Quantum-gravity-inspired Alcubierre warp-drive geometriesString T-duality, through its correspondence with path-integral duality, endows the low-energy propagator with a zero-point length l0=2πα' that softens the short-distance behavior of…Kimet Jusufi, Francisco S. N. Lobo·Sep 3, 2026SaveLearn
Does spatial curvature generate new thermodynamic criticality at the FLRW apparent horizon?We generalize the apparent-horizon thermodynamic construction of [1] to a FLRW universe with non-zero spatial curvature, non-interacting cold dark matter and holographic-type dark energy. For nonzero…Samuel Lepe, Joel Saavedra·Sep 3, 2026SaveLearn
Exact solution of the Klein-Gordon equation in a Kiselev black hole backgroundIn this work, we investigate exactly the dynamics of a relativistic spinless particle influenced by a static and uncharged black hole surrounded by a quintessence-like anisotropic fluid or Kiselev…Matheus. D. de Oliveira, Alexandre G. M. Schmidt·Sep 3, 2026SaveLearn
From Nonmetricity Operators to the Physical Spectrum: A Branch-Complete Analysis of Local Four-Derivative Symmetric Teleparallel GravityWe develop a branch-complete classical free-spectrum analysis of local parity-even symmetric teleparallel gravity containing all pure-gravity nonmetricity operators through four derivatives. After…Caglar Pala·Sep 3, 2026SaveLearn
Screened Scalar Hair and the Weak-Lensing Separation of Black Holes from Neutron Stars in Quadratic f(R) GravityQuadratic f(R) gravity carries a massive scalar degree of freedom, the scalaron, whose finite range λ screens its influence on the geometry outside a compact object. We show that this screening…Yashmitha Kumaran, Ilídio Lopes·Sep 3, 2026SaveLearn
An Attractor-Repeller model of the Local Universe : The Λ-Szekeres spacetime and Perturbation TheoryThe standard linearly perturbed Friedmann-Lemaître-Robertson-Walker (FLRW) framework provides an accurate description of the Universe on large scales but cannot fully capture the non-linear…Maharshi Sarma, Christian Marinoni, Basheer Kalbouneh·Sep 3, 2026SaveLearn
Waveform models for the gravitational-wave memory effect: III. Phenomenological frequency-domain model for nonspinning binariesWe present a phenomenological frequency-domain model for the gravitational-wave (GW) memory signal from nonspinning binary-black-hole mergers on quasicircular orbits. We develop separate amplitude…Arwa Elhashash, David A. Nichols·Sep 3, 2026SaveLearn
Emergent dark sector in group field theory cosmologyWe develop an analytical treatment of the emergent cosmological dynamics induced by local polynomial interactions in a deparametrised group field theory model, moving beyond the usual non-interacting…Andrea Calcinari, Federico Greco, Daniele Oriti et al.·Sep 3, 2026SaveLearn
Dyonic rotating cosmological black hole surrounded by quintessenceIn this work, we constructed a new metric describing a rotating cosmological black hole with electric and magnetic charges in the presence of quintessence dark energy, where the cosmological constant…M. D. de Oliveira, Alexandre G. M. Schmidt·Sep 3, 2026SaveLearn
An off-shell conformally invariant Galilean Weyl tensorWe propose a manifestly conformally invariant off-shell definition of the Weyl tensor in Galilean geometry. We also propose definitions for the electric and magnetic parts thereof. For the latter to…Quentin Vigneron, Philip K. Schwartz, James Read·Sep 3, 2026SaveLearn
Black holes in alternative theories of gravityBlack holes, with their strong gravitational fields, provide an important testing ground for theories of gravity beyond General Relativity. Among the many proposed alternatives, considerable recent…Jose Luis Blázquez-Salcedo, Fech Scen Khoo, Burkhard Kleihaus et al.·Sep 3, 2026SaveLearn
Eight Local Couplings of Gravitational Waves from Unified Field EquationsA gravitational-wave (GW) detector records a linear mixture of local couplings under the assumption that extra polarizations enter geodesic deviation. Vacuum general relativity (GR) admits two…Hong-Bo Jin, Yue-Liang Wu·Sep 3, 2026SaveLearn
On the interplay between waveform systematics and lensing signatures in gravitational-wave signalsThe exceptional gravitational-wave event GW231123 exhibited unusually high total mass and near-extremal spins, while revealing strong waveform-dependent variations in its inferred source properties.…Disha Hegde, Justin Janquart·Sep 3, 2026SaveLearn
Not All Resonances Are Created Equal: Prioritizing Tidal Resonances in EMRIsTidal perturbations from nearby compact objects can drive resonant "kicks" in extreme-mass-ratio inspirals (EMRIs), imprinting potentially detectable phase shifts in LISA-band gravitational…Béatrice Bonga, Patrick Bourg, Bram ten Brink et al.·Sep 3, 2026SaveLearn
Long-lived ringing of Bronnikov--Kim brane-world black holes and wormholesMassive-field perturbations on black-hole and wormhole backgrounds can form long-lived quasinormal ringing; this behaviour is not confined to brane-world spacetimes, but it is also not universal…Milena Skvortsova·Sep 3, 2026SaveLearn
Dynamical Selection of Horizon-BMS Goldstone Modes in Evaporating Black HolesWe investigate the dynamics of horizon soft degrees of freedom associated with near-horizon BMS supertranslations in an evaporating Vaidya-Schwarzschild black hole spacetime. Considering the dynamic…Nihar Ranjan Ghosh, Malay K. Nandy·Sep 3, 2026SaveLearn
Solutions for neutron stars in General Relativity from a complexity structure scalar boundary conditionA new condition involving the complexity factor, a structure scalar arising from the orthogonal splitting of the Riemann tensor, is generated at the boundary of a spherically symmetric anisotropic…Robert S. Bogadi, Megandhren Govender, Genly Leon et al.·Sep 3, 2026SaveLearn
Introducing SINFONIA: Symplectic, slimplectic and Magnusian (Neural) Flows for Orbital Numerical Integration and AccelerationLong-duration gravitational-wave modelling must resolve fast orbital motion together with slow dissipative evolution while preventing small numerical errors from accumulating into secular phase…Lidia J. Gomes Da Silva·Sep 3, 2026SaveLearn
Tidal forces in the quantum Oppenheimer--Snyder black holeWe investigate the tidal forces experienced by massive particles in radial free fall in the quantum Oppenheimer--Snyder black hole, a loop quantum gravity correction to the Schwarzschild geometry…Anuar Idrissov, Hernando Quevedo·Sep 3, 2026SaveLearn
Constraint closure and gravitational-wave content of shear-free cosmologies in metric f(R) gravityWe derive the consistency conditions governing the propagating content of linear shear-free perturbations of Friedmann-Lema\ıtre-Robertson-Walker cosmologies in metric f(R) gravity. The divergence…Mudhahir Al Ajmi, Amare Abebe·Sep 3, 2026SaveLearn
Non-extensive entropy signatures in compact starThe non-extensive entropy models applied to the black-hole horizon are connected to the generalized Einstein--Hilbert action, f(R), via the Wald entropy formalism. We demonstrate that quark star…B. N. Jayawiguna, M. H. Al Ghifari, A. Rohim et al.·Sep 3, 2026SaveLearn
Exceptional points and the breaking of Schwarzschild isospectrality under local potential perturbationsThe odd- and even-parity gravitational perturbations of a Schwarzschild black hole are governed by the distinct Regge-Wheeler and Zerilli potentials, yet their quasinormal-mode (QNM) spectra are…Mohamed Ould El Hadj·Sep 2, 2026SaveLearn
Evolving wormhole cosmology: modified Friedmann dynamics and observational constraintsWe construct an evolving wormhole cosmological model from a Morris--Thorne metric with a separable, time-dependent shape function in a spatially flat Friedmann--Lemaitre--Robertson--Walker…Aritra Sanyal, Kazuharu Bamba, Prabir Rudra·Sep 2, 2026SaveLearn
Coherent multipath wave response on Reissner-Nordström analogue surfaceTo uncover how the intrinsic metric of a relativistic compact object governs macroscopic wave phenomena, we establish a theoretical framework mapping the charge dependent spatial geometry of a…Peng-Yu Chen, Sen Guo, Qing-Quan Jiang et al.·Sep 2, 2026SaveLearn
Relativistic transformation of temperature for exotic cosmological fluidsWe study the relativistic transformation of temperature for effective cosmological fluids with negative pressure within a covariant thermodynamic framework. The Lorentz transformation of temperature…Soroor Pouryazdan, Babak Vakili·Sep 2, 2026SaveLearn