Description
Oct 26–30
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Oleg Komoltsev (Goethe-Universität Frankfurt am Main)(3rd week, Oct. 26-30) Symposium
As our understanding of cold, extremely dense matter grows, a multidisciplinary approach that combines recent progress in multimessenger neutron-star observations with theoretical knowledge of the equation of state (EoS) becomes increasingly essential. In this talk, I present a new physically motivated framework for encoding prior knowledge about dense matter arising from chiral effective...
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Farid Salazar (Temple University)(3rd week, Oct. 26-30) Symposium
A central goal of the future Electron-Ion Collider and of upcoming upgrades at the Large Hadron Collider is the search for a new regime of nuclear matter known as the Color Glass Condensate (CGC). In this extreme state, matter is dominated by an exceptionally dense population of gluons, the particles responsible for binding quarks inside protons and nuclei. Over the past two decades,...
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Aleksey Cherman (University of Minnesota)
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Aleksas Mazeliauskas (Institute for Theoretical Phyiscs, Heidelberg University)
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Jorge Noronha (University of Illinois Urbana-Champaign)
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Luciano Rezzolla (Institute for Theoretical Physics, Frankfurt, Germany)
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Felix Ringer (Stony Brook University)
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Dam Thanh Son (University of Chicago)
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Charlotte Van Hulse (Vrije Universiteit Brussel (VUB))
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87. What can we learn about the cold matter equation of state of QCD while evading the sign problem?Thomas Cohen (University of Maryland)(3rd week, Oct. 26-30) Symposium
The equation of state of cold matter in QCD is a central issue in particle physics, nuclear physics as well as the astrophysics of neutron stars. Unfortunately, direct lattice calculation of the equation of state as a function of density using lattice methods are not viable due to an exponentially bad sign problem when a chemical potential is included. However, this need not mean that...
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