Neutron stars and the high density equation of state
2009 (English)In: AIP Conference Proceedings: BULK NUCLEAR PROPERTIES: 5th ANL/MSU/JINA/INT FRIB Workshop, American Institute of Physics (AIP), 2009, Vol. 1128, 175-185 p.Conference paper (Other academic)
One of the key ingredients to understand the properties of neutrons stars1 (NS) is the equation of state at finite densities far beyond nuclear saturation. Investigating the phase structure of quark matter that might be realized in the core of NS inspires theory and observation. We discuss recent results of our work to point out our view on challenges and possibilities in this evolving field by means of a few examples.
Place, publisher, year, edition, pages
American Institute of Physics (AIP), 2009. Vol. 1128, 175-185 p.
IdentifiersURN: urn:nbn:se:ltu:diva-35668DOI: 10.1063/1.3146212Local ID: a4cbde00-e8f1-11de-bae5-000ea68e967bISBN: 978-0-7354-0664-3 (print)OAI: oai:DiVA.org:ltu-35668DiVA: diva2:1008921
ANL/MSU/JINA/INT FRIB Workshop : Bulk Nuclear Properties 19/11/2008 - 22/11/2008
Upprättat; 2009; 20091214 (fresan)2016-09-302016-09-30