5547 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 introduces MadNIS, a framework that accelerates Next-to-Leading Order (NLO) calculations by combining fast amplitude surrogates with neural importance sampling to achieve significant speed-ups and variance reduction in electron-positron scattering processes.
This study presents a comprehensive sensitivity atlas for Big Bang Nucleosynthesis using the PRyMordial code to quantify how 14 fundamental parameters and 63 reaction rates influence primordial abundances, incorporating new LBT helium-4 data to rank theoretical uncertainties and address the deuterium tension and lithium problem.
This paper demonstrates that the autonomous AI system PhysMaster can fully automate the complex, multi-step extraction of the Collins-Soper kernel from Lattice QCD data, reducing the workflow duration from months to hours while achieving precision consistent with state-of-the-art traditional methods and stabilizing signals at large transverse separations.
This paper investigates whether three anomalous compact objects can be modeled as dark matter admixed neutron stars using a first-principles baryonic equation of state, finding that HESS J1731-347 and PSR J1231-1411 are consistent with small fermionic dark matter fractions while XTE J1814-338 is ruled out as a candidate and instead suggests a twin star scenario.
This paper analyzes pseudoscalar contributions to production in extended scalar sector models, finding that while a 95 GeV pseudoscalar yields negligible effects, heavier pseudoscalars (100–1000 GeV) can produce cross-sections exceeding current LHC limits, thereby constraining the parameter spaces of the Two Higgs Doublet Model and its singlet extension.
The paper introduces FERMIACC, a scaffolded reasoning model built on OpenAI agents that autonomously generates and quantitatively validates high-energy physics theory hypotheses at scale.
This paper investigates how frequency chirps and field polarization influence dynamically assisted electron-positron pair production within the Dirac-Heisenberg-Wigner formalism, revealing that chirps significantly enhance pair yields through interference effects while simultaneously reducing the system's sensitivity to polarization, thereby offering a pathway for optimizing particle generation.
This paper proposes using magnetically levitated superconductors to detect ultra-light dark gravitons in the dHz to kHz range, finding that while their sensitivity to matter couplings is limited compared to existing experiments, they could serve as highly sensitive laboratory probes for dark-graviton couplings to electromagnetism.
This paper investigates the potential of the future 100 TeV FCC-hh collider to discover or exclude heavy axion-like particles (ALPs) via light-by-light scattering in pp, pPb, and PbPb collisions, demonstrating that the facility offers significant sensitivity to ALP masses up to the TeV scale compared to current LHC bounds.
This paper investigates the evolution of massive and massless neutrinos in rotating matter by solving the Dirac equation in a corotating frame, deriving a nonzero electroweak vector current analogous to the chiral vortical effect, and analyzing neutrino flavor oscillations to reveal resonance phenomena and generalize noninertial effects in astrophysical contexts.