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1. Radiative Corrections to Superallowed $\beta$ Decays in Effective Field Theory

   https://doi.org/10.1103/PhysRevLett.133.211801  

   Cirigliano, Vincenzo; Dekens, Wouter; de_Vries, Jordy; Gandolfi, Stefano; Hoferichter, Martin; Mereghetti, Emanuele (November 2024, Physical Review Letters)

   The accuracy of $V_{ud}$determinations from superallowed $\beta$decays critically hinges on control over radiative corrections. Recently, substantial progress has been made on the single-nucleon, universal corrections, while nucleus-dependent effects, typically parametrized by a quantity ${\delta }_{\mathrm{NS}}$, are much less well constrained. Here, we lay out a program to evaluate this correction from effective field theory (EFT), highlighting the dominant terms as predicted by the EFT power counting. Moreover, we compare the results to a dispersive representation of ${\delta }_{\mathrm{NS}}$and show that the expected momentum scaling applies even in the case of low-lying intermediate states. Our EFT framework paves the way toward calculations of ${\delta }_{\mathrm{NS}}$and thereby addresses the dominant uncertainty in $V_{ud}$. Published by the American Physical Society2024 

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2. Conformal field theories in a magnetic field

   https://doi.org/10.1103/PhysRevResearch.6.043093  

   Boyack, Rufus; Delacrétaz, Luca; Dupuis, Éric; Witczak-Krempa, William (November 2024, Physical Review Research)

   We study the properties of 2+1d conformal field theories (CFTs) in a background magnetic field. Using generalized particle-vortex duality, we argue that in many cases of interest the theory becomes gapped, which allows us to make a number of predictions for the magnetic response, background monopole operators, and more. Explicit calculations at large $N$for Wilson-Fisher and Gross-Neveu CFTs support our claim, and yield the spectrum of background (defect) monopole operators. Finally, we point out that other possibilities exist: certain CFTs can become metallic in a magnetic field. Such a scenario occurs, for example, with a Dirac fermion coupled to a Chern-Simons gauge field, where a non-Fermi liquid is argued to emerge. Published by the American Physical Society2024 

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3. Corrections to Diffusion in Interacting Quantum Systems

   https://doi.org/10.1103/PhysRevX.14.031020  

   Michailidis, Alexios A; Abanin, Dmitry A; Delacrétaz, Luca V (August 2024, Physical Review X)

   The approach to equilibrium in interacting classical and quantum systems is a challenging problem of both theoretical and experimental interest. One useful organizing principle characterizing equilibration is the dissipative universality class, the most prevalent one being diffusion. In this paper, we use the effective field theory (EFT) of diffusion to systematically obtain universal power-law corrections to diffusion. We then employ large-scale simulations of classical and quantum systems to explore their validity. In particular, we find universal scaling functions for the corrections to the dynamical structure factor $⟨n(x,t)n⟩$, in the presence of a single $\mathrm{U}\left(1\right)$or $\mathrm{SU}\left(2\right)$charge in systems with and without particle-hole symmetry, and present the framework to generalize the calculation to multiple charges. Classical simulations show remarkable agreement with EFT predictions for subleading corrections, pushing precision tests of effective theories for thermalizing systems to an unprecedented level. Moving to quantum systems, we perform large-scale tensor-network simulations in unitary and noisy 1D Floquet systems with conserved magnetization. We find a qualitative agreement with EFT, which becomes quantitative in the case of noisy systems. Additionally, we show how the knowledge of EFT corrections allows for fitting methods, which can improve the estimation of transport parameters at the intermediate times accessible by simulations and experiments. Finally, we explore nonlinear response in quantum systems and find that EFT provides an accurate prediction for its behavior. Our results provide a basis for a better understanding of the nonlinear phenomena present in thermalizing systems. Published by the American Physical Society2024 

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4. Mesoscale field theory for quasicrystals

   https://doi.org/10.1103/PhysRevResearch.6.043285  

   De_Donno, Marcello; Angheluta, Luiza; Elder, Ken R; Salvalaglio, Marco (December 2024, Physical Review Research)

   We present a mesoscale field theory unifying the modeling of growth, elasticity, and dislocations in quasicrystals. The theory is based on the amplitudes entering their density-wave representation. We introduce a free energy functional for complex amplitudes and assume nonconserved dissipative dynamics to describe their evolution. Elasticity, including phononic and phasonic deformations, along with defect nucleation and motion, emerges self-consistently by prescribing only the symmetry of quasicrystals. Predictions on the formation of semicoherent interfaces and dislocation kinematics are given. Published by the American Physical Society2024 

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5. Resonant shattering flares as asteroseismic tests of chiral effective field theory

   https://doi.org/10.1103/PhysRevC.111.015809  

   Neill, Duncan; Tsang, David; Drischler, Christian; Holt, Jeremy W; Newton, William G (January 2025, Physical Review C)

   Chiral effective field theory ( $\chi \mathrm{EFT}$) has proved to be a powerful microscopic framework for predicting the properties of neutron-rich nuclear matter with quantified theoretical uncertainties up to about twice the nuclear saturation density. Tests of $\chi \mathrm{EFT}$predictions are typically performed at low densities using nuclear experiments, with neutron star (NS) constraints only being considered at high densities. In this work, we discuss how asteroseismic quasinormal modes within NSs could be used to constrain specific matter properties at particular densities not just the integrated quantities to which bulk NS observables are sensitive. We focus on the crust-core interface mode, showing that measuring this mode's frequency would provide a meaningful test of $\chi \mathrm{EFT}$at densities around half the saturation density. Conversely, we use nuclear matter properties predicted by $\chi \mathrm{EFT}$to estimate that this mode's frequency is around $185\pm 50\text{Hz}$. Asteroseismic observables such as resonant phase shifts in gravitational-wave signals and multimessenger resonant shattering flare timings, therefore, have the potential to provide useful tests of $\chi \mathrm{EFT}$. Published by the American Physical Society2025 

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