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Bose-Einstein condensates in neutron stars
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA.
2017 (English)In: Universal Themes of Bose-Einstein Condensation, Cambridge University Press , 2017, p. 573-592Chapter in book (Other academic)
Abstract [en]

In the two decades since the appearance of the book Bose-Einstein Condensation in 1995, there have been a number of developments in our understanding of dense matter. After a brief overview of neutron star structure and the Bose-Einstein condensed phases that have been proposed, we describe selected topics, including neutron and proton pairing gaps; the physics of the inner crust of neutron stars, where a neutron fluid penetrates a lattice of nuclei, meson condensates; and pairing in dense quark matter. Especial emphasis is placed on basic physical effects and on connections to the physics of cold atomic gases. 

Place, publisher, year, edition, pages
Cambridge University Press , 2017. p. 573-592
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-236783DOI: 10.1017/9781316084366.031Scopus ID: 2-s2.0-85045837995ISBN: 9781316084366 (print)ISBN: 9781107085695 (print)OAI: oai:DiVA.org:kth-236783DiVA, id: diva2:1277058
Note

QC 20190109

Available from: 2019-01-09 Created: 2019-01-09 Last updated: 2019-01-09Bibliographically approved

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