NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = G.C.McLaughlin Found 34 matches. 2024VA02 Phys.Rev.Lett. 132, 052701 (2024) N.Vassh, X.Wang, M.Lariviere, T.Sprouse, M.R.Mumpower, R.Surman, Zh.Liu, G.C.McLaughlin, P.Denissenkov, F.Herwig Thallium-208: A Beacon of In Situ Neutron Capture Nucleosynthesis
doi: 10.1103/PhysRevLett.132.052701
2023LU01 Astrophys.J. 944, 144 (2023) K.A.Lund, J.Engel, G.C.McLaughlin, M.R.Mumpower, E.M.Ney, R.Surman The Influence of β-decay Rates on r-process Observables
doi: 10.3847/1538-4357/acaf56
2022OR02 Phys.Rev. C 105, L052802 (2022) R.Orford, N.Vassh, J.A.Clark, G.C.McLaughlin, M.R.Mumpower, D.Ray, G.Savard, R.Surman, F.Buchinger, D.P.Burdette, M.T.Burkey, D.A.Gorelov, J.W.Klimes, W.S.Porter, K.S.Sharma, A.A.Valverde, L.Varriano, X.L.Yan Searching for the origin of the rare-earth peak with precision mass measurements across Ce-Eu isotopic chains ATOMIC MASSES 152,153,154Ce, 152,153,154,156,157Pr, 157Nd, 161Pm, 163,165Eu; measured cyclotron frequency; deduced mass excess, solar abundances of rare-earth elements. Comparison to AME2016 and AME2020 evaluations, previous experimental data and calculations using Markov chain Monte Carlo (MCMC) technique. Canadian Penning Trap (CPT) with low-energy ion beams from the Californium Rare Isotope Breeder Upgrade(CARIBU) facility at Argonne National Laboratory. Systematics of CPT mass-measurements for Ce, Pr, Nd, Pm, Sm, Eu (Z=58-63).
doi: 10.1103/PhysRevC.105.L052802
2021HO13 Astrophys.J. 909, 21 (2021) E.M.Holmbeck, A.Frebel, G.C.McLaughlin, R.Surman, R.Fernandez, B.D.Metzger, M.R.Mumpower, T.M.Sprouse Reconstructing Masses of Merging Neutron Stars from Stellar r-process Abundance Signatures
doi: 10.3847/1538-4357/abd720
2021ZH02 Astrophys.J. 906, 94 (2021) Y.L.Zhu, K.A.Lund, J.Barnes, T.M.Sprouse, N.Vassh, G.C.McLaughlin, M.R.Mumpower, R.Surman Modeling Kilonova Light Curves: Dependence on Nuclear Inputs RADIOACTIVITY 254Cf, 254Cm, 258,259Fm, 267,269,270,271Rf, 273Db, 288Hs(SF); calculated total spontaneous fission heating, electron fractions using HFB22, HFB27, FRDM2012, UNEDF1 and ETFSI models.
doi: 10.3847/1538-4357/abc69e
2020SP04 Phys.Rev. C 101, 055803 (2020) T.M.Sprouse, R.Navarro-Perez, R.Surman, M.R.Mumpower, G.C.McLaughlin, N.Schunck Propagation of statistical uncertainties of Skyrme mass models to simulations of r-process nucleosynthesis ATOMIC MASSES Z=1-120; calculated atomic mass tables within the nuclear density functional theory (DFT) approach to nuclear structure with Skyrme energy density functionals (EDFs), and UNEDF1 parametrization. A=120-200; analyzed propagation of uncertainties in the Skyrme mass models using Bayesian statistics for the simulated r-process abundance patterns, by considering nuclear masses and the influence of the masses on β-decay and neutron capture rates.
doi: 10.1103/PhysRevC.101.055803
2019HO18 J.Phys.(London) G46, 083001 (2019) C.J.Horowitz, A.Arcones, B.Cote, I.Dillmann, W.Nazarewicz, I.U.Roederer, H.Schatz, A.Aprahamian, D.Atanasov, A.Bauswein, T.C.Beers, J.Bliss, M.Brodeur, J.A.Clark, A.Frebel, F.Foucart, C.J.Hansen, O.Just, A.Kankainen, G.C.McLaughlin, J.M.Kelly, S.N.Liddick, D.M.Lee, J.Lippuner, D.Martin, J.Mendoza-Temis, B.D.Metzger, M.R.Mumpower, G.Perdikakis, J.Pereira, B.W.O'Shea, R.Reifarth, A.M.Rogers, D.M.Siegel, A.Spyrou, R.Surman, X.Tang, T.Uesaka, M.Wang r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos
doi: 10.1088/1361-6471/ab0849
2018OR02 Phys.Rev.Lett. 120, 262702 (2018) R.Orford, N.Vassh, J.A.Clark, G.C.McLaughlin, M.R.Mumpower, G.Savard, R.Surman, A.Aprahamian, F.Buchinger, M.T.Burkey, D.A.Gorelov, T.Y.Hirsh, J.W.Klimes, G.E.Morgan, A.Nystrom, K.S.Sharma Precision Mass Measurements of Neutron-Rich Neodymium and Samarium Isotopes and Their Role in Understanding Rare-Earth Peak Formation ATOMIC MASSES 154,156,158,159,160Nd, 162,163,164Sm; measured cyclotron frequency ratios; deduced mass excess values. Comparison with AME16 evaluation.
doi: 10.1103/PhysRevLett.120.262702
2018ZH34 Astrophys.J. 863, L23 (2018) Y.Zhu, R.T.Wollaeger, N.Vassh, R.Surman, T.M.Sprouse, M.R.Mumpower, P.Moller, G.C.McLaughlin, O.Korobkin, T.Kawano, P.J.Jaffke, E.M.Holmbeck, C.L.Fryer, W.P.Even, A.J.Couture, J.Barnes Californium-254 and Kilonova Light Curves RADIOACTIVITY 254Cf(SF); calculated abundance, fission product yields, heating rates, mid-IR light curves.
doi: 10.3847/2041-8213/aad5de
2017AR04 Prog.Part.Nucl.Phys. 94, 1 (2017) A.Arcones, D.W.Bardayan, T.C.Beers, L.A.Bernstein, J.C.Blackmon, B.Messer, B.A.Brown, E.F.Brown, C.R.Brune, A.E.Champagne, A.Chieffi, A.J.Couture, P.Danielewicz, R.Diehl, M.El Eid, J.E.Escher, B.D.Fields, C.Frohlich, F.Herwig, W.R.Hix, C.Iliadis, W.G.Lynch, G.C.McLaughlin, B.S.Meyer, A.Mezzacappa, F.Nunes, B.W.O'Shea, M.Prakash, B.Pritychenko, S.Reddy, E.Rehm, G.Rogachev, R.E.Rutledge, H.Schatz, M.S.Smith, I.H.Stairs, A.W.Steiner, T.E.Strohmayer, F.X.Timmes, D.M.Townsley, M.Wiescher, R.G.T.Zegers, M.Zingale White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics
doi: 10.1016/j.ppnp.2016.12.003
2017MU08 J.Phys.(London) G44, 034003 (2017) M.R.Mumpower, G.C.McLaughlin, R.Surman, A.W.Steiner Reverse engineering nuclear properties from rare earth abundances in the r process COMPILATION A<250; compiled experimental nuclear reaction and structure data.
doi: 10.1088/1361-6471/44/3/034003
2016MU01 Prog.Part.Nucl.Phys. 86, 86 (2016); Erratum Prog.Part.Nucl.Phys. 87, 116 (2016) M.R.Mumpower, R.Surman, G.C.McLaughlin, A.Aprahamian The impact of individual nuclear properties on r-process nucleosynthesis
doi: 10.1016/j.ppnp.2015.09.001
2016SH39 Phys.Rev. C 94, 055802 (2016) T.Shafer, J.Engel, C.Frohlich, G.C.McLaughlin, M.Mumpower, R.Surman β decay of deformed r-process nuclei near A=80 and A=160, including odd-A and odd-odd nuclei, with the Skyrme finite-amplitude method RADIOACTIVITY 68,69,70,71,72Cr, 71,72,73,74,75Mn, 72,73,74,75,76Fe, 76,77Co, 80,81Cu, 84,85,86Zn, 86,87Ga, 86,87,88,89,90,91,92Ge, 89,90,91,92,93,94,95As, 92,93,94,95,96,97,98Se, 157,159,161,163,165,167Cs, 163,165,167,169,171,173,175La, 146,148,150,152,160,164,166,168,170,172,174,176Ce, 152,154,156,164,166,172,174,176,178Nd(β-); calculated half-lives using proton-neutron finite-amplitude method (pn-FAM) with Skyrme energy-density functionals (EDFs) in the quasiparticle random-phase approximation (QRPA), after optimizing the nuclear interaction to best fit the measured half-lives in A=80 and A=160 regions. Deduced r-process abundances. Comparison with other theoretical calculations and experimental values.
doi: 10.1103/PhysRevC.94.055802
2013PA23 Int.J.Mod.Phys. E22, 1330013 (2013) K.M.Patton, G.C.McLaughlin, K.Scholberg Prospects for using coherent elastic neutrino-nucleus scattering to measure the nuclear neutron form factor
doi: 10.1142/S0218301313300130
2012MU06 Phys.Rev. C 85, 045801 (2012) M.R.Mumpower, G.C.McLaughlin, R.Surman Formation of the rare-earth peak: Gaining insight into late-time r-process dynamics ATOMIC MASSES A=150-180, N=90-115; calculated effects of neutron capture rates, S(n) and β-decay rates on rare earth peak formation in elemental abundance plot using three nuclear data set simulations: ETFSI-Q, FRDM and HFB-17. R-process nucleosynthesis. Comparison between hot and cold r-process environments and with nuclear models.
doi: 10.1103/PhysRevC.85.045801
2012MU11 Phys.Rev. C 86, 035803 (2012) M.R.Mumpower, G.C.McLaughlin, R.Surman Influence of neutron capture rates in the rare earth region on the r-process abundance pattern NUCLEAR STRUCTURE Z=58-66, N=94-109, A=153-175; calculated sensitivity of rare earth elemental abundances to neutron capture rates in the rare earth region of the r-process abundance pattern. Introduced concepts of large nuclear flow and flow saturation.
doi: 10.1103/PhysRevC.86.035803
2012PA23 Phys.Rev. C 86, 024612 (2012) K.Patton, J.Engel, G.C.McLaughlin, N.Schunck Neutrino-nucleus coherent scattering as a probe of neutron density distributions NUCLEAR REACTIONS 40Ar, 74Ge, 132Xe(ν, ν), E at 0-100 MeV/c; calculated event rates in 40Ar as a function of recoil energy and neutron radius, neutron form factors, neutron rms radii, effective moments using density functional theory and Monte Carlo techniques for argon, germanium, and xenon detectors of neutrinos.
doi: 10.1103/PhysRevC.86.024612
2010KI02 Phys.Rev. C 81, 025802 (2010) L.-T.Kizivat, G.Martinez-Pinedo, K.Langanke, R.Surman, G.C.McLaughlin ψ-ray bursts black hole accretion disks as a site for the νp process
doi: 10.1103/PhysRevC.81.025802
2009AM01 J.Phys.(London) G36, 015105 (2009) Nuclear neutron form factor from neutrino-nucleus coherent elastic scattering
doi: 10.1088/0954-3899/36/1/015105
2009BE01 J.Phys.(London) G36, 025201 (2009) J.Beun, J.C.Blackmon, W.R.Hix, G.C.McLaughlin, M.S.Smith, R.Surman Neutron capture on 130Sn during r-process freeze-out
doi: 10.1088/0954-3899/36/2/025201
2009SU07 Phys.Rev. C 79, 045809 (2009) R.Surman, J.Beun, G.C.McLaughlin, W.R.Hix Neutron capture rates near A=130 that effect a global change to the r-process abundance distribution NUCLEAR REACTIONS Sn, In, Cd(n, γ); calculated σ for A=105-155, neutron capture rates, separation energies. Implications for r-process model.
doi: 10.1103/PhysRevC.79.045809
2008BE07 Phys.Rev. C 77, 035804 (2008) J.Beun, G.C.McLaughlin, R.Surman, W.R.Hix Fission cycling in a supernova r process
doi: 10.1103/PhysRevC.77.035804
2008JA05 Phys.Rev. C 77, 055501 (2008) N.Jachowicz, G.C.McLaughlin, C.Volpe Untangling supernova-neutrino oscillations with β-beam data NUCLEAR REACTIONS 2H, 16O, 208Pb(ν, ν), E=14, 18, 22 MeV; calculated σ, neutrino spectra, supernova neutrino interactions.
doi: 10.1103/PhysRevC.77.055501
2008SU04 J.Phys.(London) G35, 014059 (2008) R.Surman, J.Beun, G.C.McLaughlin, S.Kane, W.R.Hix The role of neutrinos in r-process nucleosynthesis in supernovae and gamma-ray bursts
doi: 10.1088/0954-3899/35/1/014059
2007AM06 Phys.Rev. C 75, 065502 (2007) Manipulating a neutrino spectrum to maximize the physics potential from a low-energy β beam
doi: 10.1103/PhysRevC.75.065502
2006JA08 Phys.Rev.Lett. 96, 172301 (2006) Reconstructing Supernova-Neutrino Spectra using Low-Energy Beta Beams NUCLEAR REACTIONS 2H(ν, ep), 16O, 208Pb(ν, ν'), E ≈ 18-22 MeV; calculated σ(E). Application to detector response calibration discussed.
doi: 10.1103/PhysRevLett.96.172301
2006JA16 Eur.Phys.J. A 27, Supplement 1, 43 (2006) On the importance of low-energy beta beams for supernova neutrino physics NUCLEAR REACTIONS 16O(ν, ν'X), E=14, 18, 22 MeV; calculated neutral-current σ(E). 2H(ν, ep), E=14, 18, 22 MeV; calculated charged-current σ(E).
doi: 10.1140/epja/i2006-08-005-x
2006KN01 J.Phys.(London) G32, 443 (2006) J.P.Kneller, G.C.McLaughlin, R.A.Surman Neutrino scattering, absorption and annihilation above the accretion discs of gamma ray bursts
doi: 10.1088/0954-3899/32/4/004
2005MC10 Nucl.Phys. A758, 189c (2005) Prospects for obtaining an r process from Gamma Ray Burst Disk Winds
doi: 10.1016/j.nuclphysa.2005.05.036
2004MC05 Phys.Lett. B 591, 229 (2004) Prospects for detecting a neutrino magnetic moment with a tritium source and beta-beams RADIOACTIVITY 3H, 6He(β-); 18Ne(β+); calculated neutrino spectra. Application to neutrino magnetic moment measurement discussed.
doi: 10.1016/j.physletb.2004.02.073
2004MC07 Phys.Rev. C 70, 045804 (2004) Neutrino-lead cross section measurements using stopped pions and low energy β beams NUCLEAR REACTIONS 208Pb(ν, eX), E=spectrum; calculated electron spectra, σ.
doi: 10.1103/PhysRevC.70.045804
2001MC01 Phys.Rev. D63, 053002 (2001) Use of Nuclear β Decay as a Test of Bulk Neutrinos in Extra Dimensions RADIOACTIVITY 3H(β-); 38mK(EC); calculated Kurie plots, recoil spectra, effects of bulk neutrinos in extra dimensions.
doi: 10.1103/PhysRevD.63.053002
1999MC02 Phys.Rev. C59, 2873 (1999) G.C.McLaughlin, J.M.Fetter, A.B.Balantekin, G.M.Fuller Active-Sterile Neutrino Transformation Solution for r-Process Nucleosynthesis
doi: 10.1103/PhysRevC.59.2873
1998ME25 Phys.Rev. C58, 3696 (1998) B.S.Meyer, G.C.McLaughlin, G.M.Fuller Neutrino Capture and r-Process Nucleosynthesis
doi: 10.1103/PhysRevC.58.3696
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