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Weinberg,Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity(John Wiley and Sons, New York, 1972)

7 Pith papers cite this work. Polarity classification is still indexing.

7 Pith papers citing it

years

2026 4 2025 3

verdicts

UNVERDICTED 7

representative citing papers

Relativistic Gravity-Induced Entanglement via Frame Dragging

quant-ph · 2026-06-30 · unverdicted · novelty 6.0

Derives the same entanglement phase from frame dragging via Schrödinger evolution and path-integral methods in linearized gravity, including retardation effects, under locality assumptions that would imply non-classical gravity.

Metric affine gravity with dynamical chronology protection

gr-qc · 2026-04-09 · unverdicted · novelty 6.0

A new metric-affine gravity toy model dynamically generates a global time function via projective invariance breaking to enforce stable causality, recovering mimetic gravity and yielding a broader dark sector.

From minimal-length quantum theory to modified gravity

gr-qc · 2025-11-18 · unverdicted · novelty 5.0

A systematic mapping is derived from GUP parameters in minimal-length quantum theory to higher-order curvature coefficients in extended gravity, with an application yielding an upper bound on the minimal measurable length via light deflection corrections.

Regular black holes with gravitational self-energy as dark matter

gr-qc · 2025-09-10 · unverdicted · novelty 5.0

Incorporating non-local gravitational self-energy from a T-duality-inspired model yields a regular neutral black-hole metric with extremal Planck-mass particle-black-hole solutions that are thermodynamically stable and suggested as dark matter.

citing papers explorer

Showing 7 of 7 citing papers.

  • Relativistic Gravity-Induced Entanglement via Frame Dragging quant-ph · 2026-06-30 · unverdicted · none · ref 66

    Derives the same entanglement phase from frame dragging via Schrödinger evolution and path-integral methods in linearized gravity, including retardation effects, under locality assumptions that would imply non-classical gravity.

  • Gravitational Waves from a Black Hole Falling Radially into a Thin-Shell Traversable Wormhole gr-qc · 2026-05-02 · unverdicted · none · ref 54

    Analytic gravitational waveforms from radial test-particle infall into a thin-shell traversable wormhole exhibit a characteristic pulse-gap structure from repeated throat crossings and lie within reach of ground-based detectors at ~500 Mpc.

  • Metric affine gravity with dynamical chronology protection gr-qc · 2026-04-09 · unverdicted · none · ref 70

    A new metric-affine gravity toy model dynamically generates a global time function via projective invariance breaking to enforce stable causality, recovering mimetic gravity and yielding a broader dark sector.

  • From minimal-length quantum theory to modified gravity gr-qc · 2025-11-18 · unverdicted · none · ref 83

    A systematic mapping is derived from GUP parameters in minimal-length quantum theory to higher-order curvature coefficients in extended gravity, with an application yielding an upper bound on the minimal measurable length via light deflection corrections.

  • Regular black holes with gravitational self-energy as dark matter gr-qc · 2025-09-10 · unverdicted · none · ref 29

    Incorporating non-local gravitational self-energy from a T-duality-inspired model yields a regular neutral black-hole metric with extremal Planck-mass particle-black-hole solutions that are thermodynamically stable and suggested as dark matter.

  • Semi-analytic bounds on axion-like-particle supernovae emission hep-ph · 2026-04-30 · unverdicted · none · ref 29

    Semi-analytic modeling of supernova cooling with six PNS parameters yields bounds on axion-nucleon coupling versus ALP mass that match numerical simulation results.

  • Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 astro-ph.CO · 2025-12-02 · unverdicted · none · ref 70

    Local Hubble constant anisotropy in Cosmicflows-4 data is primarily attributed to peculiar velocities and survey structure rather than cosmic-scale isotropy violation, with limited implications for the Hubble tension.