Towards grounding nuclear physics in QCD
Christian Drischler, Wick Haxton, Kenneth McElvain, Emanuele, Mereghetti, Amy Nicholson, Pavlos Vranas, Andr\'e Walker-Loud

TL;DR
This paper discusses how exascale computing and lattice QCD can enable a predictive, systematic understanding of nuclear physics rooted in the Standard Model, impacting fundamental physics and astrophysics.
Contribution
It reviews the integration of lattice QCD, effective field theories, and ab initio methods to connect QCD with nuclear properties, highlighting recent progress and challenges.
Findings
Advances in lattice QCD will provide key inputs for nuclear effective theories.
Development of non-relativistic effective theories like HOBET enhances nuclear modeling.
Coupling lattice QCD with effective theories impacts understanding of symmetries and astrophysical phenomena.
Abstract
Exascale computing could soon enable a predictive theory of nuclear structure and reactions rooted in the Standard Model, with quantifiable and systematically improvable uncertainties. Such a predictive theory will help exploit experiments that use nucleons and nuclei as laboratories for testing the Standard Model and its limitations. Examples include direct dark matter detection, neutrinoless double beta decay, and searches for permanent electric dipole moments of the neutron and atoms. It will also help connect QCD to the properties of cold neutron stars and hot supernova cores. We discuss how a quantitative bridge between QCD and the properties of nuclei and nuclear matter will require a synthesis of lattice QCD (especially as applied to two- and three-nucleon interactions), effective field theory, and ab initio methods for solving the nuclear many-body problem. While there are…
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