2998 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 recasting data from the J-PARC KOTO experiment's search for decays can establish novel limits on prompt axion-like particles in the challenging "pion chimney" mass range and extend sensitivity to a broader mass spectrum by incorporating displaced decays.
This paper presents updated observational constraints on the spatially flat CDM dynamical dark energy model using Planck 2018 and non-CMB data, finding that while the standard CDM model remains an excellent fit, current data mildly favor evolving quintessence-like dark energy and reveal tensions in the Hubble constant and CMB lensing amplitude that are partially alleviated by allowing the lensing consistency parameter to vary.
This paper introduces an eigen-microstate framework that analyzes final-state particle fluctuations in relativistic heavy-ion collisions to identify the QCD critical point by extracting dominant critical modes as a robust order parameter, offering a background-insensitive tool directly applicable to RHIC Beam Energy Scan data without relying on equilibrium assumptions.
This paper proposes and validates a method to reconstruct the local dark matter speed distribution by combining a Maxwell-Boltzmann component for old merger debris with a kinematically boosted stellar tracer for recent massive mergers, demonstrating its application to the Milky Way using Gaia data.
This paper presents a comprehensive analysis demonstrating that future electron-positron and proton-proton colliders offer an order-of-magnitude improvement in sensitivity to anomalous CP-violating interactions in the gauge-Higgs sector compared to the high-luminosity LHC, thereby providing crucial insights into new physics sources for the observed matter-antimatter asymmetry.
This review challenges the assumption that SN 1987A neutrino emissions were near-simultaneous, arguing that despite conflicting with current cosmological and experimental upper limits, the data may still correctly yield specific values for all three neutrino masses as originally suggested by Ramanath Cowsik.
This paper proposes and validates a method using Pythia 8.3 simulations to isolate the top-quark dead cone effect in decays by extrapolating hadronic momentum distributions to the forward direction, thereby successfully separating primary top radiation from secondary -quark radiation to test perturbative QCD in a new kinematic regime.
Using an improved AMPT model, this study demonstrates that the coalescence mechanism is essential for accurately reproducing the enhanced ratio observed in Au+Au collisions at RHIC, whereas fragmentation alone fails to capture this trend.
This paper presents a unified framework for studying the QCD dead-cone effect across charm, bottom, and top quark jets by combining precision LEP data with Monte Carlo simulations to validate momentum-space suppression in lighter heavy quarks and proposing a novel method to isolate the dead cone in top-quark jets despite finite lifetime and decay radiation challenges.
This paper investigates the thermodynamics of a Schwarzschild black hole within non-commutative gauge theory, demonstrating that non-commutative corrections remove temperature divergence, introduce logarithmic entropy corrections, and result in extremely sparse Hawking radiation that diverges as the black hole approaches the final stage of evaporation.