NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = I.Tews Found 29 matches. 2024PA12 Phys.Rev. C 109, 025807 (2024) P.T.H.Pang, L.Sivertsen, R.Somasundaram, T.Dietrich, S.Sen, I.Tews, M.W.Coughlin, Ch.Van Den Broeck Probing quarkyonic matter in neutron stars with the Bayesian nuclear-physics multimessenger astrophysics framework
doi: 10.1103/PhysRevC.109.025807
2024SO07 Phys.Rev. C 109, 034005 (2024) R.Somasundaram, J.E.Lynn, L.Huth, A.Schwenk, I.Tews Maximally local two-nucleon interactions at N3LO in Δ-less chiral effective field theory
doi: 10.1103/PhysRevC.109.034005
2023MA41 Phys.Rev. C 108, L031304 (2023) J.D.Martin, S.J.Novario, D.Lonardoni, J.Carlson, S.Gandolfi, I.Tews Auxiliary field diffusion Monte Carlo calculations of magnetic moments of light nuclei with chiral effective field theory interactions
doi: 10.1103/PhysRevC.108.L031304
2023RO11 Phys.Rev. C 108, 025811 (2023) H.Rose, N.Kunert, T.Dietrich, P.T.H.Pang, R.Smith, C.Van Den Broeck, S.Gandolfi, I.Tews Revealing the strength of three-nucleon interactions with the proposed Einstein Telescope
doi: 10.1103/PhysRevC.108.025811
2023SO04 Phys.Rev. C 107, 025801 (2023) R.Somasundaram, I.Tews, J.Margueron Investigating signatures of phase transitions in neutron-star cores
doi: 10.1103/PhysRevC.107.025801
2023SO08 Phys.Rev. C 107, L052801 (2023) R.Somasundaram, I.Tews, J.Margueron Perturbative QCD and the neutron star equation of state
doi: 10.1103/PhysRevC.107.L052801
2022AL20 Phys.Rev. C 106, 055804 (2022) M.G.Alford, L.Brodie, A.Haber, I.Tews Relativistic mean-field theories for neutron-star physics based on chiral effective field theory
doi: 10.1103/PhysRevC.106.055804
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
2022TE06 Few-Body Systems 63, 67 (2022) I.Tews, Z.Davoudi, A.Ekstrom, J.D.Holt, K.Becker, R.Briceno, D.J.Dean, W.Detmold, C.Drischler, T.Duguet, E.Epelbaum, A.Gasparyan, J.Gegelia, J.R.Green, H.W.Griesshammer, A.D.Hanlon, M.Heinz, H.Hergert, M.Hoferichter, M.Illa, D.Kekejian, A.Kievsky, S.Konig, H.Krebs, K.D.Launey, D.Lee, P.Navratil, A.Nicholson, A.Parreno, D.R.Phillips, M.Ploszajczak, X.-L.Ren, T.R.Richardson, C.Robin, G.H.Sargsyan, M.J.Savage, M.R.Schindler, P.E.Shanahan, R.P.Springer, A.Tichai, U.van Kolck, M.L.Wagman, A.Walker-Loud, C.-J.Yang, X.Zhang Nuclear Forces for Precision Nuclear Physics: A Collection of Perspectives
doi: 10.1007/s00601-022-01749-x
2021ES07 Phys.Rev.Lett. 127, 192701 (2021) R.Essick, I.Tews, P.Landry, A.Schwenk Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of 208Pb with Minimal Modeling Assumptions NUCLEAR STRUCTURE 208Pb; analyzed available data; deduced astrophysical constraints on the symmetry energy and the neutron skin.
doi: 10.1103/PhysRevLett.127.192701
2021ES10 Phys.Rev. C 104, 065804 (2021) R.Essick, P.Landry, A.Schwenk, I.Tews Detailed examination of astrophysical constraints on the symmetry energy and the neutron skin of 208Pb with minimal modeling assumptions NUCLEAR STRUCTURE 208Pb; analyzed correlations between selected nuclear properties such as symmetry energy, slope parameter, curvature, 208Pb skin and electric dipole polarizability using nonparametric equation of state (EOS) representation based on Gaussian processes to constrain the symmetry energy, slope parameter, and 208Pb skin from observations of neutron stars with minimal modeling assumptions, and by combining astrophysical data from heavy pulsar masses, LIGO/Virgo, and NICER with chiral effective field theory (χEFT) and constraints from PREX-II experiment for 208Pb skin thickness, and using Monte Carlo implementation of a hierarchical Bayesian inference. Relevance to neutron-skin thickness of nuclei to the crust thickness and the radius of neutron stars.
doi: 10.1103/PhysRevC.104.065804
2021SO13 Phys.Rev. C 103, 045803 (2021) R.Somasundaram, C.Drischler, I.Tews, J.Margueron Constraints on the nuclear symmetry energy from asymmetric-matter calculations with chiral NN and 3N interactions
doi: 10.1103/PhysRevC.103.045803
2020ES04 Phys.Rev. C 102, 055803 (2020) R.Essick, I.Tews, P.Landry, S.Reddy, D.E.Holz Direct astrophysical tests of chiral effective field theory at supranuclear densities
doi: 10.1103/PhysRevC.102.055803
2020LO09 Phys. Rev. Res. 2, 022033 (2020) D.Lonardoni, I.Tews, S.Gandolfi, J.Carlson Nuclear and neutron-star matter from local chiral interactions
doi: 10.1103/PhysRevResearch.2.022033
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
2019TE02 Eur.Phys.J. A 55, 97 (2019) Confronting gravitational-wave observations with modern nuclear physics constraints
doi: 10.1140/epja/i2019-12774-6
2018TE03 Phys.Rev. C 98, 024001 (2018) Large-cutoff behavior of local chiral effective field theory interactions
doi: 10.1103/PhysRevC.98.024001
2018TE05 Phys.Rev. C 98, 045804 (2018) Critical examination of constraints on the equation of state of dense matter obtained from GW170817
doi: 10.1103/PhysRevC.98.045804
2017HU17 Phys.Rev. C 96, 054003 (2017) L.Huth, I.Tews, J.E.Lynn, A.Schwenk Analyzing the Fierz rearrangement freedom for local chiral two-nucleon potentials NUCLEAR STRUCTURE 2H, 4He; calculated binding energies, radii, phase-shifts in the framework of Chiral effective field theory (EFT), by constructing leading order (LO) and next-to-leading order (NLO) potentials for all possible LO-operator pairs.Calculated energy of neutron matter at different densities.
doi: 10.1103/PhysRevC.96.054003
2017LY01 Phys.Rev. C 96, 054007 (2017) J.E.Lynn, I.Tews, J.Carlson, S.Gandolfi, A.Gezerlis, K.E.Schmidt, A.Schwenk Quantum Monte Carlo calculations of light nuclei with local chiral two- and three-nucleon interactions NUCLEAR STRUCTURE 2H; calculated deuteron wave functions, binding energy, asymptotic D/S ratio, quadrupole moment, root-mean-square (rms) matter radius, momentum distributions and tensor polarization at N2LO, deuteron energy at LO, NLO, and N2LO as function of radius. 3H, 3,4He; calculated wave functions for AV18+UIX at N22LO, energies using Green's function Monte Carlo (GFMC) method, kinetic and potential energy contributions to the GFMC energy, point-proton radii at LO, NLO, and N2LO, one-body proton and neutron distributions for 3,4He at N2LO, longitudinal charge form factor for 4He. Quantum Monte Carlo (QMC) calculations for light nuclei with local chiral NN and 3N interactions.
doi: 10.1103/PhysRevC.96.054007
2017TE01 Phys.Rev. C 95, 015803 (2017) Spectrum of shear modes in the neutron-star crust: Estimating the nuclear-physics uncertainties
doi: 10.1103/PhysRevC.95.015803
2016DY01 Phys.Rev. C 94, 034001 (2016) A.Dyhdalo, R.J.Furnstahl, K.Hebeler, I.Tews Regulator artifacts in uniform matter for chiral interactions
doi: 10.1103/PhysRevC.94.034001
2016KL06 Phys.Rev. C 94, 054005 (2016) P.Klos, J.E.Lynn, I.Tews, S.Gandolfi, A.Gezerlis, H.-W.Hammer, M.Hoferichter, A.Schwenk Quantum Monte Carlo calculations of two neutrons in finite volume NUCLEAR STRUCTURE 2n; calculated ground state, energy and nodal surface of the first excited state for a two neutron-system in a box; extracted low-energy S-wave scattering parameters from ground- and excited-state energies for different box sizes using Luscher formula. Auxiliary-field diffusion Monte Carlo (AFDMC) calculations, and chiral EFT interactions. Relevance to effective field theories of strong interaction.
doi: 10.1103/PhysRevC.94.054005
2016LY02 Phys.Rev.Lett. 116, 062501 (2016) J.E.Lynn, I.Tews, J.Carlson, S.Gandolfi, A.Gezerlis, K.E.Schmidt, A.Schwenk Chiral Three-Nucleon Interactions in Light Nuclei, Neutron-α Scattering, and Neutron Matter NUCLEAR STRUCTURE 4He; analyzed available data; deduced binding and ground-state energies. Quantum Monte Carlo calculations of light nuclei using local two- and three-nucleon (3N) interactions derived from chiral effective field theory up to next-to-next-to-leading order (N2LO).
doi: 10.1103/PhysRevLett.116.062501
2016TE01 Phys.Rev. C 93, 024305 (2016) I.Tews, S.Gandolfi, A.Gezerlis, A.Schwenk Quantum Monte Carlo calculations of neutron matter with chiral three-body forces
doi: 10.1103/PhysRevC.93.024305
2014GE06 Phys.Rev. C 90, 054323 (2014) A.Gezerlis, I.Tews, E.Epelbaum, M.Freunek, S.Gandolfi, K.Hebeler, A.Nogga, A.Schwenk Local chiral effective field theory interactions and quantum Monte Carlo applications NUCLEAR STRUCTURE 2H; calculated binding energy, quadrupole moment, magnetic moment, asymptotic D/S ratio, rms radius, asymptotic s-wave factor, and the d-state probability using the local chiral potentials. Calculated ground-state energy for a 66-neutron matter system. Local chiral effective field theory interactions to next-to-next-to-leading order and Monte Carlo calculations for neutron matter.
doi: 10.1103/PhysRevC.90.054323
2013GE03 Phys.Rev.Lett. 111, 032501 (2013) A.Gezerlis, I.Tews, E.Epelbaum, S.Gandolfi, K.Hebeler, A.Nogga, A.Schwenk Quantum Monte Carlo Calculations with Chiral Effective Field Theory Interactions
doi: 10.1103/PhysRevLett.111.032501
2013KR10 Phys.Rev. C 88, 025802 (2013) T.Kruger, I.Tews, K.Hebeler, A.Schwenk Neutron matter from chiral effective field theory interactions
doi: 10.1103/PhysRevC.88.025802
2013TE01 Phys.Rev.Lett. 110, 032504 (2013) I.Tews, T.Kruger, K.Hebeler, A.Schwenk Neutron Matter at Next-to-Next-to-Next-to-Leading Order in Chiral Effective Field Theory NUCLEAR STRUCTURE 208Pb; calculated neutron matter energy, energy per particle vs. density using N3LO potentials. Comparison with available data.
doi: 10.1103/PhysRevLett.110.032504
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