The BEF symplectic form is derived from L∞-Lagrangians via covariant phase space methods and coincides with the Barnich-Brandt form for second-order equations of motion.
Some properties of Noether charge and a proposal for dynamical black hole entropy,
4 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 4representative citing papers
Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.
In 5D Einstein-Bumblebee gravity, Kerr/CFT microscopic entropy of constructed rotating black holes matches Komar-integral entropy but not Wald entropy.
A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.
citing papers explorer
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The BEF Symplectic Form: A Lagrangian Perspective
The BEF symplectic form is derived from L∞-Lagrangians via covariant phase space methods and coincides with the Barnich-Brandt form for second-order equations of motion.
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Stationary Stars Are Axisymmetric in Higher Curvature Gravity
Stationary stellar configurations are axisymmetric in diffeomorphism-invariant metric theories of gravity that include higher curvature corrections.
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Rotating Black Holes and the Kerr/CFT Correspondence in Einstein-Bumblebee Gravity
In 5D Einstein-Bumblebee gravity, Kerr/CFT microscopic entropy of constructed rotating black holes matches Komar-integral entropy but not Wald entropy.
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A new rotating axionic AdS$_4$ black hole dressed with a scalar field
A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.