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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Constraints on neutron star radii based on chiral effective field theory interactions
K Hebeler1, J M Lattimer, C J Pethick
1TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, V6T 2A3, Canada.
Abstract:
We show that microscopic calculations based on chiral effective field theory interactions constrain the properties of neutron-rich matter below nuclear densities to a much higher degree than is reflected in commonly used equations of state. Combined with observed neutron star masses, our results lead to a radius R=9.7-13.9 km for a 1.4M⊙ star, where the theoretical range is due, in about equal amounts, to uncertainties in many-body forces and to the extrapolation to high densities.
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