Thermodynamic quantities for black p-branes in arbitrary dimensions can be derived without constructing solutions by generalizing a previous method, including cases with general scalar cosets.
ADM masses for black strings and p-branes
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abstract
An ADM mass formula is derived for a wide class of black solutions with certain spherical symmetry. By applying this formula, we calculate the ADM masses for recently discovered black strings and $p$-branes in diverse dimensions. By this, the Bogolmol'nyi equation can be shown to hold explicitly. A useful observation is made for non-extremal black $p$-branes that only for $p = 0$, i.e. for a black hole, can its ADM mass be read directly from the asymptotic behaviour of the metric component $g_{00}$.
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UNVERDICTED 2representative citing papers
Semi-holographic systems with perturbative and holographic sectors exhibit prethermal time crystals through dissipationless modes in hydrodynamic channels plus short-wavelength instabilities that produce inhomogeneities over a wide temperature range.
citing papers explorer
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Black p-brane Thermodynamics without Constructing Solutions
Thermodynamic quantities for black p-branes in arbitrary dimensions can be derived without constructing solutions by generalizing a previous method, including cases with general scalar cosets.
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On prethermal time crystals from semi-holography
Semi-holographic systems with perturbative and holographic sectors exhibit prethermal time crystals through dissipationless modes in hydrodynamic channels plus short-wavelength instabilities that produce inhomogeneities over a wide temperature range.