Effects of radiation on the Laser Interferometer Lunar Antenna (LILA)The Moon provides a promising environment for gravitational-wave (GW) observations in the midband. The Laser Interferometer Lunar Antenna (LILA) combines a lunar deformation channel (LDC) and a…James M. Trippe, Brett N. Shapiro, Chloe A. Champagne et al.·Nov 1, 2026SaveLearn
Gravitational dynamics and backward ray-traced shadows of bumblebee AdS black holesWe investigate the total observed frequency shift of photons emitted by massive geodesic particles in circular orbits near the event horizon of bumblebee AdS black holes. The cosmological effects of…Muhammad Yasir, Senyue Lou, Zelin Zhang et al.·Nov 1, 2026SaveLearn
Strong gravity physics of dynamical horizons in black hole mergers and its imprint in their gravitational radiationIn a binary black hole merger, the inspiral portion of the gravitational waveform corresponds to two distinct horizons orbiting each other, and the merger and ringdown signals correspond to the final…Vaishak Prasad·Oct 31, 2026SaveLearn
Daemon sub Ponte: The Cost of a Second Black Hole (A Scholium on an ER=EPR Thought Experiment)A thought experiment in the ER=EPR and related literature involves collecting the Hawking radiation of an old black hole, then collapsing it into a second, entangled black hole. In this short note,…Yen Chin Ong·Oct 31, 2026SaveLearn
Probing Hidden Dimensions with Multimessenger Gravitational WavesThe dimensionality of spacetime is a fundamental property of nature, yet whether our observed four-dimensional spacetime is embedded in a higher-dimensional geometry remains experimentally…Hanlin Song, Minghui Du, Peng Xu·Oct 31, 2026SaveLearn
Excess inner-horizon entropy and the thermodynamics of Kerr formationWe develop a charge-matched thermodynamic framework for the regular rotating black-hole family underlying an exact model of Kerr formation. Since the Kerr endpoint already possesses a…Francisco S. N. Lobo, Jorge Ovalle, Manuel E. Rodrigues·Oct 31, 2026SaveLearn
The structured pseudospectrum of Schwarzschild black holeThe non-Hermitian nature of black hole quasinormal modes (QNMs) can give rise to remarkable spectrum instability. Such instability is naturally characterized by the pseudospectrum for the operator.…Liang-Bi Wu, Yu-Sen Zhou, Ming-Fei Ji et al.·Oct 31, 2026SaveLearn
Dimensional dependence of critical phenomena in black hole interiorsWe numerically investigate the interior dynamics of D dimensional Reissner-Nordström (RN) black holes perturbed by a real scalar field. Strong perturbations destroy the null inner horizon and…Li-Jie Xin, Xiangdong Zhang·Oct 31, 2026SaveLearn
Near-extremal critical dynamics driven by a phantom field in Einstein-Maxwell-scalar theoryWe investigate the fully nonlinear dynamics of Einstein-Maxwell-scalar black holes in the low-mass, near-extremal region of the solution space, which is difficult to access with conventional…Zhen-Kun Jia, Lang Zhao, Lin Chen et al.·Oct 31, 2026SaveLearn
Unitary implementability of Darboux transformationsWe investigate the unitary implementability of the canonical transformations corresponding to Darboux transformations in the Hamiltonian formalism recently developed for gauge invariant perturbations…Guillermo A. Mena Marugán, Alvaro Torres-Caballeros, José Velhinho·Oct 31, 2026SaveLearn
Absorption and scattering of massless scalar waves by black holes with scalar hairWe use partial waves to study massless scalar absorption and scattering by the normal (ξ=5) and phantom (ξ=-2) Bakopoulos--Nakas black holes, described by mass M and scalar charge q. At fixed…Lina Zhang, Yun Soo Myung, Yu-Xuan Wang et al.·Oct 31, 2026SaveLearn
Charged Gravastars with Casimir Energy in Quadratic f(T) GravityWe investigate a charged gravastar configuration in the framework of modified teleparallel gravity, considering the quadratic form f(T)=T+αT2 and incorporating Casimir vacuum energy as a source…S. R. Harshitha, C. S. Varsha, V. Venkatesha et al.·Oct 31, 2026SaveLearn
Holonomy classification, gyroscope precession, and Landau levels in Gödel-type spacetimes and their superfluid analogWe derive the parallel-transport holonomies of circles centered on the symmetry axis in the homogeneous Gödel-type family of Rebouças and Tiomno, which includes the Gödel universe, the causal member…Claudio Furtado, G. Q. Garcia, Abdullah Guvendi et al.·Oct 31, 2026SaveLearn
The Fluctuation-Dissipation Theorem and Dynamical Love Number in Schwarzschild Black HolesWe study the real-time response of a Schwarzschild black hole in the Hartle-Hawking state to an external massless scalar field. Using a complexified radial contour to represent the Schwinger-Keldysh…Dimitrios Giataganas, Alex Kehagias, Antonio Riotto·Oct 31, 2026SaveLearn
Exact scalarization thresholds and onset laws for a nonminimally coupled scalar field on the Ellis wormholeWe study a real scalar field nonminimally coupled to curvature on a fixed Ellis wormhole background. The scalar perturbation decouples at linear order, and the substitution x=a z reduces its…Abdullah Guvendi, Omar Mustafa, Claudio Furtado·Oct 31, 2026SaveLearn
Nonlinear stability of Schwarzschild black holes for the Einstein-massless Dirac system in spherical symmetryIn this paper, we establish the nonlinear stability of the Schwarzschild exterior for the spherically symmetric Einstein-massless Dirac system. More precisely, we consider sufficiently small…Lamberto Tresoldi·Oct 30, 2026SaveLearn
Strong-coupling of Minkowski spacetime in f(R) gravity: a Hamiltonian perspectiveA Hamiltonian analysis of f(R) gravity in the perturbation field approximation is performed. The action principle is presented as a series expansion around a generic fixed background with constant…Aldair Pantoja·Oct 30, 2026SaveLearn
Quantum superposition of Cosmic String spacetimesSince the quantum nature of spacetime is anticipated by a theory of Quantum Gravity, the possibility of spacetime superposition would be a natural consequence. This spacetime interference phenomena…Enrique Arias, Shoshauna Gauvin, Willy Izquierdo et al.·Oct 30, 2026SaveLearn
Hyperbolic scaling of the small-exponent limit in magnetic nonlinear electrodynamicsA magnetic spacetime can approach Schwarzschild while its electromagnetic characteristics remain singular in the same parameter limit. We study this separation in fractional-power nonlinear…Jonathan A. Rebouças, R. Martínez von Dossow, Edson Otoniel·Oct 30, 2026SaveLearn
A Charged Compact Star Solution for a Conducting SphereThis paper considers the simplest charged stellar model, namely, a uniform density star with electric charge distributed on its surface. In this model, we treat the uniform density star as a…Kai Lin·Oct 30, 2026SaveLearn
Scattering of massless scalar waves by higher-dimensional regular black holes in general relativity coupled to nonlinear electrodynamicsWe study the scattering of planar massless scalar waves by the family of higher-dimensional regular black holes in general relativity coupled to nonlinear electrodynamics, which unifies the Bardeen…Bobir Toshmatov, Askar Abdikamalov, Sardor Tojiev·Oct 30, 2026SaveLearn
Neutrino Oscillation in a Static Dihole GeometryWe investigate neutrino flavor oscillations in the static equal-mass Majumdar-Papapetrou dihole geometry, restricting the propagation to the symmetry plane. Within the null approximation, we derive…Rogério Capobianco, Rafael C. R. de Lima·Oct 30, 2026SaveLearn
Finite-Depth Null Capture and Mass-History Sensitivity in Vaidya SpacetimeWe formulate a finite-depth endpoint map for past-directed null rays in dynamical black-hole spacetimes, retaining an unresolved label when no terminal is reached before a prescribed optical depth.…Jorge Luis Palamara, Jorge R. Palamara·Oct 30, 2026SaveLearn
From thermogravity to thermocosmology with a running non-conservation scaleThermogravity offers a novel approach to cosmic acceleration, deriving trace-free gravitational equations and matter non-conservation from thermodynamic processes in spacetime. We extend this…Emmanuel N. Saridakis·Oct 30, 2026SaveLearn
Homogeneous Spectral Freedom and Hadamard Consistency of Perturbative Green FunctionsPerturbative mode equations often admit formally different particular solutions whose spectral sums appear to have different short-distance singularities. We formulate a general diagnostic which…Bekir Can Lütfüoğlu·Oct 30, 2026SaveLearn