414 citations · 5.3k across the 60 of their papers we have counts for
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Investigating Signatures of Phase Transitions in Neutron-Star Cores
Rahul Somasundaram, Ingo Tews, Jérôme Margueron
Neutron stars explore matter at the highest densities in the universe such that their inner cores might undergo a phase transition from hadronic to exotic phases, e.g., quark matte…
Quantifying modeling uncertainties when combining multiple gravitational-wave detections from binary neutron star sources
Nina Kunert, Peter T. H. Pang, Ingo Tews +2
With the increasing sensitivity of gravitational-wave detectors, we expect to observe multiple binary neutron-star systems through gravitational waves in the near future. The combi…
Chiral Effective Field Theory's Impact on Advancing Quantum Monte Carlo Methods
I. Tews, D. Lonardoni, S. Gandolfi
Thirty years ago, Steven Weinberg published his seminal paper on "Nuclear Forces from chiral Lagrangians" which has revolutionized the field of theoretical nuclear physics. Nowaday…
Modeling Neutron Star Oscillations in a Fixed General Relativistic Background Including Solid Crust Dynamics
Bing-Jyun Tsao, Irina Sagert, Oleg Korobkin +4
Measurements of the gravitational-wave signals from neutron star mergers allow scientists to learn about the interior of neutron stars and the properties of dense nuclear matter. T…
Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions
S. Huth, P. T. H. Pang, I. Tews +8
Interpreting high-energy, astrophysical phenomena, such as supernova explosions or neutron-star collisions, requires a robust understanding of matter at supranuclear densities. How…
A Detailed Examination of Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of Pb with Minimal Modeling Assumptions
Reed Essick, Philippe Landry, Achim Schwenk +1
The symmetry energy and its density dependence are pivotal for many nuclear physics and astrophysics applications, as they determine properties ranging from the neutron-skin thickn…
Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement
Peter T. H. Pang, Ingo Tews, Michael W. Coughlin +3
In the past few years, new observations of neutron stars and neutron-star mergers have provided a wealth of data that allow one to constrain the equation of state of nuclear matter…
Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of Pb with Minimal Modeling Assumptions
Reed Essick, Ingo Tews, Philippe Landry +1
The symmetry energy and its density dependence are crucial inputs for many nuclear physics and astrophysics applications, as they determine properties ranging from the neutron-skin…