The f(Q)f(Q) gravity and affine EoS: Compatibility and observational constraints

This paper investigates the cosmological implications of an affine equation of state within General Relativity and f(Q)f(Q) gravity, demonstrating that while both frameworks can unify the universe's transition from decelerated to accelerated expansion, the affine model yields quintessence-like dark energy in General Relativity but phantom-like dark energy in f(Q)f(Q) gravity, with parameters constrained by Cosmic Chronometer and Supernovae type Ia data.

Romanshu Garg, G. P. Singh, Ashutosh Singh2026-03-10⚛️ gr-qc

Geometric realization of stress-tensor deformed field theory

This paper establishes a semiclassical framework demonstrating that stress-tensor deformations of quantum field theories are equivalent to gravitational actions evaluated at metric saddles, thereby creating a bidirectional link between field theory flows and classical gravity that is explicitly verified through the emergence of an induced Newton constant in a deformed free scalar theory.

Yun-Ze Li, Yunfei Xie, Song He2026-03-10⚛️ hep-th

Information paradox and island of covariant black holes in LQG

This paper investigates the information paradox in four-dimensional covariant black holes within Loop Quantum Gravity, revealing that while two distinct solutions exhibit contrasting evaporation dynamics, the application of the island prescription to the first solution successfully recovers unitarity by suppressing late-time entropy growth through the influence of the LQG parameter.

Yongbin Du, Jia-Rui Sun, Xiangdong Zhang2026-03-10⚛️ gr-qc

Novel scalar degrees of freedom emerging from hybrid metric-Palatini gravity

This paper introduces the hybrid metric-Palatini scalar-tensor (HMPST) theory as an extension of hybrid metric-Palatini gravity, demonstrating that its linear-f(R^)f(\hat{R}) subclass consistently unifies cosmological acceleration, astrophysical compact objects, and Solar System constraints through analytically tractable solutions and Yukawa-type weak-field corrections that recover General Relativity.

David S. Pereira, Salvatore Capozziello, Francisco S. N Lobo + 1 more2026-03-10⚛️ gr-qc

Bohmian Quantum Cosmology from the Wheeler-DeWitt Equation

This paper constructs a solvable Bohmian quantum cosmological model for a flat universe with a unified dark sector scalar field by mapping the Wheeler-DeWitt equation to a hyperbolic oscillator, enabling the derivation of deterministic trajectories that reproduce late-time Λ\LambdaCDM expansion while exhibiting quantum modifications at early epochs.

Spyros Basilakos, Gerasimos Kouniatalis, Emmanuel N. Saridakis + 1 more2026-03-10⚛️ gr-qc

Critical collapse of a massive scalar field in semi-classical loop quantum gravity

Numerical simulations of massive scalar field collapse within two semi-classical loop quantum gravity frameworks reveal that critical phenomena remain consistent with classical general relativity, exhibiting type II behavior for small masses and type I behavior with a finite minimum black hole mass for large masses, indicating that semi-classical LQG corrections have a negligible impact on these dynamics.

Li-Jie Xin, Xiangdong Zhang2026-03-10⚛️ gr-qc

Constraining ββ-Exponential Inflation with the latest ACT observations

This paper demonstrates that the β\beta-exponential inflationary potential, particularly when augmented with a small non-minimal coupling, successfully reconciles the higher scalar spectral index indicated by recent ACT and DESI observations with current CMB constraints by predicting a spectral tilt larger than universal attractor models while suppressing the tensor-to-scalar ratio.

Jureeporn Yuennan, Farruh Atamurotov, Salvatore Capozziello + 1 more2026-03-10⚛️ gr-qc

From Bertotti--Robinson to Vacuum: New Exact Solutions in General Relativity via Harrison and Inversion Symmetries

This paper constructs new accelerating vacuum solutions in General Relativity by applying Harrison and Inversion symmetries to electrovacuum configurations, demonstrating how external electromagnetic fields can be removed to leave non-trivial gravitational backreactions, including a new two-parameter extension of the Schwarzschild–Levi-Civita geometry and a stationary generalization.

José Barrientos, Adolfo Cisterna, Amaro Díaz + 1 more2026-03-10⚛️ hep-th

All $2Dgeneraliseddilatontheoriesfrom generalised dilaton theories from d\geq 4$ gravities

This paper demonstrates that all two-dimensional Horndeski theories can be derived from higher-dimensional pure gravity reductions, leading to a Birkhoff theorem for a class of "quasi-topological" gravities that allows for the explicit reconstruction of any static, spherically symmetric, asymptotically flat spacetime satisfying specific metric conditions as a vacuum solution, including regular black holes like the Bardeen spacetime.

Johanna Borissova2026-03-10⚛️ hep-th

Flat holography for spinor fields

This paper establishes a flat-space holographic dictionary for free massive spinor fields in four-dimensional Minkowski spacetime by utilizing hyperbolic slicing to reduce the problem to effective AdS3\mathrm{AdS}_3 systems, thereby deriving universal two-point correlation functions for dual spinning operators on the celestial sphere and clarifying the construction of spinor conformal primary wavefunctions.

Dmitry S. Ageev, Anna S. Bernakevich2026-03-10⚛️ hep-th