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NSR database version of April 11, 2024.

Search: Author = Y.Xu

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2024WA02      Phys.Rev. C 109, 014611 (2024)

B.Wang, Y.Xu, S.Goriely

Systematic study of the radiative proton capture including the compound, pre-equilibrium, and direct mechanisms

doi: 10.1103/PhysRevC.109.014611
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2024WA03      Phys.Rev. C 109, 014621 (2024)

Y.H.Wang, D.Y.Pang, W.D.Chen, Y.P.Xu, W.L.Hai, R.Y.Chen

Nuclear radii from total reaction cross section measurements at intermediate energies with complex turning point corrections to the eikonal model

doi: 10.1103/PhysRevC.109.014621
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2024XU04      Chin.Phys.C 48, 024106 (2024)

Y.-L.Xu, X.-W.Su, Zh.-H.Sun, Y.-L.Han, X.-J.Sun, D.-H.Zhang, Ch.-H.Cai

Description of elastic scattering for 7Li-induced reactions on 1p-shell nuclei

NUCLEAR REACTIONS 9Be, 10,11B, 12,13C, 15N, 16O(7Li, 7Li), E=4.5-131.8 MeV; analyzed available data; deduced σ(θ), the global phenomenological optical potentials (GPOPs), the contribution of elastic transfer by the distorted wave Born approximation (DWBA) method.

doi: 10.1088/1674-1137/ad1924
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2024ZO01      J.Phys.(London) G51, 045103 (2024)

Y.-T.Zou, J.-H.Cheng, Y.-Y.Xu, Q.Xiao, S.-M.Liu, F.-Q.Shao, T.-P.Yu

Laser-assisted two-proton radioactivity

RADIOACTIVITY 6Be, 12O, 16Ne, 19Mg, 45Fe, 48Ni, 54Zn, 67Kr(2p); calculated the two-proton radioactivity assisted by an ultra-intense laser field within a deformed one-parameter model (OPM); deduced the lasers characterized by shorter wavelengths and higher intensities exert a more significant influence on the rate of the average change in pulse duration, T1/2.

doi: 10.1088/1361-6471/ad2691
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2023JA13      Astrophys.J. 955, 51 (2023)

R.Jain, E.F.Brown, H.Schatz, A.V.Afanasjev, M.Beard, L.R.Gasques, S.S.Gupta, G.W.Hitt, W.R.Hix, R.Lau, P.Moller, W.J.Ong, M.Wiescher, Y.Xu

Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts

NUCLEAR REACTIONS 40Mg(40Mg, X)80Cr, 44Mg(40Mg, X)84Cr, 44Mg(44Mg, X)88Cr, 44Mg(38Ne, X)82Ti, 40Mg(38Ne, X)78Ti, 32Ne(32Ne, X)64Ca, 32Ne(30Ne, X)62Ca, 30Ne(30Ne, X)60Ca, 40Mg(24O, X), E not given; calculated abundances, pycnonuclear fusion rates using the reaction network with the thermal evolution code dStar. 56Fe; deduced impact of uncertainties on the depth at which nuclear heat is deposited although the total heating remains constant.

doi: 10.3847/1538-4357/acebc4
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2023LI45      Chin.Phys.C 47, 094103 (2023)

X.Liu, J.-D.Jiang, L.-J.Qi, Y.-Y.Xu, X.-J.Wu, X.-H.Li

Systematic calculations of cluster radioactivity half-lives with a screened electrostatic barrier

RADIOACTIVITY 221Fr, 221,222,223,224Ra, 226Ra, 223Ac(14C), 228Th(20O), 231Pa(23F), 230Th, 231Pa, 232,233,234U(24Ne), 234U, 233U(25Ne), 234U(26Ne), (28Mg), 236,238Pu(28Mg), 238Pu(30Mg), (32Si), 242Cm(34Si); calculated T1/2. Comparison with available data.

doi: 10.1088/1674-1137/ace351
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2023SE09      Phys.Rev. C 107, L061302 (2023)

D.Seweryniak, T.Huang, K.Auranen, A.D.Ayangeakaa, B.B.Back, M.P.Carpenter, P.Chowdhury, R.M.Clark, P.A.Copp, Z.Favier, K.Hauschild, X.-T.He, T.L.Khoo, F.G.Kondev, A.Korichi, T.Lauritsen, J.Li, C.Morse, D.H.Potterveld, G.Savard, S.Stolze, J.Wu, J.Zhang, Y.-F.Xu

Nuclear rotation at the fission limit in 254Rf

NUCLEAR REACTIONS 206Pb(50Ti, 2n)254Rf, E=244 MeV from the ATLAS-ANL facility; measured reaction products, prompt γ rays, Eγ, Iγ, Rf Kα and Kβ x-rays, (254Rf implants)γ-coin, (implants)(fission events)γ-coin using the Gammasphere array and the Argonne gas-filled analyzer (AGFA). 254Rf; deduced levels, J, π, ground-state rotational band up to 14+, kinematic moment of inertia. Systematics of ground-state bands in 250Fm, 252,254No, and 254,256Rf, and comparison with particle-number conserving cranked shell model (PNC-CSM) calculations.

doi: 10.1103/PhysRevC.107.L061302
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2023WA36      Phys.Rev. C 108, 065805 (2023)

B.Wang, Y.Xu, X.Tang

Effective energy window of the E1 photon strength function for astrophysical neutron-capture reaction rates

doi: 10.1103/PhysRevC.108.065805
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2023XI06      J.Phys.(London) G50, 085102 (2023)

Q.Xiao, J.-H.Cheng, B.-L.Wang, Y.-Y.Xu, Y.-T.Zou, T.-P.Yu

Half-lives for proton emission and α decay within the deformed Gamow-like model

RADIOACTIVITY 109I, 112,113Cs, 117La, 121Pr, 131Eu, 135Tb, 140,141Ho, 144,145,146,147Tm, 150,151Lu, 155,156,157Ta, 159,160,161Re, 164,165,166,167Ir, 170,171Au, 176,177Tl, 185Bi, 111Cs, 127Pm, 137Tb(p), 106,108Te, 108,110,112Xe, 114Ba, 144Nd, 146,148Sm, 148,150,152Gd, 150,152,154Dy, 152,154,156Er, 154,156Yb, 156,158,160,162Hf, 174Hf, 158,160,162,164,166,168W, 180W, 162,164,166,168,170,172,174Os, 186Os, 168,170,172,174,176,178,180,182,184,186,188,190Pt, 170,172,174,176,178,180,182,184,186,188Hg, 178,180,182,184,186,188,190,192,194Pb, 210Pb, 186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218Po, 194,196,198,200,202,204,206,208,210,212,214,216,218,220,222Rn, 202,204,206,208,210Ra, 214,216,218,220,222,224,226Ra, 210,212,214,216,218,220,222,224,226,228,230,232Th, 216,218,220,222,224,226,228,230,232,234,236,238U, 228,230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 246,248,250,252,254,256Fm, 252,254,256No, 256,258Rf, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288,290Fl, 290,292Lv, 294Og, 105Te, 109Te, 109Xe, 147Sm, 149,151Gd, 151,153Dy, 153,155Er, 155Yb, 157,159Hf, 161,163W, 167W, 161Os, 167,169,171,173Os, 171,173,175,177,179,181,183,185Pt, 175,177,179,181,183,185Hg, 183,185,187,189Pb, 187,189,191,193,195,197,199,201,203,205,207,209,211,213,215,217,219Po, 193,195,197,199Rn, 203,205,207,209,211,213,215,217,219,221Rn, 201,203,205,207,209,211,213,215,217,219,221,223Ra, 211,213,215,217,219,221,223,225,227Th, 221,223,225,227,229,231,233,235U, 229,231,233,235,237,239,241Pu, 233Cm, 239,241,243,245,247Cm, 237Cf, 245,247,249,251,253Cf, 249,251,253,255,257Fm, 255,257,259No, 257Rf, 261Rf, 261Sg, 265Hs, 109I, 113I, 145Pm, 147Eu, 151Tb, 151,153Ho, 155,157Tm, 155Lu, 157,159Ta, 163,165Re, 167,169,171,173,175,177Ir, 173,175,177,179,181,183,185Au, 177,179,181Tl, 187,189,191,193,195Bi, 193,195,197,199,201,203,205,207,209,211,213,215,217,219,221,223,225,227Ac, 211,213,215,217,219,221,223,225,227,229,231Pa, 219Np, 223,225,227,229,231,233,235,237Np, 229Am, 235Am, 239,241,243Am, 243,245,247,249Bk, 247Es, 251,253Es, 249,251Md, 255,257Md, 253,255Lr, 259Lr, 259Db, 261Bh, 110,112I, 114Cs, 152,154Ho, 154,156Tm, 158Lu, 158Ta, 162Ta, 160,162Re, 168Re, 166,168Ir, 172,174Ir, 170Au, 176Au, 180Tl, 186Bi, 192,194Bi, 212,214Bi, 192At, 200,202,204,206,208,210,212,214,216,218At, 200Fr, 204,206,208,210,212,214,216,218,220Fr, 216,218,220,222,224,226Ac, 212Pa, 224Pa, 228,230Pa, 236Np, 236Am, 244Bk, 248Es, 258Md, 272Rg(α); calculated T1/2 with the deformed Gamow-like model, which introduces the effects of nucleus deformation; deduced the deformed model follows the Geiger-Nuttall law. Comparison with available data.

doi: 10.1088/1361-6471/acdfeb
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2022AL01      J.Phys.(London) G49, 010501 (2022)

M.Aliotta, R.Buompane, M.Couder, A.Couture, R.J.deBoer, A.Formicola, L.Gialanella, J.Glorius, G.Imbriani, M.Junker, C.Langer, A.Lennarz, Y.A.Litvinov, W.-P.Liu, M.Lugaro, C.Matei, Z.Meisel, L.Piersanti, R.Reifarth, D.Robertson, A.Simon, O.Straniero, A.Tumino, M.Wiescher, Y.Xu

The status and future of direct nuclear reaction measurements for stellar burning

NUCLEAR REACTIONS 12C(α, γ), 22Ne(α, n), (α, γ), 12C(12C, X), E(cm)<7 MeV; analyzed available data; deduced σ, S-factors.

doi: 10.1088/1361-6471/ac2b0f
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2022HU21      Phys.Rev. C 106, L061301 (2022)

T.Huang, D.Seweryniak, B.B.Back, P.C.Bender, M.P.Carpenter, P.Chowdhury, R.M.Clark, P.A.Copp, X.-T.He, R.D.Herzberg, D.E.M.Hoff, H.Jayatissa, T.L.Khoo, F.G.Kondev, G.Morgan, C.Morse, A.Korichi, T.Lauritsen, C.Muller-Gatermann, D.H.Potterveld, W.Reviol, A.M.Rogers, S.Saha, G.Savard, K.Sharma, S.Stolze, S.Waniganeththi, G.L.Wilson, J.Wu, Y.-F.Xu, S.Zhu

Discovery of the new isotope 251Lr: Impact of the hexacontetrapole deformation on single-proton orbital energies near the Z=100 deformed shell gap

NUCLEAR REACTIONS 203Tl(50Ti, 2n)251Lr, 205Tl(50Ti, 2n)253Lr, E=237 MeV; measured reaction products, α-decay of the reaction products, Eα, Iα. 251,253Lr; deduced levels J, π, α-decay width. 251,253,255Lr; calculated single-proton levels near the Fermi surface. Calculations with particle-number conserving cranked shell model. Beam delivered to target by ATLAS linear accelerator and recoiling reaction products were separated in the Argonne Gas-Filled Analyzer (AGFA) at (ANL). Decay of the implanted reaction products was measured in pixelized double-sided Si strip detector (DSSD).

RADIOACTIVITY 251,253Lr(α)[from 203,205Tl(50Ti, 2n), E=237 MeV]; measured Eα, Iα; deduced T1/2, Q-value, α-decay branchings and widths. Comparison to other experimental data. and predictions of theoretical models.

doi: 10.1103/PhysRevC.106.L061301
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2022LA06      Phys.Rev. C 105, 044618 (2022)

H.Y.Lan, W.Luo, Y.Xu, D.L.Balabanski, G.L.Guardo, M.La Cognata, D.Lattuada, C.Matei, R.G.Pizzone, T.Rauscher, J.L.Zhou

Feasibility of studying astrophysically important charged-particle emission with the variable energy γ-ray system at the Extreme Light Infrastructure--Nuclear Physics facility

NUCLEAR REACTIONS 29Si, 47Ti, 56Fe, 73Ge, 74Se, 84Sr, 91Zr, 95Mo, 96,98Ru, 102Pd, 106Cd, 115,117,119Sn, 132Ba, 143Nd(γ, p), (γ, np), E<30 MeV; 50V, 67Zn, 87Sr, 107Ag, 113,115In, 119Sn, 123,125Te, 149,154Sm, 155,156,157,158,160Gd, 208Pb(γ, α), (γ, nα), E<30 MeV; calculated inclusive and exclusive σ(E), population of the particular excited states, energy spectra of ejectiles. TALYS-1.9 calculations with various combinations of level densities, strength functions and optical potentials available in the code.Investigated the feasibility of studying the reactions of astrophysical interest with ELI-NP facility infrastructure. Simulated achievable yields.

doi: 10.1103/PhysRevC.105.044618
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2022LU11      Eur.Phys.J. A 58, 244 (2022)

S.Luo, Y.-Y.Xu, D.-X.Zhu, B.He, P.-C.Chu, X.-H.Li

Improved Geiger-Nuttall law for α-decay half-lives of heavy and superheavy nuclei

RADIOACTIVITY 220,222,224,226,228,230,232Th, 222,224,226,228,230,232,234,236,238U, 230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 244,246,248,250,252,254,256Fm, 252,254,256No, 256,258Rf, 260Sg, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288Fl, 292Lv, 294Og, 221,223,225,227,229Th, 221,223,225,227,229,231Pa, 223,225,227,229,231,233U, 233,235,237Np, 229,231,233,235Pu, 245,247,249,251,253,255Es, 241,243,245,247,249,251,253,255,257Fm, 245,247,249,251,253,255,257Md, 251,253,255,257,259No, 224,226,228,230Pa, 224,226,228,230,232,234,236Np, 234,236,238,240,242Am, 234Bk, 240,242,244,246Es, 281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317Ts, 282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318Og, 284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319119, 287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320120(α); calculated T1/2. Comparison with available data.

doi: 10.1140/epja/s10050-022-00898-1
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2022SU04      Int.J.Mod.Phys. E31, 2250001 (2022)

Z.-H.Sun, Y.-L.Xu, X.-J.Sun, Y.-L.Han, C.-H.Cai

Global phenomenological optical model potential for 14N-nucleus elastic scattering

NUCLEAR REACTIONS 24Mg, 27Al, 28,29Si, 32S, 40Ca, 56Fe, 59Co, 58,62Ni, 70,74Ge, 90Zr, 92,100Mo, 118Sn, 208Pb(14N, 14N), E<100 MeV; analyzed available data; deduced global optical model potential parameters, σ, σ(θ).

doi: 10.1142/S021830132250001X
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2022SU13      Nucl.Sci.Eng. 196, 1031 (2022)

X.Su, Y.Xu, Y.Han

Theoretical Analysis of Cross Sections for n+46, 47, 49, 50, nat.Ti Reactions

NUCLEAR REACTIONS 46,47,49,50Ti, Ti(n, X), E<20 MeV; calculated σ, σ(θ), σ(E), σ(θ, E) using the optical model the unified Hauser-Feshbach theory, the exciton model, which includes the improved Iwamoto-Harada model, and the distorted wave Born approximation theory. Comparison with ENDF/B-VIII, JENDL-4, and JEFF33.

doi: 10.1080/00295639.2022.2049990
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2022SU23      Phys.Rev. C 106, 034614 (2022)

Y.Z.Sun, S.T.Wang, Y.P.Xu, D.Y.Pang, J.G.Li, C.X.Yuan, L.F.Wan, Y.Qiao, Y.Q.Wang, X.Y.Chen

Spectroscopic strength reduction of intermediate-energy single-proton removal from oxygen isotopes

NUCLEAR STRUCTURE C(13O, p), E=397 MeV/nucleon;C(14O, p), E=305, 349 MeV/nucleon;C(15O, p), E=308 MeV/nucleon;C(16O, p), E=450 MeV/nucleon;C(17O, p), E=629 MeV/nucleon;C(18O, p), E=573 MeV/nucleon;C(19O, p), E=635 MeV/nucleon;C(20O, p), E=415 MeV/nucleon;C(22O, p), E=414 MeV/nucleon; calculated inclusive single-proton removal σ, shell-model spectroscopic factors, reduction factors of the spectroscopic factors with the experimental data. Glauber reaction model calculations performed with MOMDIS code. Comparison to experimental data obtained at GSI and ETF(Lanzhou, China).

doi: 10.1103/PhysRevC.106.034614
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2022XU04      Eur.Phys.J. A 58, 16 (2022)

Y.-Y.Xu, H.-M.Liu, D.-X.Zhu, X.Pan, Y.-T.Zou, X.-H.Li, P.-C.Chu

An improved formula for the favored α decay half-lives

RADIOACTIVITY 146,148Sm, 148,150,152Gd, 150,152,154Dy, 152,154,156Er, 154,156Yb, 156,158,160,162Hf, 174Hf, 158,160,162,164,166,168W, 180W, 162,164,166,168,170,172,174Os, 186Os, 166,168,170,172,174,176,178,180,182,184,186,188,190Pt, 170,172,174,176,178,180,182,184,186,188Hg, 178,180,182,184,186,188,190,192,194Pb, 210Pb, 186,188,190,192,194,196,198,200,202,204,206,208,210,212,214,216,218Po, 194,196,198,200,202,204,206,208,210,212,214,216,218,220,222Rn, 202,204,206,208,210,212,214,216,218,220,222,224,226Ra, 208,210,212,214,216,218,220,222,224,226,228,230,232Th, 218,220,222,224,226,228,230,232,234,236,238U, 230,232,234,236,238,240,242,244Pu, 234,236,238,240,242,244,246,248Cm, 238,240,242,244,246,248,250,252,254Cf, 244,246Fm, 252,254,256No, 256,258Rf, 260Sg, 266,268,270Hs, 270Ds, 282Ds, 286Cn, 286,288Fl, 290,292Lv, 294Og, 105,107,109Te, 113I, 109,111Xe, 145Pm, 147Sm, 147Eu, 149,151Gd, 151,153Dy, 151,153Ho, 153,155Er, 153,155,157Tm, 155Yb, 155,157Lu, 157,159,161Hf, 157,159,161Ta, 159,161,163,165,167W, 159,161,163,165Re, 161,163,165,167,169,171,173Os, 165,167,169,171,173Ir, 177Ir, 165,167,169,171,173Pt, 177Pt, 181,183,185Pt, 171,173,175,177,179,181,183,185Au, 173,175Hg, 179Hg, 183Hg, 185Hg, 177,179,181Tl, 185,187,189,191Pb, 185,187,189,191,193,195,197Bi, 191,193,195,197,199,201Po, 205,207,209Po, 213,215,217,219Po, 187Po, 191,193,195,197,199,201,203,205,207,209,211,213,215,217,219At, 195,197,199,201,203,205,207,209Rn, 215,217Rn, 197,199,201,203,205,207,209,211,213,215,217,219Fr, 201,203,205Ra, 209,211Ra, 217Ra, 207,209,211,213,215,217,219,221Ac, 227Ac, 209,211,213Th, 219Th, 211,213,215,217,219,221,223,225,227,229,231Pa, 221U, 229U, 233U, 219Np, 223,225Np, 233Np, 231Pu, 235Pu, 239Pu, 233Cm, 239,241Cf, 245Cf, 253Cf, 241,243,245,247Es, 251,253,255Es, 241Fm, 247Fm, 251No, 253,255Lr, 259Lr, 261Rf, 257Db, 263Sg, 263,265Hs, 267Ds, 148Eu, 152,154Ho, 154,156Tm, 156,158Lu, 158Ta, 162,164Re, 164,166,168,170,172Ir, 170,172,174,176,178Au, 184Au, 188Bi, 196Bi, 192,194,196,198,200,202At, 214,216At, 256,258,260Rf, 260Sg, 262,264Hs, 268,270,272Hs, 266Ds, 270Ds, 276,278Ds, 270Cn, 280,282Cn, 284,286,288Fl, 288,290,292,294,296Lv, 294,296,298,300,302,304Og, 296,298,300,302,304,306,308120, 302,304,306,308,310,312122, 308,310,312,314,316,318124, 314,316,318,320,322,324,326126, 320,322,324,326,328,330,332128(α); calculated T1/2 using the modified Hatsukawa formula. Comparison with available data.

doi: 10.1140/epja/s10050-022-00666-1
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2022XU07      Chin.Phys.C 46, 064102 (2022)

Y.-P.Xu, D.-Y.Pang, C.-X.Yuan, X.-Y.Yun

Quenching of single-particle strengths of carbon isotopes 9-12, 14-20C with knockout reactions for incident energies 43-2100 MeV/nucleon

NUCLEAR REACTIONS 9Be, C(9C, 8C), (10C, 9C), (11C, 10C), (12C, 11C), (14C, 13C), (15C, 14C), (16C, 15C), (17C, 16C), (18C, 17C), (19C, 18C), (20C, 19C), E=43-2100 MeV/nucleon; analyzed available data; deduced the quenching of single-particle strengths of carbon isotopes, dependence on the proton-neutron asymmetry.

doi: 10.1088/1674-1137/ac5236
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2022XU10      Eur.Phys.J. A 58, 163 (2022)

Y.-Y.Xu, D.-X.Zhu, X.Chen, X.-J.Wu, B.He, X.-H.Li

A unified formula for α decay half-lives

RADIOACTIVITY 109I, 151Eu, 149,151Tb, 155Lu, 157Ta, 169Re, 171,173,175Ir, 175Pt, 179Pt, 185Hg, 171Hg, 177Hg, 181Hg, 181,183Tl, 187Tl, 179,181,183,185,187,189Pb, 187,189Bi, 209,211,213Bi, 211Po, 187,189Po, 203Po, 191,193,195At, 193Rn, 205Rn, 211,213Rn, 219,221Rn, 221,223Fr, 213Ra, 215,217,219,221,223Ra, 207Ra, 223,225Ac, 217Th, 221,223,225,227,229Th, 217Pa, 225Pa, 229Pa, 219U, 223,225,227U, 231U, 227,229,231Np, 235,237Np, 229Pu, 233Pu, 241Pu, 229Am, 233,235,237,239,241,243Am, 235Cm, 241,243,245,247Cm, 245,247,249Bk, 237Cf, 243Cf, 247,249,251Cf, 249Es, 243,245,247Fm, 251,253Fm, 257Fm, 245,247,249,251,253,255,257Md, 253,255,257,259No, 255Lr, 255,257,259,261Rf, 257,259Db, 263Db, 259,261,263,265Sg, 261Bh, 263Hs, 269Hs, 205Ac, 217Ac, 257Lr, 154Ho, 156Lu, 162Ta, 158Ta, 160Re, 168Re, 170,172,174Ir, 180,182,184,186Au, 178Tl, 184,186Tl, 186,188,190,192,194Bi, 212,214Bi, 206At, 210,212At, 218At, 192At, 200At, 198Fr, 212,214Fr, 218,220Fr, 214,216At, 220At, 208At, 222,224,226At, 216,218Pa, 228,230Pa, 224Np, 228,230Np, 236Np, 234Am, 242Am, 242,244,246,248Es, 252,254Es, 244,246Md, 250Md, 256,258Md, 254,256Lr, 256Db, 281,282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317Ts, 282,283,284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318Og, 284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319119, 287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320120, 254No, 256,258Rf(α); calculated T1/2; deduced formula. Comparison with NUBASE2020 values.

doi: 10.1140/epja/s10050-022-00812-9
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2022XU13      Chin.Phys.C 46, 114103 (2022)

Y.-Y.Xu, D.-X.Zhu, Y.-T.Zou, X.-J.Wu, B.He, X.-H.Li

Systematic study on α-decay half-lives of uranium isotopes with a screened electrostatic barrier

RADIOACTIVITY 216,217,218U, 221U, 222,223,224,225,226,227,228U, 229U, 230,231,232U, 233U, 234,235,236,237,238,239,240,241,242,243U(α); calculated T1/2 using the Gamow model with a screened electrostatic barrier. Comparison with available data.

doi: 10.1088/1674-1137/ac7fe8
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2022XU14      Int.J.Mod.Phys. E31, 2250093 (2022)

Y.Xu, X.Su, Y.Han, X.Sun, D.Zhang, C.Cai

Optical potential for the elastic scattering of 6Li projectile on 1p-shell nuclei

NUCLEAR REACTIONS 6,7Li, 9Be, 10,11B, 12,13,14C, 15N, 16,18O(6Li, 6Li), E=2-210 MeV; analyzed available data; deduced σ(θ), a set of global optical potential parameters by fitting the experimental data of elastic scattering angular distributions.

doi: 10.1142/S0218301322500938
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2022ZH39      Chin.Phys.C 46, 044106 (2022)

D.-X.Zhu, H.-M.Liu, Y.-Y.Xu, Y.-T.Zou, X.-J.Wu, P.-C.Chu, X.-H.Li

Two-proton radioactivity within Coulomb and proximity potential model

RADIOACTIVITY 19Mg, 45Fe, 48Ni, 54Zn, 67Kr(2p); calculated T1/2 using the Coulomb and proximity potential model (CPPM). Comparison with available data.

doi: 10.1088/1674-1137/ac45ef
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2021AB12      Phys.Rev. C 104, L061901 (2021)

M.S.Abdallah, B.E.Aboona, J.Adam, L.Adamczyk, J.R.Adams, J.K.Adkins, G.Agakishiev, I.Aggarwal, M.M.Aggarwal, Z.Ahammed, I.Alekseev, D.M.Anderson, A.Aparin, E.C.Aschenauer, M.U.Ashraf, F.G.Atetalla, A.Attri, G.S.Averichev, V.Bairathi, W.Baker, J.G.Ball Cap, K.Barish, A.Behera, R.Bellwied, P.Bhagat, A.Bhasin, J.Bielcik, J.Bielcikova, I.G.Bordyuzhin, J.D.Brandenburg, A.V.Brandin, I.Bunzarov, J.Butterworth, X.Z.Cai, H.Caines, M.Calderon de la Barca Sanchez, D.Cebra, I.Chakaberia, P.Chaloupka, B.K.Chan, F.-H.Chang, Z.Chang, N.Chankova-Bunzarova, A.Chatterjee, S.Chattopadhyay, D.Chen, J.Chen, J.H.Chen, X.Chen, Z.Chen, J.Cheng, M.Chevalier, S.Choudhury, W.Christie, X.Chu, H.J.Crawford, M.Csanad, M.Daugherity, T.G.Dedovich, I.M.Deppner, A.A.Derevschikov, A.Dhamija, L.Di Carlo, L.Didenko, P.Dixit, X.Dong, J.L.Drachenberg, E.Duckworth, J.C.Dunlop, N.Elsey, J.Engelage, G.Eppley, S.Esumi, O.Evdokimov, A.Ewigleben, O.Eyser, R.Fatemi, F.M.Fawzi, S.Fazio, P.Federic, J.Fedorisin, C.J.Feng, Y.Feng, P.Filip, E.Finch, Y.Fisyak, A.Francisco, C.Fu, L.Fulek, C.A.Gagliardi, T.Galatyuk, F.Geurts, N.Ghimire, A.Gibson, K.Gopal, X.Gou, D.Grosnick, A.Gupta, W.Guryn, A.I.Hamad, A.Hamed, Y.Han, S.Harabasz, M.D.Harasty, J.W.Harris, H.Harrison, S.He, W.He, X.H.He, Y.He, S.Heppelmann, S.Heppelmann, N.Herrmann, E.Hoffman, L.Holub, Y.Hu, H.Huang, H.Z.Huang, S.L.Huang, T.Huang, X.Huang, Y.Huang, T.J.Humanic, G.Igo, D.Isenhower, W.W.Jacobs, C.Jena, A.Jentsch, Y.Ji, J.Jia, K.Jiang, X.Ju, E.G.Judd, S.Kabana, M.L.Kabir, S.Kagamaster, D.Kalinkin, K.Kang, D.Kapukchyan, K.Kauder, H.W.Ke, D.Keane, A.Kechechyan, M.Kelsey, Y.V.Khyzhniak, D.P.Kikola, C.Kim, B.Kimelman, D.Kincses, I.Kisel, A.Kiselev, A.G.Knospe, H.S.Ko, L.Kochenda, L.K.Kosarzewski, L.Kramarik, P.Kravtsov, L.Kumar, S.Kumar, R.Kunnawalkam Elayavalli, J.H.Kwasizur, R.Lacey, S.Lan, J.M.Landgraf, J.Lauret, A.Lebedev, R.Lednicky, J.H.Lee, Y.H.Leung, C.Li, C.Li, W.Li, X.Li, Y.Li, X.Liang, Y.Liang, R.Licenik, T.Lin, Y.Lin, M.A.Lisa, F.Liu, H.Liu, H.Liu, P.Liu, T.Liu, X.Liu, Y.Liu, Z.Liu, T.Ljubicic, W.J.Llope, R.S.Longacre, E.Loyd, N.S.Lukow, X.F.Luo, L.Ma, R.Ma, Y.G.Ma, N.Magdy, D.Mallick, S.Margetis, C.Markert, H.S.Matis, J.A.Mazer, N.G.Minaev, S.Mioduszewski, B.Mohanty, M.M.Mondal, I.Mooney, D.A.Morozov, A.Mukherjee, M.Nagy, J.D.Nam, Md.Nasim, K.Nayak, D.Neff, J.M.Nelson, D.B.Nemes, M.Nie, G.Nigmatkulov, T.Niida, R.Nishitani, L.V.Nogach, T.Nonaka, A.S.Nunes, G.Odyniec, A.Ogawa, S.Oh, V.A.Okorokov, B.S.Page, R.Pak, J.Pan, A.Pandav, A.K.Pandey, Y.Panebratsev, P.Parfenov, B.Pawlik, D.Pawlowska, H.Pei, C.Perkins, L.Pinsky, R.L.Pinter, J.Pluta, B.R.Pokhrel, G.Ponimatkin, J.Porter, M.Posik, V.Prozorova, N.K.Pruthi, M.Przybycien, J.Putschke, H.Qiu, A.Quintero, C.Racz, S.K.Radhakrishnan, N.Raha, R.L.Ray, R.Reed, H.G.Ritter, M.Robotkova, O.V.Rogachevskiy, J.L.Romero, D.Roy, L.Ruan, J.Rusnak, N.R.Sahoo, H.Sako, S.Salur, J.Sandweiss, S.Sato, W.B.Schmidke, N.Schmitz, B.R.Schweid, F.Seck, J.Seger, M.Sergeeva, R.Seto, P.Seyboth, N.Shah, E.Shahaliev, P.V.Shanmuganathan, M.Shao, T.Shao, A.I.Sheikh, D.Shen, S.S.Shi, Y.Shi, Q.Y.Shou, E.P.Sichtermann, R.Sikora, M.Simko, J.Singh, S.Singha, M.J.Skoby, N.Smirnov, Y.Sohngen, W.Solyst, P.Sorensen, H.M.Spinka, B.Srivastava, T.D.S.Stanislaus, M.Stefaniak, D.J.Stewart, M.Strikhanov, B.Stringfellow, A.A.P.Suaide, M.Sumbera, B.Summa, X.M.Sun, X.Sun, Y.Sun, Y.Sun, B.Surrow, D.N.Svirida, Z.W.Sweger, P.Szymanski, A.H.Tang, Z.Tang, A.Taranenko, T.Tarnowsky, J.H.Thomas, A.R.Timmins, D.Tlusty, T.Todoroki, M.Tokarev, C.A.Tomkiel, S.Trentalange, R.E.Tribble, P.Tribedy, S.K.Tripathy, T.Truhlar, B.A.Trzeciak, O.D.Tsai, Z.Tu, T.Ullrich, D.G.Underwood, I.Upsal, G.Van Buren, J.Vanek, A.N.Vasiliev, I.Vassiliev, V.Verkest, F.Videbaek, S.Vokal, S.A.Voloshin, F.Wang, G.Wang, J.S.Wang, P.Wang, Y.Wang, Y.Wang, Z.Wang, J.C.Webb, P.C.Weidenkaff, L.Wen, G.D.Westfall, H.Wieman, S.W.Wissink, J.Wu, Y.Wu, B.Xi, Z.G.Xiao, G.Xie, W.Xie, H.Xu, N.Xu, Q.H.Xu, Y.Xu, Z.Xu, Z.Xu, C.Yang, Q.Yang, S.Yang, Y.Yang, Z.Ye, Z.Ye, L.Yi, K.Yip, Y.Yu, H.Zbroszczyk, W.Zha, C.Zhang, D.Zhang, J.Zhang, S.Zhang, S.Zhang, X.P.Zhang, Y.Zhang, Y.Zhang, Y.Zhang, Z.J.Zhang, Z.Zhang, Z.Zhang, J.Zhao, C.Zhou, X.Zhu, M.Zurek, M.Zyzak

Global Λ-hyperon polarization in Au+Au collisions at √ sNN = 3 GeV

doi: 10.1103/PhysRevC.104.L061901
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2021BE28      Phys.Rev. C 104, 044332 (2021)

A.Berceanu, Y.Xu, Y.F.Niu

Temperature effects on neutron-capture cross sections and rates through electric dipole transitions in hot nuclei

NUCLEAR STRUCTURE 126,128,130,132,134,136,138,140,142,144,146Sn; calculated E1 transition strengths as a function of excitation energy for temperatures T=0 MeV, ratio between neutron-capture rate using relativistic quasiparticle random phase approximation (RQRPA) model, and for T=1 and 2 MeV using self-consistent finite-temperature relativistic random-phase approximation (FTRRPA) model, based on DD-ME2 energy density functional. 126,136,146Sn; calculated transition densities of neutrons and protons for the low-lying peaks at T=0 for 8.33-MeV peak in 126Sn, 6.04- and 8.28-MeV peaks in 136Sn, and 5.11- and 7.54-MeV peaks in 146Sn using RQRPA model based on DD-ME2 energy density functional, main single-particle transition configurations for selected low-lying dipole states, E1 transition strength as function of excitation energy. Self-consistent QRPA and finite-temperature RPA model based on relativistic energy density functionals.

doi: 10.1103/PhysRevC.104.044332
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2021KE02      Nucl.Phys. A1005, 122039 (2021)

W.Ke, Y.Xu, S.Bass

Quantifying heavy quark transport coefficients with an improved transport model

doi: 10.1016/j.nuclphysa.2020.122039
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2021SU05      Nucl.Sci.Eng. 195, 239 (2021)

X.Su, Y.Xu, Y.Han

Calculations and Evaluations of the n + 48Ti Reaction Below 200 MeV

NUCLEAR REACTIONS 48Ti(n, X), (n, n), (n, n'), E<200 MeV; analyzed available data; calculated σ, σ(θ). Comparison with the EXFOR library.

doi: 10.1080/00295639.2020.1808388
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2021XU04      Phys.Rev. C 104, 044301 (2021)

Y.Xu, S.Goriely, E.Khan

Systematical studies of the E1 photon strength functions combining the Skyrme-Hartree-Fock-Bogoliubov plus quasiparticle random-phase approximation model and experimental giant dipole resonance properties

NUCLEAR STRUCTURE 70,72,74Ge, 80,82Se, 89Y, 90,91,92,94Zr, 93Nb, 96,100Mo, 103Rh, 107Ag, 115In, 119,120,124Sn, 124,126,128Te, 127I, 128,134Xe, 133Ce, 138Ba, 140Ce, 141Pr, 143,145,146Nd, 144,150Sm, 165Ho, 181Ta, 188Os, 197Au, 206,208Pb, 209Bi, 239Pu; calculated E1 photon strength function using BSk27+QRPA, and compared with extracted strength from experimental photoabsorption cross sections. A=70-190; calculated parameters of giant-dipole resonances (GDR) using BSk27+QRPA, and compared with compiled in the RIPL-3 database. A=25-250; calculated E1 strength functions and compared with compiled data in RIPL3 for 60 nuclei from 25Mg to 239U, and comparison between ARC E1 strength function for 25 nuclei from 96Mo to 240Pu. 115,120,125,130,135,140,145,150,155Sn; calculated E1 photon strength functions from empirical Lorentzian model SMLO, D1M+QRPA, BSk7+QRPA, and the present BSk27+QRPA. 115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155Sn; calculated neutron capture reaction rates at the temperature of T9=1 using present BSk27+QRPA model and compared with those from BSk7+QRPA, D1M+QRPA, SMLO. Z=1-110, N=0-255; calculated neutron capture reaction rates at T9=1 present BSk27+QRPA model and compared with those from previous D1M+QRPA model. 43,44Sc, 44,45Ti; calculated temperature-dependent E1 strength functions using present BSk27+QRPA, and compared with shell-model calculationsSystematic investigation of E1 photon strength functions for about 10, 000 nuclei with Z=8-124 lying between the proton and neutron drip lines by combining simultaneously microscopic Hartree-Fock-Bogoliubov plus quasiparticle random-phase approximation (HFB+QRPA) model and the constraints from available experimental results for photon strength functions from giant dipole resonance (GDR) data, and other types of experiments. Relevance to future measurement of the photonuclear excitation using the Extreme Light Infrastructure (ELI-NP) facilities, and to improve study of r and p nucleosynthesis processes.

doi: 10.1103/PhysRevC.104.044301
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2021XU07      Chin.Phys.C 45, 114103 (2021)

Y.-L.Xu, Y.-L.Han, X.-W.Su, X.-J.Sun, H.-Y.Liang, H.-R.Guo, C.-H.Cai

Description of elastic scattering induced by the unstable nuclei 9, 10, 11, 13, 14C

NUCLEAR REACTIONS 208Pb(9C, 9C), (11C, 11C), E=222-227 MeV; 27Al, 58Ni, 208Pb(10C, 10C), E=29.1-256 MeV; 28Si, 208Pb(9C, 9C), E<500 MeV; 28Si, 208Pb(11C, 11C), E<500 MeV; 28Si(13C, 13C), E=25-60 MeV; 40Ca, 56Fe, 60Ni, 66Zn, 88Sr(14C, 14C), E=51 MeV; 92,100Mo(14C, 14C), E=71 MeV; 28Si(14C, 14C), E<500 MeV; analyzed available data; deduced σ, σ(θ), global optical model potentials.

doi: 10.1088/1674-1137/ac1fe1
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2021YA04      Nucl.Phys. A1005, 121854 (2021)

X.Yao, W.Ke, Y.Xu, S.A.Bass, T.Mehen, B.Muller

Quarkonium Production in Heavy Ion Collisions: From Open Quantum System to Transport Equation

doi: 10.1016/j.nuclphysa.2020.121854
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2020MU07      Phys.Rev. C 101, 055801 (2020)

M.Munch, C.Matei, S.D.Pain, M.T.Febbraro, K.A.Chipps, H.J.Karwowski, C.Aa.Diget, A.Pappalardo, S.Chesnevskaya, G.L.Guardo, D.Walter, D.L.Balabanski, F.D.Becchetti, C.R.Brune, K.Y.Chae, J.Frost-Schenk, M.J.Kim, M.S.Kwag, M.La Cognata, D.Lattuada, R.G.Pizzone, G.G.Rapisarda, G.V.Turturica, C.A.Ur, Y.Xu

Measurement of the 7Li(γ, t)4He ground-state cross section between Eγ = 4.4. and 10 MeV

NUCLEAR REACTIONS 7Li(γ, t), E=4.4-10 MeV from High Intensity Gamma-ray Source (HIγS) at TUNL; measured E(t), I(t), Eα, Iα, Eγ and Iγ, αt-coin, ground state σ(E) using the SIDAR silicon detector array. 3H(α, γ), E(cm)=0-7 MeV; deduced astrophysical S-factor from R-matrix analysis. Comparison with model predictions, and with previous experimental results. Relevance to primordial Li problem and the mirror α-capture reactions.

doi: 10.1103/PhysRevC.101.055801
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetL0260. Data from this article have been entered in the XUNDL database. For more information, click here.


2020SO09      Phys.Rev. C 101, 044903 (2020)

Ta.Song, P.Moreau, Y.Xu, V.Ozvenchuk, E.Bratkovskaya, J.Aichelin, S.A.Bass, P.B.Gossiaux, M.Nahrgang

Traces of nonequilibrium effects, initial condition, bulk dynamics, and elementary collisions in the charm observables

doi: 10.1103/PhysRevC.101.044903
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2020XU03      Chin.Phys.C 44, 034101 (2020)

Y.-L.Xu, Y.-L.Han, H.-Y.Liang, Z.-D.Wu, H.-R.Guo, C.-H.Cai

Applicability of 9Be global optical potential to description of 8, 10, 11B elastic scattering

NUCLEAR REACTIONS 12C, 27Al, 28Si, 58Ni, 208Pb(8B, 8B), 9Be, 12C, 16O, 28Si, 58Ni, 120Sn, 208Pb(10B, 10B), 12C, 28Si, 58Ni, 208Pb, 209Bi(11B, 11B), E<50 MeV; analyzed available data. 8,10,11B; calculated σ; deduced global phenomenological optical model potentials.

doi: 10.1088/1674-1137/44/3/034101
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2020XU04      Chin.Phys.C 44, 034101 (2020)

Y.-L.Xu, Y.-L.Han, H.-Y.Liang, Z.-D.Wu, H.-R.Guo, C.-H.Cai

Applicability of 9Be global optical potential to description of 8, 10, 11B elastic scattering

NUCLEAR REACTIONS 27Al, 58Ni, 208Pb, 12C, 28Si(8B, 8B), E<100 MeV; 27Al, 28Si, 58Ni, 120Sn, 16O, 9Be, 208Pb(10B, 10B), E<100 MeV; 28Si, 58Ni, 209Bi, 12C, 209Bi(11B, 11B), E<100 MeV; analyzed available data. 9Be; deduced optical model potential parameters, σ, σ(θ).

doi: 10.1088/1674-1137/44/3/034101
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2020XU07      J.Phys.(London) G47, 085105 (2020)

Y.-G.Xu, X.-D.Cheng, J.-L.Zhang, R.-M.Wang

Studying two-body nonleptonic weak decays of hyperons with topological diagram approach

doi: 10.1088/1361-6471/ab97c7
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2020XU10      Chin.Phys.C 44, 124103 (2020)

Y.-L.Xu, Y.-L.Han, X.-W.Su, X.-J.Sun, H.-Y.Liang, H.-R.Guo, C.-H.Cai

Global optical model potential describing 12C-nucleus elastic scattering

NUCLEAR REACTIONS 24Mg, 28Si, 32S, 39K, 40,42,48Ca, 50Cr, 56Fe, Fe, 58,64Ni, Ni, 90,91,92,94,96Zr, 92Mo, 116,117,118,119,120,122,124Sn, 194,198Pt, 208Pb, 209Bi(12C, 12C), E<200 MeV; analyzed available data; deduced a new global optical model potential parameters.

doi: 10.1088/1674-1137/abb4d0
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2020ZH02      Phys.Lett. B 801, 135170 (2020), Corrigendum Phys.Lett. B 803, 135278 (2020)

N.T.Zhang, X.Y.Wang, D.Tudor, B.Bucher, I.Burducea, H.Chen, Z.J.Chen, D.Chesneanu, A.I.Chilug, L.R.Gasques, D.G.Ghita, C.Gomoiu, K.Hagino, S.Kubono, Y.J.Li, C.J.Lin, W.P.Lin, R.Margineanu, A.Pantelica, I.C.Stefanescu, M.Straticiuc, X.D.Tang, L.Trache, A.S.Umar, W.Y.Xin, S.W.Xu, Y.Xu

Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies

NUCLEAR REACTIONS 12C(13C, p)24Na, E=4.640-10.995 MeV; measured reaction products, Eγ, Iγ; deduced σ, branching ratio, S-factor.

doi: 10.1016/j.physletb.2019.135170
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0970.


2019CA14      Phys.Rev. C 99, 054907 (2019)

S.Cao, G.Coci, S.K.Das, W.Ke, S.Y.F.Liu, S.Plumari, T.Song, Y.Xu, J.Aichelin, S.Bass, E.Bratkovskaya, X.Dong, P.B.Gossiaux, V.Greco, M.He, M.Nahrgang, R.Rapp, F.Scardina, X.-N.Wang

Toward the determination of heavy-quark transport coefficients in quark-gluon plasma

doi: 10.1103/PhysRevC.99.054907
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2019KE08      Phys.Rev. C 100, 064911 (2019)

W.Ke, Y.Xu, S.A.Bass

Modified Boltzmann approach for modeling the splitting vertices induced by the hot QCD medium in the deep Landau-Pomeranchuk-Migdal region

doi: 10.1103/PhysRevC.100.064911
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2019SU03      Phys.Rev. C 99, 024605 (2019)

Y.Z.Sun, S.T.Wang, Z.Y.Sun, X.H.Zhang, D.Yan, B.H.Sun, J.W.Zhao, Y.P.Xu, D.Y.Pang, Y.H.Yu, K.Yue, S.W.Tang, C.Dong, Y.X.Zhao, F.Fang, Y.Sun, Z.H.Cheng, X.M.Liu, P.Ma, H.R.Yang, C.G.Lu, L.M.Duan

Two-neutron removal cross sections from 15, 16C at around 240 MeV/nucleon

NUCLEAR REACTIONS 12C(15C, X), (15C, 13C), (16C, X), (16C, 14C)8Li/10Be/11Be/12B/13B/15C/16C/17N, E=237, 239 MeV/nucleon, [secondary 15,16C beams from 9Be(18O, X), E=280 MeV/nucleon primary reaction followed by in-flight fragment separator RIBLL2 at HIRFL-Lanzhou]; measured reaction products, particle identification spectra, time of flight of fragments, and two-neutron removal σ(E) using multiwire drift chambers for particle detection and identification, and plastic scintillators for time of flight measurements. Comparison with previous experimental values, and theoretical calculations for two-neutron removal σ based on eikonal-model and shell-model structure information. Systematics of odd-even staggering in two-neutron removal σ from 15,16,17,18,19,20C projectiles.

doi: 10.1103/PhysRevC.99.024605
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetS0188.


2019WA01      Phys.Scr. 94, 015302 (2019)

S.T.Wang, Y.P.Xu, D.Y.Pang

Energy dependence of the reduced single-particle strength for strongly-bound proton removal on 16C

NUCLEAR REACTIONS 12C(16C, 15B), E=400 MeV/nucleon; analyzed available data; deduced reduction factors of the one-proton σ.

doi: 10.1088/1402-4896/aaed64
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2019XU02      Phys.Rev. C 99, 014902 (2019)

Y.Xu, S.A.Bass, P.Moreau, T.Song, M.Nahrgang, E.Bratkovskaya, P.Gossiaux, J.Aichelin, S.Cao, V.Greco, G.Coci, K.Werner

Resolving discrepancies in the estimation of heavy quark transport coefficients in relativistic heavy-ion collisions

doi: 10.1103/PhysRevC.99.014902
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2019XU05      Phys.Rev. C 99, 034618 (2019)

Y.Xu, Y.Han, H.Liang, Z.Wu, H.Guo, C.Cai

Global optical model potential for the weakly bound projectile 9Be

NUCLEAR REACTIONS Mg(9Be, 9Be), E=14.0, 20.0, 26.0 MeV; 27Al(9Be, 9Be), E=12.0, 14.0, 18.0, 20.0, 22.0, 25.0, 28.0, 32.0, 33.0, 35.0.40.0, 47.5 MeV; 28Si(9Be, 9Be), E=12.0, 13.0, 14.0, 17.0, 20.0, 23.0, 26.0, 30.0, 45.0, 50.0, 60.0 MeV; 40Ca(9Be, 9Be), E=14.0, 20.0, 26.0, 45.0.50.0, 60.0 MeV; 58Ni(9Be, 9Be), E=20.0, 26.0 MeV; 64Zn(9Be, 9Be), E=17.0, 19.0, 21.0, 23.0, 26.0, 28.0, 28.4, 28.97 MeV; 89Y(9Be, 9Be), E=18.6, 20.6, 22.7, 24.7, 26.7, 28.7, 33.2 MeV; Ag(9Be, 9Be), E=26.0 MeV; 144Sm(9Be, 9Be), E=30.0, 31.5, 33.0, 34.0, 35.0, 37.0, 39.0, 41.0, 44.0, 48.0 MeV; 208Pb(9Be, 9Be), E=37.0, 37.8, 38.0, 38.2, 38.5, 38.7, 39.0, 9.5, 40.0, 41.0, 42.0, 44.0, 46.0, 47.2, 48.0, 50.0, 60.0, 68.0, 75.0 MeV; 209Bi(9Be, 9Be), E=37.0, 37.8, 38.0, 38.2, 38.5, 38.7, 39.0, 39.5, 40.0, 41.0, 42.0, 44.0, 46.0, 48.0 MeV; analyzed elastic σ(θ, E) data for global phenomenological energy-dependent optical model potential parameters for 9Be. 9Be, 12,13C, 27Al, 64Zn, 89Y, 144Sm(9Be, X), E=10-300 MeV; 28Si, Cu(9Be, X), E=10-500 MeV; 89Y(α, X), (6He, X), (8He, X), (6Li, X), (7Li, X), (9Be, X), (11B, X); calculated reaction σ(E) using optical model and compared with experimental data. 9Be(9Be, 9Be), E=14.0, 20.0, 26.0 MeV; 12C(9Be, 9Be), E=13.0, 14.0, 14.5, 17.3, 19.0, 20.0, 21.0, 26.0, 153.8 MeV; 13C(9Be, 9Be), E=19.46, 25.05 MeV; 16O(9Be, 9Be), E=20.0, 25.94 MeV; calculated elastic σ(θ, E) using optical model parameters and compared with experimental data.

doi: 10.1103/PhysRevC.99.034618
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2019YA01      Nucl.Phys. A982, 755c (2019)

X.Yao, W.Ke, Y.Xu, S.Bass, B.Muller

Quarkonium production in heavy ion collisions: coupled Boltzmann transport equations

doi: 10.1016/j.nuclphysa.2018.10.005
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2018HE01      Chin.Phys.C 42, 015001 (2018)

J.-J.He, I.Lombardo, D.Dell'Aquila, Y.Xu, L.-Y.Zhang, W.-P.Liu

Thermonuclear 19F(p, α0)16O reaction rate

NUCLEAR REACTIONS 19F(p, α), E<1 MeV; analyzed available data; deduced reaction rate, σ, σ(θ), S-factor using theoretical R-matrix extrapolations.

doi: 10.1088/1674-1137/42/1/015001
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2018HU09      Nucl.Sci.Eng. 191, 262 (2018)

J.Hu, Y.Xu, Y.Han

Calculation and Evaluations for n+64, 66, 67, 68, 70, natZn Reactions

NUCLEAR REACTIONS 64,66,67,68,70Zn, Zn(n, X), E<200 MeV; calculated σ(θ), σ(E), σ(θ, E). Comparison with experimental data, JEFF-3.2 and JENDL-4.0 evaluated nuclear data libraries.

doi: 10.1080/00295639.2018.1469334
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2018KE05      Phys.Rev. C 98, 064901 (2018)

W.Ke, Y.Xu, S.A.Bass

Linearized Boltzmann-Langevin model for heavy quark transport in hot and dense QCD matter

doi: 10.1103/PhysRevC.98.064901
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2018LA06      Astrophys.J. 859, 62 (2018)

R.Lau, M.Beard, S.S.Gupta, H.Schatz, A.V.Afanasjev, E.F.Brown, A.Deibel, L.R.Gasques, G.W.Hitt, W.R.Hix, L.Keek, P.Moller, P.S.Shternin, A.W.Steiner, M.Wiescher, Y.Xu

Nuclear Reactions in the Crusts of Accreting Neutron Stars

doi: 10.3847/1538-4357/aabfe0
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2018LA14      Phys.Rev. C 98, 054601 (2018)

H.Y.Lan, Y.Xu, W.Luo, D.L.Balabanski, S.Goriely, M.La Cognata, C.Matei, A.Anzalone, S.Chesnevskaya, G.L.Guardo, D.Lattuada, R.G.Pizzone, S.Romano, C.Spitaleri, A.Taffara, A.Tumino, Z.C.Zhu

Determination of the photodisintegration reaction rates involving charged particles: Systematic calculations and proposed measurements based on the facility for Extreme Light Infrastructure--Nuclear Physics

NUCLEAR REACTIONS 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te(γ, p), E(cm)=8-20 MeV; 74Se, 84Sr, 92Mo, 96Ru, 102Pd, 106Cd, 112Sn, 120Te, 132Ba, 144Sm, 148Gd, 184Os(γ, α), E(cm)=6-20 MeV; calculated σ(E), proton and α-particle spectra and yields, Gamow windows at T9=2.5 and minimum required energies of the incident γ beam satisfying the measurable criteria of the minimum detectable limit and the particle identification. Z=10-100, N=10-160; calculated ratios of the (γ, p) and (γ, α) astrophysical reaction rates at T9=2.5 for 3000 targets of stable and proton-rich nuclei. Optical potential model calculations using Woods-Saxon and microscopic folding JLMB optical model potentials. Relevance to p-process nucleosynthesis, and the measurements of six (γ, p) and eight (γ, α) reactions based on the γ-beam facility and the Extreme Light Infrastructure Silicon Strip Array (ELISSA) for the detection of charged particles at ELI-NP, Bucharest facility.

doi: 10.1103/PhysRevC.98.054601
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2018XU01      Phys.Rev. C 97, 014615 (2018)

Y.Xu, Y.Han, J.Hu, H.Liang, Z.Wu, H.Guo, C.Cai

Global phenomenological optical model potential for the 7Li projectile nucleus

NUCLEAR REACTIONS 9Be(7Li, 7Li), E=15.75, 24.0, 30.0, 63.0, 130.0 MeV; 12C(7Li, 7Li), E=7.5, 9.0, 12.0, 15.0, 36.0, 131.8 MeV; 16O(7Li, 7Li), E=26.0, 36.0, 42.0, 50.0 MeV; 11B, 12,13C, 24Mg(7Li, 7Li), E=34.0 MeV; 24,26Mg(7Li, 7Li), E=88.7 MeV; 27Al(7Li, 7Li), E=6.0, 7.0, 8.0, 9.0, 10.0, 11.0, 12.0, 13.0, 14.0, 16.0, 18.0, 19.0, 24.0 MeV; 28Si(7Li, 7Li), E=8.0, 8.5, 9.0, 10.0, 11.0, 11.5, 13.0, 15.0, 16.0, 21.0, 26.0, 36.0, 177.8 MeV; 40,44,48Ca(7Li, 7Li), E=34.0; 40Ca(7Li, 7Li), E=88.7 MeV; 46,48Ti(7Li, 7Li), E=17.0 MeV; 54Fe(7Li, 7Li), E=36.0, 42.0, 48.0 MeV; 56Fe, 65Cu, 90Zr(7Li, 7Li), E=34.0 MeV; 58Ni(7Li, 7Li), E=14.22, 16.25.18.28, 19.0, 20.31.34.0, 42.0 MeV; 60,62Ni, 64,68Zn(7Li, 7Li), E=34.0 MeV; 80Se(7Li, 7Li), E=14.0, 14.5, 15.0, 15.5, 16.0, 17.0, 18.0, 19.0, 20.0, 23.0, 26.0 MeV; 89Y(7Li, 7Li), E=60.0 MeV; 116Sn(7Li, 7Li), E=18.0, 19.0, 20.0, 21.0, 22.0, 23.0, 24.0, 26.0, 30.0, 35.0 MeV; 120Sn(7Li, 7Li), E=19.5, 20.0, 20.5, 22.0, 24.0, 25.0, 26.0, 28.0, 30.044.0 MeV; 138Ba(7Li, 7Li), E=21.0, 22.0, 23.0, 24.0, 28.0, 30.0, 32.0, 52.0 MeV; 140Ce, 142Nd(7Li, 7Li), E=52.0 MeV; 144Sm(7Li, 7Li), E=21.6, 22.1, 22.6.23.0, 25.0, 27.0, 29.0, 30.0, 32.0, 35.0, 40.8, 52.0 MeV; 208Pb(7Li, 7Li), E=27.0, 29.0, 33.0, 39.0, 42.0, 52.0 MeV; 232Th(7Li, 7Li), E=24.0, 26.0, 30.0, 32.0, 35.0, 40.0, 44.0 MeV; analyzed σ(θ, E) experimental data by global phenomenological optical model potential. 13C, 27Al, 64Zn, 116Sn, 138Ba, (7Li, X), E<300 MeV; 28Si, Cu, 208Pb(7Li, X), E<400 MeV; calculated reaction σ(E) using optical model, and compared with experimental data.

doi: 10.1103/PhysRevC.97.014615
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2018XU02      Phys.Rev. C 97, 014907 (2018)

Yi.Xu, J.E.Bernhard, S.A.Bass, M.Nahrgang, S.Cao

Data-driven analysis for the temperature and momentum dependence of the heavy-quark diffusion coefficient in relativistic heavy-ion collisions

doi: 10.1103/PhysRevC.97.014907
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2018XU03      Int.J.Mod.Phys. E27, 1850023 (2018)

Y.Xu, Y.Han, Q.Shen

The proton microscopic optical potential based on Skyrme interaction

NUCLEAR REACTIONS 54,56Fe, 51V, 40Ca, 28Si, 27Al, 59Co, 58,60Ni, 63Cu, 90Zr, 120Sn, 208Pb, 232Th, 238U(p, p), E<100 MeV; calculated σ, σ(θ). Comparison with available data.

doi: 10.1142/S0218301318500234
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2018XU10      Phys.Rev. C 98, 024619 (2018)

Y.Xu, Y.Han, J.Hu, H.Liang, Z.Wu, H.Guo, C.Cai

6Li global phenomenological optical model potential

NUCLEAR REACTIONS 24Mg, 48Ca(6Li, 6Li), E=240.0 MeV; 25,26Mg, 39K, 91Zr(6Li, 6Li), E=34.0 MeV; 27Al(6Li, 6Li), E=7.0, 8.0, 10.0, 12.0, 18.0, 34.0 MeV; 28Si(6Li, 6Li), E=7.5, 9.0, 11.0, 13.0, 16.0, 20.0, 21.0, 25.0, 27.0, 34.0, 46.0, 99.0, 135.0, 154.0, 210.0, 240.0, 318.0, 350.0 MeV; 40Ca(6Li, 6Li), E=50.6, 99.0, 156.0, 210.0, 240.0 MeV; 54Fe(6Li, 6Li), E=38.0, 44.0, 50.0 MeV; 59Co(6Li, 6Li), E=12.0, 18.0, 26.0, 30.0 MeV; 58Ni(6Li, 6Li), E=9.85, 11.21, 12.13, 13.04, 14.04, 34.0, 50.6, 73.7, 90.0, 99.0, 210.0, 240.0 MeV; 65Cu(6Li, 6Li), E=25.0 MeV; 64Zn(6Li, 6Li), E=10.77, 11.69, 12.0, 12.43, 13.0, 13.54, 13.8, 14.92, 15.0, 16.30, 16.5, 18.0, 18.14, 19.98, 22.0 MeV; 72,74,76Ge(6Li, 6Li), E=28.0 MeV; 80Se(6Li, 6Li), E=14.0, 14.5, 15.0, 15.5, 16.0, 17.0, 18.0, 19.0, 20.0, 22.19, 23.0, 26.0 MeV; 89Y(6Li, 6Li), E=60.0 MeV; 90Zr(6Li, 6Li), E=11.0, 12.0, 13.0, 15.0, 17.0, 19.0, 21.0, 25.0, 30.0, 34.0, 60.0, 70.0, 73.7, 99.0, 156.0, 210.0, 240.0 MeV; 92,94,96Zr(6Li, 6Li), E=70.0 MeV; 112Sn(6Li, 6Li), E=21.0, 22.0, 23.0, 25.0, 30.0, 35.0 MeV; 116Sn(6Li, 6Li), E=20.0, 21.0, 22.0, 23.0, 24.0, 26.0, 30.0, 35.0, 40.0 MeV; 118Sn(6Li, 6Li), E=42.0 MeV; 120Sn(6Li, 6Li), E=30.0, 44.0, 90.0 MeV; 124Sn(6Li, 6Li), E=73.7 MeV; 138Ba(6Li, 6Li), E=21.0, 22.0, 23.0, 24.0, 26.0, 28.0 MeV; 144Sm(6Li, 6Li), E=21.0, 22.1, 22.6, 24.1, 26.0, 28.0, 30.1, 32.2, 35.1, 42.3 MeV; 208Pb(6Li, 6Li), E=25.0, 29.0, 31.0, 33.0, 35.0, 36.0, 37.0, 39.0, 42.0, 43.0, 46.0, 48.0, 50.6, 73.7, 88.0, 90.0, 99.0, 156.0, 210.0 MeV; 209Bi(6Li, 6Li), E=24.0, 26.0, 28.0, 29.9, 30.0, 32.0, 32.8, 34.0, 36.0, 40.0, 44.0, 50.0 MeV; 232Th(6Li, 6Li), E=26.0, 30.0, 32.0, 35.0, 40.0, 44.0 MeV; analyzed differential σ(θ, E) data; deduced a new set of 6Li global phenomenological energy-dependent optical potential parameters based on the form of the Woods-Saxon potential within the optical model. 63,65Cu, 64Zn, 112,116Sn, 138Ba, 208Pb(6Li, X), E<400 MeV; calculated reaction σ(E), and compared with experimental data.

doi: 10.1103/PhysRevC.98.024619
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2018XU11      Phys.Rev. C 98, 044622 (2018)

Y.P.Xu, D.Y.Pang, X.Y.Yun, S.Kubono, C.A.Bertulani, C.X.Yuan

Possible determination of high-lying single-particle components with (d, p) reactions

NUCLEAR REACTIONS 12C, 24Mg, 28Si, 40Ca(d, p), E=51.93 MeV; analyzed experimental σ(θ) distributions, spectroscopic amplitudes for neutrons in normal and high-lying single-particle components in the ground and excited states by fitting the angular distributions of the ground and the j-forbidden excited states simultaneously, effects of one-step transfer (OST), two-step transfer (TST) and inelastic excitation processes in neutron pickup reactions. Coupled reaction channel calculations.

doi: 10.1103/PhysRevC.98.044622
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2018XU12      Int.J.Mod.Phys. E27, 1850099 (2018)

Y.-Li.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

Global phenomenological optical model potentials for 8, 10, 11B projectiles

NUCLEAR REACTIONS 28,30Si, 40Ca, 58Ni, 208Pb, 209Bi(11B, 11B), E<100 MeV; 7Li, 9Be, 12C, 28Si, 58Ni, 208Pb(8B, 8B), E < 100 MeV; 16O, 28Si, 120Sn, 208Pb, 232Th(10B, 10B), E<100 MeV; analyzed available data for 11B; deduced global phenomenological optical model potential for 11B, calculated σ.

doi: 10.1142/S0218301318500994
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2017GU06      Phys.Rev. C 95, 034614 (2017)

H.Guo, H.Liang, Y.Xu, Y.Han, Q.Shen, C.Cai, T.Ye

Microscopic optical potential for 6He

NUCLEAR REACTIONS 12C(6He, 6He), E=8.79, 9.18, 9.9, 18, 230, 250 MeV; 27Al(6He, 6He), E=9.54, 11.0, 12.0, 13.4 MeV; 51V(6He, 6He), E=15.4, 23.0 MeV; 58Ni(6He, 6He), E=9.0, 10.0, 12.2, 16.5, 21.7 MeV; 64Zn(6He, 6He), E=10.0, 13.6 MeV; 65Cu(6He, 6He), E=19.56, 22.6, 30.05 MeV; 120Sn(6He, 6He), E=17.4, 18.05, 19.8, 20.05 MeV; 197Au(6He, 6He), E=10.1, 27.0 MeV; 209Bi(6He, 6He), E=14.71, 16.26, 17.8, 19.0, 19.14, 22.02, 22.5 MeV; 208Pb(6He, 6He), E=14.0, 16, 18, 22, 27, 56.6 MeV; 9Be(6He, 6He), E=16.2, 16.8, 21.3, 150 MeV; calculated differential σ(θ, E) relative to Rutherford cross section using microscopic optical potential (MOP) and global phenomenological 6He optical potential (GOP) based on experimental data. 28Si(6He, X), E<330 MeV; calculated total σ(E) using MOP and GOP. Comparison with experimental data. Isospin-dependent nucleon microscopic optical potential derived by using Green's function method through the nuclear matter approximation and the local density approximation based on the Skyrme nucleon-nucleon effective interaction.

doi: 10.1103/PhysRevC.95.034614
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2017GU11      Nucl.Sci.Eng. 186, 156 (2017)

H.Guo, Y.Xu, Y.Han, Q.Shen, T.Ye, W.Sun

Calculation and Evaluation for the n+51V Reaction

NUCLEAR REACTIONS 51V(n, n), E<300 MeV; calculated σ, σ(E), σ(θ), σ(θ, E). Optical model, distorted wave Born approximation theory, Hauser-Feshbach theory, evaporation model, exciton model, and intranuclear cascade model, comparison with the experimental data and the evaluated results in ENDF/B-VII.1 and JENDL-4 libraries.

doi: 10.1080/00295639.2016.1273008
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2017HE19      Phys.Rev. C 96, 045801 (2017)

J.J.He, A.Parikh, Y.Xu, Y.H.Zhang, X.H.Zhou, H.S.Xu

Thermonuclear 46Cr (p, γ) 47Mn rate in type-I x-ray bursts

NUCLEAR REACTIONS 46Cr(p, γ)47Mn, T9=0.01-2.0; analyzed astrophysical thermonuclear reaction rates, and proton resonances in 47Mn using known structure information and parameters in the ENSDF database for the mirror nucleus 47Ti. Comparison with previous statistical model and shell-model calculations. Pointed out need for experimental studies of the level structure of 47Mn near the proton threshold to improve model predictions. Relevance to Type-I x-ray bursts (XRBs).

doi: 10.1103/PhysRevC.96.045801
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2017WE03      Chin.Phys.C 41, 054104 (2017)

C.Wen, Y-P.Xu, D.-Y.Pang, Y.-L.Ye

Quenching of neutron spectroscopic factors of radioactive carbon isotopes with knockout reactions within a wide energy range

NUCLEAR REACTIONS C(15C, X), E=54, 62 MeV; Be(15C, X), E=103, 700 MeV; C(16C, X), E=55, 83 MeV; Be(16C, X), E=62, 700 MeV; C(17C, X), E=49, 79, 904 MeV; Be(17C, X), E=62, 700 MeV; C(18C, X), E=43, 80 MeV; Be(18C, X), E=700 MeV; C(19C, X), E=243, 910 MeV; Be(19C, X), E=57, 64, 88, 700 MeV; analyzed available data; deduced quenching factors of one-neutron spectroscopic factors. Comparison with systematics.

doi: 10.1088/1674-1137/41/5/054104
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2017XU05      Phys.Rev. C 96, 024621 (2017)

Y.Xu, H.Guo, Y.Han, Q.Shen

New extended Skyrme interaction for nuclear properties and nuclear reactions

NUCLEAR STRUCTURE 16O, 40,48Ca, 56,60Ni, 88Sr, 90Zr, 114Sn, 146Gd, 204Hg, 206,208Pb; calculated relative deviations of charge radii and energies per nucleon using SkC17, SkC, and GS2 Skyrme interactions. 208Pb; calculated neutron and proton single-particle energy levels near the Fermi surface using various Skyrme interactions, and compared with experimental data.

NUCLEAR REACTIONS 56Fe, 208Pb(n, X), E=0.1-100 MeV; calculated total and non-elastic σ(E) using SkC17, SkC, GS2, and SkOP4 Skyrme interactions, and compared with experimental data. 24Mg, 54,58Fe, 59Co, 90Zr, 93Nb, 92,96,98,100Mo, 120Sn, 206,208Pb(n, n), E=11.0 MeV; 28Si, 40Ca, 56Fe, 90Zr, 120Sn, 208Pb(n, n), E=65.0 MeV; 56Fe, 208Pb(n, n), E=1.68-96.0 MeV; 100Mo(n, n), E=0.34-26.0 MeV; 12C(n, n), E=0.5-94.8 MeV; 238U(n, n), E=4.5=10 MeV; 181Ta(n, n), E=0.32-15.2 MeV; 54Fe(polarized n, n), E=9.94, 13.92, 16.93 MeV; 89Y(polarized n, n), E=9.95, 13.93, 16.93 MeV; 208Pb(polarized n, n), E=5.97, 6.97, 7.96, 8.96, 9.95, 13.9, 23.0 MeV;calculated σ(θ, E), analyzing powers using different Skyrme interaction parameters; deduced SkC17 Skyrme interaction by simultaneously fitting variety of experimental data. Extended Skyrme interaction involving additional momentum- and density-dependent terms.

doi: 10.1103/PhysRevC.96.024621
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2017XU06      Phys.Rev. C 96, 024902 (2017)

Y.Xu, P.Moreau, T.Song, M.Nahrgang, S.A.Bass, E.Bratkovskaya

Traces of nonequilibrium dynamics in relativistic heavy-ion collisions

doi: 10.1103/PhysRevC.96.024902
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2017XU08      Nucl.Phys. A967, 668 (2017)

Y.Xu, M.Nahrgang, J.E.Bernhard, S.Cao, S.A.Bass

A data-driven analysis of the heavy quark transport coefficient

doi: 10.1016/j.nuclphysa.2017.05.035
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2017XU09      Int.J.Mod.Phys. E26, 1750065 (2017)

Y.Xu, H.Guo, Y.Han, Q.Shen

Isospin dependence of the nucleon density distributions

NUCLEAR STRUCTURE 40,48Ca, 124Sn, 208Pb; calculated proton density distributions, rms radii. Comparison with available data.

doi: 10.1142/S0218301317500653
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2016MA82      Nuovo Cim. C 39, 360 (2016)

C.Matei, D.L.Balabanski, O.Tesileanu, Y.Xu, M.La Cognata, C.Spitaleri

Nuclear astrophysics measurements with ELISSA at ELI-NP

NUCLEAR REACTIONS 3H(α, γ), E(cm)<9 MeV; Calculated S-factor. Comparison with available data.

doi: 10.1393/ncc/i2016-16360-4
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2016XU02      Int.J.Mod.Phys. E25, 1650013 (2016)

Y.-L.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

The neutron microscopic optical potential based on skyrme interaction

NUCLEAR REACTIONS 24Mg, 54,56Fe, 59Co, 90Zr, 93Nb, 92,96,98,100Mo, 120Sn, 206,208Pb(n, n), E=11 MeV; 12C, 16O, 23Na, 14N, 232Th, 235,238U, 239Pu(n, X), E=0.1-100 MeV; calculated σ(θ), σ. Comparison with experimental data.

doi: 10.1142/S0218301316500130
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2016XU05      Astrophys.J. 827, 17 (2016)

Y.Xu, B.Xiong, Y.C.Chang, C.Y.Ng

Absolute Integral Cross Sections for the State-selected Ion-Molecule Reaction N+2(X2Σg+; ν+ = 0-2) + C2H2 in the Collision Energy Range of 0.03-10.00 eV

NUCLEAR REACTIONS C, H(14N, p), (14N, E), E=0.03-10.00 eV; measured reaction products; deduced integral σ for charge and hydrogen-atom transfers.

doi: 10.3847/0004-637X/827/1/17
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2015DE34      Phys.Part. and Nucl.Lett. 12, 703 (2015)

A.S.Denikin, S.M.Lukyanov, N.K.Skobelev, Yu.G.Sobolev, E.I.Voskoboynik, Yu.E.Penionzhkevich, W.H.Trzaska, G.P.Tyurin, V.Burjan, V.Kroha, J.Mrazek, S.Piskor, V.Glagolev, Y.Xu, S.V.Khlebnikov, M.N.Harakeh, K.A.Kuterbekov, Yu.Tuleushev

Inelastic scattering and clusters transfer in 3, 4He + 9Be reactions

NUCLEAR REACTIONS 9Be(α, α), (α, α'), (α, 3He), (α, t), (3He, 6Li), (3He, 6Be), E ∼ 50 MeV; measured reaction products, spectra of total energies; deduced σ(θ), optical potential parameters. Comparison with DWBA calculations.

doi: 10.1134/S1547477115050052
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0789.


2015HE25      Nucl.Instrum.Methods Phys.Res. B361, 517 (2015)

M.He, Y.Xu, Y.Guan, H.Shen, L.Du, C.Hongtao, K.Dong, S.Jiang, X.Yang, X.Wang, X.d.Ruan, J.Liu, S.Wu, Q.Zhao, L.Cai, F.Pang

Determination of cross sections of 60Ni(n, 2n)59Ni induced by 14 MeV neutrons with accelerator mass spectrometry

NUCLEAR REACTIONS 60Ni(n, 2n), E≈14 MeV; measured reaction products; deduced σ. Comparison with ENDF/B-VII.0 and JENDL-3.3 evaluated nuclear libraries.

doi: 10.1016/j.nimb.2015.01.060
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Data from this article have been entered in the EXFOR database. For more information, access X4 dataset32736.


2015XU04      Int.J.Mod.Phys. E24, 1550005 (2015)

Y.-L.Xu, H.-R.Guo, Y.-L.Han, Q.-B.Shen

Applicability of the systematic helium-3 potential for triton-nucleus reactions

NUCLEAR REACTIONS 28Si, 58Ni, 116Sn, 208Pb(t, t), (3He, 3He), E<60 MeV/nucleon; calculated σ; deduced optical model potential parameters. Comparison with available data.

doi: 10.1142/S0218301315500056
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2015ZH41      Phys.Rev. C 92, 054616 (2015)

Q.Z.Zhao, X.M.Wang, W.Wang, M.He, K.J.Dong, C.J.Xiao, X.D.Ruan, H.T.Shen, S.Y.Wu, X.R.Yang, L.Dou, Y.N.Xu, L.Cai, F.F.Pang, H.Zhang, Y.J.Pang, S.Jiang

Determination of the α-decay half-life of 210Po based on film and slice bismuth samples at room temperature

RADIOACTIVITY 210Po(α)[from 209Po(n, γ), E=thermal]; measured Eα, Iα, T1/2 for a film sample of Bi2O3 and slice sample of Bi metal; deduced no difference in T1/2 using samples with two different physical configurations. Comparison with the recommended value in the ENSDF database.

doi: 10.1103/PhysRevC.92.054616
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2014GU01      Nucl.Phys. A922, 84 (2014)

H.Guo, Y.Xu, H.Liang, Y.Han, Q.Shen

Microscopic optical model potential for triton

NUCLEAR REACTIONS A=6-232(t, t), (t, X), E=threshold-60 MeV/nucleon; calculated triton microscopic optical model potential, reaction σ, elastic scattering σ(θ). Compared with some data.

doi: 10.1016/j.nuclphysa.2013.11.007
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2014HA17      Nucl.Data Sheets 118, 132 (2014)

Y.Han, Y.Xu, H.Liang, H.Guo, C.Cai, Q.Shen

Theoretical Calculation of Actinide Nuclear Reaction Data

doi: 10.1016/j.nds.2014.04.018
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2014XU01      J.Phys.(London) G41, 015101 (2014)

Y.Xu, H.Guo, Y.Han, Q.Shen

New Skyrme interaction parameters for a unified description of the nuclear properties

NUCLEAR REACTIONS 28Si, 56Fe, 208Pb(n, X), (n, n), 27Al, 90Zr, 208Pb, 232Th(p, p), E<100 MeV; calculated σ, σ(θ). Skyrme-Hartree-Fock approach, comparison with available data.

doi: 10.1088/0954-3899/41/1/015101
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2014XU09      Phys.Rev. C 90, 024604 (2014)

Y.Xu, S.Goriely, A.J.Koning, S.Hilaire

Systematic study of neutron capture including the compound, pre-equilibrium, and direct mechanisms

NUCLEAR REACTIONS 16,18O, 22Ne, 26Mg, 27Al, 37Cl, 48Ca, 61Ni, 97Mo, 112Sn, 176Lu, 208Pb, 232Th(n, γ), E=0.001-10 MeV; calculated total capture σ(E) for three processes of compound-nucleus capture (CNC), pre-equilibrium capture (PEC), and direct capture (DIC) using Hauser-Feshbach model, the exciton model, and potential model, respectively, and Compared with experimental data. Z=8-100, N=10-180; calculated total neutron-capture cross sections and astrophysical reaction rates using TALYS code for about 8000 nuclei. Impact of the newly determined reaction rates on the r process abundances.

doi: 10.1103/PhysRevC.90.024604
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2013HA04      Ann.Nucl.Energy 55, 75 (2013)

Y.Han, Y.Xu, C.Cai, Q.Shen

Double differential cross sections of light charged particle emission of n + 27Al reaction

NUCLEAR REACTIONS 27Al(n, xp), (n, xd), (n, xt), (n, xα), (n, 3He), E<40 MeV; calculated σ(E, θ), σ(E). Comparison with available data.

doi: 10.1016/j.anucene.2012.11.031
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2013XU06      Phys.Rev. C 87, 044605 (2013)

Y.P.Xu, D.Y.Pang

Toward a systematic nucleus-nucleus potential for peripheral collisions

NUCLEAR REACTIONS 40Ca(6Li, 6Li), E=99.0, 156.0, 210.0, 240.0 MeV; 48Ca(6Li, 6Li), E=240.0 MeV; 58Ni(6Li, 6Li), E=12, 20, 34.0, 73.7, 90.0, 99.0, 240.0 MeV; 58Fe(6Li, 6Li), E=15 MeV; 65Cu(6Li, 6Li), E=25 MeV; 70Ge(6Li, 6Li), E=28 MeV; 89Y(6Li, 6Li), E=60.0 MeV; 90Zr(6Li, 6Li), E=70.0, 73.7, 99.0, 210.0, 240.0 MeV; 92,94,96Zr(6Li, 6Li), E=70.0 MeV; 116Sn(6Li, 6Li), E=20, 240.0; 120Sn(6Li, 6Li), E=44.0, 90.0; 124Sn(6Li, 6Li), E=73.7 MeV; 144Sm(6Li, 6Li), E=21, 30.1, 32.2, 35.1, 42.3 MeV; 208Pb(6Li, 6Li), E=25, 31.0, 33.0, 35.0, 39.0, 50.6, 73.7, 90.0, 99.0, 156.0, 210.0 MeV; 209Bi(6Li, 6Li), E=32.8, 36.0, 40.0 MeV; 40,48Ca(7Li, 7Li), E=34.0, 88.0 MeV; 44Ca(7Li, 7Li), E=34.0; 48Ca(7Li, 7Li), E=88 MeV; 54Fe(7Li, 7Li), E=36.0, 42.0, 48.0 MeV; 56Fe(7Li, 7Li), E=34.0; 58Ni(7Li, 7Li), E=34.0, 42.0, 73.7, 90, 99 MeV; 59Co(7Li, 7Li), E=12, 18 MeV; 60Ni(7Li, 7Li), E=34.0 MeV; 65Cu(7Li, 7Li), E=2 MeV; 80Se(7Li, 7Li), E=14, 23 MeV; 89Y(7Li, 7Li), E=60.0 MeV; 90Zr(7Li, 7Li), E=34.0, 70, 99 MeV; 118Sn(7Li, 7Li), E=48.0 MeV; 120Sn(7Li, 7Li), E=90 MeV; 124Sn(7Li, 7Li), E=73.7 MeV; 144Sm(7Li, 7Li), E=21.6, 30.1, 35.1, 40.8, 42.3, 52.0 MeV; 208Pb(7Li, 7Li), E=27, 33.0, 39.0, 42.0, 52.0, 73.7 MeV; 208Pb(12C, 12C), E=58.9.64.9, 74.9, 84.9 MeV; 208Pb(16O, 16O), E=80, 90, 102 MeV; 12C, 28Si, 40Ca, 90Zr, 208Pb(16O, 16O), E=94 MeV/nucleon; 60Ni, 120Sn, 208Pb(40Ar, 40Ar), E=44 MeV/nucleon; 40Ca, 58Ni, 96Mo(32S, 32S), E=151.5, 107.3, 180 MeV; analyzed σ(E, θ) data; deduced optical model parameters, and comparison with experimental data. 27Al, 40Ca, 54,56,57Fe, 64,66,68Zn, 89Y, Ag(12C, X), E=30, 83 MeV/nucleon; 12C, 27Al, 64Zn, 93Nb, 107Ag, 118Sn, 144,150,154Sm(20Ne, X), E=30 MeV/nucleon; 12C, 27Al, 51V, 54Fe, 107Ag, 118Sn, 208Pb(40Ar, X), E=44 MeV/nucleon; 27Al, 64Zn, 93Nb, 118Sn, 144Sm, 181Ta, 208Pb(40Ca, X), E=77 MeV/nucleon; analyzed total reaction cross sections with optical model calculations. A single-folding model based on Bruyeres Jeukenne-Lejeune-Mahaux (JLMB) nucleon-nucleus potential.

doi: 10.1103/PhysRevC.87.044605
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2013XU07      Astrophys.J. 769, 72 (2013)

Y.Xu, Y.C.Chang, Z.Lu, C.Y.Ng

Absolute Integral Cross Sections and Product Branching Ratios for the Vibrationally Selected Ion-Molecule Reactions: N+2(X2Σ+g+ =0-2) + CH4

doi: 10.1088/0004-637X/769/1/72
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2013XU14      Nucl.Phys. A918, 61 (2013)

Y.Xu, K.Takahashi, S.Goriely, M.Arnould, M.Ohta, H.Utsunomiya

NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number A ≤ 16

COMPILATION 2,3H, 3He, 6,7Li, 7,9Be, 10,11B, 12,13C, 13,14,15N(p, X), (α, X), E≈0.1 keV-1 MeV;2,3H, 3He(d, X), E≈0.1 keV-1 MeV;3He(3He, 2p), E≈0.1 keV-1 MeV; compiled, evaluated Q-value, σ, S-factor, reaction rates using DWBA, potential models; deduced model parameters.

doi: 10.1016/j.nuclphysa.2013.09.007
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2013zu01      Hyperfine Interactions 220, 87 (2013)

Y.Zuo, Y.Zheng, Y.Xu, B.Cui, L.Li, Y.Ma, F.Ping, D.Yuan, S.Gao, S.Zhu

Production of 62Zn radioactive nuclear beam and on-line PAC investigation of quadrupole interaction in nano-magnetic material Fe73.5Cu1Nb3Si13.5B9

NUCLEAR REACTIONS 63Cu(p, 2n), E=22.9 MeV; Cd(p, X)111In, E=16.9 MeV; 186W(d, p), E=12.6 MeV; measured reaction products, Eγ, Iγ; deduced σ, spin rotation functions, quadrupole interaction frequencies. Perturbed angular correlation (PAC) and positron annihilation spectroscopy (PAS).

doi: 10.1007/s10751-013-0848-Z
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2012CO01      Astrophys.J. 744, 158 (2012)

A.Coc, S.Goriely, Y.Xu, M.Saimpert, E.Vangioni

Standard Big Bang Nucleosynthesis up to CNO with an Improved Extended Nuclear Network

NUCLEAR REACTIONS 7Li(d, γ), (t, n), (t, p), (d, n), 8Li(α, n), 11B(d, n), (d, p), (n, γ), 11C(d, p), (n, α), E<10 MeV; calculated astrophysical reaction rates. TALYS code, comparison with NACRE compilations.

doi: 10.1088/0004-637X/744/2/158
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2012HA16      Ann.Nucl.Energy 46, 179 (2012)

Y.Han, Y.Xu, H.Liang, H.Guo, C.Cai, Q.Shen

The analysis of n+237Np reactions for energies up to 200 MeV

NUCLEAR REACTIONS 237Np(n, γ), (n, F), (n, 2n), (n, xn), (n, xp), (n, xd), (n, xt), (n, xα) E<200 MeV; calculated σ, σ(θ, E), σ(θ), σ(E). Optical model, the intra-nuclear cascade model, the unified Hauser-Feshbach theory, comparison with ENDF/B-VII and JENDL-3 libraries and available data.

doi: 10.1016/j.anucene.2012.03.013
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2012HA24      Nucl.Sci.Eng. 172, 102 (2012)

Y.Han, Y.Xu, H.Liang, H.Guo, C.Cai, Q.Shen

Theoretical Calculations and Analysis of n + 27Al Reaction

NUCLEAR REACTIONS 27Al(n, X), (n, n), (n, n'), (n, p), (n, γ), (n, d), (n, t), (n, α), (n, 2n), (n, xn), (n, xp), (n, xα), E<200 MeV; calculated σ, σ(θ), σ(E), σ(θ, E). Comparison with ENDF/B-VII and JENDL-3 evaluated nuclear libraries.

doi: 10.13182/NSE11-28
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2012XU09      Phys.Rev. C 86, 045801 (2012)

Y.Xu, S.Goriely

Systematic study of direct neutron capture

NUCLEAR STRUCTURE Z=8-102; calculated E1, E2, and M1 neutron direct capture reaction rates of astrophysical interest for 6400 nuclei at temperature T9=1.

NUCLEAR REACTIONS 16O, 18O, 22Ne, 26Mg, 27Al, 36S, 37Cl, 46,48Ca, 122,132Sn(n, γ), E=1-10000 keV; calculated total neutron direct capture cross sections. Comparison with experimental data.

doi: 10.1103/PhysRevC.86.045801
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2011GU15      Phys.Rev. C 83, 064618 (2011)

H.Guo, Y.Xu, H.Liang, Y.Han, Q.Shen

4He microscopic optical model potential

NUCLEAR REACTIONS 12C, 58Ni, 116Sn, 208Pb(α, X), E=20-300 MeV; calculated radial dependence of real and imaginary parts of the potential, volume integral and rms radii. 12C, 16O, 28Si, 40Ca, 58,60Ni, 112,116,120,124Sn, 208Pb, 209Bi(α, X), E=5-200 MeV; calculated reaction σ(E). 62,64Ni, 63,65Cu, 64,66,68,70Zn, 70,72Ge(α, α), E=25.0 MeV; 94Mo, 107Ag, 116,122,124Sn(α, α), E=25.2 MeV; 20,22Ne, 24,26Mg, 28Si, 40Ar, 40,42,44,48Ca, 56Fe, 56,58,60,62Ni, 90Zr, 124Sn, 208Pb(α, α), E=104 MeV; 16O, 46,48Ti, 58Ni, 116Sn, 197Au(α, α), E=240 MeV; 12C, 58Ni, 90Zr, 116Sn, 144Sm, 208Pb(α, α), E=386.0 MeV; calculated σ(θ). 12C(α, α), E=120.0-400 MeV; 58Ni(α, α), E=29.0-386 MeV; 24Mg(α, α), E=39.0-172.5 MeV; 107Ag(α, α), E=15.0-43.0 MeV; 116Sn(α, α), E=23.3-386 MeV; 124Sn(α, α), E=23.3-104 MeV; 208Pb(α, α), E=23.6-386.0 MeV; 209Bi(α, α), E=19.0-104 MeV; calculated σ(E, θ); deduced 4He microscopic optical model potential by Green¬Ěs function method. Comparison with experimental data.

doi: 10.1103/PhysRevC.83.064618
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2011HA28      Ann.Nucl.Energy 38, 1852 (2011)

Y.Han, Y.Xu, H.Liang, H.Guo, Q.Shen

Calculation and evaluations for n + 63, 65, nat.Cu reactions

NUCLEAR REACTIONS Cu, 63,65Cu(n, X), (n, n), (n, n'), (n, γ), (n, p), (n, d), (n, α), (n, 2n), (n, 3n), E<250 MeV; calculated σ, σ(θ). Optical model, preequilibrium theory, comparison with ENDF/B-VII.0, JENDL-3.3 evaluated nuclear libraries and experimental data.

doi: 10.1016/j.anucene.2011.05.016
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2011HA29      Ann.Nucl.Energy 38, 1950 (2011)

Y.Han, Y.Xu, H.Liang, H.Guo, Q.Shen

Double differential cross sections of n + 63, 65, nat.Cu reactions

NUCLEAR REACTIONS Cu, 63,65Cu(n, X), (n, xn), (n, xp), (n, xα), (n, xd), (n, xt), E<200 MeV; calculated σ(θ, E). Optical model, unified Hauser-Feshbach and exciton model, comparison with ENDF/B-VII.0, JENDL-3.3 evaluated nuclear libraries and experimental data.

doi: 10.1016/j.anucene.2011.05.001
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2011HA44      J.Korean Phys.Soc. 59, 855s (2011)

Y.Han, Y.Xu, H.Liang, H.Guo, Q.Shen, C.Cai

The Theoretical Calculation of Cross Section and Spectrum for n+238U Reaction up to 150 MeV

NUCLEAR REACTIONS 238U(n, f), (n, xn), (n, d), (n, t), (n, p), (n, α), E=0-200 MeV; calculated σ, dσ(E, θ) using different reaction models.

doi: 10.3938/jkps.59.855
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2010HA06      Phys.Rev. C 81, 024616 (2010)

Y.Han, Y.Xu, H.Liang, H.Guo, Q.Shen

Global phenomenological optical model potential for nucleon-actinide reactions at energies up to 300 MeV

NUCLEAR REACTIONS 232Th, 233,235,238U, 237Np, 239,240,242Pu, 241Am(n, X), E=0.01-300 MeV; calculated total σ. 235,238U(n, n), E=0.01-300 MeV; calculated σ. 232Th, 235,238U, 239Pu(n, n'), E=0.1-300 MeV; calculated non-inelastic σ. 232Th, 235,238U, 239Pu(n, n), (n, n'), E=0.14-15.2 MeV; 238U(n, n), E=96 MeV; calculated σ(θ) for elastic σ, inelastic σ and elastic+inelastic σ. 232Th, 238U(p, X), E=0-300 MeV; calculated σ. 232Th, 235,238U(p, p), (p, p'), E=16-95 MeV; calculated σ(θ). global phenomenological optical model potential. Deduced of neutron and proton global optical model potential parameters. Comparison and analysis with experimental data.

doi: 10.1103/PhysRevC.81.024616
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2010YU04      Nucl.Phys. A834, 97c (2010)

Z.Yu, G.-Z.Liu, M.-F.Zhu, Y.Xu, E.-G.Zhao

Thermal neutron stars including the hyperon-hyperon interactions

doi: 10.1016/j.nuclphysa.2010.01.029
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2010ZH03      Chin.Phys.Lett. 27, 022102 (2010)

Y.-N.Zheng, D.-M.Zhou, D.-Q.Yuan, Y.zuo, P.fan, M.Mihara, K.Matsuta, M.Fukuda, T.Minamisono, T.Suzuki, Y.-J.Xu, J.-Z.Zhu, Z.-Q.Wang, H.-L.Luo, X.-Z.Zhang, S.-Y.Zhu

Nuclear Structure and Magnetic Moment of the Unstable 12B-12N Mirror Pair

NUCLEAR MOMENTS 12B, 12N; measured β-NMR spectra; deduced magnetic moments, magic numbers. Comparison with shell model calculations.

doi: 10.1088/0256-307X/27/2/022102
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2010ZH38      Nucl.Phys. A834, 761c (2010)

Y.Zheng, Y.Zuo, D.Yuan, D.Zhou, Y.Xu, P.Fan, J.Zhu, Z.Wang, S.Zhu

Investigation of Radiation Damage in Stainless steel, Tungsten and Tantalum by Heavy Ion Irradiations

doi: 10.1016/j.nuclphysa.2010.01.139
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2009IJ01      Phys.Rev. C 80, 034322 (2009)

Q.A.Ijaz, W.C.Ma, H.Abusara, A.V.Afanasjev, Y.B.Xu, R.B.Yadav, Y.C.Zhang, M.P.Carpenter, R.V.F.Janssens, T.L.Khoo, T.Lauritsen, D.T.Nisius

Excited superdeformed bands in 154Dy and cranked relativistic mean field interpretation

NUCLEAR REACTIONS 122Sn(36S, 4n), E=165 MeV; measured Eγ, Iγ, γγ-coin using Gammasphere array. 154Dy; deduced levels, J, π, superdeformed bands, dynamic moments of inertia, neutron single particle energies. Comparison with the cranked relativistic mean field calculations.

doi: 10.1103/PhysRevC.80.034322
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2009LU19      Phys.Rev. A 80, 051201 (2009)

H.Y.Lu, J.S.Liu, C.Wang, W.T.Wang, Z.L.Zhou, A.H.Deng, C.Q.Xia, Y.Xu, X.M.Lu, Y.H.Jiang, Y.X.Leng, X.Y.Liang, G.Q.Ni, R.X.Li, Z.Z.Xu

Efficient fusion neutron generation from heteronuclear clusters in intense femtosecond laser fields

NUCLEAR REACTIONS 2H(γ, xnyp), E not given; measured densities and average kinetic energies of deuterium ions; deduced fusion neutron yields as a function of laser energy.

doi: 10.1103/PhysRevA.80.051201
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2009TA07      Phys.Rev. C 79, 051901 (2009)

Z.Tang, Y.Xu, L.Ruan, G.van Buren, F.Wang, Z.Xu

Spectra and radial flow in relativistic heavy ion collisions with Tsallis statistics in a blast-wave description

doi: 10.1103/PhysRevC.79.051901
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2009XU02      Chem.Phys. 18, 1421 (2009)

Y.Xu, W.Xu, Y.-G.Ma, X.-Z.Cai, J.-G.Chen, G.-T.Fan, G.-W.Fan, W.Guo, W.Luo, Q.-Y.Pan, W.-Q.Shen, L.-F.Yang

Determination of the stellar reaction rate for 12C(α, γ)16O: using a new expression with the reaction mechanism

NUCLEAR REACTIONS 12C(α, γ);E not given; calculated astrophysical reaction rates.

doi: 10.1088/1674-1056/18/4/023
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2009XU06      Nucl.Phys. A830, 701c (2009)

Y.Xu, and the STAR collaboration

Measurements of neutral and charged kaon production at high pT up to 15 GeV/c at STAR

doi: 10.1016/j.nuclphysa.2009.09.059
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2009YA25      Chin.Phys.C 33, Supplement 1, 196 (2009)

W.-F.Yang, Z.-Z.Zhao, S.-G.Yuan, Y.-B.Xu, X.T.Lu

Dependence of the cross sections for Ir isotopes on the values of Qgg in the heavy ion collision

NUCLEAR REACTIONS 197Au(12C, X)184Ir/185Ir/186Ir/187Ir/189Ir/190Ir/192Ir/194Ir/195Ir/196Ir, E=47 MeV/nucleon; measured Eγ, Iγ; deduced σ.

doi: 10.1088/1674-1137/33/S1/063
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2009YU11      Chin.Phys.C 33, Supplement 1, 191 (2009)

S.-G.Yuan, Y.-B.Xu, H.-J.Ding, W.-F.Yang, Y.-H.Xiao, Y.-N.Niu

Gamma decay of the lowly excited states of 189Re

RADIOACTIVITY 189W(β-) [from 192Os(n, α)189Re, E=14 MeV];measured Eγ, Iγ, X-γ-coin., γ-γ-coin.; deduced decay scheme, J, π, energies.

doi: 10.1088/1674-1137/33/S1/061
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2007XU04      J.Radioanal.Nucl.Chem. 272, 227 (2007)

Y.B.Xu, S.D.Zhang, H.J.Ding, X.T.Lu, W.F.Yang, S.G.Yuan, Y.H.Xiao, Y.N.Niu

Production cross section of 236Th in the interaction of 238U with 60 MeV/u 18O ions

NUCLEAR REACTIONS 238U(18O, 20Ne), E=60 MeV/nucleon; measured Eγ, Iγ; deduced σ.

doi: 10.1007/s10967-007-0505-6
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2006QI03      Yuan.Wul.Ping. 23, 400 (2006); Nucl.Phys.Rev. 23, 404 (2006)

Z.Qin, X.-l.Wu, H.-j.Ding, W.Wu, W.-x.Huang, X.-g.Lei, Y.-b.Xu, X.-h.Yuan, B.Guo, W.-f.Yang, Z.-g.Gan, H.-m.Fan, J.-S.Guo, H.-s.Xu, G.-q.Xiao

Alpha-decay Properties of 266Bh

RADIOACTIVITY 266Bh(α) [from 243Am(26Mg, X), E=162 MeV]; measured decay products, Eα, Iα, α-α correl.; deduced T1/2. Comparison with Q-N systematics.

ATOMIC MASSES 266Bh, 262Db; measured decay products, Eα, Iα, α-α correl.; deduced Q-value. Comparison with Q-N systematics.


2006TA02      Phys.Rev.Lett. 96, 034301 (2006); Erratum Phys.Rev.Lett. 96, 179903 (2006)

R.P.Taleyarkhan, C.D.West, R.T.Lahey, Jr., R.I.Nigmatulin, R.C.Block, Y.Xu

Nuclear Emissions During Self-Nucleated Acoustic Cavitation

NUCLEAR REACTIONS 2H(d, n), E not given; measured Eγ, En for deuterated benzene and acetone mixtures. Acoustic inertial confinement.

doi: 10.1103/PhysRevLett.96.034301
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Note: The following list of authors and aliases matches the search parameter Y.Xu: , Y.B.XU, Y.F.XU, Y.G.XU, Y.J.XU, Y.L.XU, Y.N.XU, Y.P.XU, Y.S.XU, Y.W.XU, Y.Y.XU