NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = A.Bauswein Found 9 matches. 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
2021LE05 Phys.Rev. C 103, 025806 (2021) J.-F.Lemaitre, S.Goriely, A.Bauswein, H.-T.Janka Fission fragment distributions and their impact on the r-process nucleosynthesis in neutron star mergers NUCLEAR REACTIONS 235U(n, F), E=thermal; calculated energy of fission fragments with or without the phenomenological distance correction. 235U, 239Pu, 251Cf(n, F), E=thermal; calculated isotopic and isobaric fission yields, evaporated neutron distributions as a function of the fragment mass number, total mean number of evaporated neutrons per fission, evaporated neutron distribution of spontaneous fission of 252Cf. Improved scission-point yield (SPY) model, and comparison with GEF model calculations, and with experimental and evaluated data for fission yields. NUCLEAR STRUCTURE Z=70-124, N=80-290; calculated peak multiplicity for the raw preneutron isobaric yields with corrected distance, mean prompt neutron multiplicity per fission, peak multiplicity for the smooth preneutron isobaric yields with corrected distance, mean available energy release per fission, peak multiplicity for the smooth preneutron isobaric yields without corrected distance, isolines of mean available energy release per fission, and mean prompt neutron multiplicity per fission for 3000 nuclei. Z=84-92, N=118-140; Z=92-104, N=140-160; calculated isobaric fission yields for A=70-160 fragments, abundances of A=50-240 nuclei. Z=93-104, A=272-291; Z=99-110, A=328-347; calculated postneutron fission-fragment distributions (FFDs). Analyzed impact of fission on the r-process nucleosynthesis in binary neutron star mergers. Improved scission-point yield (SPY) model, and comparison with GEF model calculations, and with experimental and evaluated data for fission yields.
doi: 10.1103/PhysRevC.103.025806
2019BA44 Ann.Phys.(New York) 411, 167958 (2019) Equation of state constraints from multi-messenger observations of neutron star mergers
doi: 10.1016/j.aop.2019.167958
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
2017BA10 Acta Phys.Pol. B48, 651 (2017) A.Bauswein, R.A.Pulpillo, J.A.Clark, O.Just, S.Goriely, H.-T.Janka, N.Stergioulas Neutron-star Mergers and Nuclear Physics
doi: 10.5506/APhysPolB.48.651
2016BA17 Eur.Phys.J. A 52, 56 (2016) A.Bauswein, N.Stergioulas, H.-T.Janka Exploring properties of high-density matter through remnants of neutron-star mergers
doi: 10.1140/epja/i2016-16056-7
2015ME10 Phys.Rev. C 92, 055805 (2015) J.Mendoza-Temis, M.-R.Wu, K.Langanke, G.Martinez-Pinedo, A.Bauswein, H.-T.Janka Nuclear robustness of the r process in neutron-star mergers ATOMIC MASSES A=108-288; calculated r-process abundances of slow ejecta for different mass models at different phases of the evolution in neutron star mergers using three-dimensional relativistic smoothed particle hydrodynamic simulation, and extended nuclear network of 7300 nuclei from free nucleons up to 313Ds, including spontaneous, β- and neutron-induced fission, fission yield distributions from the ABLA code. Comparison with observed r-process abundances. NUCLEAR REACTIONS 278Am(n, F); calculated fission fragment distributions as functions of charge, neutron number, and mass number for neutron using the ABLA code.
doi: 10.1103/PhysRevC.92.055805
2013GO17 Phys.Rev.Lett. 111, 242502 (2013) S.Goriely, J.-L.Sida, J.-F.Lemaitre, S.Panebianco, N.Dubray, S.Hilaire, A.Bauswein, H.-T.Janka New Fission Fragment Distributions and r-Process Origin of the Rare-Earth Elements
doi: 10.1103/PhysRevLett.111.242502
2012GO14 J.Phys.:Conf.Ser. 337, 012039 (2012) S.Goriely, A.Bauswein, H.-T.Janka R-process nucleosynthesis during the decompression of neutron star crust material COMPILATION A=65-250; compiled ejectile mass distribution, abundance mass distribution, mean mass, charge time dependence, relative T1/2 for spontaneous fission, β-delayed fission, neutron-induced fission and neutron capture using NETGEN library supplemented with TALYS calculations based on HFB-21 nuclear mass model.
doi: 10.1088/1742-6596/337/1/012039
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