2338 papers
This paper presents a systematic calculation of non-dissipative, quantum-origin second-order hydrodynamic corrections to the stress-energy tensor and currents for free boson and Dirac fields in thermal vorticity, deriving their Kubo formulae via equilibrium correlators and demonstrating that the axial current receives vorticity-proportional corrections independent of anomalous terms.
This paper validates the accuracy of prior-informed Fisher-matrix analyses by comparing them against real gravitational-wave data from GWTCs, demonstrating that while priors are crucial for handling parameter degeneracies, the Fisher approximation remains a reliable tool for future Einstein Telescope science-case studies.
The paper demonstrates that the standard low-energy effective field theory of quantum gravity predicts unobservably small vacuum fluctuations in interferometers, implying that any future detection of large gravitationally-induced length variations would signal a fundamental breakdown of this theory.
This paper presents a new general solution for gravitational field equations in quantum fluctuation modified gravity that encompasses various Kiselev black hole configurations, while analyzing their energy conditions, Hawking temperatures, and constraints on metric fluctuation parameters.
This paper reports a 100-fold improvement in sensitivity for detecting new gravity-like forces at micrometer scales using optically levitated microspheres, establishing the first multi-component vector force measurements and setting stringent new upper limits on Yukawa-type interactions in the 5–10 μm range.
This paper introduces a new set of non-orbit-averaged, gauge-invariant post-Newtonian equations up to 2.5 order that accurately describe the non-adiabatic evolution of eccentric black-hole binaries across all eccentricities, revealing the limitations of traditional orbit-averaged approximations like Peters' equations at the first pericenter passage.
This paper establishes a rigorous quantum optical framework for analyzing diffraction-induced vacuum field injection in DECIGO's Fabry-Perot cavities, demonstrating that while such losses slightly increase radiation pressure noise, cavity detuning combined with homodyne detection and optical-spring locking can effectively mitigate these effects to enhance the detector's sensitivity to primordial gravitational waves.
This paper demonstrates that classical-quantum gravity theories based on completely positive dynamics can be embedded into a fully quantum framework and, as a consequence, can violate fundamental conservation laws like angular momentum even when the underlying equations are rotationally symmetric.
This paper analyzes DESI DR2 data using a model-independent method to present potential evidence for physics beyond the standard CDM model, specifically suggesting a temporary acceleration of the universe's expansion at , a subsequent deceleration at , and a dark energy equation of state parameter less than -1 at .
This paper presents a systematic framework for deriving non-relativistic effective field theories from relativistic theories with generic, potentially non-analytic self-interactions, establishing an effective fluid description and extending the formalism to cosmological settings to analyze ultra-light dark matter models, boson stars, and dark matter halo cores.
This paper investigates a specific gravity model with effective curvature-matter interaction, demonstrating through statistical analysis of distance modulus data and a comparative study of early-Universe epochs that it predicts an earlier onset of structure formation and a higher matter-radiation equality redshift than standard CDM cosmology while remaining consistent with observed recombination data.
This paper investigates the Lorentzian gravitational path integral for 4D Gauss-Bonnet gravity, demonstrating that complex deformation of the coupling effectively resolves degeneracies arising from anti-linear symmetries and ensures compatibility with the KSW criterion for No-boundary geometries.
This paper provides an exact analytical solution for gravitational wave propagation in ghost-free bimetric gravity during a late-time de Sitter epoch, deriving new observational bounds from GW170817 and demonstrating that massless and massive graviton components maintain coherence even when temporally resolved.
This paper advocates for comparing astrophysical population-synthesis models directly to gravitational-wave data in observable space rather than reconstructing the underlying population, demonstrating that this approach respects model validity domains and enables unbiased inference of the observable compact-binary population using LIGO-Virgo-KAGRA data.
This paper demonstrates that nonvanishing spatial curvature in an initially empty universe generates primordial matter through quantum gravity effects, which is characterized by a stiff equation of state and alters the early universe's expansion history via modified Friedmann equations.
This paper investigates interacting -essence dark energy models with non-pressureless dark matter under two interaction scenarios, demonstrating through autonomous system analysis and extensive observational constraints that these models successfully reproduce cosmological evolution, yield values of 67–70 km/s/Mpc, and remain statistically competitive with the standard CDM model.
This paper presents a new black hole solution in bumblebee gravity with non-commutative corrections, analyzing its horizon properties, light propagation, and shadow to derive observational constraints from Event Horizon Telescope data and Solar System experiments.
This paper demonstrates that black holes with significant synchronized or resonant bosonic hair are dynamically unstable, causing their event horizons to be ejected from the center of their scalar environments in a process termed "splitting."
This paper proposes using linear Paul traps with single or multi-ion configurations to detect megahertz gravitational waves via graviton-photon conversion or relative-motion excitations, demonstrating that entangling vibrational qubits enhances signal probability by a factor of to surpass the standard quantum limit.
This paper presents a numerical study demonstrating that while massive particles scattering off Reissner-Nordström black holes are confined to a narrow range of deflection angles due to an event horizon, those interacting with naked singularities are scattered in all directions by a repulsive core, leading to distinct observable signatures in tidal disruption events.