Author: sylvia
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research-publ
How Well Do We Know the Neutron-Matter Equation of State at the Densities Inside Neutron Stars? A Bayesian Approach with Correlated Uncertainties
We introduce a new framework for quantifying correlated uncertainties of the infinite-matter equation of state derived from chiral effective field theory (χEFT). Bayesian machine learning via Gaussian processes with physics-based […]
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research-publ
Quantifying uncertainties and correlations in the nuclear-matter equation of state
We perform statistically rigorous uncertainty quantification (UQ) for chiral effective field theory (χEFT) applied to infinite nuclear matter up to twice nuclear saturation density. The equation of state (EOS) is […]
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research-publ
Gravitational wave signatures from the phase-transition-induced collapse of a magnetized neutron star
Strong magnetic fields make neutron stars potential sources of detectable electromagnetic and gravitational-wave signals. Hence, inferring these magnetic fields is critical to understand the emissions of neutron stars. However, due […]