4400 papers
Hep-Th, or high-energy theoretical physics, explores the fundamental building blocks of our universe and the forces that govern them. Researchers in this field use complex mathematics to understand everything from subatomic particles to the behavior of black holes, often pushing the boundaries of what we know about space and time.
At Gist.Science, we monitor the arXiv repository to ensure you stay ahead of the curve in this rapidly evolving discipline. For every new preprint uploaded to arXiv under this category, our team generates both accessible plain-language overviews and detailed technical summaries, making cutting-edge research understandable regardless of your background.
Below are the latest papers in high-energy theoretical physics, curated to help you navigate the most significant recent discoveries.
This paper investigates dynamical mass generation for fermions with and without bare mass in two-dimensional space-time coupled to a massive vector field using Schwinger-Dyson equations, revealing that purely dynamical masses originating from different bare masses converge at a specific coupling constant where a duality relation is satisfied.
This paper demonstrates that while the renormalization-group flow driven by BCS interactions induces a "drag mechanism" that pushes higher-dimensional fermionic operators toward strong coupling, it simultaneously preserves a parametric hierarchy that prevents these operators from destabilizing the infrared-stable non-Fermi-liquid fixed point in dimensions.
This paper investigates holographic entanglement entropy and complexity in Coulomb-branch geometries featuring flat-space bubbles, demonstrating that these regions correspond to a reduction in effective infrared degrees of freedom and entanglement relative to the standard vacuum.
This review examines how quantum anomalies and vacuum topology in QCD resolve the problem and generate hadron mass, while connecting these nonperturbative dynamics to modern studies of nucleon spin structure and partonic observables.
This paper demonstrates that a two-dimensional effective dilaton gravity theory derived from four-dimensional Einstein-Maxwell theory successfully reproduces the semiclassical thermodynamic phase structure of charged AdS black holes, while showing that one-loop Kaluza-Klein photon corrections only induce constant shifts in entropy and charge parameters without qualitatively altering this phase structure.
This paper investigates the hydrodynamic properties of a strongly coupled non-Abelian plasma dual to a four-dimensional AdS black brane with a nonminimal curvature-gauge coupling, demonstrating that this higher-derivative interaction significantly modifies the DC color conductivity and shear viscosity-to-entropy density ratio, potentially violating their respective universal bounds depending on the sign of the coupling constant.
This paper investigates the bipartite entanglement entropy of Bethe states across various integrable spin chains, systematically identifying the specific solutions that minimize and maximize entanglement, revealing that while the ground state often minimizes entropy in the XXX model, this correspondence breaks down in higher-spin and non-compact chains, and further developing an optimization algorithm to explore maximum entanglement for off-shell states.
This paper investigates the short-time behavior of real-time pseudo entropy, demonstrating that its initial imaginary and real responses are fundamentally governed by the symmetrized covariance and commutator, respectively, between the physical Hamiltonian and the modular Hamiltonian, thereby revealing pseudo entropy as a time-oriented modular response rather than a mere branch artifact.
This paper derives a universal expression for the leading finite-volume effects on smeared vector-vector spectral densities using two distinct approaches, demonstrating that these effects are exponentially suppressed and governed by the pion form factor, thereby providing a framework to reliably estimate and control volume extrapolations in lattice QCD calculations.
This paper establishes a systematic framework within worldline effective field theory to define and compute the dynamical tidal response of neutron stars by matching gravitational-wave scattering amplitudes between the effective theory and full stellar perturbation theory, thereby resolving coordinate ambiguities and recovering key physical features like static limits, resonant behaviors, and dissipative effects.