NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.W.Holt Found 47 matches. 2024SH02 Phys.Rev. C 109, 015804 (2024) E.Shin, E.Rrapaj, J.W.Holt, S.K.Reddy Chiral effective field theory calculation of neutrino reactions in warm neutron-rich matter
doi: 10.1103/PhysRevC.109.015804
2023DA15 Phys.Rev. C 108, 034003 (2023) D.Davesne, J.W.Holt, J.Navarro, A.Pastore Landau sum rules with noncentral quasiparticle interactions
doi: 10.1103/PhysRevC.108.034003
2023HE08 J.Phys.(London) G50, 060501 (2023) C.Hebborn, F.M.Nunes, G.Potel, W.H.Dickhoff, J.W.Holt, M.C.Atkinson, R.B.Baker, C.Barbieri, G.Blanchon, M.Burrows, R.Capote, P.Danielewicz, M.Dupuis, C.Elster, J.E.Escher, L.Hlophe, A.Idini, H.Jayatissa, B.P.Kay, K.Kravvaris, J.J.Manfredi, A.Mercenne, B.Morillon, G.Perdikakis, C.D.Pruitt, G.H.Sargsyan, I.J.Thompson, M.Vorabbi, T.R.Whitehead Optical potentials for the rare-isotope beam era
doi: 10.1088/1361-6471/acc348
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
2021BR12 Phys.Rev.Lett. 127, 062701 (2021) Normalizing Flows for Microscopic Many-Body Calculations: An Application to the Nuclear Equation of State
doi: 10.1103/PhysRevLett.127.062701
2021LI15 Phys.Rev. C 103, 025807 (2021) Proton pairing in neutron stars from chiral effective field theory
doi: 10.1103/PhysRevC.103.025807
2021LI48 Phys.Rev. C 104, L032802 (2021) Y.Lim, A.Bhattacharya, J.W.Holt, D.Pati Radius and equation of state constraints from massive neutron stars and GW190814
doi: 10.1103/PhysRevC.104.L032802
2021WE09 Phys.Rev. C 103, 064002 (2021) Constraining the nonanalytic terms in the isospin-asymmetry expansion of the nuclear equation of state
doi: 10.1103/PhysRevC.103.064002
2021WH01 Phys.Rev.Lett. 127, 182502 (2021) T.R.Whitehead, Y.Lim, J.W.Holt Global Microscopic Description of Nucleon-Nucleus Scattering with Quantified Uncertainties NUCLEAR REACTIONS 14N, 16O, 34S, 56Fe, 90Zr, 121Sb, 138Ba, 182W, 208Pb(n, n), E<75 MeV; 16O, 27Al, 48Ti, 60Ni, 80Se, 120Sn, 182W, 194Pt, 206Pb(p, p), E<135 MeV; analyzed available data; deduced s(θ), optical potentials from a set of five nuclear forces from chiral effective field theory for 1800 target nuclei.
doi: 10.1103/PhysRevLett.127.182502
2020WH01 Phys.Rev. C 101, 064613 (2020) T.R.Whitehead, Y.Lim, J.W.Holt Neutron elastic scattering on calcium isotopes from chiral nuclear optical potentials NUCLEAR STRUCTURE 40,48Ca; calculated matter density distributions using mean-field theory with the Skyrme Skχ450 effective interaction constrained by chiral effective field theory. NUCLEAR REACTIONS 40,48Ca(n, n), E=3.2, 30, 85 MeV; calculated real, imaginary, and spin-orbit terms of the microscopic chiral optical potential. 40Ca(n, n), E=3.2, 5.3, 6.52, 11.9, 16.9, 21.7, 25.5, 30, 40, 65, 85, 107.5, 155, 185 MeV; 48Ca(n, n), E=7.97, 11.9, 16.9 MeV; calculated differential σ(E, θ). 48Ca(polarized n, n), E=11.9, 16.9 MeV; calculated vector analyzing powers Ay(E, θ). Calculated used the chiral optical potential, and Koning-Delaroche phenomenological optical potential. 40,48Ca(n, x), E=10-200 MeV; calculated total σ(E) using the chiral optical potential. Comparison with experimental data. Improved microscopic optical potential based on nuclear two- and three-body interactions from chiral effective field theory.
doi: 10.1103/PhysRevC.101.064613
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
2019LI43 Phys.Rev. C 100, 035802 (2019) Predicting the moment of inertia of pulsar J0737-3039A from Bayesian modeling of the nuclear equation of state
doi: 10.1103/PhysRevC.100.035802
2019LI53 Eur.Phys.J. A 55, 209 (2019) Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
doi: 10.1140/epja/i2019-12917-9
2019WH01 Phys.Rev. C 100, 014601 (2019) T.R.Whitehead, Y.Lim, J.W.Holt Proton elastic scattering on calcium isotopes from chiral nuclear optical potentials NUCLEAR REACTIONS 40Ca(p, p), E=2.35, 35, 100 MeV; calculated real, imaginary, and spin-orbit terms of the microscopic optical potential from chiral EFT, and from fits to the Koning-Delaroche (KD) form. 40,42,44,48Ca; calculated nucleon density distributions in mean field theory using the Skyrme Skχ450 effective interaction. 40Ca(p, p), E=2.35, 25, 35, 45, 55, 65, 80, 135, 160 MeV; 42,44,48Ca(p, p), E=25, 35, 45 MeV; 40,42,44,48Ca(p, X), E=20-50 MeV; calculated differential elastic σ(θ, E), and total reaction σ(E) using microscopic optical potentials calculated from chiral effective field theory, and from the chiral optical potential by the Koning-Delaroche (KD) phenomenological imaginary part, and using the reaction code TALYS. Comparison with experimental data.
doi: 10.1103/PhysRevC.100.014601
2018HO05 Phys.Rev. C 97, 054325 (2018) J.W.Holt, N.Kaiser, T.R.Whitehead Tensor Fermi liquid parameters in nuclear matter from chiral effective field theory
doi: 10.1103/PhysRevC.97.054325
2018LI39 Phys.Rev.Lett. 121, 062701 (2018) Neutron Star Tidal Deformabilities Constrained by Nuclear Theory and Experiment
doi: 10.1103/PhysRevLett.121.062701
2017HO06 Phys.Rev. C 95, 034326 (2017) Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral effective field theory
doi: 10.1103/PhysRevC.95.034326
2017LI20 Phys.Rev. C 95, 065805 (2017) Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory
doi: 10.1103/PhysRevC.95.065805
2016HO10 Phys.Rev. C 93, 064603 (2016) J.W.Holt, N.Kaiser, G.A.Miller Microscopic optical potential for exotic isotopes from chiral effective field theory
doi: 10.1103/PhysRevC.93.064603
2016RR01 Phys.Rev. C 93, 065801 (2016) Microscopically constrained mean-field models from chiral nuclear thermodynamics
doi: 10.1103/PhysRevC.93.065801
2016WE08 Phys.Rev. C 93, 055802 (2016) C.Wellenhofer, J.W.Holt, N.Kaiser Divergence of the isospin-asymmetry expansion of the nuclear equation of state in many-body perturbation theory
doi: 10.1103/PhysRevC.93.055802
2015DA02 Phys.Rev. C 91, 014323 (2015) D.Davesne, J.W.Holt, A.Pastore, J.Navarro Effect of three-body forces on response functions in infinite neutron matter
doi: 10.1103/PhysRevC.91.014323
2015RR01 Phys.Rev. C 91, 035806 (2015) E.Rrapaj, J.W.Holt, A.Bartl, S.Reddy, A.Schwenk Charged-current reactions in the supernova neutrino-sphere NUCLEAR REACTIONS 1n(ν, e-)p, E=1-100 MeV; 1H(ν-bar, e+)n, E=1-100 MeV; calculated neutrino absorption rates due to charged-current reactions in the outer regions of a newly born neutron star called the neutrino-sphere, momentum-, density-, and temperature-dependent nucleon self-energies in the Hartree-Fock approximation.
doi: 10.1103/PhysRevC.91.035806
2015SA22 Phys.Rev. C 91, 054311 (2015) F.Sammarruca, L.Coraggio, J.W.Holt, N.Itaco, R.Machleidt, L.E.Marcucci Toward order-by-order calculations of the nuclear and neutron matter equations of state in chiral effective field theory
doi: 10.1103/PhysRevC.91.054311
2015WE10 Phys.Rev. C 92, 015801 (2015) C.Wellenhofer, J.W.Holt, N.Kaiser Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory
doi: 10.1103/PhysRevC.92.015801
2014CO09 Phys.Rev. C 89, 044321 (2014) L.Coraggio, J.W.Holt, N.Itaco, R.Machleidt, L.E.Marcucci, F.Sammarruca Nuclear-matter equation of state with consistent two- and three-body perturbative chiral interactions NUCLEAR STRUCTURE 3H, 3He; calculated neutron-proton phase shifts, binding energy, Gamow-Teller transition matrix element, nuclear matter energy per particle. Equation of state (EOS) for two- and three-body perturbative chiral interactions in the framework of the perturbative Goldstone expansion and regulator functions. Comparison with experimental data.
doi: 10.1103/PhysRevC.89.044321
2014DO13 Nucl.Phys. A930, 1 (2014) Non-degenerate shell-model effective interactions from the Okamoto-Suzuki and Krenciglowa-Kuo iteration methods
doi: 10.1016/j.nuclphysa.2014.08.036
2014KU16 Nucl.Phys. A928, 30 (2014) Core polarization, Brown-Rho scaling and a memory of Gerry's Princeton Years
doi: 10.1016/j.nuclphysa.2014.05.006
2014MA80 Phys.Rev. C 90, 044003 (2014) S.Maurizio, J.W.Holt, P.Finelli Nuclear pairing from microscopic forces: Singlet channels and higher-partial waves
doi: 10.1103/PhysRevC.90.044003
2014TZ01 Chin.J.Phys.(Taiwan) 52, 1450 (2014) Y.Tzeng, S.-Y.T.Tzeng, T.T.S.Kuo, J.W.Holt Binding Energy of 16O in the Ring Diagram Method with Chiral Two- and Three-Nucleon Low Momentum Interactions NUCLEAR STRUCTURE 16O; calculated charge density, binding and ground state energies. Comparison with available data.
doi: 10.6122/CJP.20140430
2014WE05 Phys.Rev. C 89, 064009 (2014) C.Wellenhofer, J.W.Holt, N.Kaiser, W.Weise Nuclear thermodynamics from chiral low-momentum interactions
doi: 10.1103/PhysRevC.89.064009
2014WL01 Phys.Rev.Lett. 113, 182503 (2014) G.Wlazlowski, J.W.Holt, S.Moroz, A.Bulgac, K.J.Roche Auxiliary-Field Quantum Monte Carlo Simulations of Neutron Matter in Chiral Effective Field Theory
doi: 10.1103/PhysRevLett.113.182503
2013CO02 Phys.Rev. C 87, 014322 (2013) L.Coraggio, J.W.Holt, N.Itaco, R.Machleidt, F.Sammarruca Reduced regulator dependence of neutron-matter predictions with perturbative chiral interactions
doi: 10.1103/PhysRevC.87.014322
2013HO04 Phys.Rev. C 87, 014338 (2013) Chiral Fermi liquid approach to neutron matter
doi: 10.1103/PhysRevC.87.014338
2013HO14 Phys.Rev. C 88, 024614 (2013) J.W.Holt, N.Kaiser, G.A.Miller, W.Weise Microscopic optical potential from chiral nuclear forces
doi: 10.1103/PhysRevC.88.024614
2012HO02 Nucl.Phys. A876, 61 (2012) Quasiparticle interaction in nuclear matter with chiral three-nucleon forces
doi: 10.1016/j.nuclphysa.2011.12.001
2011HO13 Eur.Phys.J. A 47, 128 (2011) Nuclear energy density functional from chiral two-nucleon and three-nucleon interactions
doi: 10.1140/epja/i2011-11128-x
2011HO14 Nucl.Phys. A870-871, 1 (2011) Second-order quasiparticle interaction in nuclear matter with chiral two-nucleon interactions
doi: 10.1016/j.nuclphysa.2011.09.006
2010HO01 Phys.Rev. C 81, 024002 (2010) Density-dependent effective nucleon-nucleon interaction from chiral three-nucleon forces
doi: 10.1103/PhysRevC.81.024002
2009HO02 Phys.Rev. C 79, 054331 (2009) Chiral three-nucleon interaction and the 14C-dating β decay RADIOACTIVITY 14C(β-); calculated Gamow-Teller matrix elements, B(GT) using universal low momentum chiral nucleon-nuclear potential N3LO. Comparison with experimental data.
doi: 10.1103/PhysRevC.79.054331
2009SI09 Phys.Rev. C 79, 054004 (2009) L.-W.Siu, J.W.Holt, T.T.S.Kuo, G.E.Brown Low-momentum NN interactions and all-order summation of ring diagrams of symmetric nuclear matter
doi: 10.1103/PhysRevC.79.054004
2008HO01 Phys.Rev.Lett. 100, 062501 (2008) J.W.Holt, G.E.Brown, T.T.S.Kuo, J.D.Holt, R.Machleidt Shell Model Description of the 14C Dating β Decay with Brown-Rho-Scaled NN Interactions RADIOACTIVITY 14C(β-); calculated Gamow-Teller matrix elements and β-decay half life using the shell model and medium modified Bonn-B potential.
doi: 10.1103/PhysRevLett.100.062501
2007BR03 Phys.Rep. 439, 161 (2007) G.E.Brown, J.W.Holt, C.-H.Lee, M.Rho Vector manifestation and matter formed in relativistic heavy-ion processes
doi: 10.1016/j.physrep.2006.12.002
2007HO06 Nucl.Phys. A785, 322 (2007) J.W.Holt, G.E.Brown, Jason D.Holt, T.T.S.Kuo Nuclear matter with Brown-Rho-scaled Fermi liquid interaction
doi: 10.1016/j.nuclphysa.2006.12.099
2007HO17 Phys.Rev. C 76, 034325 (2007) J.D.Holt, N.Pietralla, J.W.Holt, T.T.S.Kuo, G.Rainovski Microscopic restoration of proton-neutron mixed symmetry in weakly collective nuclei NUCLEAR STRUCTURE 92Zr, 94Mo, 96Ru, 98Pd, 100Cd; calculated B(M1) and g-factors using the shell model and the microscopic low-momentum nucleon-nucleon interaction.
doi: 10.1103/PhysRevC.76.034325
2006OR09 Phys.Rev.Lett. 97, 062504 (2006) J.N.Orce, J.D.Holt, A.Linnemann, C.J.McKay, S.R.Lesher, C.Fransen, J.W.Holt, A.Kumar, N.Warr, V.Werner, J.Jolie, T.T.S.Kuo, M.T.McEllistrem, N.Pietralla, S.W.Yates Identification of Mixed-Symmetry States in an Odd-Mass Nearly Spherical Nucleus NUCLEAR REACTIONS 93Nb(n, n'), E=1.5-3 MeV; 94Zr(p, 2n), E=11.5-19 MeV; measured Eγ, Iγ, γγ-coin, DSA. 93Nb deduced levels J, π, configurations, T1/2, B(M1), B(E2). Comparison with shell model predictions.
doi: 10.1103/PhysRevLett.97.062504
2005HO29 Phys.Rev. C 72, 041304 (2005) J.D.Holt, J.W.Holt, T.T.S.Kuo, G.E.Brown, S.K.Bogner Low momentum shell model effective interactions with all-order core polarizations NUCLEAR STRUCTURE 18O, 18F; calculated levels, J, π. All-order summation of core-polarization diagrams.
doi: 10.1103/PhysRevC.72.041304
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