Dense Matter in Nuclear Astrophysics
ORAL · L12 · ID: 50009
Presentations
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Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae
ORAL
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Publication: https://arxiv.org/abs/2110.05544
Presenters
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Luca Boccioli
University of Notre Dame
Authors
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Luca Boccioli
University of Notre Dame
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Grant J Mathews
University of Notre Dame
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Evan P O'Connor
Stockholm Univ
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In-Saeng J Suh
University of Notre Dame
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Response function for hot and dense nuclear matter from chiral effective field theory
ORAL
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Presenters
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Eunkyoung Shin
Cyclotron Institute and Department of Physics and Astronomy
Authors
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Eunkyoung Shin
Cyclotron Institute and Department of Physics and Astronomy
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Jeremy W Holt
Texas A&M University
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Ermal Rrapaj
University of California, Berkeley
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Sanjay K Reddy
University of Washington
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Constructing an Equation of State from Pure Neutron Matter Calculations
ORAL
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Presenters
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Liam Brodie
Washington University, St. Louis
Authors
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Liam Brodie
Washington University, St. Louis
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Alexander Haber
Washington University, St. Louis
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Mark Alford
Washington University, St. Louis
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Ingo Tews
Los Alamos National Laboratory
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Speed of Sound for Hadronic and Quark Phases in a Magentic Field
ORAL
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Presenters
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Aric A Hackebill
The Graduate Center, City University of
Authors
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Aric A Hackebill
The Graduate Center, City University of
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Efrain J Ferrer
University of Texas Rio Grande Valley
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The Effect of Charge, Isospin, and Strangeness in the QCD Phase Diagram Critical End Point
ORAL
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Presenters
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krishna P aryal
Kent State University
Authors
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krishna P aryal
Kent State University
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Veronica Dexheimer
Kent State University
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Neutron Tunneling: A New Mechanism to Power Explosive Phenomena in Neutron Stars, Magnetars, and Neutron Star Mergers
ORAL
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Publication: The Astrophysical Journal 912, 105 (2021)
Presenters
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Carlos A Bertulani
Texas A&M University–Commerce
Authors
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Carlos A Bertulani
Texas A&M University–Commerce
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Ejecta Composition Effects on Kilonova Parameter Inference
ORAL
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Presenters
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Marko Ristic
Rochester Institute of Technology
Authors
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Marko Ristic
Rochester Institute of Technology
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Erika M Holmbeck
Carnegie Observatories
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Ryan Wollaeger
Los Alamos National Lab, Los Alamos National Laboratory
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Oleg Korobkin
Los Alamos National Laboratory
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Richard W O'Shaughnessy
Rochester Institute of Technology
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Eve Chase
Los Alamos National Lab, Los Alamos National Laboratory
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Chris Fryer
Los Alamos National Lab, Los Alamos Natl Lab, Los Alamos National Laboratory
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Chris J Fontes
Los Alamos National Laboratory
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Using cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars and their time-evolution
ORAL
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Publication: arXiv:2111.05864 [astro-ph.HE]
Presenters
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Ilias Cholis
Oakland University
Authors
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Ilias Cholis
Oakland University
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Iason Krommydas
National Technical Univeristy of Athens
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