2693 papers
Quantum gravity represents the frontier where the very large meets the very small, attempting to unify Einstein's theory of gravity with the strange rules of quantum mechanics. This field explores the fundamental fabric of spacetime, seeking to understand how the universe behaves at its most extreme scales, from the heart of black holes to the moment of the Big Bang. Because these concepts often involve complex mathematics, they can feel distant to non-specialists, yet they hold the key to a complete picture of physical reality.
At Gist.Science, we bridge this gap by processing every new preprint in this category directly from arXiv. Our team provides both plain-language explanations and detailed technical summaries for each paper, ensuring that groundbreaking research is accessible to everyone, from curious students to seasoned researchers. Below are the latest papers in quantum gravity, offering fresh insights into the nature of our cosmos.
This paper investigates a dark matter model based on a symplectic gauge group, analyzing its thermodynamic properties near the confinement phase transition and exploring the resulting gravitational-wave production and relic abundances in the early universe.
This paper investigates perturbative deviations from General Relativity in the Starobinsky model by deriving an effective energy density that includes a mass-dependent correction term, which is numerically shown to diminish with distance and vanish as the model parameter increases, thereby recovering the relativistic limit.
This paper proposes a geometrical Yang-Mills framework that unifies local Lorentz and internal gauge symmetries within an extended space-time, thereby enabling the transfer of topological insights from Euclidean to Lorentzian theories and establishing a novel correspondence between gravity and the weak force.
This paper constructs a family of singularity-free, higher-dimensional Kerr-Anti-de Sitter-like black holes in even spacetime dimensions that feature non-spherical horizons and negatively curved conformal infinity.
This paper calculates universal leading-order logarithmic temperature corrections to the thermodynamic entropy of four-dimensional near-extremal Reissner-Nordström de Sitter black holes by analyzing one-loop contributions and zero modes in the cold and Nariai extremal limits within a path integral framework.
By incorporating spin-induced orbital precession into gravitational-wave searches for the first time, this study significantly improves detection sensitivity for neutron star-black hole binaries, leading to a 16% downward revision of their estimated merger rate and the identification of four new subthreshold candidates likely of terrestrial origin.
This paper investigates interacting dark energy using recent observational data, including DESI DR2, and finds only mild evidence for interaction that remains inconclusive when weighed against the standard CDM model through various statistical criteria.
This paper establishes conditions under which lower-dimensional symmetries of a foliated spacetime's base space, specifically arising from non-commuting Killing vectors, can be lifted to generate irreducible Killing tensors of higher rank in the full spacetime, a mechanism demonstrated through examples ranging from generalized Lense-Thirring metrics to rotating black holes in Einstein-Maxwell-Dilaton-Axion theory.
This study demonstrates that strong magnetic field gradients in post-merger environments can significantly suppress or slow the magneto-rotational instability (MRI), limiting its ability to amplify poloidal magnetic fields to only specific regions and late times ( ms) after a binary neutron star merger.
This study utilizes axisymmetric simulations of a rotating, magnetized progenitor to demonstrate that prompt stellar convection generates early-time gravitational wave signals with amplitudes comparable to or exceeding the bounce signal, while magnetic fields modulate signal strength by decelerating core rotation and influencing mode excitation.