About: A small amount of mini-charged dark matter could cool the baryons in the early Universe

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scientific article published in Nature

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) article publié dans la revue scientifique Nature (fr) scientific article published in Nature (en) im Mai 2018 veröffentlichter wissenschaftlicher Artikel (de) наукова стаття, опублікована в Nature в травні 2018 (uk)
publication date	wds:Q59069177-89B0F00C-4BEE-420F-863D-32F034C8698A
publication date	2018-05-30 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q59069177-1C6F9302-7180-4474-B49C-2EB67FFA855D
language of work or name	English
exact match	wds:Q59069177-7D1039DB-50F6-4611-BC0F-DDA9A53D6CD8
exact match	https://scigraph.springernature.com/pub.10.1038/s41586-018-0151-x
cites work	wds:Q59069177-09C87049-AD92-46C9-B102-3D70CCB245DF wds:Q59069177-13114FAC-61BA-47B9-8414-D587E928C204 wds:Q59069177-15B6EAD0-E693-4B38-B0F5-FB07C4656C0D wds:Q59069177-26247537-FF71-4287-9BDD-CBB0C4B49EF6 wds:Q59069177-30494BC2-9EA4-4AD8-AE7E-2267667EBE06 wds:Q59069177-3633DB2E-120D-4272-89F9-51F510E0F33E wds:Q59069177-3E1748CF-9684-4DBF-A815-FC28D24BEE02 wds:Q59069177-45F8519D-D82D-4E2A-ABB9-3AA6DD15E37A wds:Q59069177-4CDCCD93-A78D-4B9D-AB30-3C0553D8C694 wds:Q59069177-4CDF39B8-B757-40B8-81C5-2A5566F05D0A wds:Q59069177-62349051-7E77-469B-B4C2-9B3A7E1B3F8D wds:Q59069177-6D64B9B6-87D3-499C-AAEC-10B7BE016B39 wds:Q59069177-7164566C-4E29-4F15-8423-DAD899F398AD wds:Q59069177-7544971A-32B3-42B8-9A38-BF1207203562 wds:Q59069177-757E2C82-0087-40E8-8809-0F328B19FC99 wds:Q59069177-7EFA73A5-B01F-4446-BD4F-1CA192D764D8 wds:Q59069177-85BD3C31-3070-44A7-A9F4-F9E55E0A918E wds:Q59069177-8711F6C1-EC95-4616-B239-C1DC7CBA6B33 wds:Q59069177-8D25F153-E9C5-4796-9043-424C2BA9016F wds:Q59069177-8FB698EA-CEEA-41D4-B92A-C5414565244B wds:Q59069177-95ED43DA-5550-4F65-9C97-26302C2A1857 wds:Q59069177-C408B291-A95F-4079-A38B-E701F0EF0AEB wds:Q59069177-CD391BF3-62A1-41B2-848A-4F1519129034 wds:Q59069177-CE053657-80AF-4F69-A187-4F53938FF676 wds:Q59069177-E54BDB4D-F3FC-44DA-BA29-550D672B2368 wds:Q59069177-F13A842E-2D8B-4A39-9259-0503A18477AC wds:Q59069177-FCF01922-37CD-4C54-8D8E-B471A2E353F1 wds:Q59069177-FF5236A0-A68C-4A7A-B33B-2DBDCBED13C0
cites work	Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges Constraining the unexplored period between the dark ages and reionization with observations of the global 21 cm signal Cosmology at low frequencies: The 21cm transition and the high-redshift Universe 21 Centimeter Tomography of the Intergalactic Medium at High Redshift On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line Evolution of the 21 cm signal throughout cosmic history Two U(1)'s and ϵ charge shifts Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 /R = 4kpc/ to UGC 2885 /R = 122 kpc/ LEP shines light on dark matter A new radio-X-ray probe of galaxy cluster magnetic fields Cold dark matter: Controversies on small scales Single explanation for both baryon and dark matter densities Recombination of the Primeval Plasma The Spin Temperature of Intergalactic Neutral Hydrogen Hydrogen Epoch of Reionization Array (HERA) Search for an intermediate-range interaction The nongravitational interactions of dark matter in colliding galaxy clusters On the local dark matter density Possible interaction between baryons and dark-matter particles revealed by the first stars. An absorption profile centred at 78 megahertz in the sky-averaged spectrum Turning off the lights: How dark is dark matter? Dark matter self-interactions via collisionless shocks in cluster mergers Charting the parameter space of the global 21-cm signal Constraining dark matter-baryon scattering with linear cosmology A new model of the galactic magnetic field Light Dark Matter from Forbidden Channels TheFermiGalactic Center GeV Excess and Implications for Dark Matter Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure.
author name string	wds:Q59069177-36F24F70-96D7-4897-AD8A-2B6B6764025A wds:Q59069177-C642332E-19D1-4C19-81C6-CE630F9DE4DF
author name string	Abraham Loeb Julian B Muñoz
rdfs:label	A small amount of mini-charged dark matter could cool the baryons in the early Universe (en) A small amount of mini-charged dark matter could cool the baryons in the early Universe (nl)
skos:prefLabel	A small amount of mini-charged dark matter could cool the baryons in the early Universe (en) A small amount of mini-charged dark matter could cool the baryons in the early Universe (nl)
name	A small amount of mini-charged dark matter could cool the baryons in the early Universe (en) A small amount of mini-charged dark matter could cool the baryons in the early Universe (nl)
author	wds:Q59069177-8FBEE77C-E0DC-4CAB-B1CE-1C90933535F9
author	Avi Loeb
title	wds:Q59069177-F48F8638-6863-4BA7-BC8C-617D255F86F3
title	A small amount of mini-charged dark matter could cool the baryons in the early Universe (en)
page(s)	wds:Q59069177-6C0D5A86-B689-4E3E-946A-9A0DC0BA08B8
page(s)	684-686
instance of	wds:Q59069177-945942D0-5495-4903-8BFA-BD70EBCD5219
instance of	scholarly article
main subject	wds:Q59069177-060D5282-A5E7-4F7D-9F53-BB7BD2A402C1
main subject	dark matter
PubMed ID	wds:Q59069177-4901B21E-CC3F-4162-8F1E-93DDFD02DDEB
PubMed ID	http://rdf.ncbi.nlm.nih.gov/pubchem/reference/29849153
PubMed ID	29849153
published in	wds:Q59069177-FD760259-17AA-4B8E-B3E2-AA7EE2BF17A2
published in	Nature
issue	wds:Q59069177-63B53EA5-23B5-41D3-9CB3-8E0A2EEEDEE9
volume	wds:Q59069177-D419F314-3354-4707-954D-335D99CCE56D
issue	7707
volume	557
DOI	wds:Q59069177-0EA10310-2766-4C36-AC16-BAEA4842EF65
DOI	http://dx.doi.org/10.1038/S41586-018-0151-X

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