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 demonstrates that high-energy collisions at future linear colliders can rival the discovery potential of conventional modes for doubly charged Higgs bosons within the 2HDMcT framework, achieving significance through significantly enhanced production cross sections that compensate for reduced effective luminosity.
This paper proposes utilizing the Bethe-Heitler process () as a laboratory to generate and validate high-fidelity bipartite and genuine tripartite entanglement, specifically identifying thousands of GHZ and W states below 5 GeV center-of-mass energy through event simulations.
This paper presents a confining density functional equation of state for hybrid stars that reveals the existence of "thermal twin stars" at finite temperatures, suggesting that the presence of such disconnected branches serves as a new criterion to exclude strong color superconductivity and assess the explodability of core-collapse supernovae.
This paper proposes that an inflationary dark Schwinger mechanism can generate the observed dark matter relic abundance for a wide mass range (0.1 eV to GeV) by producing dark electrons that interact via light dark photons, a process that remains viable even when purely gravitational production is negligible and successfully evades isocurvature constraints.
This paper presents a PYTHIA8-based Monte Carlo study of jet substructure observables, including angularities and the primary Lund Plane with a focus on the dead cone effect, for light and heavy flavor jets in 200 GeV collisions at RHIC to test non-perturbative physics models and enable feasible measurements at sPHENIX.
This paper proposes a novel numerical method using diffusion models to efficiently search for phenomenologically viable parameters in the modular flavor model, successfully reproducing quark observables and confirming spontaneous CP violation through an inverse problem approach.
This paper proposes a TeV-scale neutrinophilic two-Higgs-doublet model augmented by flavor symmetry and five flavons to realize Trimaximal mixing, successfully explaining lepton masses under normal ordering while predicting a sub-threshold neutrinoless double-beta decay mass and enabling low-scale leptogenesis to account for the universe's matter-antimatter asymmetry.
This paper proposes a modular -symmetric inverse seesaw model that successfully explains neutrino masses and mixing, predicts near-maximal Dirac CP violation and testable neutrinoless double beta decay signals, and accounts for the observed baryon asymmetry through resonant leptogenesis.
This paper combines numerical simulations and semi-analytic modeling to demonstrate that ultralight bosons can form "gravitational molecules" around comparable-mass binaries, where eccentricity-induced ionization drives efficient orbital circularization and significantly alters the stochastic gravitational wave background.
This paper presents the public release of FeynRules and UFO model files for the SMEFT, enabling the simulation of dimension-five and dimension-six operators involving right-handed neutrinos, including a specialized implementation for Majorana four-fermion operators compatible with MadGraph5_aMC@NLO.