Integrability of R2 gravity cosmological models with radiationWe consider cosmological R2 gravity models with radiation. We find the general solution to the trace equation R=0 in the spatially flat Friedmann-Lemaitre-Robertson-Walker (FLRW) metric. We…Vsevolod R. Ivanov, Sergey Yu. Vernov·Jun 16, 2026SaveLearn
Lagrangian Extensions of Newtonian Gravity constrained by Solar System testsWe explore an extension to Newtonian gravity through a generalised Lagrangian function with the introduction of a second dynamical scalar field. Building on previous research into gravity with…Pedro H. Dalprá, Júlio C. Fabris, Hermano Velten et al.·Jun 16, 2026SaveLearn
Adaptive ray tracing, image diagnostics, and photon ring signatures of rotating dark-matter-dressed black holesWe study the optical appearance of rotating black holes embedded in dark matter environments using a phenomenological ray tracing framework. Rather than focusing on a single geometry, we compare two…Mohsen Fathi·Jun 16, 2026SaveLearn
Energy conditions in static, spherically symmetric spacetimes and effective geometriesClassical energy conditions are investigated in generic static and spherically symmetric spacetimes. In setups with nonconstant gtt grr, the appearance of horizons can signal the violation of…Zi-Liang Wang, Emmanuele Battista·Jun 16, 2026SaveLearn
Thermodynamic constraints and future singularities in Unimodular Gravity driven by phantom and non-phantom fluidsThis work investigates future cosmological singularities in a flat FLRW universe filled with a single barotropic fluid, (p = (γ- 1)ρ), within the framework of unimodular gravity. In this setting,…Norman Cruz, Samuel Lepe, Guillermo Palma et al.·Jun 16, 2026SaveLearn
Geometric properties of slowly rotating black holes embedded in matter environmentsExtreme mass-ratio inspirals (EMRIs) provide a precise probe of strong-field gravity, where small deviations from vacuum Kerr geometry can accumulate over many orbital cycles. In realistic…Sayak Datta, Chiranjeeb Singha·Jun 16, 2026SaveLearn
Null Raychaudhuri Equation and the Impossibility of Traversable Wormholes in Unimodular GravityWe formulate the traversability of wormhole throats as a local and covariant null defocusing condition derived from the Raychaudhuri equation. Since unimodular gravity preserves the local geometric…Erick Pastén, Marco Bosquez, Norman Cruz·Jun 16, 2026SaveLearn
Matter environments around black holes: geodesics, light rings, and ultracompact configurationsAstrophysical black holes are invariably embedded in matter environments whose gravitational influence can alter key strong-field features of the spacetime. In this work, we investigate the impact of…Dylan S. Fonseca, Caio F. B. Macedo, Mateus Malato Corrêa et al.·Jun 16, 2026SaveLearn
Internal structure of Hayward black holesRegular black holes, free of central singularities, provide an ideal laboratory for probing the geometric structure of spacetime. The global structure of some regular black holes, e.g. Hayward black…Caiying Shao, Jun-Qi Guo, Yu Tian et al.·Jun 16, 2026SaveLearn
Dynamical Formation of Black Holes due to Boundary Effect in Vacuum GravityWe prove the dynamical formation of a marginally outer trapped surface in pure vacuum spacetime from smooth asymptotically flat Cauchy data which initially contain no MOTS. The mechanism is a…Puskar Mondal, Shing-Tung Yau·Jun 16, 2026SaveLearn
Dynamical Tidal Response of Schwarzschild Black HolesDynamical Love numbers capture the conservative response of an object to a time-dependent external tidal gravitational field. We compute the dynamical Love numbers of Schwarzschild black holes in…Oscar Combaluzier--Szteinsznaider, Daniel Glazer, Austin Joyce et al.·Jun 16, 2026SaveLearn
Null integrability and photon phenomenology in the accelerated Schwarzschild black holeUniformly accelerated black holes provide a controlled setting to isolate how translatory acceleration and conical defects modify photon dynamics and observable optics. We analyse null geodesics in…Shokoufe Faraji, Eva Hackmann·Jun 16, 2026SaveLearn
Sequential simulation-based inference for extreme mass ratio inspiralsExtreme mass-ratio inspirals pose a difficult challenge in terms of both search and parameter estimation for upcoming space-based gravitational-wave detectors such as LISA. Their signals are long and…Philippa S. Cole, James Alvey, Lorenzo Speri et al.·Jun 16, 2026SaveLearn
Relativistic magnetohydrodynamics in the early UniverseWe review the conservation laws of magnetohydrodynamics (MHD) in an expanding homogeneous and isotropic Universe that can be applied to the study of early Universe physics during the epoch of…Alberto Roper Pol, Antonino Salvino Midiri·Jun 16, 2026SaveLearn
Shadow, Emission, and Strong-Field Lensing of Dilatonic Black HolesWe study the shadow and strong-field optical properties of a static, spherically symmetric dyon-like dilatonic black hole. The photon sphere radius, critical impact parameter, and shadow radius are…Kuantay Boshkayev, Ainur Urazalina, Aidana Kurmanbek et al.·Jun 15, 2026SaveLearn
CASPER: Interpretable ResNet based Classifier with FastShap Explainer for Gravitational Wave DetectionTraditional matched filtering has been the standard for Gravitational waves (GW) detection ever since LIGO was established, even though it requires pre-computed waveform templates and provides no…R. Rai, R. Verma, Somya·Jun 15, 2026SaveLearn
Exciting the Vacuum: Non-Thermal Particle Bursts and Multi-Messenger Signals from Binary Black HolesWe investigate particle production in the dynamical curved spacetime of a binary black hole system. Particle production is a well-known feature of quantum field theory in curved spacetime, underlying…Sohrab Rahvar·Jun 15, 2026SaveLearn
Boundary conditions and Hilbert spaces in no-roll quantum cosmologyWe construct Hilbert spaces for the minisuperspace quantum cosmology of a closed Universe in the limit of extreme slow-roll inflation, in which the scalar field is approximated as constant. In this…Steffen Gielen·Jun 15, 2026SaveLearn
Improving low-latency multi-messenger follow-up of neutron star-black hole mergers with mode-by-mode filteringRapid parameter estimation for neutron star-black hole (NSBH) mergers is essential for deciding whether, where, and how electromagnetic facilities should follow up gravitational-wave alerts. Current…Francesco Iacovelli, Digvijay Wadekar, Javier Roulet et al.·Jun 15, 2026SaveLearn
Quantum fate of the Choptuik naked singularityClassical critical collapse provides a dynamical route from smooth initial data to a naked singularity, representing a sharper violation of predictability than ordinary black hole singularities. We…Chih-Hung Wu·Jun 15, 2026SaveLearn
Fixed-quadrupole static tidal response of Schwarzschild black holes in a cubic Weyl effective field theoryStatic Love numbers of four-dimensional Schwarzschild black holes vanish in general relativity. We study how the fixed-quadrupole static tidal solution is modified by the parity-even cubic Weyl…Edilberto O. Silva·Jun 15, 2026SaveLearn
Non-linear stability of the matter dominated universeWe numerically study non-linear perturbations of the Einstein-de Sitter spacetime as a solution to the Gowdy-symmetric Einstein-Euler system for a polytropic equation of state. The results suggest…David Fajman, Elliot Marshall·Jun 15, 2026SaveLearn
Kinetic Theory of Cosmological Magnetogenesis at Second Order: A New Density-Gradient Source and Comparison with the Harrison MechanismWe derive and compare three mechanisms of cosmological magnetogenesis: the Thomson-scattering velocity-difference mechanism of Takahashi et al.\ (2005), a new density-gradient source identified here…Bob Osano·Jun 15, 2026SaveLearn
Generalized Unimodular Gravity and Cosmological PerturbationsThe generalized unimodular theory is revisited and its consequence for cosmology is discussed. The usual matter components of the universe are obtained in a pure geometric way. This result gives a…Júlio C. Fabris, Alexander Yu. Kamenshchik·Jun 15, 2026SaveLearn
Ultraviolet Structure of Real-time Gravitational Wave Linear Response in a Resonant Scalar FieldWe study the real-time linear response of gravitational waves in a time-dependent resonant scalar field in a Minkowski background. In the Schwinger-Keldysh formalism, we develop an adiabatic…Han Lai, Atsuhisa Ota·Jun 15, 2026SaveLearn