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NSR database version of May 1, 2024.

Search: Author = G.Grams

Found 8 matches.

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2024GR04      Eur.Phys.J. A 60, 90 (2024)

G.Grams, J.Margueron

Effects of dilute neutron matter on the neutron star crust equation of state

doi: 10.1140/epja/s10050-024-01309-3
Citations: PlumX Metrics

2023GR08      Eur.Phys.J. A 59, 270 (2023)

G.Grams, W.Ryssens, G.Scamps, S.Goriely, N.Chamel

Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: III. From atomic nuclei to neutron stars

doi: 10.1140/epja/s10050-023-01158-6
Citations: PlumX Metrics

2022GR02      Phys.Rev. C 105, 035806 (2022)

G.Grams, R.Somasundaram, J.Margueron, S.Reddy

Properties of the neutron star crust: Quantifying and correlating uncertainties with improved nuclear physics

doi: 10.1103/PhysRevC.105.035806
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2022GR03      Eur.Phys.J. A 58, 56 (2022)

G.Grams, J.Margueron, R.Somasundaram, S.Reddy

Confronting a set of Skyrme and χ_EFTpredictions for the crust of neutron stars

doi: 10.1140/epja/s10050-022-00706-w
Citations: PlumX Metrics

2022GR10      Phys.Rev. C 106, 044305 (2022)

G.Grams, R.Somasundaram, J.Margueron, E.Khan

Nuclear incompressibility and speed of sound in uniform matter and finite nuclei

NUCLEAR STRUCTURE ^{98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153,154,155,156,157,158,159,160,161,162}Sn, ^{174,175,176,177,178,179,180,181,182,183,184,185,186,187,188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208,209,210,211,212,213,214,215,216,217,218,219,220,221,222,223,224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260}Pb, ^90,92,94Zr; calculated surface tension, incompressibility, contributions from the surface and Coulomb terms to the incompressibility, speed of sound in finite nuclei matter. ^{100,106,114,120}Sn, ^180,200,208Pb; binding energies, isoscalar giant monopole resonance energy (ISGMR). Compressible liquid-drop model extended with a density-dependent surface term. Bayesian approach coupled to a Markov-Chain Monte Carlo exploration of the parameter space to confront the model predictions. Comparison to experimental results, EDF calculations and AME2020 data.

doi: 10.1103/PhysRevC.106.044305
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2021GR10      Few-Body Systems 62, 116 (2021)

G.Grams, J.Margueron, R.Somasundaram, S.Reddy

Properties of Neutron Star Crust with Improved Nuclear Physics: Impact of Chiral EFT Interactions and Experimental Nuclear Masses

doi: 10.1007/s00601-021-01697-y
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2018GR04      Phys.Rev. C 97, 035807 (2018)

G.Grams, S.Giraud, A.F.Fantina, F.Gulminelli

Distribution of nuclei in equilibrium stellar matter from the free-energy density in a Wigner-Seitz cell

doi: 10.1103/PhysRevC.97.035807
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2017GR10      Phys.Rev. C 95, 055807 (2017)

G.Grams, A.M.Santos, P.K.Panda, C.Providencia, D.P.Menezes

Nuclear pasta phases within the quark-meson coupling model

doi: 10.1103/PhysRevC.95.055807
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