A Role for Bose-Einstein Condensation in Astrophysics

dc.contributor.author	Ninham, Barry W.
dc.contributor.author	Brevik, Iver Håkon
dc.contributor.author	Malyi, Oleksandr I.
dc.contributor.author	Boström, Mathias
dc.date.accessioned	2024-01-15T15:52:30Z
dc.date.available	2024-01-15T15:52:30Z
dc.date.created	2023-06-27T14:30:34Z
dc.date.issued	2023
dc.identifier.citation	Substantia. 2023, 7 (2), 35-39.	en_US
dc.identifier.issn	2532-3997
dc.identifier.uri	https://hdl.handle.net/11250/3111604
dc.description.abstract	We revive a 60-year-old idea that might explain a remarkable new observation of a periodic low-frequency radio emission from a source at galactic distances (GLEAM-X J162759.5-523504.3). It derives from the observation that a high-density high-temperature charged boson plasma is a superconducting superfluid with a Meissner effect.	en_US
dc.language.iso	eng	en_US
dc.publisher	© 2023 Firenze University Press	en_US
dc.rights	Navngivelse 4.0 Internasjonal	*
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/deed.no	*
dc.title	A Role for Bose-Einstein Condensation in Astrophysics	en_US
dc.title.alternative	A Role for Bose-Einstein Condensation in Astrophysics	en_US
dc.type	Peer reviewed	en_US
dc.type	Journal article	en_US
dc.description.version	publishedVersion	en_US
dc.source.pagenumber	35-39	en_US
dc.source.volume	7	en_US
dc.source.journal	Substantia	en_US
dc.source.issue	2	en_US
dc.identifier.doi	10.36253/Substantia-2091
dc.identifier.cristin	2158751
cristin.ispublished	true
cristin.fulltext	original
cristin.qualitycode	1

Except where otherwise noted, this item's license is described as Navngivelse 4.0 Internasjonal