Nuclear Science References (NSR)

NUCLEAR STRUCTURE ²⁰⁸Pb; calculated symmetry energy and its slope of nuclear matter, neutron skin thickness, proton and neutron density profiles using Thomas-Fermi approximation. Investigated nuclear pasta structures in a three-dimensional geometry with reflection symmetry using RMF model with Thomas-Fermi approximation; deduced similarity of droplets and bubbles in body-centered cubic (bcc) and face-centered cubic (fcc) lattices, with impact on properties of neutron stars, supernova dynamics, and binary neutron star mergers.

doi: 10.1103/PhysRevC.103.055812
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2019MA60 Phys.Rev. C 100, 025802 (2019)

K.Maslov, N.Yasutake, D.Blaschke, A.Ayriyan, H.Grigorian, T.Maruyama, T.Tatsumi, D.N.Voskresensky

Hybrid equation of state with pasta phases, and third family of compact stars

doi: 10.1103/PhysRevC.100.025802
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2017YA29 Phys.Rev. C 96, 065804 (2017)

Y.Yamamoto, H.Togashi, T.Tamagawa, T.Furumoto, N.Yasutake, Th.A.Rijken

Neutron-star radii based on realistic nuclear interactions

doi: 10.1103/PhysRevC.96.065804
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2016YA01 Eur.Phys.J. A 52, 19 (2016)

Y.Yamamoto, T.Furumoto, N.Yasutake, Th.A.Rijken

Hyperon-mixed neutron star with universal many-body repulsion

NUCLEAR REACTIONS ¹⁶O(¹⁶O, ¹⁶O), E=70 MeV/nucleon; calculated σ(θ) using G-matrix folding potentials.

doi: 10.1140/epja/i2016-16019-0
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2014MA13 Phys.Rev. C 89, 035801 (2014)

T.Maruyama, J.Hidaka, T.Kajino, N.Yasutake, T.Kuroda, T.Takiwaki, M.-K.Cheoun, C.-Y.Ryu, G.J.Mathews

Rapid spin deceleration of magnetized protoneutron stars via asymmetric neutrino emission

doi: 10.1103/PhysRevC.89.035801
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2014YA13 Phys.Rev. C 89, 065803 (2014)

N.Yasutake, R.Lastowiecki, S.Benic, D.Blaschke, T.Maruyama, T.Tatsumi

Finite-size effects at the hadron-quark transition and heavy hybrid stars

doi: 10.1103/PhysRevC.89.065803
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2014YA26 Phys.Rev. C 90, 045805 (2014)

Y.Yamamoto, T.Furumoto, N.Yasutake, Th.A.Rijken

Hyperon mixing and universal many-body repulsion in neutron stars

NUCLEAR REACTIONS ¹⁶O(¹⁶O, ¹⁶O), E=70 MeV/nucleon; analyzed differential elastic σ(θ) data with the G-matrix folding potentials; deduced multi-Pomeron exchange potential (MPPs) and used as input to hyperon mixing in neutron stars.

NUCLEAR STRUCTURE ¹³C, ²⁸Si, ⁵¹V, ⁸⁹Y, ¹³⁹La, ²⁰⁸Pb; calculated energy spectra of hypernuclei using MPPs deduced from analysis of ¹⁶O(¹⁶O, ¹⁶O) reaction, composition of hyperonic neutron-star matter in the case of extended soft core (ESC) baryon-baryon interaction, equation of state (EoS) in neutron matter with hyperon mixing; derived mass-radius relations of neutron stars. Comparison with experimental data for energy spectra of hypernuclei.

doi: 10.1103/PhysRevC.90.045805
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2013YA15 Phys.Rev. C 88, 022801 (2013)

Y.Yamamoto, T.Furumoto, N.Yasutake, Th.A.Rijken

Multi-Pomeron repulsion and the neutron-star mass

NUCLEAR REACTIONS ¹⁶O(¹⁶O, ¹⁶O), E=70 MeV/nucleon; analyzed σ(θ) data using G-matrix folding potential derived from extended soft core (ESC) model with three-nucleon interaction (TNA) and multi-Pomeron exchange potential (MPP); deduced fitting parameters for the neutron matter equation of state (EoS); calculated neutron-star mass by solving the Tolmann-Oppenheimer-Volkof equation.

doi: 10.1103/PhysRevC.88.022801
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2011YA24 J.Phys.:Conf.Ser. 312, 042027 (2011)

N.Yasutake, T.Maruyama, T.Tatsumi

Pasta Structures of Quark-Hadron Phase Transition in Proto-Neutron Stars

doi: 10.1088/1742-6596/312/4/042027
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2005YA18 Nucl.Phys. A758, 43c (2005)

N.Yasutake, M.Hashimoto, Y.Eriguchi, K.Arai

Evolutionary transition between rapidly rotating compact stars after supernova explosion

doi: 10.1016/j.nuclphysa.2005.05.165
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