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Horizon Strings as 3d Black Hole Microstates
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We propose that 3d black holes are an ensemble of tensionless null string states. These microstates typically have non-zero winding. We evaluate their partition function in the limit of large excitation numbers and show that their combinatorics reproduces the Bekenstein-Hawking entropy and its semiclassical logarithmic corrections.
Forward citations
Cited by 4 Pith papers
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Null-strings Gauged, Reloaded and Quantized, I: Canonical Quantization in the Light-Cone Gauge
Light-cone Schrödinger quantization of null-strings with Carroll-Weyl symmetry yields D-3 physical modes, a discrete spectrum, and no critical dimension.
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An Inconsistency in the Null Strings Literature: The Tale of an Overlooked Symmetry
The paper claims a new local symmetry of null strings forces a third constraint, giving D−3 physical degrees of freedom.
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Towards Quantizing Null p-branes: Light-Cone Gauge Analysis and Physical Hilbert Space
Quantized null p-branes in light-cone gauge have physical Hilbert spaces split into p+1 classes of standing-wave states.
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A time-like window into tensionless worldsheets
Kasner worldsheets near their null horizons reproduce the tensionless, Carrollian string physics previously found for Rindler worldsheets, with a Bogoliubov-map identification that depends on an arbitrary regularizati...
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