Does Eternal Inflation Violate the Smeared Null Energy Condition?The smeared null energy condition (SNEC) imposes a semilocal bound on the negative energy accumulated along null geodesics. In eternal inflation, rare stochastic upward fluctuations of the inflaton…Dong-Hui Yu, Yong Cai·Jun 6, 2026SaveLearn
Rotation-Induced Effective Anisotropy in White Dwarfs as a Newtonian Benchmark with Relativistic Scale AssessmentWe develop a one-dimensional Newtonian reduction for uniformly rotating cold white dwarfs in which the angle-averaged centrifugal support is represented by an effective anisotropic term. From the…Aray Muratkhan, Aliya Taukenova, Saken Toktarbay et al.·Jun 6, 2026SaveLearn
Renormalization-group improved Schwarzschild black hole: shadow, ringdown, and strong cosmic censorshipA renormalization-group (RG) improved Schwarzschild-like black hole (BH) is studied here, with a lapse that interpolates between a classical Schwarzschild exterior and a quantum-smoothed interior set…Ahmad Al-Badawi, Faizuddin Ahmed, İzzet Sakallı·Jun 6, 2026SaveLearn
Energy-momentum and dark energy in SU(∞)-QGR quantum gravitySU(∞) Quantum GRavity (QGR) is a recently proposed fundamentally quantum approach to gravity and cosmology. In this model the Hilbert space of the Universe represents SU(∞) symmetry.…Houri Ziaeepour·Jun 6, 2026SaveLearn
Hotspot Images from Magnetic Reconnection Processes in the plunging Region of a Kerr Black HoleEmploying the hotspot imaging technique, this work investigates the plasma motion trajectories prior to and following the Comisso-Asenjo mechanism within the plunging region. After a concise overview…Xiao-Xiong Zeng, Yun Hong, Ke Wang·Jun 6, 2026SaveLearn
Traversable Wormhole Solutions in massive F(T) gravityWe study traversable wormhole geometries in an F(T) teleparallel framework augmented by a perturbative de Rham-Gabadadze-Tolley (dRGT) graviton-mass term. Adopting the static, spherically symmetric…Alexandre Landry, Yassine Sekhmani, Sunil K Maurya et al.·Jun 6, 2026SaveLearn
Spacetime Bartnik Mass Positivity and Temporal Monotonicity for Black HolesWe define a quasilocal mass of Bartnik type, and establish its positivity and temporal monotonicity properties for two classes of domains associated with black holes. More precisely, we first show…Lars Andersson, Marcus Khuri, Marc Mars et al.·Jun 5, 2026SaveLearn
Stochastic scalar-tensor inflation and beyondDuring cosmological inflation, inhomogeneities arising from quantum vacuum fluctuations are stretched to become super-Hubble and effectively classical. As many scenarios of the origin involve…Yoann Launay·Jun 5, 2026SaveLearn
Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing arraysSearches for gravitational waves (GWs) from isolated supermassive black hole binaries (SMBHBs) in pulsar timing array (PTA) data require simultaneous estimation of signal and noise parameters, so the…Xuan Tao, Boris Goncharov, Yiqian Qian et al.·Jun 5, 2026SaveLearn
Loss of the scaling attractor in self-gravitating domain wall networksDomain-wall(DW) networks are known to approach a relativistic scaling regime on fixed radiation- and matter-dominated backgrounds, forming the basis of the no-frustration conjecture. However, this…Zhen-Min Zeng·Jun 5, 2026SaveLearn
From (Hidden) Symmetries to Stealth SolutionsIn a recent paper, Arxiv:2605.23077, we have demonstrated that (conformal) Killing vectors give rise to stealth vector solutions of a specific bumblebee-type Proca theory supplemented by fine tuned…David Kubiznak, Robert B. Mann, Marek Milička·Jun 5, 2026SaveLearn
Vanishing of all redshift modes in Schwarzschild ringdownSeveral studies of black hole ringdown from particles plunging into black holes have identified contributions decaying at integer multiples of the surface gravity, called redshift modes, horizon…Adrien Kuntz, Matteo Della Rocca·Jun 5, 2026SaveLearn
Fuzzy-novaeWe propose a novel phenomenological model of quantum gravitational collapse inspired by loop quantum gravity that ensures a completely regular spacetime evolution. By incorporating quantum…Francesco Fazzini, Waleed Sherif·Jun 5, 2026SaveLearn
Accelerating scaling solutions from dark matter particle creationThis article opens new window to obtain accelerating scaling attractors without any need of dark energy. We study cosmological dynamics in a two-fluid system where pressureless dark matter (DM)…Sudip Halder, Jaume de Haro, Supriya Pan et al.·Jun 5, 2026SaveLearn
Dynamical Black Hole Thermodynamics in Modified GravityWe investigate the dynamical and thermodynamic evolution of a Schwarzschild black hole in Modified Gravity (MOG) perturbed by a scalar gravitational wave breathing mode. By evaluating the linearized…Nikko John Leo S. Lobos, Emmanuel T. Rodulfo·Jun 5, 2026SaveLearn
Distinguishing Black Holes and Neutron Stars via Optical Images Illuminated by Thick Accretion DisksThis paper investigates the optical images of neutron stars within the framework of the radiatively inefficient accretion flow model, taking into account a polytropic equation of state. After…Chen-Yu Yang, Xiao-Xiong Zeng·Jun 5, 2026SaveLearn
Melvin--Bonnor and Bertotti--Robinson spacetimes with Baryonic chargeIn this work, we exploit a dictionary that maps solutions of the Einstein--Scalar--Maxwell theory to those of gauged Skyrme--Maxwell--Einstein models in (3+1) dimensions, allowing gravitating…José Barrientos, Fabrizio Canfora, Adolfo Cisterna et al.·Jun 5, 2026SaveLearn
Thermodynamic and Dynamical Properties of Phantom Charged Black Holes in 4D Einstein-Gauss-Bonnet GravityWe present charged black hole solutions of regularized four dimensional Einstein Gauss Bonnet gravity coupled to a phantom electromagnetic field. We investigate the combined effects of higher…Bilel Hamil·Jun 5, 2026SaveLearn
Cosmological perturbations in Energy-Momentum Squared GravityWe present a fully covariant and gauge-invariant analysis of linear cosmological perturbations in Energy-Momentum Squared Gravity. Working within the 1+3 formalism, we derive the exact propagation…Peter K. S. Dunsby, Maria-Alexia Caldis, Eduardo Bittencourt·Jun 5, 2026SaveLearn
Quantum spacetime from constraints: wave equations and fieldsIn previous works, we showed that both time and space can emerge from entanglement within a globally constrained quantum Universe, with no background coordinates. By extending the Page and Wootters…Tommaso Favalli·Jun 5, 2026SaveLearn
Resonant interactions from dynamical perturbers on generic orbits around an extreme mass ratio inspiralExtreme mass-ratio inspirals (EMRIs) are binary systems where a compact object slowly inspirals into its much larger compact partner. Since we anticipate such systems to exist within and be…Makana Silva, Harrison G. Blake-Goszyk, Christopher M. Hirata·Jun 5, 2026SaveLearn
Correlation and Data-Analysis Distinctiveness of Time-Delay Interferometry ConfigurationsTime-Delay Interferometry (TDI) is essential for space-based gravitational wave (GW) missions, as it suppresses laser frequency noise and achieve the required sensitivity. Beyond the standard…Gang Wang·Jun 5, 2026SaveLearn
Entropy in Loop Quantum CosmologyThe Generalized First Law (GFL) and the Generalized Second Law (GSL) of thermodynamics are studied for cosmological scenarios with spatial curvature through an apparent horizon. We focus on effective…Alejandro Corichi, Omar Gallegos·Jun 5, 2026SaveLearn
Radial Oscillations of Viscous Stars at Finite TemperatureWe study the radial oscillation spectrum of relativistic stars within Israel-Stewart and Navier-Stokes theories, extending previous analyses to include heat diffusion and a thermodynamically…Amanda Guerrieri, Gabriel S. Rocha, Gabriel S. Denicol et al.·Jun 4, 2026SaveLearn
Measuring a Black Hole's Area Immediately after Merger: A Direct-Wave Test of Hawking's Area LawBlack-hole area is the geometric variable behind horizon thermodynamics. We introduce a gravitational-wave method to infer a Kerr-equivalent horizon area from direct waves in the near-merger signal,…Adrian Ka-Wai Chung, Kelvin Ka-Ho Lam, Anna Liu et al.·Jun 4, 2026SaveLearn