Resources

Author(s): Caio V. P. de Brito, David Wagner, Gabriel S. Denicol, and Dirk H. Rischke A standard lore in relativistic fluid dynamics is that the widely-used moment expansion for the single particle distribution function converges. The authors challenge this assumption, demonstrating in a simple example that the moment expansion does not produce decreasing multipole coefficients of a series of orthogonal polynomials. This divergence can nevertheless...

Author(s): J. McCullough et al. (DES Collaboration) The authors use the Dark Energy Survey Year 3 galaxy-shear catalog to demonstrate that the challenge of intrinsic alignment (IA) modeling can be effectively circumvented when using a subsample of blue, star-forming galaxies, which are virtually devoid of IA effects. In particular, goodness of fit and agreement with Planck results improve both for Ωₘ and 𝑆₈ . [Phys. Rev. D 113, 103509] Published...

Author(s): Anthony Francis, Patrick Fritzsch, Rohith Karur, Jangho Kim, Giovanni Pederiva, Dimitra A. Pefkou, Antonio Rago, Andrea Shindler, André Walker-Loud, and Savvas Zafeiropoulos We present a nonperturbative determination of the pion valence parton distribution function (PDF) moment ratios $⟨{x}^{n−1}⟩/⟨x⟩$ up to $n=6$, using the gradient flow in lattice quantum chromodynamics (QCD). As a testing ground, we employ SU(3) isosymmetric gauge...

Author(s): Alan Price and Frank Krauss Especially at proposed future lepton colliders, the description of electroweak radiation at high perturbative accuracy will be critical to achieve the high precision goals for sensitivity to rare Standard Model processes or new physics. The authors present an algorithm based on the Yennie-Frautschi-Suura theorem and demonstrate the first process-independent inclusion of electroweak corrections at next-to...

Author(s): M. Gatti et al. The authors present the largest (270 million galaxies) galaxy weak-lensing mass map to date from combined analysis of Dark Energy Camera All Data Everywhere (DECADE) and Dark Energy Survey Year-3 data. They further showcase its potential for cosmological applications by detecting cosmic filaments directly from the mass map. [Phys. Rev. D 113, L081303] Published Thu Apr 23, 2026

Author(s): Oliver Just, Zewei Xiong, and Gabriel Martínez-Pinedo Nuclear reactions of any sort are computationally difficult to include in any sort of astrophysical simulation. The combination of a large number of species to keep track of and stiff differential equations will bog down these computations. Thus, there is a strong impetus to developed simplified models or approximate methods to allow for nuclear reactions to be included. In this...

Author(s): Danat Issa, Beverly Lowell, Jonatan Jacquemin-Ide, Matthew Liska, and Alexander Tchekhovskoy Launching jets from collapsar black holes requires strong magnetic field and rapid rotation. However, strong fields can spin down the collapsar black holes before the jet can be launched. In this work, the authors study the effect of neutrino cooling on this jet launching process. They show that neutrino cooled disks can continue to feed angular...