3949 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 establishes the precise late-time oscillating and decaying tails of charged scalar fields on near-extremal Reissner--Nordström spacetimes and proves the existence of asymptotic instabilities along future null infinity and the event horizon using purely physical-space methods without assuming smallness of the scalar field charge.
By analyzing 85 binary black hole mergers from the O4a observing run, this study finds no statistically significant evidence for orbital eccentricity, thereby ruling out single-single gravitational wave captures in nuclear star clusters as the dominant formation channel for all observed LIGO-Virgo-KAGRA events.
Motivated by the linguistic coincidence that both bird calls and gravitational waves are described as "chirps," this satirical paper humorously proposes that Northern cardinal vocalizations can be modeled as gravitational waves from a precessing black hole binary, suggesting a whimsical link between ornithology and cosmology.
This paper investigates the minisuperspace quantum cosmology of Cosmological Einsteinian Cubic Gravity by deriving its Hamiltonian formulation via canonical transformations, performing Wheeler-DeWitt quantization to obtain exact and WKB-type wave functions for various spatial geometries, and analyzing the resulting strong correlations between coordinates and momenta in the presence of an inflationary scalar field.
This paper evaluates the utility of the coprecessing frame for modeling gravitational waveforms from eccentric, precessing compact binaries using numerical relativity simulations, finding that while it facilitates surrogate modeling by reducing amplitude and phase modulations, it fails to fully separate precession effects from eccentricity, resulting in waveform mismatches that remain too high for precise characterization.
This paper humorously proposes that Mexican Burrowing Toads could serve as inexpensive gravitational wave detectors by amplifying cosmic signals through their nervous systems, though the authors found no evidence of such events in their recordings, ironically concluding that the lack of detection validates their unconventional approach.
This paper proposes that continuous gravitational waves generated by rapid charge-discharge processes in neutron star magnetospheres, particularly from outer gaps with strains around , could be detectable by future observatories like the Einstein Telescope, offering a new method to probe magnetospheric physics.
This paper investigates gravitational wave turbulence within the Hadad-Zakharov metric by addressing the compatibility of Einstein equations and utilizing a new GPU-based code to demonstrate the emergence of Kolmogorov-Zakharov spectra, dual cascades, and intermittent coherent structures, thereby confirming the propagation of genuine physical degrees of freedom.
This paper investigates two distinct single-field brane inflation scenarios—radial and angular—within a warped deformed conifold geometry, where moduli stabilization via D7-brane Kuperstein embeddings generates the inflaton potentials, demonstrating that embedding these models in the warm inflation paradigm with dissipation enables them to satisfy current observational constraints from Planck and ACT, whereas their cold inflation counterparts fail.
This paper investigates the gravitational waveform degeneracy between quasi-circular binary systems and Lagrange three-body systems up to 0.5PN order, demonstrating that while stable triples can mimic binary waveforms with high overlap for nearly symmetric masses, the unique degeneracy occurring at 0.5PN involves an unstable configuration.