2489 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.
Through numerical relativity simulations of equal-mass black hole scattering, this study reveals that systems with anti-aligned spins, high momenta, and incident angles near the merger threshold experience the most significant mass gain and spin-up, with maximum increases of 15% in mass and 0.3 in spin, while noting that high initial prograde spins can paradoxically lead to spin-down despite angular momentum growth.
This paper demonstrates the robust emergence of Schrödinger symmetry in spherically-symmetric static mini-superspace models containing Maxwell and massless scalar fields through canonical transformations, identifying specific spacetime solutions and proposing a physical interpretation where symmetry generators either map solutions within a theory or generate new theories with transformed configurations.
This paper presents remarkably simple, dimension-independent covariant expressions for graviton and ghost propagators in Anti-de Sitter spacetime, achieved by selecting a special gauge-fixing condition that ensures improved infrared behavior and is unattainable in flat spacetime.
This paper presents a general framework for simulating polarized emission from inspiraling hotspots around Kerr black holes, revealing that their inward spiral motion produces distinctive, unwinding polarimetric Q-U loop signatures that differ significantly from the closed loops of stable orbits, thereby offering a new method to probe accretion physics and spacetime geometry.
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.
This paper constructs the phase space for an arbitrary cut of a null hypersurface in Minkowski spacetime and demonstrates its symplectomorphism to the infrared phase space of asymptotically flat gravity, explicitly mapping cut fluctuations to leading soft graviton modes and the supertranslation Goldstone mode to the product of the cut's size and its null time offset.
This paper analyzes perturbations of strongly coupled Yang-Mills plasma by demonstrating that while classical spectral truncation methods are limited by convergence boundaries, an exact WKB analysis combined with Seiberg--Witten theory provides a systematic framework to resum quasinormal modes, yielding an accurate spectrum that remains valid from the large wave number regime all the way to zero.
This paper demonstrates that LISA observations of extreme-mass-ratio inspirals embedded in active galactic nucleus accretion disks can simultaneously constrain disk surface density and accretion rates using fully Bayesian analysis, thereby enabling the study of sub-microparsec accretion physics and improving cosmological measurements without requiring electromagnetic counterparts.
This paper proposes a generic mechanism where a light axion spectator induces a post-inflationary "tachyonic encore" that reshapes inflationary observables by enhancing the curvature power spectrum and suppressing the tensor-to-scalar ratio, thereby reconciling otherwise disfavored inflaton potentials with current CMB constraints while predicting observable local non-Gaussianity.
This paper formulates Maxwell's equations in Schwarzschild spacetime using a tetrad-based framework to demonstrate how static observers perceive gravitational corrections as geometrical modifications to the medium, while freely falling observers experience additional kinematical effects that mix charge and current densities and intertwine electric and magnetic fields due to local radial boosts.