Lower BNS merger rates from GWTC-4 data produce tensions of factors 3.6-18 with SGRB rates, 0.9-4.1 with r-process rates, and 2.3-5.1 with Galactic DNS rates.
Coello-P´ erez EA (2026), Low-energy collective excitations in atomic nuclei, Encyclopedia of Nuclear Physics, Elsevier
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The universality assumption in the Koonin-Pratt formula for femtoscopic correlations introduces potentially large intrinsic uncertainty when extracting strong interactions between hadrons like nucleons.
A review of random phase approximation, Lorentz integral transform coupled-cluster, projected generator-coordinate, and self-consistent Green's functions methods for nuclear giant resonances, with benchmark comparisons on 16O and 40Ca.
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Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
Lower BNS merger rates from GWTC-4 data produce tensions of factors 3.6-18 with SGRB rates, 0.9-4.1 with r-process rates, and 2.3-5.1 with Galactic DNS rates.
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Can the strong interactions between hadrons be determined using femtoscopy?
The universality assumption in the Koonin-Pratt formula for femtoscopic correlations introduces potentially large intrinsic uncertainty when extracting strong interactions between hadrons like nucleons.
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Nuclear giant resonances from first principles
A review of random phase approximation, Lorentz integral transform coupled-cluster, projected generator-coordinate, and self-consistent Green's functions methods for nuclear giant resonances, with benchmark comparisons on 16O and 40Ca.