Requiring causal stable thermodynamically consistent extensions of neutron-star EOS models to perturbative QCD constrains high-density behavior and disfavors purely nucleonic descriptions for all stable stars.
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Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.
Fully heavy pentaquark fragmentation functions PQ5Q1.0 are completed for charm and bottom flavors and used to compute NLL/NLO+ semi-inclusive production rates at future colliders.
citing papers explorer
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As above, so below: assessing extremeness of the neutron-star equation of state based on the unstable branch
Requiring causal stable thermodynamically consistent extensions of neutron-star EOS models to perturbative QCD constrains high-density behavior and disfavors purely nucleonic descriptions for all stable stars.
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Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective
Tripling fluctuations in a BEC-BCS-inspired model provide a microscopic derivation of quarkyonic matter that reproduces the speed of sound peak and baryon momentum shell in a simplified dense-matter framework.
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Fully Heavy Pentaquarks with JETHAD: A High-Energy Viewpoint
Fully heavy pentaquark fragmentation functions PQ5Q1.0 are completed for charm and bottom flavors and used to compute NLL/NLO+ semi-inclusive production rates at future colliders.