5257 papers
Hep-Ph explores the fundamental forces that govern how particles interact and behave at the smallest scales imaginable. This field bridges the gap between theoretical predictions and experimental reality, helping scientists understand the building blocks of our universe without getting lost in complex mathematics. Whether investigating the Higgs boson or searching for new physics beyond current models, these studies push the boundaries of human knowledge about matter and energy.
At Gist.Science, we process every new preprint in this category as soon as it appears on arXiv. We strip away the dense jargon to offer both accessible plain-language explanations and detailed technical summaries, ensuring that groundbreaking research is understandable to everyone from students to seasoned experts. Below are the latest papers in this dynamic field, ready for you to explore with clarity and depth.
This paper incorporates the resonance into heavy-baryon chiral perturbation theory calculations to show that it restores power counting for the axial-vector charge, significantly reduces the QED radiative correction to the ratio, and increases pion-induced radiative corrections to inverse beta decay by a factor of 1.2–1.3.
This paper investigates how bubble nucleation history and plasma-induced friction influence primordial black hole formation during cosmological first-order phase transitions, demonstrating that friction significantly alters black hole mass and formation time while leaving distinct signatures in the stochastic gravitational-wave spectrum.
This paper employs QCD light-cone sum rules to calculate the form factors and predict the branching fractions and various polarization asymmetries for the semileptonic decay , providing theoretical benchmarks for future experimental investigations.
The paper introduces Neural Boltzmann Equations (NBEs), a novel framework combining physics-inspired neural distribution functions, Monte Carlo integration with importance sampling, and natural gradient optimization to efficiently solve high-dimensional particle dynamics in the early universe, enabling precision calculations of cosmological parameters like the effective number of relativistic neutrino degrees of freedom.
This paper utilizes high-resolution numerical simulations to demonstrate that multifield fuzzy dark matter halos exhibit distinct wave dynamics, including synchronized core random walks and suppressed granule-induced heating, which collectively offer a potentially better match to astrophysical observations than single-field models.
This paper derives a systematic method for generating integration-by-parts identities for dimensionally regulated loop integrals with non-linear measurement constraints by utilizing vectors tangent to the constraint hypersurface, thereby avoiding derivatives of distributions and enabling the calculation of differential distributions like transverse-momentum spectra in processes such as and production.
This paper investigates the glueball content of the resonance by analyzing light-cone distribution amplitudes and a tetra-mixing scheme to predict branching ratios for heavy quarkonium radiative decays and electroproduction cross sections, offering testable theoretical predictions for current BESIII and Belle-II experiments.
This paper demonstrates that exclusive vector meson production at small serves as a novel probe of nuclear shell structure, as self-consistent nuclear densities derived from the quark-meson coupling model significantly modify coherent diffractive patterns, particularly for intermediate-mass nuclei like calcium isotopes where production offers a clean signal free from saturation effects.
This paper proposes a generalized chiral model with two free parameters that relaxes LHC constraints by suppressing dilepton decays, while simultaneously explaining neutrino masses and viable dark matter phenomenology through a combined and scalar-mediated annihilation mechanism.
This paper presents a non-perturbative path integral framework for modeling the one-point matter probability distribution function with arbitrary spherically symmetric window functions, demonstrating that while the most probable density profiles differ significantly for overdensities depending on the filter, the overall PDF is largely filter-independent and accurately validated against N-body simulations for scales larger than 10 Mpc/h.