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Information recovery from evaporating rotating charged black holes
Zhi-Wei Wang, Samuel L. Braunstein, Saurya Das
In classical gravity, nothing can escape from a black hole, not even light. In particular, this happens for stationary black holes because their horizons are null. We show, on the…
Life in a random universe: Sciama's argument reconsidered
Zhi-Wei Wang, Samuel L. Braunstein
Random sampling in high dimensions has successfully been applied to phenomena as diverse as nuclear resonances, neural networks and black hole evaporation. Here we revisit an elega…
Information recovery from evaporating black holes
Samuel L. Braunstein, Saurya Das, Zhi-Wei Wang
We show that the apparent horizon and the region near of an evaporating charged, rotating black hole are timelike. It then follows that for black holes in nature, which invar…
Noether charge astronomy
Zhi-Wei Wang, Samuel L. Braunstein
Noether's theorem identifies fundamental conserved quantities, called Noether charges, from a Hamiltonian. To-date Noether charges remain largely elusive within theories of gravity…