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NSR database version of April 27, 2024.

Search: Author = Y.Y.Zhang

Found 4 matches.

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2021CA31      Phys.Rev. C 104, 065502 (2021)

M.Cadeddu, N.Cargioli, F.Dordei, C.Giunti, Y.F.Li, E.Picciau, C.A.Ternes, Y.Y.Zhang

New insights into nuclear physics and weak mixing angle using electroweak probes

NUCLEAR REACTIONS ¹³³Cs, ¹²⁷I(ν, ν), E=2-100 MeV; analyzed coherent elastic neutrino-nucleus scattering data in cesium-iodide crystal from the COHERENT experiment, and from atomic parity violation (APV) experiment. ¹³³Cs, ¹²⁷I; deduced most precise neutron rms radii, and the neutron skin values, independent low-energy weak mixing angle with uncertainty and compared with standard model prediction. ¹²⁷I, ¹³³Cs, ²⁰⁸Pb; calculated rms proton and neutron point and physical radii and the neutron skins using nonrelativistic Skyrme-Hartree-Fock (SHF) and relativistic mean-field (RMF) nuclear models, point neutron skin predictions for ²⁰⁸Pb and ¹³³Cs according to different models and comparisons with data from PREX-I, PREX-II, and COHERENT+APV experiments.

doi: 10.1103/PhysRevC.104.065502
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2021ZH04      Nucl.Phys. A1005, 122003 (2021)

Y.-Y.Zhang, G.-Y.Qin, X.-N.Wang

Parton Energy Loss in the Generalized High-Twist Approach

doi: 10.1016/j.nuclphysa.2020.122003
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2018CA04      Phys.Rev.Lett. 120, 072501 (2018)

M.Cadeddu, C.Giunti, Y.F.Li, Y.Y.Zhang

Average CsI Neutron Density Distribution from COHERENT Data

NUCLEAR REACTIONS ¹³³Cs, ¹²⁷I(ν, X), E ∼ 10 KeV; analyzed available data; calculated average neutron rms radius of ¹³³Cs and ¹²⁷I using the symmetrized Fermi and Helm form factors.

doi: 10.1103/PhysRevLett.120.072501
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2018CA29      Phys.Rev. D 98, 113010 (2018), Erratum Phys.Rev. D 101, 059902 (2020)

M.Cadeddu, C.Giunti, K.A.Kouzakov, Y.F.Li, A.I.Studenikin, Y.Y.Zhang

Neutrino charge radii from COHERENT elastic neutrino-nucleus scattering

NUCLEAR REACTIONS ¹³³Cs, ¹²⁷I(ν, ν), E<50 MeV; analyzed available data; calculated coherent elastic neutrino-nucleus scattering; deduced boundson the neutrino charge and transition radii.

doi: 10.1103/PhysRevD.98.113010
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