Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions
A. R. Counsell🇬🇧 · F. Gittins🇳🇱 · N. Andersson🇬🇧 · I. Tews🇺🇸
Apr 9, 2025#9↳ gr-qcPRL30 citations
Author
Tews, Ingo
INSPIRE profile1227844ORCID0000-0003-2656-6355
7 papers·7,873 citations in this corpus
Emulators for Scarce and Noisy Data: Application to Auxiliary-Field Diffusion Monte Carlo for Neutron Matter
Cassandra L. Armstrong · Pablo Giuliani · Kyle Godbey · Rahul Somasundaram · Ingo Tews
Feb 7, 2025#1nucl-thPRL27 citations
Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of Pb with Minimal Modeling Assumptions
Reed Essick · Ingo Tews · Philippe Landry · Achim Schwenk
Feb 22, 2021#3nucl-thPRL225 citations
Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii
Mohammad Al-Mamun · Andrew W. Steiner · Joonas Nättilä · Jacob Lange · Richard O'Shaughnessy · Ingo Tews · Stefano Gandolfi · Craig Heinke · Sophia Han
Sep 1, 2020#11↳ astro-ph.HEPRL111 citations
Chiral Three-Nucleon Interactions in Light Nuclei, Neutron- Scattering, and Neutron Matter
J. E. Lynn · I. Tews · J. Carlson · S. Gandolfi · A. Gezerlis · K. E. Schmidt · A. Schwenk
Sep 14, 2015#5nucl-thPRL323 citations
Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions
A. Gezerlis🇩🇪 · I. Tews🇩🇪 · E. Epelbaum🇩🇪 · S. Gandolfi🇺🇸 · K. Hebeler🇺🇸 · A. Nogga🇩🇪 · A. Schwenk🇩🇪
Mar 27, 2013#1*nucl-thPRL350 citations
Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
I. Tews🇩🇪 · T. Krueger🇩🇪 · K. Hebeler🇺🇸 · A. Schwenk🇩🇪
Jun 4, 2012#1*nucl-thPRL454 citations
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