NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = A.W.Steiner Found 37 matches. 2023LI09 Phys.Rev. C 107, 015804 (2023) Z.Lin, A.W.Steiner, J.Margueron Uncertainty quantification for neutrino opacities in core-collapse supernovae and neutron star mergers
doi: 10.1103/PhysRevC.107.015804
2022DU06 Phys.Rev. C 105, 035803 (2022) Hot and dense matter equation of state probability distributions for astrophysical simulations
doi: 10.1103/PhysRevC.105.035803
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
2019BE34 Phys.Rev. C 100, 055801 (2019) S.Beloin, S.Han, A.W.Steiner, K.Odbadrakh Simultaneous fitting of neutron star structure and cooling data
doi: 10.1103/PhysRevC.100.055801
2019DU10 Phys.Rev. C 99, 025803 (2019) Hot and dense homogeneous nucleonic matter constrained by observations, experiment, and theory
doi: 10.1103/PhysRevC.99.025803
2019GA36 J.Phys.(London) G46, 103001 (2019) S.Gandolfi, J.Lippuner, A.W.Steiner, I.Tews, X.Du, M.Al-Mamun From the microscopic to the macroscopic world: from nucleons to neutron stars
doi: 10.1088/1361-6471/ab29b3
2018BE02 Phys.Rev. C 97, 015804 (2018) S.Beloin, S.Han, A.W.Steiner, D.Page Constraining superfluidity in dense matter from the cooling of isolated neutron stars
doi: 10.1103/PhysRevC.97.015804
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
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
2017HA24 Phys.Rev. C 96, 035802 (2017) Cooling of neutron stars in soft x-ray transients
doi: 10.1103/PhysRevC.96.035802
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
2016ST08 Eur.Phys.J. A 52, 18 (2016) A.W.Steiner, J.M.Lattimer, E.F.Brown Neutron star radii, universal relations, and the role of prior distributions
doi: 10.1140/epja/i2016-16018-1
2015BE27 Phys.Rev. C 92, 025803 (2015) Hypernuclei and the hyperon problem in neutron stars NUCLEAR STRUCTURE 3,4H, 4,5,6,8He, 6,7,8,9Li, 7,8,9,10Be, 9,10,11,12B, 12,13,14C, 14,15,16N, 16,18O, 27,28Al, 28Si, 32S, 40Ca, 51V, 56Fe, 89Y, 139La, 208Pb, 209Bi; analyzed binding energies of known single-hyperon hypernuclei with three- and four-parameter fits; investigated interaction between hyperons and nuclear/neutron matter by calculating Monte Carlo probability distribution of incompressibility for neutron star models.
doi: 10.1103/PhysRevC.92.025803
2015ST02 Phys.Rev. C 91, 015804 (2015) A.W.Steiner, S.Gandolfi, F.J.Fattoyev, W.G.Newton Using neutron star observations to determine crust thicknesses, moments of inertia, and tidal deformabilities
doi: 10.1103/PhysRevC.91.015804
2014DE28 Phys.Rev. C 90, 025802 (2014) A.T.Deibel, A.W.Steiner, E.F.Brown Magnetar giant flare oscillations and the nuclear symmetry energy
doi: 10.1103/PhysRevC.90.025802
2014GA06 Eur.Phys.J. A 50, 10 (2014) S.Gandolfi, J.Carlson, S.Reddy, A.W.Steiner, R.B.Wiringa The equation of state of neutron matter, symmetry energy and neutron star structure
doi: 10.1140/epja/i2014-14010-5
2014LA06 Eur.Phys.J. A 50, 40 (2014) Constraints on the symmetry energy using the mass-radius relation of neutron stars
doi: 10.1140/epja/i2014-14040-y
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
2012CA04 Nucl.Phys. A876, 77 (2012) B.V.Carlson, R.Donangelo, S.R.Souza, W.G.Lynch, A.W.Steiner, M.B.Tsang Fermi breakup and the statistical multifragmentation model NUCLEAR REACTIONS 16O(p, X), E=62 MeV fragmentation; calculated charge, mass yields using Fermi breakup model and microcanonical statistical multifragmentation model.
doi: 10.1016/j.nuclphysa.2011.12.009
2012ST09 Phys.Rev. C 85, 055804 (2012) Deep crustal heating in a multicomponent accreted neutron star crust
doi: 10.1103/PhysRevC.85.055804
2012TS04 Phys.Rev. C 86, 015803 (2012) M.B.Tsang, J.R.Stone, F.Camera, P.Danielewicz, S.Gandolfi, K.Hebeler, C.J.Horowitz, J.Lee, W.G.Lynch, Z.Kohley, R.Lemmon, P.Moller, T.Murakami, S.Riordan, X.Roca-Maza, F.Sammarruca, A.W.Steiner, I.Vidana, S.J.Yennello Constraints on the symmetry energy and neutron skins from experiments and theory NUCLEAR STRUCTURE 208Pb; analyzed neutron-skin thickness, symmetry energy constraints. Contributions of three-body forces in neutron matter models.
doi: 10.1103/PhysRevC.86.015803
2011CA34 J.Phys.:Conf.Ser. 312, 082017 (2011) B.V.Carlson, R.Donangelo, S.R.Souza, W.G.Lynch, A.W.Steiner, M.B.Tsang Fermi breakup and the Statistical Multifragmentation Model NUCLEAR REACTIONS 16O(γ, X), E=50 MeV; calculated breakup Z=4-7 isotopes yields, σ using Fermi breakup model and statistical multifragmentation.
doi: 10.1088/1742-6596/312/4/082017
2009SO07 Phys.Rev. C 79, 054602 (2009) S.R.Souza, B.V.Carlson, R.Donangelo, W.G.Lynch, A.W.Steiner, M.B.Tsang Statistical multifragmentation model with Skyrme effective interactions NUCLEAR STRUCTURE 150Nd; calculated temperature and charge distributions for breakup of the nucleus, average multiplicity and yields of light particles Li, Be, B, C, N and O. 10Be, 20Ne, 31P, 40Ca; calculated internal free energy as a function of temperature. Statistical multifragmentation and Thomas-Fermi (SMM-TF) model with Skyrme interaction.
doi: 10.1103/PhysRevC.79.054602
2009SO15 Phys.Rev. C 80, 041602 (2009) S.R.Souza, M.B.Tsang, B.V.Carlson, R.Donangelo, W.G.Lynch, A.W.Steiner Isospin effects and the density dependence of the nuclear symmetry energy NUCLEAR REACTIONS 58Ni(40Ar, X), (40Ca, X), E not given; calculated isoscaling parameters as a function of the excitation energy of the source, and Isotopic distribution of primary fragments Li, Be, B, C, N and O using improved statistical multifragmentation model (ISMM), SLy4 and Gs Skyrme effective interactions.
doi: 10.1103/PhysRevC.80.041602
2009SO16 Phys.Rev. C 80, 044606 (2009) S.R.Souza, M.B.Tsang, B.V.Carlson, R.Donangelo, W.G.Lynch, A.W.Steiner Temperature effects in nuclear isoscaling
doi: 10.1103/PhysRevC.80.044606
2009ST03 Phys.Rev. C 79, 015802 (2009) Superfluid response and the neutrino emissivity of neutron matter
doi: 10.1103/PhysRevC.79.015802
2009TS02 Phys.Rev.Lett. 102, 122701 (2009) M.B.Tsang, Y.Zhang, P.Danielewicz, M.Famiano, Z.Li, W.G.Lynch, A.W.Steiner Constraints on the Density Dependence of the Symmetry Energy
doi: 10.1103/PhysRevLett.102.122701
2008LI09 J.Phys.(London) G35, 014044 (2008) B.-A.Li, L.-W.Chen, C.M.Ko, P.G.Krastev, A.W.Steiner, G.-C.Yong Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
doi: 10.1088/0954-3899/35/1/014044
2008SO13 Phys.Rev. C 78, 014605 (2008) S.R.Souza, M.B.Tsang, R.Donangelo, W.G.Lynch, A.W.Steiner Probing the symmetry energy from the nuclear isoscaling
doi: 10.1103/PhysRevC.78.014605
2008ST07 Phys.Rev. C 77, 035805 (2008) Neutron star inner crust: Nuclear physics input
doi: 10.1103/PhysRevC.77.035805
2007RE07 Nucl.Phys. A785, 24c (2007) Cool Dense Matter and Neutron Star Phenomenology
doi: 10.1016/j.nuclphysa.2006.11.130
2006LI61 Phys.Lett. B 642, 436 (2006) Constraining the radii of neutron stars with terrestrial nuclear laboratory data
doi: 10.1016/j.physletb.2006.09.065
2006ST19 Phys.Rev. C 74, 045808 (2006) High-density symmetry energy and direct Urca process
doi: 10.1103/PhysRevC.74.045808
2005ST17 Phys.Rep. 411, 325 (2005) A.W.Steiner, M.Prakash, J.M.Lattimer, P.J.Ellis Isospin asymmetry in nuclear and neutron stars
doi: 10.1016/j.physrep.2005.02.004
2005ST31 Phys.Rev. C 72, 041601 (2005) Isospin diffusion in heavy-ion collisions and the neutron skin thickness of lead NUCLEAR STRUCTURE 208Pb; analyzed correlation between neutron skin thickness of lead and isospin diffusion in heavy-ion collisions. NUCLEAR REACTIONS 124Sn(112Sn, X), E not given; analyzed correlation between isospin diffusion in heavy-ion collisions and the neutron skin thickness of lead.
doi: 10.1103/PhysRevC.72.041601
2003PR04 Nucl.Phys. A715, 835c (2003) M.Prakash, J.M.Lattimer, A.W.Steiner, D.Page Observability of neutron stars with quarks
doi: 10.1016/S0375-9474(02)01514-2
2000ST21 Phys.Lett. 486B, 239 (2000) A.W.Steiner, M.Prakash, J.M.Lattimer Quark-Hadron Phase Transitions in Young and Old Neutron Stars
doi: 10.1016/S0370-2693(00)00780-2
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