:Q92911857-0E9D2CA3-1A66-4D76-A933-BC3CD92D6A3F wds:Q74414443-9CD8758B-D679-4AB2-A6B4-5BBD200D95FA

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