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.

⚛️ phenomenology

Classification of order-two T-duality orbifolds at the SO(12) free fermionic point

This paper classifies all order-two T-duality orbifolds on the SO(12) lattice at the free fermionic point of type II string theories, presenting their parametric spectra, identifying minimal Hodge numbers and orientifoldable configurations, and arguing that the appearance of spin-3/2 states in twisted sectors necessitates a supersymmetric vacuum with vanishing energy.

Alon E. Faraggi, Stefan Groot Nibbelink, Benjamin Percival2026-09-24
⚛️ phenomenology

Chiral Phase Structure and In-Medium Modifications of Charmed Meson Masses within SU(4) extended Linear-Sigma Models

This paper extends the Polyakov-loop-enhanced linear-sigma model to four flavors to demonstrate that open-charm DD-mesons serve as precise indicators of chiral restoration with significant mass increases across the crossover transition, while hidden-charm states remain largely unaffected, collectively mapping a chiral phase boundary consistent with lattice-QCD predictions and devoid of a critical endpoint.

Nourhan M. Rfeek (Assiut U.), Alexandra Friesen (JINR), Yuri Kalinovsky (JINR), Saleh O. Allehabi (Islamic U. of Madinah (…)2026-09-24
🔬 condensed matter

Analytical Solution of the Nonlinear Boltzmann Equation For Multicomponent Systems

This paper presents exact analytical solutions to the nonlinear relativistic Boltzmann equation for homogeneous, isotropic, massless multicomponent systems, identifying three distinct solution classes for two-component systems that include a novel hybrid structure featuring a non-equilibrium Maxwell-Jüttner distribution coupled with nontrivial dynamics.

Linyuan Wei, Yi Wang, Jin Hu, Baoyi Chen2026-09-24
⚛️ high-energy experiments

Benchmark Dark SMEFT Scenarios from the Interplay of Flavor Physics and Dark Matter Searches

This paper investigates the interplay between low-energy flavor physics and dark matter phenomenology within the dimension-6 dark Standard Model Effective Field Theory, demonstrating that correlated multi-operator configurations are necessary to satisfy current constraints and defining tightly constrained benchmark regions for future collider searches.

Lipika Kolay, Soumitra Nandi, Ipsita Ray2026-09-24
⚛️ phenomenology

Towards Foundation Models on Hardware Accelerators for Particle Physics

This paper demonstrates that knowledge distillation from a large foundation model into an efficient, attention-free Deep Sets network significantly improves background rejection for real-time top quark jet tagging on hardware accelerators, particularly in the low signal efficiency regime critical for collider triggers.

Maya Benyas, Julia Gonski, Qibin Liu, P. Alex May, Vinicius Mikuni, Benjamin Nachman, Tanvi Wamorkar, Liangyu Wu2026-09-24
⚛️ phenomenology

Supernova Gamma-Ray Echo as an Astrophysical Near Detector for Galactic Neutrino Propagation

This paper proposes using the delayed 511 keV gamma-ray echo from a core-collapse supernova as an astrophysical "near detector" to directly measure the emitted neutrino fluence, thereby enabling a precise test of neutrino propagation effects such as pseudo-Dirac oscillations, decay, or dark matter interactions by comparing this source flux with the flux observed at Earth.

Garv Chauhan, Yago Porto2026-09-24