About: Inflation from N-forms and its stability

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scholarly article in Journal of High Energy Physics, 2009 no. 9, September 2009

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована у вересні 2009 (uk) im September 2009 veröffentlichter wissenschaftlicher Artikel (de) scholarly article in Journal of High Energy Physics, 2009 no. 9, September 2009 (en)
publication date	wds:Q58200809-2C9FB3EB-EB5C-4991-AD0A-01C11CAB6B5B
publication date	2009-09-21 00:00:00Z (xsd:dateTime)
exact match	wds:Q58200809-B06DB3C0-7822-4063-B864-B4EF5AD0652A
exact match	https://scigraph.springernature.com/pub.10.1088/1126-6708/2009/09/092
cites work	wds:Q58200809-02E49556-35E4-4459-8315-02452D2C3A81 wds:Q58200809-11AA37C1-E496-4859-AADB-B4280FD41B78 wds:Q58200809-1307515B-B55B-4FB8-ADDC-557804944FF2 wds:Q58200809-1530A7CE-456F-42E0-8C1A-755B325705F2 wds:Q58200809-2EEAEFB5-FB15-4987-A9DB-953A7CE6FC1F wds:Q58200809-69CC8045-21D4-4DC2-ABD3-80ADA0EB083C wds:Q58200809-6A31515D-1DA5-474D-B9B8-68F347888307 wds:Q58200809-6A6F8793-80A3-4CF1-9915-12B1321CEBDA wds:Q58200809-7A274FC0-6365-4E83-9950-36BD8EB61BAC wds:Q58200809-7BF9A306-F2D7-4A2B-B450-C525108688B8 wds:Q58200809-807599DB-608C-40FC-91E1-55E6FC12AA12 wds:Q58200809-8490523C-3227-4C5A-B46B-1A01D128B803 wds:Q58200809-8A2D2E5D-C42D-41EA-B695-125B035961AA wds:Q58200809-8ACA401A-F258-4FD0-AAF7-4A29CE319BF7 wds:Q58200809-9429C7AC-EF31-4C73-91FC-9DBF90212568 wds:Q58200809-A8B5F4A5-3412-494C-858F-481A46D31D8B wds:Q58200809-C1C9462B-B5CE-44EC-BB8C-50E7AF21F893 wds:Q58200809-C21CD898-5FE0-4422-B052-D1107B1F9E24 wds:Q58200809-CCA9031F-5DF3-4E9B-AEE3-5C33CEC0796B wds:Q58200809-CE7B1B89-E8FC-4D51-8FBA-D9C699EADC2E wds:Q58200809-E7C0ECEE-6F88-4688-85A8-FAD1C7982E65 wds:Q58200809-F198FB23-B997-4AD5-B388-D248833B5882 wds:Q58200809-F593C187-73A8-4B72-9DAE-73FC0BAAF372 wds:Q58200809-F795495A-A791-43DA-A66B-8D79E112133F wds:Q58200809-F8A30267-DAFA-4F4A-98DB-1D36B9C28C5F
cites work	Cosmology and the fate of dilatation symmetry Inflationary universe: A possible solution to the horizon and flatness problems Mach's Principle and a Relativistic Theory of Gravitation Significance of the largest scale CMB fluctuations in WMAP DYNAMICS OF DARK ENERGY Chaotic inflation Brane inflation Theory of cosmological perturbations Reheating after inflation. Is the low-l microwave background cosmic? A new type of isotropic cosmological models without singularity Particle physics models of inflation and the cosmological density perturbation A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems Inflationary universe with anisotropic hair. Cosmology and astrophysical constraints of Gauss–Bonnet dark energy Gauss-Bonnet quintessence: Background evolution, large scale structure, and cosmological constraints Constraining dark energy anisotropic stress Examination of Evidence for a Preferred Axis in the Cosmic Radiation Anisotropy Low-order multipole maps of cosmic microwave background anisotropy derived fromWMAP A new nonsymmetric gravitational theory CMB anisotropies and inflation from non-standard spinors Dark energy anisotropic stress and large scale structure formation Microscopic and macroscopic behaviors of Palatini modified gravity theories Primordial magnetic fields via spontaneous breaking of Lorentz invariance Cuscuton cosmology: Dark energy meets modified gravity
author name string	wds:Q58200809-525D019B-0089-4513-A586-1280607E864C wds:Q58200809-F472DB9E-9AB7-485E-BC1E-465418D87C41
author name string	Tomi S Koivisto Cyril Pitrou
rdfs:label	Inflation from N-forms and its stability (en) Inflation from N-forms and its stability (nl)
skos:prefLabel	Inflation from N-forms and its stability (en) Inflation from N-forms and its stability (nl)
name	Inflation from N-forms and its stability (en) Inflation from N-forms and its stability (nl)
author	wds:Q58200809-53DF8D6C-D2CF-4659-B940-E970DA18BBD7
author	David F. Mota
title	wds:Q58200809-2F7F5E00-C6B8-4AFE-9BFF-D8324DAEFBF1
title	Inflation from N-forms and its stability (en)
page(s)	wds:Q58200809-ACAB192A-4C8F-46EB-A23E-BE0C1EC38E7B
page(s)	092-092
instance of	wds:Q58200809-03C96855-670B-45DF-BB3D-7B2A393530A9
instance of	scholarly article
published in	wds:Q58200809-1175E4E6-6C8B-41B9-B6E5-EC0D7BE64EED
published in	Journal of High Energy Physics
issue	wds:Q58200809-E19809EA-3298-4E8B-B29E-8575D1D446E5
volume	wds:Q58200809-7ADB40AB-C463-4776-9C68-A5E775CD659C
issue	09
volume	2009
DOI	wds:Q58200809-BA4E1373-C12C-4BD6-AB30-F1E3CEB4FEC3
DOI	http://dx.doi.org/10.1088/1126-6708/2009/09/092
DOI	10.1088/1126-6708/2009/09/092
arXiv ID	wds:Q58200809-80259C17-04B5-42A9-BC40-B56C342FED78
arXiv ID	0903.4158
ADS bibcode	wds:Q58200809-24ADE560-3EB6-4721-851A-865FF65CDF84
ADS bibcode	2009JHEP...09..092K
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58200809
is cites work of	Possibility of anisotropic curvature in cosmology Cosmic microwave background anomalies from imperfect dark energy CMB statistics in noncommutative inflation Non-Gaussianity and Statistical Anisotropy from Vector Field Populated Inflationary Models Inflation with stable anisotropic hair: is it cosmologically viable? Unifying static analysis of gravitational structures with a scale-dependent scalar field gravity as an alternative to dark matter
is cites work of	wds:Q58200752-DC117296-2B6A-46A7-8322-9C4276ECE926 wds:Q58200675-94593518-9A8D-4B30-A17E-31557D56633C wds:Q58200748-B90AC9FC-FB74-4D55-9F61-B6F5A9370026

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