NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = C.Horowitz Found 124 matches. Showing 1 to 100. [Next]2024RE05 Phys.Rev. C 109, 035803 (2024) B.T.Reed, F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz Density dependence of the symmetry energy in the post-PREX-CREX era
doi: 10.1103/PhysRevC.109.035803
2023AN15 J.Phys.(London) G50, 120501 (2023) A.M.Ankowski, A.Ashkenazi, S.Bacca, J.L.Barrow, M.Betancourt, A.Bodek, M.E.Christy, L.Doria, S.Dytman, A.Friedland, O.Hen, C.J.Horowitz, N.Jachowicz, W.Ketchum, T.Lux, K.Mahn, C.Mariani, J.Newby, V.Pandey, A.Papadopoulou, E.Radicioni, F.Sanchez, C.Sfienti, J.M.Udias, L.Weinstein, L.Alvarez-Ruso, J.E.Amaro, C.A.Arguelles, A.B.Balantekin, S.Bolognesi, V.Brdar, P.Butti, S.Carey, Z.Djurcic, O.Dvornikov, S.Edayath, S.Gardiner, J.Isaacson, W.Jay, A.Klustova, K.S.McFarland, A.Nikolakopoulos, A.Norrick, S.Pastore, G.Paz, M.H.Reno, I.Ruiz Simo, J.E.Sobczyk, A.Sousa, N.Toro, Y.-D.Tsai, M.Wagman, J.G.Walsh, G.Yang Electron scattering and neutrino physics
doi: 10.1088/1361-6471/acef42
2022DE26 Phys.Rev. C 106, 045803 (2022) A.Deibel, M.E.Caplan, C.J.Horowitz Nuclear fission reaction simulations in compact stars NUCLEAR REACTIONS 232,233Th, 235,236,237,238,239,240,241U(n, γ), (n, F), E=1 MeV; analyzed σ(E); deduced abundance per baryon time evolution for different initial actinide enrichment in cooling white dwarf, heating rate per baryon, total fission heating per baryon versus time, final temperature. Reaction network simulations of fission chain reactions in a cooling white dwarf.
doi: 10.1103/PhysRevC.106.045803
2021DE06 Phys.Lett. B 814, 136115 (2021) R.T.deSouza, V.Singh, S.Hudan, Z.Lin, C.J.Horowitz Effect of increasing neutron-excess on the fusion cross-section in 12-15C + 12C at above-barrier energies NUCLEAR REACTIONS 12C(12C, X), (13C, X), (14C, X), (15C, X), E(cm)<20 MeV; analyzed available data; deduced fusion σ using the FSUGOLD and NL3 interactions, TDHF model with a SLy4d interaction; deduced the stronger dependence on neutron-excess attributable to dynamics.
doi: 10.1016/j.physletb.2021.136115
2021HO06 Phys.Rev.Lett. 126, 131101 (2021) Actinide Crystallization and Fission Reactions in Cooling White Dwarf Stars NUCLEAR REACTIONS 235,238U, 232Th(n, F), (n, γ), E<1 MeV; calculated composition of solid, 235U enrichment fraction, criticality conditions. ENDF/B-VII.1 library.
doi: 10.1103/PhysRevLett.126.131101
2021RE05 Phys.Rev.Lett. 126, 172503 (2021) B.T.Reed, F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz Implications of PREX-2 on the Equation of State of Neutron-Rich Matter NUCLEAR STRUCTURE 208Pb; analyzed available data for the neutron skin thickness; deduced the slope of the symmetry energy, the impact of stiff symmetry energy on some critical neutron-star observables.
doi: 10.1103/PhysRevLett.126.172503
2020FA09 Phys.Rev. C 102, 065805 (2020) F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz, B.Reed GW190814: Impact of a 2.6 solar mass neutron star on the nucleonic equations of state
doi: 10.1103/PhysRevC.102.065805
2020HO16 Phys.Rev. C 102, 044321 (2020) C.J.Horowitz, J.Piekarewicz, B.Reed Insights into nuclear saturation density from parity-violating electron scattering NUCLEAR STRUCTURE 208Pb; calculated charge density, saturation density of nuclear matter, baryon density, extrapolation factor as a function of the neutron skin thickness for several nonrelativistic and relativistic energy density functionals (EDFs) using PREX experimental result for the weak radius of 208Pb, and symmetrized two parameter Fermi function. Comparison with other theoretical predictions.
doi: 10.1103/PhysRevC.102.044321
2020HU08 Phys.Rev. C 101, 061601 (2020) S.Hudan, R.T.deSouza, A.S.Umar, Z.Lin, C.J.Horowitz Enhanced dynamics in fusion of neutron-rich oxygen nuclei at above-barrier energies NUCLEAR REACTIONS 12C(16O, X), (17O, X), (18O, X), (19O, X), E(cm)=7-20 MeV; calculated above-barrier fusion σ(E) using static and dynamical microscopic model. Comparison with experimental data, and with CCFULL, TDHF and FHF calculations.
doi: 10.1103/PhysRevC.101.061601
2020KO22 Phys.Rev. C 102, 022501 (2020) O.Koshchii, J.Erler, M.Gorchtein, C.J.Horowitz, J.Piekarewicz, X.Roca-Maza, C.-Y.Seng, H.Spiesberger Weak charge and weak radius of 12C NUCLEAR REACTIONS 12C(e, e), E=155 MeV; calculated parity-violating (PV) asymmetry; deduced weak charge, weak radius and neutron skin of 12C nucleus. Parity-violating electron scattering (PVEC), based on model-independent assessment of the uncertainties. Relevance to experiments at the upcoming MESA facility in Mainz, to quantification of generic isospin symmetry-breaking (ISB) effects, test of unitarity of Cabibbo-Kobayashi-Maskawa (CKM) matrix, and new physics searches with superallowed β decays.
doi: 10.1103/PhysRevC.102.022501
2020LI43 Phys.Rev. C 102, 045801 (2020) Z.Lin, M.E.Caplan, C.J.Horowitz, C.Lunardini Fast neutrino cooling of nuclear pasta in neutron stars: Molecular dynamics simulations
doi: 10.1103/PhysRevC.102.045801
2020RE08 Phys.Rev. C 101, 045803 (2020) Large sound speed in dense matter and the deformability of neutron stars
doi: 10.1103/PhysRevC.101.045803
2020RE16 Phys.Rev. C 102, 064308 (2020) B.T.Reed, Z.Jaffe, C.J.Horowitz, C.Sfienti Measuring the surface thickness of the weak charge density of nuclei NUCLEAR REACTIONS 48Ca, 208Pb(polarized e-, e-), E=855, 950, 2220 MeV; calculated differential σ(θ) and parity violating asymmetry including Coulomb distortions, radius and surface thickness parameters, weak charge density versus radius for 855 MeV beam energy, log derivative of parity violating asymmetry with respect to the log of the surface thickness parameter or the log of the weak radius versus scattering angle; evaluated statistical uncertainties and figure of merit (FOM) for proposed experiments at the A1 spectrometer facility of the MAMI accelerator to measure the surface thickness of the weak charge density of a heavy nucleus, further to present PREX-II and CREX parity violating electron scattering experiments probing the weak charge densities. Fermi function fit with relativistic and non-relativistic mean field models.
doi: 10.1103/PhysRevC.102.064308
2019HO02 Phys.Lett. B 789, 675 (2019) Weak radius of the proton NUCLEAR STRUCTURE 1H; analyzed available data for proton radius; deduced new experiment for large weak radius with parity violating electron scattering.
doi: 10.1016/j.physletb.2018.12.029
2019HO13 Ann.Phys.(New York) 411, 167992 (2019) Neutron rich matter in the laboratory and in the heavens after GW170817
doi: 10.1016/j.aop.2019.167992
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
2018BR08 Phys.Rev.Lett. 120, 182701 (2018) E.F.Brown, A.Cumming, F.J.Fattoyev, C.J.Horowitz, D.Page, S.Reddy Rapid Neutrino Cooling in the Neutron Star MXB 1659-29
doi: 10.1103/PhysRevLett.120.182701
2018CA21 Phys.Rev.Lett. 121, 132701 (2018) M.E.Caplan, A.S.Schneider, C.J.Horowitz Elasticity of Nuclear Pasta
doi: 10.1103/PhysRevLett.121.132701
2018FA05 Phys.Rev.Lett. 120, 172702 (2018) F.J.Fattoyev, J.Piekarewicz, C.J.Horowitz Neutron Skins and Neutron Stars in the Multimessenger Era NUCLEAR STRUCTURE 208Pb; calculated neutron star dimensionless tidal polarizability as a function of the neutron-skin thickness of 208Pb, mass-vs-radius relations.
doi: 10.1103/PhysRevLett.120.172702
2018FA08 Phys.Rev. C 98, 025801 (2018) F.J.Fattoyev, E.F.Brown, A.Cumming, A.Deibel, C.J.Horowitz, B.-A.Li, Z.Lin Deep crustal heating by neutrinos from the surface of accreting neutron stars NUCLEAR REACTIONS 1H, Fe(p, π+), Fe(α, π+), E=290-550 MeV/nucleon; calculated multiplicity of pion production as a function of beam energy, total energy per accreted nucleon deposited by neutrinos in the inner crust for a neutron star using the four equations of state, total energy deposited by neutrinos into the inner crust; investigated a new mechanism of deep crustal heating of neutron stars in mass-transferring binaries by neutrinos from decay of charged pions produced at the surface of the neutron stars through p+p, p+Fe and α+Fe collisions.
doi: 10.1103/PhysRevC.98.025801
2018SC11 Phys.Rev. C 98, 055801 (2018) A.S.Schneider, M.E.Caplan, D.K.Berry, C.J.Horowitz Domains and defects in nuclear pasta
doi: 10.1103/PhysRevC.98.055801
2018VA03 Phys.Rev. C 97, 031601 (2018) J.Vadas, V.Singh, B.B.Wiggins, J.Huston, S.Hudan, R.T.deSouza, Z.Lin, C.J.Horowitz, A.Chbihi, D.Ackermann, M.Famiano, K.W.Brown Probing the fusion of neutron-rich nuclei with re-accelerated radioactive beams NUCLEAR REACTIONS 28Si(39K, X), (47K, X), E=2-3 MeV/nucleon, [ions of 39K from a source, and 47K from a thermalized radioactive beam charge bred in an ion trap, injected into the ReA3 linac at NSCL-MSU facility]; measured reaction products, particles by ΔE-TOF, fusion σ(E); deduced impact of additional neutrons on fusion. Comparison with Wong parametrization, and with different models including coupled-channel calculations using CCFULL code.
doi: 10.1103/PhysRevC.97.031601
2017BO24 Phys.Rev.Lett. 119, 242702 (2017) R.Bollig, H.-T.Janka, A.Lohs, G.Martinez-Pinedo, C.J.Horowitz, T.Melson Muon Creation in Supernova Matter Facilitates Neutrino-Driven Explosions
doi: 10.1103/PhysRevLett.119.242702
2017CA06 Prog.Part.Nucl.Phys. 94, 68 (2017) J.Carlson, M.P.Carpenter, R.Casten, C.Elster, P.Fallon, A.Gade, C.Gross, G.Hagen, A.C.Hayes, D.W.Higinbotham, C.R.Howell, C.J.Horowitz, K.L.Jones, F.G.Kondev, S.Lapi, A.Macchiavelli, E.A.McCutchan, J.Natowitz, W.Nazarewicz, T.Papenbrock, S.Reddy, M.J.Savage, G.Savard, B.M.Sherrill, L.G.Sobotka, M.A.Stoyer, M.B.Tsang, K.Vetter, I.Wiedenhoever, A.H.Wuosmaa, S.Yennello White paper on nuclear astrophysics and low-energy nuclear physics, Part 2: Low-energy nuclear physics
doi: 10.1016/j.ppnp.2016.11.002
2017CU02 Phys.Rev. C 95, 025806 (2017) A.Cumming, E.F.Brown, F.J.Fattoyev, C.J.Horowitz, D.Page, S.Reddy Lower limit on the heat capacity of the neutron star core
doi: 10.1103/PhysRevC.95.025806
2017FA05 Phys.Rev. C 95, 055804 (2017) F.J.Fattoyev, C.J.Horowitz, B.Schuetrumpf Quantum nuclear pasta and nuclear symmetry energy
doi: 10.1103/PhysRevC.95.055804
2017HO05 Phys.Rev. C 95, 025801 (2017) C.J.Horowitz, O.L.Caballero, Z.Lin, E.O'Connor, A.Schwenk Neutrino-nucleon scattering in supernova matter from the virial expansion
doi: 10.1103/PhysRevC.95.025801
2017LI41 Phys.Rev. C 96, 055804 (2017) Neutrino scattering in supernovae and the universal spin correlations of a unitary gas
doi: 10.1103/PhysRevC.96.055804
2017SI03 Phys.Lett. B 765, 99 (2017) V.Singh, J.Vadas, T.K.Steinbach, B.B.Wiggins, S.Hudan, R.T.deSouza, Z.Lin, C.J.Horowitz, L.T.Baby, S.A.Kuvin, V.Tripathi, I.Wiedenhover, A.S.Umar Fusion enhancement at near and sub-barrier energies in 19O + 12C NUCLEAR REACTIONS 12C(18O, X), (19O, X), E(cm)<20 MeV; measured reaction products; deduced σ. comparison with a state-of-the-art microscopic model.
doi: 10.1016/j.physletb.2016.12.017
2016BE36 Phys.Rev. C 94, 055801 (2016) D.K.Berry, M.E.Caplan, C.J.Horowitz, G.Huber, A.S.Schneider "Parking-garage" structures in nuclear astrophysics and cellular biophysics
doi: 10.1103/PhysRevC.94.055801
2016SA24 Phys.Rev. C 93, 055801 (2016) I.Sagert, G.I.Fann, F.J.Fattoyev, S.Postnikov, C.J.Horowitz Quantum simulations of nuclei and nuclear pasta with the multiresolution adaptive numerical environment for scientific simulations NUCLEAR STRUCTURE 16O, 208Pb, 238U; calculated nuclear ground states, binding energies, shapes of light and heavy nuclei with different geometries with and without spin-orbit forces via three-dimensional (3D) Skyrme Hartree-Fock (SHF) simulations of nuclear pasta with Multi-resolution ADaptive Numerical Environment for Scientific Simulations (MADNESS); deduced that pasta phase remains in waffle geometry. Relevance to exotic shapes of neutron star and supernova matter.
doi: 10.1103/PhysRevC.93.055801
2016SC09 Phys.Rev. C 93, 065806 (2016) A.S.Schneider, D.K.Berry, M.E.Caplan, C.J.Horowitz, Z.Lin Effect of topological defects on "nuclear pasta" observables
doi: 10.1103/PhysRevC.93.065806
2015CA07 Phys.Rev. C 91, 065802 (2015) M.E.Caplan, A.S.Schneider, C.J.Horowitz, D.K.Berry Pasta nucleosynthesis: Molecular dynamics simulations of nuclear statistical equilibrium
doi: 10.1103/PhysRevC.91.065802
2015LI27 Phys.Rev. C 92, 014313 (2015) Full weak-charge density distribution of 48Ca from parity-violating electron scattering NUCLEAR REACTIONS 48Ca(e, e), E=2 GeV; calculated ground state electromagnetic charge and weak charge densities of 48Ca versus radius, σ(θ), six Fourier Bessel coefficients, full radial structure of weak charge density, neutron density, parity violating asymmetry parameter. Comparison with experimental data. 1n; deduced size, surface thickness, shell oscillations, and saturation density of the neutron distribution.
doi: 10.1103/PhysRevC.92.014313
2015UM03 Phys.Rev. C 92, 025808 (2015) A.S.Umar, V.E.Oberacker, C.J.Horowitz, P.-G.Reinhard, J.A.Maruhn Swelling of nuclei embedded in neutron-gas and consequences for fusion NUCLEAR REACTIONS 28O(28O, X), E(cm)=2-14 MeV; 60Ca(60Ca, X), E(cm)=34-58 MeV; calculated pycnonuclear fusion cross sections and Astrophysical S factor as a function of external neutron-gas density, up to 500 neutrons for 28O and 1040 for 60Ca using Sao Paulo potential and incoming wave boundary condition (IWBC) method. Relevance to study of fusion of neutron rich nuclei at radioactive ion beam facilities, and to the study of composition and heating of the crust of accreting neutron stars.
doi: 10.1103/PhysRevC.92.025808
2014HA01 Phys.Rev. C 89, 014319 (2014) G.Hagen, T.Papenbrock, A.Ekstrom, K.A.Wendt, G.Baardsen, S.Gandolfi, M.Hjorth-Jensen, C.J.Horowitz Coupled-cluster calculations of nucleonic matter NUCLEAR STRUCTURE A=10-1000; N=66, 132; calculated relative finite-size corrections for the kinetic energy in pure neutron matter, E/A of nuclear and neutron matter. Coupled-cluster computations of equation of state (EoS) for symmetric nuclear matter and neutron matter using optimized nucleon-nucleon (NN) potential NNLOopt at next-to-next-to leading order. Comparison with benchmark calculations.
doi: 10.1103/PhysRevC.89.014319
2014HO05 Eur.Phys.J. A 50, 48 (2014) C.J.Horowitz, K.S.Kumar, R.Michaels Electroweak measurements of neutron densities in CREX and PREX at JLab, USA
doi: 10.1140/epja/i2014-14048-3
2014HO07 Phys.Rev. C 89, 045503 (2014) Parity violating elastic electron scattering from 27Al and the Qweak measurement NUCLEAR REACTIONS 27Al(e, e), E=250, 1160 MeV; calculated parity violating asymmetry, differential σ(θ), proton-, and neutron-charge-radii using plane wave Born approximation, FSUgold, and RMF models. Estimate of inelastic scattering and impurity contributions. Comparison with data from Qweak experiment.
doi: 10.1103/PhysRevC.89.045503
2014PI06 Phys.Rev. C 90, 015803 (2014) J.Piekarewicz, F.J.Fattoyev, C.J.Horowitz Pulsar glitches: The crust may be enough NUCLEAR STRUCTURE 208Pb; calculated binding energy per nucleon, charge radius, and neutron-skin thickness, fraction of the crustal moment of inertia as a function of the neutron-skin thickness of 208Pb using relativistic mean-field models FSUGold and NL3. Comparison with experimental data. Calculated fractional moment of inertia of neutron stars of various masses using a representative set of relativistic mean-field models.
doi: 10.1103/PhysRevC.90.015803
2014SC26 Phys.Rev. C 90, 055805 (2014) A.S.Schneider, D.K.Berry, C.M.Briggs, M.E.Caplan, C.J.Horowitz Nuclear ``waffles"
doi: 10.1103/PhysRevC.90.055805
2013ER04 Phys.Rev. C 87, 044320 (2013) J.Erler, C.J.Horowitz, W.Nazarewicz, M.Rafalski, P.-G.Reinhard Energy density functional for nuclei and neutron stars NUCLEAR STRUCTURE 208Pb; calculated neutron skin radius, electric dipole polarizability, mass-radius relations, correlation of nuclear matter properties with neutron star mass. Z=100, N=140-260; calculated S2n of even-even nuclei. Z=4-120, N=4-300; calculated two neutron and two proton drip lines. Self-consistent nuclear density functional theory (DFT) with Skyrme energy density functionals and covariance analysis.
doi: 10.1103/PhysRevC.87.044320
2013SC26 Phys.Rev. C 88, 065807 (2013) A.S.Schneider, C.J.Horowitz, J.Hughto, D.K.Berry Nuclear "pasta" formation
doi: 10.1103/PhysRevC.88.065807
2012BA01 J.Phys.(London) G39, 015104 (2012) S.Ban, C.J.Horowitz, R.Michaels Parity violating electron scattering measurements of neutron densities NUCLEAR REACTIONS 40,48Ca, 112,120,124Sn, 208Pb(e, e), E=1.05, 1.8 GeV; calculated error estimates for neutron radius measurements, surface thickness of neutron density.
doi: 10.1088/0954-3899/39/1/015104
2012HO07 Phys.Rev. C 85, 032501 (2012) C.J.Horowitz, Z.Ahmed, C.-M.Jen, A.Rakhman, P.A.Souder, M.M.Dalton, N.Liyanage, K.D.Paschke, K.Saenboonruang, R.Silwal, G.B.Franklin, M.Friend, B.Quinn, K.S.Kumar, D.McNulty, L.Mercado, S.Riordan, J.Wexler, R.W.Michaels, G.M.Urciuoli Weak charge form factor and radius of 208Pb through parity violation in electron scattering NUCLEAR STRUCTURE 208Pb; calculated weak charge form factor, weak charge radius, weak charge density using point neutron radius from Lead Radius Experiment (PREX) parity-violating asymmetry measurement. Distorted wave electron scattering calculations, Helm model.
doi: 10.1103/PhysRevC.85.032501
2012HO23 Prog.Theor.Phys.(Kyoto), Suppl. 196, 451 (2012) Multi-Messenger Observations of Neutron Rich Matter
doi: 10.1143/PTPS.196.451
2012HO24 Phys.Rev. C 86, 045503 (2012) Impact of spin-orbit currents on the electroweak skin of neutron-rich nuclei NUCLEAR STRUCTURE 22O, 48Ca, 90Zr, 118,132Sn, 138Ba, 158Dy, 176Yb, 208Pb; calculated proton-, neutron-, charge-, weak-charge radii, neutron and weak skins. NL3 and FSU relativistic mean-field approximation. Spin-orbit contributions to the electroweak skin of neutron-rich nuclei.
doi: 10.1103/PhysRevC.86.045503
2012HO25 Phys.Rev. C 86, 065806 (2012) C.J.Horowitz, G.Shen, E.O'Connor, C.D.Ott Charged-current neutrino interactions in core-collapse supernovae in a virial expansion
doi: 10.1103/PhysRevC.86.065806
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
2012UM02 Phys.Rev. C 85, 055801 (2012) A.S.Umar, V.E.Oberacker, C.J.Horowitz Microscopic sub-barrier fusion calculations for the neutron star crust NUCLEAR REACTIONS 12C, 16,24,28O(16O, X), (24O, X), E(cm)=2-13 MeV; calculated nuclear density contours, potential barriers, fusion σ(E), astrophysical S factor. Time-dependent Hartree-Fock theory with density-constrained Hartree-Fock calculations. Comparison with Sao Paulo static barrier penetration model and experimental data.
doi: 10.1103/PhysRevC.85.055801
2011GO21 Phys.Rev. C 84, 015502 (2011) M.Gorchtein, C.J.Horowitz, M.J.Ramsey-Musolf Model dependence of the γ Z dispersion correction to the parity-violating asymmetry in elastic ep scattering NUCLEAR REACTIONS 1H(polarized e, e), E=2.2375-5.498 GeV; calculated total photoabsorption cross section, differential cross section for inclusive electroproduction; deduced theory uncertainty at the kinematics of the Q-Weak experiment. Comparison with experimental data.
doi: 10.1103/PhysRevC.84.015502
2011HO12 Int.J.Mod.Phys. E20, 2077 (2011) Multi-Messenger Observations of Neutron-Rich Matter
doi: 10.1142/S0218301311020332
2011HO22 J.Phys.:Conf.Ser. 312, 042003 (2011) Neutron rich matter, neutron stars, and their crusts
doi: 10.1088/1742-6596/312/4/042003
2011SH11 Phys.Rev. C 83, 035802 (2011) New equation of state for astrophysical simulations
doi: 10.1103/PhysRevC.83.035802
2011SH22 Phys.Rev. C 83, 065808 (2011) G.Shen, C.J.Horowitz, E.O'Connor Second relativistic mean field and virial equation of state for astrophysical simulations
doi: 10.1103/PhysRevC.83.065808
2010FA18 Phys.Rev. C 82, 055803 (2010) F.J.Fattoyev, C.J.Horowitz, J.Piekarewicz, G.Shen Relativistic effective interaction for nuclei, giant resonances, and neutron stars NUCLEAR STRUCTURE 40,48Ca, 90Zr, 132Sn, 208Pb; calculated binding energy, charge radii, neutron skin thickness, charge and neutron densities, centroid energies of giant-monopole resonances (GMR) using relativistic mean-field (RMF) theory and NL3, FSU and IU-FSU interactions. Equation of state for neutron-star structure. Comparison with experimental data.
doi: 10.1103/PhysRevC.82.055803
2010SH15 Phys.Rev. C 82, 015806 (2010) Equation of state of dense matter from a density dependent relativistic mean field model
doi: 10.1103/PhysRevC.82.015806
2010SH26 Phys.Rev. C 82, 045802 (2010) Equation of state of nuclear matter in a virial expansion of nucleons and nuclei NUCLEAR STRUCTURE Z=3-60, A=12-160; calculated free energy/nucleon and mass fractions using equation of state (EOS) model of nuclear matter at subnuclear density in a virial expansion for a nonideal gas of neutrons, protons, α particles, and 8980 species of nuclei at temperatures of 0.158 to 15.8 MeV.
doi: 10.1103/PhysRevC.82.045802
2009HO03 Phys.Rev. C 79, 065803 (2009) Structure of accreted neutron star crust
doi: 10.1103/PhysRevC.79.065803
2008AR06 Phys.Rev. C 78, 015806 (2008) A.Arcones, G.Martinez-Pinedo, E.O'Connor, A.Schwenk, H.-Th.Janka, C.J.Horowitz, K.Langanke Influence of light nuclei on neutrino-driven supernova outflows NUCLEAR REACTIONS 3H(ν-bar, ν-bar), (ν-bar, e+), E=11-100 MeV; calculated σ.
doi: 10.1103/PhysRevC.78.015806
2008CA24 Phys.Rev. C 78, 045805 (2008) O.L.Caballero, S.Postnikov, C.J.Horowitz, M.Prakash Shear viscosity of the outer crust of neutron stars: Ion contributions
doi: 10.1103/PhysRevC.78.045805
2008GO12 Phys.Rev. C 77, 044606 (2008) Analyzing power in elastic scattering of electrons off a spin-0 target NUCLEAR REACTIONS 4He(e, e), E=3 GeV; 208Pb(e, e), E=850, 2700 MeV; calculated analyzing power. Comparison with experimental data.
doi: 10.1103/PhysRevC.77.044606
2008HO06 Phys.Rev. C 77, 045807 (2008) C.J.Horowitz, H.Dussan, D.K.Berry Fusion of neutron-rich oxygen isotopes in the crust of accreting neutron stars NUCLEAR REACTIONS 24O(24O, X);28Ne(28Ne, X), E=1, 1.5, 2, 3, 4, 6, 8; calculated astrophysical S-factor, reaction rates. O, Ne, Ti, Se; radial distribution functions, screening potentials, thermonuclear fusion reaction rates.
doi: 10.1103/PhysRevC.77.045807
2008HO07 Phys.Rev. C 78, 015801 (2008) Shell states of neutron-rich matter
doi: 10.1103/PhysRevC.78.015801
2008HO09 Phys.Rev. C 78, 035806 (2008) Shear viscosity and thermal conductivity of nuclear "pasta"
doi: 10.1103/PhysRevC.78.035806
2007OC01 Phys.Rev. C 75, 055803 (2007) E.O'Connor, D.Gazit, C.J.Horowitz, A.Schwenk, N.Barnea Neutrino breakup of A = 3 nuclei in supernovae NUCLEAR REACTIONS 3H(ν, X), 3He(ν, X), E not given; calculated mass fraction of nucleons, average neutral current inclusive inelastic cross section per nucleon, and neutrino energy loss for inelastic excitations at supernova temperature and desities using the cirial equation of state.
doi: 10.1103/PhysRevC.75.055803
2006CA36 Phys.Rev.C 74, 065801 (2006) O.L.Caballero, C.J.Horowitz, D.K.Berry Neutrino scattering in heterogeneous supernova plasmas
doi: 10.1103/PhysRevC.74.065801
2006HO09 Phys.Lett. B 638, 153 (2006) The virial equation of state of low-density neutron matter
doi: 10.1016/j.physletb.2006.05.055
2006HO12 Nucl.Phys. A776, 55 (2006) Cluster formation and the virial equation of state of low-density nuclear matter
doi: 10.1016/j.nuclphysa.2006.05.009
2006HO18 Eur.Phys.J. A 30, 303 (2006) Links between heavy ion and astrophysics
doi: 10.1140/epja/i2006-10124-7
2006HO22 Phys.Lett. B 642, 326 (2006) The neutrino response of low-density neutron matter from the virial expansion
doi: 10.1016/j.physletb.2006.09.042
2006NO08 Phys.Lett. B 639, 465 (2006) A.Nogga, A.C.Fonseca, A.Gardestig, C.Hanhart, C.J.Horowitz, G.A.Miller, J.A.Niskanen, U.van Kolck Realistic few-body physics in the dd → απ0 NUCLEAR REACTIONS 2H(d, π0), E=293 MeV; calculated σ, related matrix elements. Effective field theory with four-body theory.
doi: 10.1016/j.physletb.2006.04.058
2005CO18 Phys.Rev. C 72, 034602 (2005) Vector analyzing power in elastic electron-nucleus scattering NUCLEAR REACTIONS 4He(e, e), E=3 GeV; 208Pb(e, e), E=200, 850 MeV; 16O, 40Ca, 90Zr(e, e), E=850 MeV; calculated σ(θ), vector analyzing power.
doi: 10.1103/PhysRevC.72.034602
2005HO07 Eur.Phys.J. A 24, Supplement 2, 167 (2005) Parity violation in astrophysics NUCLEAR REACTIONS 208Pb(polarized e, e), E=850 MeV; calculated Ay(θ).
doi: 10.1140/epjad/s2005-04-042-x
2005HO27 Phys.Rev. C 72, 035801 (2005) C.J.Horowitz, M.A.Perez-Garcia, D.K.Berry, J.Piekarewicz Dynamical response of the nuclear "pasta" in neutron star crusts
doi: 10.1103/PhysRevC.72.035801
2004GA22 Phys.Rev. C 69, 044606 (2004) A.Gardestig, C.J.Horowitz, A.Nogga, A.C.Fonseca, C.Hanhart, G.A.Miller, J.A.Niskanen, U.van Kolck Survey of charge symmetry breaking operators for dd → απ0 NUCLEAR REACTIONS 2H(d, π0), E=228.5, 231.8 MeV; calculated pion production total σ, charge symmetry breaking amplitudes; deduced reaction mechanism features. Effective field theory approach.
doi: 10.1103/PhysRevC.69.044606
2004HO11 Phys.Rev. C 69, 045804 (2004) C.J.Horowitz, M.A.Perez-Garcia, J.Piekarewicz Neutrino-"pasta" scattering: The opacity of nonuniform neutron-rich matter
doi: 10.1103/PhysRevC.69.045804
2004HO23 Phys.Rev. C 70, 065806 (2004) C.J.Horowitz, M.A.Perez-Garcia, J.Carriere, D.K.Berry, J.Piekarewicz Nonuniform neutron-rich matter and coherent neutrino scattering
doi: 10.1103/PhysRevC.70.065806
2003HO15 Phys.Rev. C 68, 025803 (2003) C.J.Horowitz, M.A.Perez-Garcia Realistic neutrino opacities for supernova simulations with correlations and weak magnetism
doi: 10.1103/PhysRevC.68.025803
2002HO21 Phys.Rev. C 66, 055803 (2002) Constraining URCA cooling of neutron stars from the neutron radius of 208Pb NUCLEAR STRUCTURE 208Pb; analyzed neutron, proton radii, application to astrophysical data.
doi: 10.1103/PhysRevC.66.055803
2002HO23 Acta Phys.Hung.N.S. 16, 113 (2002) The Lead Nucleus as a Miniature Surrogate or a Neutron Star NUCLEAR STRUCTURE 208Pb; calculated matter densities, neutron skin thickness. Application to neutron star studies discussed.
doi: 10.1556/APH.16.2002.1-4.13
2001HO01 Phys.Rev. C63, 011303 (2001) Density Dependence of Charge Symmetry Breaking
doi: 10.1103/PhysRevC.63.011303
2001HO03 Phys.Rev. C63, 025501 (2001) C.J.Horowitz, S.J.Pollock, P.A.Souder, R.Michaels Parity Violating Measurements of Neutron Densities NUCLEAR REACTIONS 208Pb(e, e), E=0.85 GeV; 138Ba(e, e), E=1.0 GeV; calculated σ(q), parity violating asymmetry, sensitivity to neutron radius.
doi: 10.1103/PhysRevC.63.025501
2001HO17 Phys.Rev.Lett. 86, 5647 (2001) Neutron Star Structure and the Neutron Radius of 208Pb NUCLEAR STRUCTURE 208Pb; calculated binding energies, neutron and proton radii. Relativistic effective field theory, implications for neutron star structure discussed.
doi: 10.1103/PhysRevLett.86.5647
2001HO33 Phys.Rev. C64, 062802 (2001) Neutron Radii of 208Pb and Neutron Stars NUCLEAR STRUCTURE 208Pb; calculated neutron, proton density distributions, radii. Relativistic effective field theory, implications for neutron star radii discussed.
doi: 10.1103/PhysRevC.64.062802
1999HO17 Phys.Rev.Lett. 82, 5198 (1999) Nucleosynthesis in Supernovae NUCLEAR REACTIONS 1n(ν, e), 1H(ν, e+), E ≈ 10-25 MeV; analyzed σ in supernova environment; deduced implications for nucleosynthesis.
doi: 10.1103/PhysRevLett.82.5198
1999HO20 Phys.Rev. C60, 022801 (1999) High Energy Solar Neutrinos and p-Wave Contributions to 3He(p, νe+)4He NUCLEAR REACTIONS 3He(p, e+ν), E not given; 3He(p, p), E < 30 MeV; calculated p-wave contribution to S factor. Application the solar neutrino spectra discussed.
doi: 10.1103/PhysRevC.60.022801
1998HO12 Phys.Rev. C57, 3430 (1998) Parity Violating Elastic Electron Scattering and Coulomb Distortions NUCLEAR REACTIONS 4He, 16O, 48Ca, 138Ba, 208Pb(e, e), E=850 MeV; 12C(e, e), E=200 MeV; calculated parity-violating asymmetry vs θ; 208Pb(e, e), E=502, 850, 3000 MeV; calculated parity-violating asymmetry vs momentum transfer; deduced Coulomb distortion effects.
doi: 10.1103/PhysRevC.57.3430
1998HO18 Nucl.Phys. A640, 281 (1998) Macroscopic Parity Violation and Supernova Asymmetries
doi: 10.1016/S0375-9474(98)00444-8
1996GA03 Phys.Rev. C53, 1143 (1996) S.Gardner, C.J.Horowitz, J.Piekarewicz Isospin-Violating Meson-Nucleon Vertices as an Alternate Mechanism of Charge-Symmetry Breaking
doi: 10.1103/PhysRevC.53.1143
1996KI05 Phys.Rev. C53, 2468 (1996) H.Kim, S.Schramm, C.J.Horowitz Delta Excitations in Neutrino-Nucleus Scattering NUCLEAR REACTIONS 16O(ν, μ), E=1 GeV; calculated double differential σ. Quasielastic scattering, Δ-hole excitation.
doi: 10.1103/PhysRevC.53.2468
1996KI06 Phys.Rev. C53, 3131 (1996) H.Kim, S.Schramm, C.J.Horowitz Detection of Atmospheric Neutrinos and Relativistic Nuclear Structure Effects
doi: 10.1103/PhysRevC.53.3131
1995GA31 Phys.Rev.Lett. 75, 2462 (1995) S.Gardner, C.J.Horowitz, J.Piekarewicz Charge-Symmetry-Breaking Potentials from Isospin-Violating Meson-Baryon Coupling Constants NUCLEAR REACTIONS 1H(polarized n, n), E=183 MeV; analyzed n, p analyzing power difference data; deduced charge symmetry breaking potential characteristics. Polarized target.
doi: 10.1103/PhysRevLett.75.2462
1995KI01 Phys.Rev. C51, 792 (1995) H.Kim, C.J.Horowitz, M.R.Frank Relativistic Models for Quasielastic (e, e') at Large Momentum Transfers NUCLEAR REACTIONS 40Ca(e, e'), E not given; calculated transverse response functions. 56Fe(e, e'), E not given; calculated longitudinal response functions. Relativistic model, momentum dependent scalar, vector mean fields.
doi: 10.1103/PhysRevC.51.792
1995KI08 Phys.Rev. C51, 2739 (1995) H.Kim, J.Piekarewicz, C.J.Horowitz Relativistic Nuclear Structure Effects in Quasielastic Neutrino Scattering
doi: 10.1103/PhysRevC.51.2739
1994GA21 Phys.Rev. C50, 1137 (1994) S.Gardner, C.J.Horowitz, J.Piekarewicz Dynamical Color Correlations in a SU(2)(c) Quark Exchange Model of Nuclear Matter
doi: 10.1103/PhysRevC.50.1137
1994HO04 Phys.Rev. C49, 1337 (1994) C.J.Horowitz, H.O.Meyer, D.K.Griegel Role of Heavy-Meson Exchange in Pion Production Near Threshold NUCLEAR REACTIONS 1H(p, pπ0), E < 400 MeV; calculated σ vs E, pion momentum; deduced heavy meson exchange role.
doi: 10.1103/PhysRevC.49.1337
1994HO09 Phys.Rev. C49, 3042 (1994) Parity Violation in Heavy Nuclei in a Relativistic Hartree-Fock Approximation NUCLEAR STRUCTURE 207Pb; calculated parity violating matrix element. Relativistic Hartree-Fock approximation.
doi: 10.1103/PhysRevC.49.3042
1994HO15 Phys.Rev. C50, 2540 (1994) Relativistic Treatment of Spin-Transfer Observables in Quasielastic (p(pol), n(pol) Scattering NUCLEAR REACTIONS 40Ca(e, e'), E not given; calculated transverse response function. 12C, 2H, 40Ca(polarized p, n), E not given; calculated spin-transfer observables. Relativistic PWIA.
doi: 10.1103/PhysRevC.50.2540
1994HO18 Nucl.Phys. A577, 137c (1994) Relativistic Models of the Spin-Isospin-Weak Quasielastic Response NUCLEAR REACTIONS 12C, 40Ca(polarized p, n), E=495 MeV; calculated spin response functions longitudinal to transverse ratio. Relativistic formalism.
doi: 10.1016/0375-9474(94)90846-X
1994SC13 Phys.Rev. C49, 2777 (1994) Meson Exchange Effects in Parity Violating Electron-Deuteron Scattering NUCLEAR REACTIONS 2H(e, e'X), E not given; calculated parity violating response functions ratio, asymmetry; deduced heavy meson exchange effects contribution.
doi: 10.1103/PhysRevC.49.2777
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