Stanisław Burzyński

Supersymmetric dark matter

The Confrontation between General Relativity and Experiment

Theory of core-collapse supernovae

Phase-shift analysis ofNNscattering below 160 MeV: Indication for a strong tensor force

Particle dark matter: evidence, candidates and constraints

Probing the early universe: a review of primordial nucleosynthesis beyond the standard big bang

Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments

Nuclear charge-density-distribution parameters from elastic electron scattering

Accurate nucleon-nucleon potential with charge-independence breaking

Energy levels of A = 21–44 nuclei (VII)

Terrestrial in situ cosmogenic nuclides: theory and application

Presupernova Evolution with Improved Rates for Weak Interactions

The evolution and explosion of massive stars

Quasinormal modes of black holes and black branes

Intercalibration of standards, absolute ages and uncertainties in 40Ar/39Ar dating

Elastic magnetic electron scattering from nuclei

Updated nucleosynthesis constraints on unstable relic particles

Accurate determination of the 17O16O + n coupling constant and spectroscopic factor

Spin-isospin strength distributions inf-pshell nuclei: A study of theV51(n,p) andCo59(n,p) reactions at 198 MeV

0° polarization transfer inH2(p→,n→)pp at 54 and 71 MeV

The 3H(α, γ)7Li reaction in the energy range from 0.7 to 2.0 Mev

A facility for monoenergetic polarized neutrons of 30–70 MeV

Gamow-Teller strength inNi60,62,64(n,p) reactions at 198 MeV

Neutron-proton spin-correlation parameterAzzat 68 MeV