NSR Query Results

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NSR database version of April 27, 2024.

Search: Author = Y.Z.Qian

Found 20 matches.

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2022LI28      Few-Body Systems 63, 43 (2022)

W.P.Liu, Z.H.Li, J.J.He, X.D.Tang, G.Lian, J.Su, Y.P.Shen, Z.An, F.Q.Chao, J.J.Chang, L.H.Chen, H.Chen, X.J.Chen, Y.H.Chen, Z.J.Chen, B.Q.Cui, X.C.Du, X.Fang, C.B.Fu, L.Gan, B.Guo, Z.Y.Han, X.Y.Guo, G.Z.He, J.R.He, A.Heger, S.Q.Hou, H.X.Huang, N.Huang, B.L.Jia, L.Y.Jiang, S.Kubono, J.M.Li, M.C.Li, K.A.Li, E.T.Li, T.Li, Y.J.Li, M.Lugaro, X.B.Luo, H.Y.Ma, S.B.Ma, D.M.Mei, W.Nan, W.K.Nan, N.C.Qi, Y.Z.Qian, J.C.Qin, J.Ren, C.S.Shang, L.T.Sun, W.L.Sun, W.P.Tan, I.Tanihata, S.Wang, P.Wang, Y.B.Wang, Q.Wu, S.W.Xu, S.Q.Yan, L.T.Yang, Y.Yang, X.Q.Yu, Q.Yue, S.Zeng, L.Zhang, H.Zhang, H.Y.Zhang, L.Y.Zhang, N.T.Zhang, P.Zhang, Q.W.Zhang, T.Zhang, X.P.Zhang, X.Z.Zhang, W.Zhao, J.F.Zhou, Y.Zho

Progress of Underground Nuclear Astrophysics Experiment JUNA in China

NUCLEAR REACTIONS 12C(α, γ), 13C(α, n), 25Mg(p, γ), 19F(p, α), E(cm)<600 keV; measured reaction products; deduced yields near the Gamow window. Comparison with available data.

doi: 10.1007/s00601-022-01735-3
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2022SC17      J.Phys.(London) G49, 110502 (2022)

H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations

Horizons: nuclear astrophysics in the 2020s and beyond

doi: https://dx.doi.org/10.1088/1361-6471/ac8890
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2020FI02      Phys.Rev. C 101, 025804 (2020)

T.Fischer, G.Guo, A.A.Dzhioev, G.Martinez-Pinedo, M.-R.Wu, A.Lohs, Y.-Z.Qian

Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current-neutrino interactions and inverse neutron decay

NUCLEAR REACTIONS 1H(ν-bar, e+)n, 1n(ν, e-)p, E<100 MeV; derived expressions for medium-dependent charged-current reactions in fully inelastic kinematics, including contribution from weak magnetism; implemented weak reaction rates in the supernova model; simulated core-collapse supernova explosions and proto-neutron star (PNS) deleptonization; analyzed subsequent neutrino signal depending on the treatment of weak interactions; investigated nuclear medium dependence at the mean-field level, with the inverse neutron decay as new opacity source; calculated complete nucleosynthesis outcome from core-collapse supernova explosion simulation.

doi: 10.1103/PhysRevC.101.025804
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2014QI02      J.Phys.(London) G41, 044002 (2014)

Y.-Z.Qian

Diverse, massive-star-associated sources for elements heavier than Fe and the roles of neutrinos

doi: 10.1088/0954-3899/41/4/044002
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2013XU02      Phys.Rev. C 87, 015805 (2013)

X.D.Xu, B.Sun, Z.M.Niu, Z.Li, Y.-Z.Qian, J.Meng

Reexamining the temperature and neutron density conditions for r-process nucleosynthesis with augmented nuclear mass models

ATOMIC MASSES A=80, 130, 195; calculated T9-neutron density conditions required for waiting-point nuclei with RMF, HFB-17, FRDM, and WS* nuclear mass models. Effects of uncertainty in S(n) for 78Ni, 82Zn, 191Tb, and 197Tm on the required T9-nn conditions. Precise mass measurements required for 76Ni, 78Ni, 82Zn, 131,132Cd. Relevance to r-process nucleosynthesis.

doi: 10.1103/PhysRevC.87.015805
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2011BA20      Phys.Rev.Lett. 106, 201104 (2011)

P.Banerjee, W.C.Haxton, Y.-Z.Qian

Long, Cold, Early r Process? Neutrino-Induced Nucleosynthesis in He Shells Revisited

NUCLEAR REACTIONS 4He(ν, nν), 3He(n, p), 3H(t, 2n), 4He(ν, νp), E ∼ 30 keV; calculated r-process yields; deduced ν-driven r-process mechanism.

doi: 10.1103/PhysRevLett.106.201104
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2010QI07      Nucl.Phys. A834, 627c (2010)

Y.-Z.Qian

Inferring stellar sources for the elements from astrophysical observations

doi: 10.1016/j.nuclphysa.2010.01.108
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2007NI12      667, L159 (2007)

H.Ning, Y.-Z.Qian, B.S.Meyer

r-Process Nucleosynthesis in Shocked Surface Layers of O-Ne-Mg Cores

doi: 10.1086/522372
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2005QI01      Nucl.Phys. A752, 550c (2005)

Y.-Z.Qian

Nuclear physics and astrophysics of the r-process

doi: 10.1016/j.nuclphysa.2005.02.118
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2004OL02      Phys.Rev. D 69, 027701 (2004)

K.A.Olive, M.Pospelov, Y.-Z.Qian, G.Manhes, E.Vangioni-Flam, A.Coc, M.Casse

Reexamination of the 187Re bound on the variation of fundamental couplings

RADIOACTIVITY 187Re(β-); analyzed T1/2 data; deduced bound on variability of fine-structure constant.

doi: 10.1103/PhysRevD.69.027701
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2004QI02      Nucl.Phys. A746, 335c (2004)

Y.-Z.Qian

The r-process: recent progress and needs for nuclear data

doi: 10.1016/j.nuclphysa.2004.09.041
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2003QI05      Prog.Part.Nucl.Phys. 50, 153 (2003)

Y.-Z.Qian

The Origin of the Heavy Elements: Recent Progress in the Understanding of the r-Process

doi: 10.1016/S0146-6410(02)00178-3
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2002QI06      Astrophys.J. 569, L103 (2002)

Y.-Z.Qian

Neutrino-Induced Fission and r-Process Nucleosynthesis

doi: 10.1086/340643
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2000QI01      Phys.Rep. 333-334, 77 (2000)

Y.-Z.Qian, G.J.Wasserburg

Stellar Abundances in the Early Galaxy and Two r-Process Components

doi: 10.1016/S0370-1573(00)00017-X
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1999QI03      Astrophys.J. 524, 213 (1999)

Y.-Z.Qian, P.Vogel, G.J.Wasserburg

Probing r-Process Production of Nuclei Beyond 209Bi with Gamma Rays

doi: 10.1086/307805
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1997HA16      Phys.Rev.Lett. 78, 2694 (1997)

W.C.Haxton, K.Langanke, Y.-Z.Qian, P.Vogel

Neutrino-Induced Nucleosynthesis and the Site of the r Process

NUCLEAR STRUCTURE A=124-126; A=183-187; analyzed postprocessed abundance distributions. A ≈ 195; analyzed postprocessing neutron emission probabilities; deduced consistency with neutrino induced nucleosynthesis, strong argument for a supernova r-process site.

doi: 10.1103/PhysRevLett.78.2694
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1997HO10      Nucl.Phys. A621, 397c (1997)

R.D.Hoffman, S.E.Woosley, Y.-Z.Qian

Model Independent r-Process Nucleosynthesis - Constraints on the Key Parameters

doi: 10.1016/S0375-9474(97)00278-9
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1997QI01      Phys.Rev. C55, 1532 (1997)

Y.-Z.Qian, W.C.Haxton, K.Langanke, P.Vogel

Neutrino-Induced Neutron Spallation and Supernova r-Process Nucleosynthesis

NUCLEAR STRUCTURE A=76-195; calculated r-process associated ν(e) capture rates, average neutron number, multiple neutron probabilities.

doi: 10.1103/PhysRevC.55.1532
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1997QI02      Nucl.Phys. A621, 363c (1997)

Y.-Z.Qian

Neutrino-Nucleus Interaction and Supernova r-Process Nucleosynthesis

doi: 10.1016/S0375-9474(97)00272-8
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1996FU16      Nucl.Phys. A606, 167 (1996)

G.M.Fuller, Y.-Z.Qian

Neutrino Gravitational Redshift and the Electron Fraction above Nascent Neutron Stars

doi: 10.1016/0375-9474(96)00268-0
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