5243 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 ultralight dark matter fields generate low-frequency stochastic metric fluctuations detectable by pulsar timing arrays, establishing current and future PTA observations as the most sensitive probes of ultralight dark matter density within the solar system for masses between and eV.
This paper investigates large- parton distribution functions within large momentum effective theory by factorizing the matching coefficient into hard and soft components to resum threshold double logarithms and leading renormalons, demonstrating that perturbative matching remains reliable when both active and spectator quark momenta significantly exceed the QCD scale.
This paper proposes an optimal analysis leveraging machine learning-based flavor tagging at the FCC-ee to achieve unprecedented precision in measuring hadronic cross-section ratios, thereby significantly enhancing sensitivity to flavor non-universal and flavor-violating four-fermion interactions within the SMEFT framework and simplified models addressing -meson anomalies.
This paper proposes that future Tera-Z factories like CEPC and FCC-ee can detect triple boson signatures via the decay chain , offering a promising avenue to probe new gauge symmetries and significantly improve current bounds on dark photon kinetic mixing parameters.
This paper investigates the viability of neutralino dark matter within five-dimensional gauge-mediated supersymmetry breaking models with a TeV gravitino, analyzing four distinct scenarios to determine their allowed parameter spaces, consistency with experimental limits, and prospects for detection at the HL-LHC and direct detection experiments.
This report discusses the prospects for sensitive tests of Standard Model predictions and searches for new physics through unique studies of CP violation in charmed hadrons, hyperons, and tau leptons, as well as CPT invariance tests in neutral kaon mixing, at a future high-luminosity Super Tau-Charm Facility operating between 2.0 and 7.0 GeV.
This paper proposes a scenario where an additional scalar field coupled to the Higgs and right-handed neutrinos enables electroweak-scale leptogenesis while simultaneously triggering a strong first-order phase transition, thereby creating a testable correlation between the baryon asymmetry of the Universe and observable gravitational wave signals.
This paper proposes and evaluates analysis strategies using kinematic observables and machine learning to measure longitudinally polarized and bosons in associated Higgs production at the LHC, projecting that the High-Luminosity LHC will achieve 5 discovery significance and percent-level cross-section precision for these states in the and channels.
This paper presents a theoretical study using the SHELL transport model showing that the suppression of high relative transverse momentum in groomed jet substructures in heavy-ion collisions arises from partonic energy loss and selection bias, while the broadening of the groomed jet radius in photon-tagged jets provides direct evidence of medium-induced gluon radiation effects.
This paper utilizes multimessenger constraints from IceCube and Fermi-LAT data to demonstrate that hadronuclear ($pp$) processes in NGC 1068 allow for a larger neutrino emission region compared to photohadronic scenarios, while also challenging shock acceleration models that require cosmic-ray spectra extending to 1 GeV with spectral indices .