Ultra-dense hydrogen H(0) as dark matter in the universe: new possibilities for the cosmological red-shift and the cosmic microwave background radiation
Crossref DOI link: https://doi.org/10.1007/s10509-019-3632-y
Published Online: 2019-08-29
Published Print: 2019-08
Update policy: https://doi.org/10.1007/springer_crossmark_policy
Holmlid, Leif https://orcid.org/0000-0003-4155-4985
Text and Data Mining valid from 2019-08-01
Version of Record valid from 2019-08-29
Article History
Received: 26 November 2018
Accepted: 19 August 2019
First Online: 29 August 2019