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NSR database version of April 27, 2024.

Search: Author = P.Landry

Found 4 matches.

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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
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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
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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
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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
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