Determining the Equation of State of Cold, Dense Matter with X-ray Observations of Neutron Stars
by Slavko Bogdanov, Anna L. Watts, Deepto Chakrabarty, Zaven Arzoumanian, Sebastien Guillot, Keith C. Gendreau, Frederick K. Lamb, Thomas Maccarone, M. Coleman Miller, Feryal Ozel, Paul S. Ray, and Colleen A. Wilson-Hodge
Published onMay 31, 2019
Determining the Equation of State of Cold, Dense Matter with X-ray Observations of Neutron Stars
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Abstract
X-ray observations from multiple next-generation X-ray telescopes proposed for deployment in the 2020s and beyond, using several complementary techniques that require different combinations of high time resolution, superb spectral resolution, and high spatial resolution can provide definitive constraints on the state of cold, ultra-dense matter.
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