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Nuclear Astrophysics V

ORAL · KD · ID: 15341

Presentations

  • Fission in White Dwarfs as a New Supernova Mechanism I

    ORAL

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    Publication: C. J. Horowitz & M. E. Caplan, Phys. Rev. Lett. 126, 131101 (2020) (arXiv:2103.02122)

    Presenters

    • Matthew E Caplan

      Illinois State University

    Authors

    • Matthew E Caplan

      Illinois State University

    • Charles J Horowitz

      Indiana University Bloomington

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  • Fission in White Dwarfs as a New Supernova Mechanism II

    ORAL

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    Publication: C. J. Horowitz & M. E. Caplan, Phys. Rev. Lett. 126, 131101 (2020) (arXiv:2103.02122)

    Presenters

    • Charles J Horowitz

      Indiana University Bloomington

    Authors

    • Charles J Horowitz

      Indiana University Bloomington

    • Matthew E Caplan

      Illinois State University

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  • Quantified Nuclear Mass Model for Nuclear Astrophysics Simulations

    ORAL

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    Presenters

    • Rahul Jain

      Michigan State University

    Authors

    • Rahul Jain

      Michigan State University

    • Leo Neufcourt

      Michigan State University, Facility for Rare Isotope Beams

    • Witold Nazarewicz

      Michigan State University

    • Samuel A Giuliani

      European Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*), Trento, Italy

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  • Contribution of Collapsars and Hypernovae to the origin and early evolution of heavy element explosive nucleosynthesis

    ORAL

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    Publication: Y. Yamazaki et al. (2021) arXiv:2102.05891 <br>H Sasaki et al. (2021) arXiv:2106.01679

    Presenters

    • Grant J Mathews

      University of Notre Dame

    Authors

    • Grant J Mathews

      University of Notre Dame

    • Yuta Yamazaki

      NAOJ

    • Hirozaku Sasaki

      NAOJ

    • Motohiko Kusakabe

      Beihang Univ.

    • Toshitaka Kajino

      Natl Astronomical Observ, Beihang Univ.

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  • Corrected Beta-Equilibrium in Neutron Star Mergers

    ORAL

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    Presenters

    • Ziyuan Zhang

      Washington University, St. Louis

    Authors

    • Ziyuan Zhang

      Washington University, St. Louis

    • Mark Alford

      Washington University, St. Louis

    • Alexander Haber

      Washington University, St. Louis

    • Steven P Harris

      University of Washington

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  • Response function for supernova and neutron star crust with chiral effective theory

    ORAL

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    Presenters

    • Eunkyoung Shin

      Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA

    Authors

    • Eunkyoung Shin

      Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA

    • Jeremy W Holt

      Cyclotron Institute and Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843, USA

    • Ermal Rrapaj

      1 Department of Physics, University of California, Berkeley, California 94720, USA. 2 School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455,

    • Sanjay K Reddy

      Institute for Nuclear Theory and Department of Physics, University of Washington, Seattle, Washington 98195, USA

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  • Applying Bayesian Methods to R-Matrix Predictions of Nuclear Reaction Observables

    ORAL

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    Publication: https://arxiv.org/abs/2105.06541

    Presenters

    • Daniel M Odell

      Ohio University

    Authors

    • Daniel M Odell

      Ohio University

    • Carl R Brune

      Ohio University

    • Daniel R Phillips

      Ohio University

    • Som N Paneru

      Michigan State University

    • Maheshwor Poudel

      Ohio University

    • Richard J deBoer

      University of Notre Dame, The Joint Institute for Nuclear Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA

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  • Fresh approaches to using solar isotopic abundances to determine heavy element origins

    ORAL

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    Publication: Markov Chain Monte Carlo Predictions of Neutron-rich Lanthanide Properties as a Probe of r-process Dynamics, N. Vassh, G.C. McLaughlin, M.R. Mumpower, and R. Surman, Astrophys. J. 907, 98, 2021<br><br>I-129 and Cm-247 in meteorites constrain the last astrophysical source of solar r-process elements, B. Côté, M. Eichler, A. Yagüe, N. Vassh, M.R. Mumpower, B. Világos, B. Soós, A. Arcones, T.M. Sprouse, R. Surman, M. Pignatari, B. Wehmeyer, T. Rauscher, and M. Lugaro, Science, 26 Feb 2021: Vol. 371, Issue 6532, pg. 945-948<br><br>

    Presenters

    • Nicole Vassh

      Notre Dame, University of Notre Dame

    Authors

    • Nicole Vassh

      Notre Dame, University of Notre Dame

    • Matthew R Mumpower

      Los Alamos National Laboratory

    • Benoit Côté

      University of Victoria

    • Gail C McLaughlin

      North Carolina State University

    • Rebecca A Surman

      University of Notre Dame

    View abstract →