@inproceedings{aa98c7cfb4604540b48a6162c47acc12,
title = "Astrophysical and laboratory constraints for the dense matter equation of state",
abstract = "New measurements of neutron star masses and radii have lead to powerful constraints on the dense matter equation of state. In the vicinity of the nuclear saturation density, the symmetry energy is the least well understood aspect of the nuclear force. Independent constraints from a variety of nuclear experiments are now able to refine the parameters of the symmetry energy.",
keywords = "dense matter, equation of state, neutron stars, nuclear symmetry energy",
author = "Lattimer, \{James M.\}",
year = "2012",
doi = "10.1063/1.4763414",
language = "English",
isbn = "9780735410961",
series = "AIP Conference Proceedings",
pages = "319--326",
booktitle = "Origin of Matter and Evolution of Galaxies 2011",
note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",
}