Dense nuclear matter equation of state from heavy-ion collisions

A Sorensen, K Agarwal, KW Brown, Z Chajęcki… - Progress in Particle and …, 2024 - Elsevier
The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

[HTML][HTML] Science requirements and detector concepts for the electron-ion collider: EIC yellow report

RA Khalek, A Accardi, J Adam, D Adamiak, W Akers… - Nuclear Physics A, 2022 - Elsevier
This report describes the physics case, the resulting detector requirements, and the evolving
detector concepts for the experimental program at the Electron-Ion Collider (EIC). The EIC …

Generative image dynamics

Z Li, R Tucker, N Snavely… - Proceedings of the IEEE …, 2024 - openaccess.thecvf.com
We present an approach to modeling an image-space prior on scene motion. Our prior is
learned from a collection of motion trajectories extracted from real video sequences …

Quantum simulation for high-energy physics

CW Bauer, Z Davoudi, AB Balantekin, T Bhattacharya… - PRX quantum, 2023 - APS
It is for the first time that quantum simulation for high-energy physics (HEP) is studied in the
US decadal particle-physics community planning, and in fact until recently, this was not …

Ab initio predictions link the neutron skin of 208Pb to nuclear forces

B Hu, W Jiang, T Miyagi, Z Sun, A Ekström, C Forssén… - Nature Physics, 2022 - nature.com
Heavy atomic nuclei have an excess of neutrons over protons, which leads to the formation
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …

Neutron stars and the nuclear matter equation of state

JM Lattimer - Annual Review of Nuclear and Particle Science, 2021 - annualreviews.org
Neutron stars provide a window into the properties of dense nuclear matter. Several recent
observational and theoretical developments provide powerful constraints on their structure …

Multimessenger constraints on the neutron-star equation of state and the Hubble constant

T Dietrich, MW Coughlin, PTH Pang, M Bulla, J Heinzel… - Science, 2020 - science.org
Observations of neutron-star mergers with distinct messengers, including gravitational
waves and electromagnetic signals, can be used to study the behavior of matter denser than …

Nuclear effective field theory: status and perspectives

HW Hammer, S König, U Van Kolck - Reviews of Modern Physics, 2020 - APS
The nuclear-physics landscape has been redesigned as a sequence of effective field
theories (EFTs) connected to the standard model through symmetries and lattice simulations …

Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory

CD Capano, I Tews, SM Brown, B Margalit, S De… - Nature …, 2020 - nature.com
The properties of neutron stars are determined by the nature of the matter that they contain.
These properties can be constrained by measurements of the star's size. We obtain stringent …

[HTML][HTML] 50 Years of quantum chromodynamics: Introduction and Review

F Gross, E Klempt, SJ Brodsky, AJ Buras… - The European Physical …, 2023 - Springer
Quantum Chromodynamics, the theory of quarks and gluons, whose interactions can be
described by a local SU (3) gauge symmetry with charges called “color quantum numbers” …