Abstract
One interesting property of black holes is that they obey thermodynamic laws. The entropy of black holes is given by the area of the horizon and it is naturally expected to be understood from the statistical mechanical viewpoint. However there has not been many things known about black hole microstates in the gravity, even though their holographic understanding has been well- known. In microstate geometry program which is a conjecture about black hole microstates, typical microstates are described as smooth and entropyless (i.e., horizonless) supergravity so- lutions which have the same mass, angular momentum, and charges as that of black holes. In this thesis, a new class of black hole microstates are suggested and studied in addition to the known microstate solutions and discussed in the context of microstate geometry program.
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