activity
20222026
most citedThe nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions

5 citations · 9 across the 8 of their papers we have counts for

collaborators

9 papers

nucl-th2026

Extending multi-messenger constraints on neutron star matter through the inclusion of direct Urca cooling

M. Dio Danarianto, Guilherme Grams, Thibeau Wouters +1

The properties and behavior of strongly interacting matter at extreme densities can not only be determined through terrestrial experiments or through theoretical considerations, bu…

astro-ph.HE2026

Unified study of nuclear physics and dark matter constraints through gravitational-wave observations of binary neutron star mergers

Nina Kunert, Guilherme Grams, William Newton +5

Understanding the properties of strongly interacting matter at extreme densities is a central problem in fundamental physics, with neutron star mergers offering a natural laborator…

gr-qc2026

Investigating the impact of quasi-universal relations on neutron star constraints in third-generation detectors

Natalie Williams, Anna Puecher, Guilherme Grams +2

Gravitational-wave observations of binary neutron star systems can shed light on the currently unknown dense matter equation of state. The equation of state determines a large numb…

nucl-th2025★ 5 cited

The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions

Jérôme Margueron, Christian Drischler, Mariana Dutra +10

Systematic comparisons across theoretical predictions for the properties of dense matter, nuclear physics data, and astrophysical observations (also called meta-analyses) are perfo…

nucl-th2025★ 4 cited

Neutron Star Inner Crust at Finite Temperatures: A Comparison Between Compressible Liquid Drop and Extended Thomas-Fermi Approaches

Guilherme Grams, Nikolai N. Shchechilin, Théau Diverrès +3

We investigate the effects of temperature on the properties of the inner crust of a non-accreting neutron star. To this aim, we employ two different treatments: the compressible li…

nucl-ex2025

Fingerprints of triaxiality in the charge radii of neutron-rich Ruthenium

Bernhard Maass, Wouter Ryssens, Michael Bender +19

We present the first measurements with a new collinear laser spectroscopy setup at the Argonne Tandem Linac Accelerator System utilizing its unique capability to deliver neutron-ri…

nucl-th2024

Gravitational wave asteroseismology of neutron stars with unified EOS: on the role of high-order nuclear empirical parameters

Guilherme Grams, César V. Flores, César H. Lenzi

We analyze the sensitivity of non-radial fluid oscillation modes and tidal deformations in neutron stars to high-order nuclear empirical parameters (NEP). In particular, we study t…

nucl-th2024

Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: IV. Improved description of the isospin dependence of pairing

Guilherme Grams, Nikolai N. Shchechilin, Adrian Sanchez-Fernandez +3

Providing reliable data on the properties of atomic nuclei and infinite nuclear matter to astrophysical applications remains extremely challenging, especially when treating both pr…

nucl-th2022

Neutron star crust properties: comparison between the compressible liquid-drop model and the extended Thomas-Fermi approach

Guilherme Grams, Jerome Margueron, Rahul Somasundaram +2

We present a detailed analysis of three models predicting the properties of non-uniform matter in the crust of neutron stars: the compressible liquid-drop model, the fourth order E…