Presently under construction in Lund, Sweden, the European Spallation Source (ESS) will
be the world's brightest neutron source. As such, it has the potential for a particle physics …

We review standard and non-standard neutrino physics probes that are based on nuclear
measurements. We pay special attention on the discussion of prospects to extract new …

Based on the covariant density functional theory, the magnetic dipole (M 1) resonance is
described in the framework of relativistic random-phase approximation with density …

When the next galactic core-collapse supernova occurs, we must be ready to obtain as
much information as possible. Although many present and future detectors are well …

Magnetic dipole (M1) excitations of magic nuclei Ca 48, Zr 90, and Sn 132 are investigated
by a self-consistent Hartree-Fock (HF) plus subtracted second random-phase approximation …

Neutrinos carry most of the energy released by a core-collapse supernova. SNOLAB has
two neutrino-capable detectors, SNO+ and HALO, that have complementary neutrino flavour …

We calculate the response of a lead-based detector, such as the Helium and Lead
Observatory (HALO) or its planned upgrade HALO-1kt to a Galactic core-collapse …

A large number of the presently running neutrino and dark-matter experiments use thallium-
doped cesium-iodide CsI [Tl] crystals, sodium-doped cesium-iodide CsI [Na] crystals, or …

We report the present status of the feasible constraints from nuclear physics on the
ambiguity in the neutrino reactions applied to the astrophysics. With the advance of the multi …

Core-collapse supernovae (CCSNe) are amongst the most rare and energetic events in the
galaxy. In the Milky Way, they are predicted to happen as infrequently as 1.64±0.46 times …