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NSR database version of May 24, 2024.

Search: Author = P.Yin

Found 18 matches.

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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
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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
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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
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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
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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
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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
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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
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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
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2018WA23      J.Phys.(London) G45, 105102 (2018)

P.Wang, P.Yin, X.Shang, W.Zuo

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
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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
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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
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2017YI06      Chin.Phys.C 41, 114102 (2017)

P.Yin, J.Dong, W.Zuo

Effect of tensor correlations on the depletion of nuclear Fermi sea within the extended BHF approach

doi: 10.1088/1674-1137/41/11/114102
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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
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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
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2013YI01      Phys.Rev. C 87, 014314 (2013)

P.Yin, J.-Y.Li, P.Wang, W.Zuo

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
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2013YI04      Phys.Rev. C 88, 015804 (2013)

P.Yin, W.Zuo

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
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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
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1984WA08      Phys.Lett. 140B, 249 (1984)

X.-H.Wang, P.-C.Yin

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
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Note: The following list of authors and aliases matches the search parameter P.Yin: , P.C.YIN, P.L.YIN