Equation of State of Dense Matter and Consequences for Neutron Stars

There is currently tremendous interest in the role of hyperons and other exotic forms of matter in neutron stars. This is particularly so following the measurement by Demorest et al. of a star with a mass almost 2 solar masses. Given that we know of no physical mechanism to stop the occurrence of h...

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Bibliographic Details
Main Authors: Thomas A. W., Whittenbury D. L., Carroll J. D., Tsushima K., Stone J. R.
Format: Article
Language:English
Published: EDP Sciences 2013-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136303004

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