NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = R.Lau Found 7 matches. 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
2020LA17 J.Phys.(London) G47, 035205 (2020) Sensitivity studies on the excited states of nuclei in beta decays in the r-process of neutron star mergers RADIOACTIVITY 194,195,196Lu(β-); calculated stellar beta decay rates.
doi: 10.1088/1361-6471/ab6c76
2018LA02 Nucl.Phys. A970, 1 (2018) Sensitivity tests on the rates of the excited states of positron decays during the rapid proton capture process of the one-zone X-ray burst model RADIOACTIVITY 60Zn, 64Ge, 68Se, 72Kr, 76Sr, 80Zr, 84Mo, 88Ru, 92Pd, 96Cd, 101,102,103,104,105,106Sn, 106Sb (β+), (EC); calculated gs T1/2 of waiting point of rapid proton capture nuclei, estimated 1st excited state T1/2 using one-zone X-ray burst model with and weak rates library. Compared with other calculations and available (stellar) data.
doi: 10.1016/j.nuclphysa.2017.10.009
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
2018LE17 Phys.Rev. C 98, 054322 (2018) S.M.Lenzi, M.A.Bentley, R.Lau, C.Aa.Diget Isospin-symmetry breaking corrections for the description of triplet energy differences NUCLEAR STRUCTURE A=18, 22, 26, 30, 34, 38, 42, 46, 50, 54, 58, 62, 66; calculated triplet energy differences (TEDs) between analog states in T=1 isobaric nuclei for various orbitals using large-scale shell model with monopole-pairing type single isotensor schematic interaction; deduced charge-independence breaking of the nuclear interaction. Comparison with experimental data.
doi: 10.1103/PhysRevC.98.054322
2014SC01 Nature(London) 505, 62 (2014) H.Schatz, S.Gupta, P.Moller, M.Beard, E.F.Brown, A.T.Deibel, L.R.Gasques, W.R.Hix, L.Keek, R.Lau, A.W.Steiner, M.Wiescher Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts NUCLEAR STRUCTURE 105Zr; calculated single-particle energy levels, J, π, hexadecapole deformation parameters.
doi: 10.1038/nature12757
2011ES06 Phys.Rev.Lett. 107, 172503 (2011) A.Estrade, M.Matos, H.Schatz, A.M.Amthor, D.Bazin, M.Beard, A.Becerril, E.F.Brown, R.Cyburt, T.Elliot, A.Gade, D.Galaviz, S.George, S.S.Gupta, W.R.Hix, R.Lau, G.Lorusso, P.Moller, J.Pereira, M.Portillo, A.M.Rogers, D.Shapira, E.Smith, A.Stolz, M.Wallace, M.Wiescher Time-of-Flight Mass Measurements for Nuclear Processes in Neutron Star Crusts ATOMIC MASSES 53,54,55Sc, 57Ti, 60,61V, 63Cr, 65,66Mn, 67,68Fe, 68,69,70,71Co, 74Ni; measured time of flight; deduced masses. Stellar nucleosynthesis implications.
doi: 10.1103/PhysRevLett.107.172503
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