Minisymposium: Solid State Physics in Neutron Stars: Crystallography and Superfluidity
FOCUS · D08 · ID: 1738193
Presentations
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Nuclear pasta and the deep inner crust
ORAL · Invited
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Publication: "Glassy quantum nuclear pasta in neutron star crusts", Physical Review C, Volume 105, Issue 2, article id.025806<br>"From neutron skins and neutron matter to the neutron star crust", Physics Letters B, Volume 834, article id. 137481<br>"Stretching nuclear pasta", in prep
Presenters
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William G Newton
Texas A&M University–Commerce
Authors
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William G Newton
Texas A&M University–Commerce
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Jirina R Stone
University of Oxford
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Mark A Kaltenborn
George Washington University
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Amber Stinson
Texas A&M University-Commerce
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Rebecca Preston
Texas A&M University–Commerce
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Lauren E Balliet
Texas A&M University–Commerce
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Michael Ross
Texas A&M University–Commerce
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Shuxi Wang
Texas A&M University
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Diffusion and Magnetic Fields in Simulations of Neutron Star Crusts
ORAL
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Presenters
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Matthew E Caplan
Illinois State University
Authors
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Matthew E Caplan
Illinois State University
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The role of A=33 mass chain in Urca Cooling of Accreting Neutron Star Crusts
ORAL
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Presenters
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Rahul Jain
Michigan State University
Authors
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Rahul Jain
Michigan State University
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Hendrik Schatz
Michigan State University
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Wei Jia Ong
Lawrence Livermore Natl Lab, LLNL, Lawrence Livermore National Laboratory, Lawerence Livermore National Laboratory
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Kirby Hermansen
Michigan State University
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Nabin Rijal
Michigan State University
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Hannah Berg
Michigan State University
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Paul A Deyoung
Hope College, Department of Physics, Hope College
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Eric Flynn
Michigan State University
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Caley M Harris
Michigan State University
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Sean N Liddick
Michigan State University, FRIB, FRIB/NSCL, Facility for Rare Isotope Beams, Michigan State University, East Lansing, MI 48824, USA, FRIB/MSU
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Stephanie M Lyons
Pacific Northwest National Laboratory
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Sara Miskovich
Stanford Linear Accelerator Center
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Fernando Montes
Facility for Rare Isotope Beams
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Timilehin H Ogunbeku
FRIB, Facility for Rare Isotope Beams, Mississippi State University
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Alicia R Palmisano
University of Tennessee, Knoxville, UTK
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Andrea Richard
Lawrence Livermore National Laboratory
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Mackenzie Smith
Michigan State University
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Mallory K Smith
Facility for Rare Isotope Beams, FRIB, Michigan State University
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Artemis Spyrou
Michigan State University, Department of Physics, Michigan State University
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Constraint on the mass and radius of GRB 200415A using the high-frequency QPOs
ORAL
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Publication: arXiv:2303.03150 [astro-ph,HE]
Presenters
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Hajime Sotani
Authors
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Hajime Sotani
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Equation of state for spin-polarized asymmetric nuclear matter with the cluster variational method
ORAL
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Publication: [1] H. Togashi, K. Nakazato, Y. Takehara, S. Yamamuro, H. Suzuki, and M. Takano, Nucl. Phys. A 961 (2017) 78.<br>[2] http://www.np. phys.waseda.ac.jp/EOS/
Presenters
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Hajime Togashi
Daegu Univ
Authors
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Hajime Togashi
Daegu Univ
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Masatoshi Takano
Waseda Univ
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Quasiparticle properties of an impurity trapped in a superfluid quantized vortex
ORAL
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Presenters
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Kazunari Ochi
Kochi University
Authors
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Kazunari Ochi
Kochi University
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Eiji Nakano
Kochi University
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Kei Iida
Kochi University
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Hiroyuki Tajima
University of Tokyo
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Junichi Takahashi
Waseda University
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Time-Dependent Slef-Consistent Band Theory for the Inner Crust of Neutron Stars: Anti-Entrainment Effects in the Slab Phase
ORAL
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Publication: [1] K. Sekizawa, S. Kobayashi, and M. Matsuo, Time-dependent extension of the self-consistent band theory for neutron star matter: Anti-entrainment effects in the slab phase, Phys. Rev. C 105, 045807 (2022).
Presenters
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Kazuyuki Sekizawa
Tokyo Institute of Technology
Authors
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Kazuyuki Sekizawa
Tokyo Institute of Technology
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Kenta Yoshimura
Tokyo Institute of Technology
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Masayuki Matsuo
Niigata University
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Superfluid and Finite-Temperature Extensions of Self-Consistent Band Theory for the Inner Crust of Neutron Stars
ORAL
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Publication: K. Yoshimura and K. Sekizawa, Superfluid extension of the self-consistent time-dependent band theory for neutron star matter: Anti-entrainment vs. superfluid effects in the slab phase, arXiv:2306.03327 [nucl-th].
Presenters
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Kenta Yoshimura
Tokyo Institute of Technology
Authors
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Kenta Yoshimura
Tokyo Institute of Technology
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Kazuyuki Sekizawa
Tokyo Institute of Technology
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