id:"swepub:oai:DiVA.org:ltu-35668"
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- Klähn, ThomasArgonne National Laboratory, Argonne, IL (author)
Neutron stars and the high density equation of state
- Article/chapterEnglish2009
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- American Institute of Physics (AIP),2009
- printrdacarrier
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- LIBRIS-ID:oai:DiVA.org:ltu-35668
- https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-35668URI
- https://doi.org/10.1063/1.3146212DOI
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- Language:English
- Summary in:English
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- Upprättat; 2009; 20091214 (fresan)
- 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.
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- Roberts, CraigArgonne National Laboratory, Argonne, IL (author)
- Blaschke, DavidUniversity of Wroclaw (author)
- Sandin, Fredrik (author)
- Argonne National Laboratory, Argonne, ILUniversity of Wroclaw (creator_code:org_t)
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- In:AIP Conference Proceedings: American Institute of Physics (AIP), s. 175-1859780735406643
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