NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 11, 2024.

Search: Author = A.W.Steiner

Found 37 matches.

Back to query form

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
Citations: PlumX Metrics

2022DU06      Phys.Rev. C 105, 035803 (2022)

X.Du, A.W.Steiner, J.W.Holt

Hot and dense matter equation of state probability distributions for astrophysical simulations

doi: 10.1103/PhysRevC.105.035803
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2019DU10      Phys.Rev. C 99, 025803 (2019)

X.Du, A.W.Steiner, J.W.Holt

Hot and dense homogeneous nucleonic matter constrained by observations, experiment, and theory

doi: 10.1103/PhysRevC.99.025803
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2017HA24      Phys.Rev. C 96, 035802 (2017)

S.Han, A.W.Steiner

Cooling of neutron stars in soft x-ray transients

doi: 10.1103/PhysRevC.96.035802
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2015BE27      Phys.Rev. C 92, 025803 (2015)

P.F.Bedaque, A.W.Steiner

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2014LA06      Eur.Phys.J. A 50, 40 (2014)

J.M.Lattimer, A.W.Steiner

Constraints on the symmetry energy using the mass-radius relation of neutron stars

doi: 10.1140/epja/i2014-14040-y
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2012ST09      Phys.Rev. C 85, 055804 (2012)


Deep crustal heating in a multicomponent accreted neutron star crust

doi: 10.1103/PhysRevC.85.055804
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2009ST03      Phys.Rev. C 79, 015802 (2009)

A.W.Steiner, S.Reddy

Superfluid response and the neutrino emissivity of neutron matter

doi: 10.1103/PhysRevC.79.015802
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2008ST07      Phys.Rev. C 77, 035805 (2008)


Neutron star inner crust: Nuclear physics input

doi: 10.1103/PhysRevC.77.035805
Citations: PlumX Metrics

2007RE07      Nucl.Phys. A785, 24c (2007)

S.Reddy, A.W.Steiner

Cool Dense Matter and Neutron Star Phenomenology

doi: 10.1016/j.nuclphysa.2006.11.130
Citations: PlumX Metrics

2006LI61      Phys.Lett. B 642, 436 (2006)

B.-A.Li, A.W.Steiner

Constraining the radii of neutron stars with terrestrial nuclear laboratory data

doi: 10.1016/j.physletb.2006.09.065
Citations: PlumX Metrics

2006ST19      Phys.Rev. C 74, 045808 (2006)


High-density symmetry energy and direct Urca process

doi: 10.1103/PhysRevC.74.045808
Citations: PlumX Metrics

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
Citations: PlumX Metrics

2005ST31      Phys.Rev. C 72, 041601 (2005)

A.W.Steiner, B.-A.Li

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

Back to query form