Atsushi Tamii

TL;DR: The extracted E1 polarizability leads to a neutron skin thickness close to that of a neutron star, thereby constraining the symmetry energy and its density dependence relevant to the description of neutron stars.

TL;DR: In this paper, precise measurements of deuteron vector and tensor analyzing powers were performed via elastic scattering at three incoming deuterons energies of 140, 200, and 270 MeV at the same angles.

TL;DR: A high-resolution magnetic spectrometer called "Grand Raiden" is operated at the RCNP ring cyclotron facility in Osaka for nuclear physics studies at intermediate energies as discussed by the authors. But it is not suitable for high-dimensional data.

TL;DR: The experimental results are in good agreement with ab initio calculations based on chiral effective field theory interactions and with state-of-the-art density-functional calculations, implying a neutron skin in ^{48}Ca of 0.14-0.20 fm.

TL;DR: In this article, the authors measured the angular distribution of the cross section, the proton analyzing power, and all proton polarization transfer coefficients at 250 MeV, compared with theoretical predictions based on exact solutions of the three nucleon Faddeev equations and modern realistic nucleon-nucleon potentials combined with three-Nucleon forces (3NF), namely, the Tucson-Melbourne (TM) $2.