NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.Yin Found 19 matches. 2023YI03 Eur.Phys.J. A 59, 163 (2023) P.-L.Yin, C.Chen, C.S.Fischer, C.D.Roberts D-Baryon axialvector and pseudoscalar form factors, and associated PCAC relations
doi: 10.1140/epja/s10050-023-01066-9
2023YI06 Phys.Rev. C 108, 034002 (2023) P.Yin, X.L.Shang, J.N.Hu, J.Y.Fu, E.Epelbaum, W.Zuo Pairing properties of semilocal coordinate- and momentum-space regularized chiral interactions
doi: 10.1103/PhysRevC.108.034002
2022CH55 Phys.Rev. C 106, 064312 (2022) J.Chen, B.P.Kay, T.L.Tang, I.A.Tolstukhin, C.R.Hoffman, H.Li, P.Yin, X.Zhao, P.Maris, J.P.Vary, G.Li, J.L.Lou, M.L.Avila, Y.Ayyad, S.Bennett, D.Bazin, J.A.Clark, S.J.Freeman, H.Jayatissa, C.Muller-Gatermann, A.Munoz-Ramos, D.Santiago-Gonzalez, D.K.Sharp, A.H.Wuosmaa, C.X.Yuan Probing the quadrupole transition strength of 15C via deuteron inelastic scattering NUCLEAR REACTIONS 1H(15C, p), 2H(15C, d);E=7.1 MeV/nucleon; measured reaction products, Ep, Ip, deuteron spectrum; deduced elastic and inelastic scattering σ(θ). 15C; deduced B(E2), proton quadrupole matrix element, ratio of neutron and proton matrix elements, proton deformation length, core polarization parameters, neutron effective charge; calculated levels, J, π, B(E2), magnetic dipole moments. Comparison to data on 17O and other C isotopes. Ab initio no-core configuration interaction (NCCI) calculations with Daejeon16 interaction. HELIOS spectrometer at ATLAS in-flight facility (Argonne National Laboratory).
doi: 10.1103/PhysRevC.106.064312
2022DU14 Phys.Rev. C 106, 054608 (2022) W.Du, S.Pal, M.Sharaf, P.Yin, S.Sarker, A.M.Shirokov, J.P.Vary Calculations of the np → dγ reaction in chiral effective field theory NUCLEAR REACTIONS 1H(n, dγ), E(cm)=0.000000012625, 0.0000005, 0.0005, 0.005, 0.001, 0.01 MeV; calculated scattering phase shift, σ(E) via the M1 reaction channel. Chiral effective field theory calculations employing the LENPIC (Low Energy Nuclear Physics International Collaboration) nucleon-nucleon interaction up to the fifth order (N4LO). Bayesian analysis for the error estimation. Comparison to available experimental results and other theoretical predictions. Bayaesian analysis for the error estimation.
doi: 10.1103/PhysRevC.106.054608
2022YI05 J.Phys.(London) G49, 125102 (2022) P.Yin, W.Du, W.Zuo, X.Zhao, J.P.Vary Sub Coulomb barrier d+208Pb scattering in the time-dependent basis function approach NUCLEAR REACTIONS 208Pb(d, d), E=3-7 MeV; calculated σ using the non-perturbative time-dependent basis function (tBF) approach; deduced the higher-order inelastic scattering effects are noticeable for sub barrier scatterings with the tBF method.
doi: 10.1088/1361-6471/ac79c3
2021SH15 Phys.Rev. C 103, 034316 (2021) X.-L.Shang, J.-M.Dong, W.Zuo, P.Yin, U.Lombardo Exact solution of the Brueckner-Bethe-Goldstone equation with three-body forces in nuclear matter
doi: 10.1103/PhysRevC.103.034316
2018DU05 Phys.Rev. C 97, 064620 (2018) W.Du, P.Yin, Y.Li, G.Chen, W.Zuo, X.Zhao, J.P.Vary Coulomb excitation of the deuteron in peripheral collisions with a heavy ion NUCLEAR REACTIONS U(d, d'), E=4.7, 19.4, 85.5 MeV/nucleon; calculated low and intermediate energy Coulomb excitations of uranium, internal charge distributions of 2H target before, during and after scattering, rms charge radii, rms momentum and rms orbital angular momentum, intrinsic energy of 2H during scattering using ab-initio nonperturbative, time-dependent basis function (tBF) method with JISP16 nucleon-nucleon interaction. Discussed excitation mechanism and dynamics.
doi: 10.1103/PhysRevC.97.064620
2018NA04 Phys.Rev. C 97, 024909 (2018) J.L.Nagle, R.Belmont, K.Hill, J.Orjuela Koop, D.V.Perepelitsa, P.Yin, Z.-W.Lin, D.McGlinchey Minimal conditions for collectivity in e+e- p+p collisions
doi: 10.1103/PhysRevC.97.024909
2018WA23 J.Phys.(London) G45, 105102 (2018) Proton spectral functions in finite nuclei based on the extended Brueckner-Hartree-Fock approach NUCLEAR STRUCTURE 12C, 27Al, 56Fe, 197Au; calculated radial density and asymmetry distributions, proton spectral function as a function of missing energy.
doi: 10.1088/1361-6471/aad8f5
2018YI05 Chin.Phys.C 42, 114102 (2018) Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach
doi: 10.1088/1674-1137/41/11/114102
2017MA48 Phys.Rev. C 96, 024302 (2017) N.N.Ma, H.F.Zhang, P.Yin, X.Ju.Bao, H.F.Zhang Weizsacker-Skyrme-type nuclear mass formula incorporating two combinatorial radial basis function prescriptions and their application NUCLEAR STRUCTURE Z=10-118, N=10-180; calculated binding energies, odd-even staggering (OES) of nuclear binding energies, S(n), S(2n), S(p), S(2p), Q(α), Q(β-), Q(β+), Q(EC) of 2267 nuclei using WS-LZ, WS-LZ1, and WS-LZ2 mass formulas, and compared with experimental values. Z=8, A=26-28; Z=9, A=27-31; Z=10, A=30-34; Z=11, A=33-37; Z=12, A=35-40; Z=13, A=21, 22, 38-43; Z=14, A=22, 23, 40-45; Z=15, A=24-26, 42-47; Z=16, A=26-28, 45-49; Z=17, A=28-30, 44, 46-51; Z=18, A=30, 31, 48-53; Z=19, A=32-34, 52-56; Z=20, A=34, 35, 53-58; Z=21, A=36-38, 53-61; Z=22, A=38-40, 55, 57-63; Z=23, A=40-42, 44, 56, 57, 59-66; Z=24, A=42-44, 58-60, 63-68; Z=25, A=44-46, 48, 62, 67-71; Z=26, A=45-48, 67-74; Z=27, A=47-49, 52, 69-76; Z=28, A=48-52, 74-79; Z=29, A=52-56, 77-82; Z=30, A=54-57, 82-85; Z=31, A=56-60, 84-87; Z=32, A=58-62, 86-90; Z=33, A=60-64, 88-92; Z=34, A=64-66, 90-95; Z=35, A=67, 68, 93-98; Z=36, A=69, 70, 98-101; Z=37, A=71-73, 100-103; Z=38, A=73-75, 103-107; Z=39, A=76-79, 104-109; Z=40, A=78-82, 106-112; Z=41, A=81-84, 109-115; Z=42, A=83, 84, 112-117; Z=43, A=85, 86, 114-120; Z=44, A=87-89, 117-124; Z=45, A=89-91, 120-126; Z=46, A=91-93, 123-128; Z=47, A=93-95, 124-130; Z=48, A=95-97, 129-133; Z=49, A=97-101, 128, 133-135; Z=50, A=99-101, 136-138; Z=51, A=103, 137-140; Z=52, A=105, 141-143; Z=53, A=107, 114, 140-145; Z=54, A=109, 147, 148; Z=55, A=115, 116, 148-152; Z=56, A=115-120, 149-153; Z=57, A=116-123, 149-155; Z=58, A=119-125, 152-157; Z=59, A=121-127, 154, 156-159; Z=60, A=124-129, 156, 158-161; Z=61, A=126-132, 160-163; Z=62, A=128-135, 162-165; Z=63, A=130-137, 164-167; Z=64, A=133-139, 143, 164-169; Z=65, A=135-140, 142, 165, 167-171; Z=66, A=138-142, 169-173; Z=67, A=140-143, 171-175; Z=68, A=142-145, 173-177; Z=69, A=144-146, 149, 150, 177-179; Z=70, A=148-153, 179-181; Z=71, A=150-154, 181-185; Z=72, A=153-157, 187-189; Z=73, A=155-158, 178, 189-192; Z=74, A=157-161, 192-194; Z=75, A=159-162, 167, 194-198; Z=76, A=161-165, 197-202; Z=77, A=164-166, 170, 198, 200-204; Z=78, A=166-169, 203-206; Z=79, A=169, 170, 174, 204-210; Z=80, A=171-173, 209-216; Z=81, A=178, 190, 212, 214-218; Z=82, A=215-220; Z=83, A=185, 194, 219-224; Z=84, A=223-227; Z=85, A=198, 225-229; Z=86, A=230, 231; Z=87, A=202, 232, 233; Z=88, A=201, 235; Z=89, A=206, 237; Z=90, A=238, 239; Z=91, A=220, 222, 239-241; Z=92, A=217, 220-222, 241-243; Z=93, A=219-224, 226, 232, 242-245; Z=94, A=247; Z=95, A=230-234, 236, 237, 246-249; Z=96, A=232, 235, 252; Z=97, A=234-242, 248, 252-254; Z=98, A=238, 239, 241, 243, 255, 256; Z=99, A=239-246, 248-250, 256-258; Z=100, A=241-245, 247, 258-260; Z=101, A=245-250, 252-254, 256, 259-262; Z=102, A=248-251, 258-264; Z=103, A=251-254, 257-266; Z=104, A=253-255, 259, 260, 262-268; Z=105, A=255-258, 260-270; Z=106, A=258, 259, 263-273; Z=107, A=260-275; Z=108, A=263, 267-273; Z=109, A=265-279; Z=110, A=267, 268, 271-281; Z=111, A=272-283; Z=112, A=276-285; Z=113, A=278-287; Z=114, A=285-289; Z=115, A=287-291; Z=116, A=289-293; Z=117, A=291-294; Z=118, A=293-295; calculated binding energies, Q(α), Q(β-), Q(β+), Q(EC) based on the WS-LZ2 mass formula for 988 nuclei. Weizsacker-Skyrme (WS)-type nuclear mass formulas.
doi: 10.1103/PhysRevC.96.024302
2017YI01 Nucl.Phys. A961, 200 (2017) P.Yin, X.Fan, J.Dong, W.Guo, W.Zuo Model-dependence of neutrino emissivities and neutrino luminosities of neutron stars from the direct Urca processes and the modified Urca processes
doi: 10.1016/j.nuclphysa.2017.03.001
2017YI06 Chin.Phys.C 41, 114102 (2017) Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach
doi: 10.1088/1674-1137/41/11/114102
2016OR04 Phys.Rev. C 93, 044910 (2016) J.D.Orjuela Koop, R.Belmont, P.Yin, J.L.Nagle Exploring the beam-energy dependence of flow-like signatures in small-system d+Au collisions
doi: 10.1103/PhysRevC.93.044910
2013WA03 Phys.Rev. C 87, 014328 (2013) P.Wang, S.-X.Gan, P.Yin, W.Zuo Three-body force effect on off-shell mass operator and spectral functions in nuclear matter
doi: 10.1103/PhysRevC.87.014328
2013YI01 Phys.Rev. C 87, 014314 (2013) Three-body force effect on nucleon momentum distributions in asymmetric nuclear matter within the framework of the extended Brueckner-Hartree-Fock approach
doi: 10.1103/PhysRevC.87.014314
2013YI04 Phys.Rev. C 88, 015804 (2013) Three-body force effect on neutrino emissivities of neutron stars within the framework of the Brueckner-Hartree-Fock approach
doi: 10.1103/PhysRevC.88.015804
2011ZH07 Phys.Rev. C 83, 035801 (2011) D.-R.Zhang, P.-L.Yin, W.Wang, Q.-C.Wang, W.-Z.Jiang Effects of a weakly interacting light U boson on the nuclear equation of state and properties of neutron stars in relativistic models
doi: 10.1103/PhysRevC.83.035801
1984WA08 Phys.Lett. 140B, 249 (1984) Boosted Bag and Nucleon EM Form Factors NUCLEAR STRUCTURE 1H; calculated electromagnetic form factor. Cloudy bag model, Lorentz-boost rule.
doi: 10.1016/0370-2693(84)90929-8
Back to query form Note: The following list of authors and aliases matches the search parameter P.Yin: , P.C.YIN, P.L.YIN |