26 citations · 57 across the 4 of their papers we have counts for
4 papers
Representing Equations of State With Strong First-Order Phase Transitions
Lee Lindblom, Steve M. Lewis, Fridolin Weber
Parametric representations of the high-density nuclear equation of state are used in constructing models for interpreting the astrophysical observations of neutron stars. This stud…
Neural Simulation-Based Inference of the Neutron Star Equation of State directly from Telescope Spectra
Len Brandes, Chirag Modi, Aishik Ghosh +6
Neutron stars provide a unique opportunity to study strongly interacting matter under extreme density conditions. The intricacies of matter inside neutron stars and their equation…
Deducing Neutron Star Equation of State Parameters Directly From Telescope Spectra with Uncertainty-Aware Machine Learning
Delaney Farrell, Pierre Baldi, Jordan Ott +6
Neutron stars provide a unique laboratory for studying matter at extreme pressures and densities. While there is no direct way to explore their interior structure, X-rays emitted f…
Neutron Star Pulsations and Instabilities
Lee Lindblom
Gravitational radiation (GR) drives an instability in certain modes of rotating stars. This instability is strong enough in the case of the r-modes to cause their amplitudes to gro…