A self-consistent angular momentum constraint in black hole spacetimes shows MSS chaos bound violations in charged Kiselev black holes are often parameter artifacts while higher-curvature geometries exhibit genuine violations at large charge-to-mass ratios.
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Stress-tensor deformations of QFTs are mapped to gravitational actions at metric saddles, with bidirectional examples and an induced Newton constant from the one-loop effective action of a massive scalar.
Bouncing solutions in quadratic curvature gravity with a scalar field satisfy null, weak, and dominant energy conditions but violate the strong one when using the scalar-field energy-momentum tensor, while all four conditions are violated near the bounce in the effective tensor formulation.
Generalizing primordial gravitational waves to a three-mode Bogoliubov transformation yields classical behavior via quantum discord for large squeeze parameters when only two of three modes are considered, while the quantum Poincare sphere shows non-classicality for positive squeeze or nonzero cosθ,
Non-Abelian monopoles in modified gravity exhibit substantial structural and property differences from their Einstein-gravity counterparts, especially at strong Higgs self-coupling.
citing papers explorer
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Physical constraints on the Maldacena-Shenker-Stanford chaos-bound in black hole spacetimes
A self-consistent angular momentum constraint in black hole spacetimes shows MSS chaos bound violations in charged Kiselev black holes are often parameter artifacts while higher-curvature geometries exhibit genuine violations at large charge-to-mass ratios.
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Geometric realization of stress-tensor deformed field theory
Stress-tensor deformations of QFTs are mapped to gravitational actions at metric saddles, with bidirectional examples and an induced Newton constant from the one-loop effective action of a massive scalar.
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Energy conditions of bouncing solutions in quadratic curvature gravity coupled with a scalar field
Bouncing solutions in quadratic curvature gravity with a scalar field satisfy null, weak, and dominant energy conditions but violate the strong one when using the scalar-field energy-momentum tensor, while all four conditions are violated near the bounce in the effective tensor formulation.
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Non-classicality of Primordial Gravitational Waves in Three-mode Representation Through Quantum Poincare Sphere
Generalizing primordial gravitational waves to a three-mode Bogoliubov transformation yields classical behavior via quantum discord for large squeeze parameters when only two of three modes are considered, while the quantum Poincare sphere shows non-classicality for positive squeeze or nonzero cosθ,
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Non-Abelian monopoles in modified gravity
Non-Abelian monopoles in modified gravity exhibit substantial structural and property differences from their Einstein-gravity counterparts, especially at strong Higgs self-coupling.
- Thermodynamics, Phase Transitions, and Geodesic Structure of F(R)-Phantom Banados-Teitelboim-Zanelli (BTZ) Black Holes