About: Neutron limit on the strongly-coupled chameleon field

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) article scientifique publié en 2016 (fr) գիտական հոդված (hy) scholarly article (en) наукова стаття, опублікована в березні 2016 (uk) im März 2016 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q57432777-5CBB43C5-8D2F-420E-B561-BD67786BAE6A
publication date	2016-03-11 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q57432777-557507B2-E394-4734-A265-853DA8BA7772
language of work or name	English
cites work	wds:Q57432777-0ECDE7AB-26D4-492E-9637-A1290EB0FFA4 wds:Q57432777-2E069EB9-1ADA-4BD3-82A5-6C270BE87D6D wds:Q57432777-3BBD5D6E-E830-4072-B4DB-CCAA027AB0AF wds:Q57432777-50296077-820E-490B-8C1A-B274188B8FA7 wds:Q57432777-57B11B99-532C-41C6-B50A-208DA1EB907F wds:Q57432777-6C7AC1CD-3ED8-4C7F-BBF1-36DBD98B7208 wds:Q57432777-6E806BD7-600F-4D2F-BFDD-B4FF3A32D3CD wds:Q57432777-747EF2C9-24F4-45FE-967C-AA0FDC3B3BD5 wds:Q57432777-8A8ACE19-D108-45E8-8EB6-B02E61155838 wds:Q57432777-8CCF98F8-9664-47C9-BF6A-654F1BADC79F wds:Q57432777-9EAAEF2E-21D6-43E4-BBDA-8389D8865E27 wds:Q57432777-A6DF2C31-4B10-41BE-B85F-4053B3168392 wds:Q57432777-B088098C-90CB-4D0D-9732-3E60939C311B wds:Q57432777-C826DD9F-5047-4EDE-B4DD-6210B5CB921D wds:Q57432777-CAB2630B-9D2D-4F5C-9D2C-E0947058C3C9 wds:Q57432777-F5125DF6-430E-4AFE-A1BD-332708003B1F wds:Q57432777-FAB5E35E-2F80-4548-B0BE-1B7B4A5D0E52
cites work	Measurements of Ω and Λ from 42 High‐Redshift Supernovae Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant Cosmological consequences of a rolling homogeneous scalar field Search for chameleons with CAST Chameleon cosmology Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function ASTROPHYSICS. Atom-interferometry constraints on dark energy Search for Chameleon Particles Using a Photon-Regeneration Technique Detecting dark energy in orbit: The cosmological chameleon Search for chameleon scalar fields with the axion dark matter experiment. The Hubble Space Telescope Cluster Supernova Survey. V. Improving the dark-energy constraints above z > 1 and building an early-type-hosted supernova sample Controlling neutron orbital angular momentum. Gravity Resonance Spectroscopy Constrains Dark Energy and Dark Matter Scenarios Beyond the cosmological standard model Facilities for Fundamental Neutron Physics Research at the NIST Cold Neutron Research Facility.
author name string	wds:Q57432777-10888BE0-CBE8-4F6F-9E66-0CECD3CB50BE wds:Q57432777-1B12C22D-F3CC-4F8B-AF89-0CFECED27179 wds:Q57432777-219BAAAD-2A3C-48E9-85A9-36F68F4FFBFE wds:Q57432777-23D65E4F-0039-440E-BC6C-0B3779873316 wds:Q57432777-381A250E-6E9D-45EF-A4E3-F52705D0C880 wds:Q57432777-3B87F89D-F5BA-4395-BC6F-EA38DC2E8023 wds:Q57432777-4AF2B137-2934-447C-A09E-9368A845829E wds:Q57432777-5A81F37E-9A8B-4698-9ADA-4894A8B454D7 wds:Q57432777-7E89CABF-4470-4141-8FB4-2BDC7A316F24 wds:Q57432777-8CE2495A-98D9-424F-BEB7-E9E76328C012 wds:Q57432777-9AB05EED-BC35-44D4-A94A-FBB0AA81B7B9 wds:Q57432777-B1CC7AE3-1A50-4787-8DC4-0F161E14D4ED wds:Q57432777-BB4B0620-7E62-4BC6-BEB1-F897A5396517 wds:Q57432777-FB4DFA9D-A76D-4B62-BFCF-CA6CD1D82E64
author name string	K. Li M. Arif D. Sarenac B. Heacock R. Haun A. R. Young J. Nsofini C. B. Shahi D. A. Pushin D. G. Cory M. G. Huber P. Saggu V. Skavysh W. M. Snow
rdfs:label	Neutron limit on the strongly-coupled chameleon field (en) Neutron limit on the strongly-coupled chameleon field (nl)
skos:prefLabel	Neutron limit on the strongly-coupled chameleon field (en) Neutron limit on the strongly-coupled chameleon field (nl)
name	Neutron limit on the strongly-coupled chameleon field (en) Neutron limit on the strongly-coupled chameleon field (nl)
title	wds:Q57432777-730726A7-A9C4-42D8-A2F8-89386E6F677D
title	Neutron limit on the strongly-coupled chameleon field (en)
Internet Archive ID	wds:Q57432777-C5E0C220-0068-4787-8FA3-323D29B31C1C
Internet Archive ID	arxiv-1601.06897
instance of	wds:Q57432777-383BF98E-0A89-42C3-A1B8-8A9ABEE12957
instance of	scholarly article
published in	wds:Q57432777-524B4C29-8B37-403F-A403-402DC6DA378B
published in	Physical Review D
issue	wds:Q57432777-F2B0EB25-1261-446D-9540-96DA195E6313
volume	wds:Q57432777-35EA8454-8835-4906-8BA9-46D7DFD898FB
issue	6
volume	93
DOI	wds:Q57432777-31EAD21D-A5E8-4551-AABB-340EEE441AB1
DOI	http://dx.doi.org/10.1103/PHYSREVD.93.062001
DOI	10.1103/PHYSREVD.93.062001
arXiv ID	wds:Q57432777-01B9E4E3-AA1A-472A-A457-CE71945CEB5E
arXiv ID	1601.06897
ADS bibcode	wds:Q57432777-54904229-B01E-45A4-B07F-3B4FDD6DB954
ADS bibcode	2016PhRvD..93f2001L
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q57432777

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