Black holes

Black holes are intriguing objects in general relativity which exhibit thermodynamic behavior and can be assigned temperature and entropy. Understanding its thermodynamic properties is a fundamental issue in black hole physics. Surprisingly, recently the study of black holes has also been relevant to explore the properties of realistic theories such as QCD, plasma and superconductors in the context of the gauge/gravity correspondence.
Black holes first appeared as classical solutions of general relativity. Almost a century ago, Schwarzschild presented the first explicit black hole solution. More general black hole solutions were only discovered much later. All black hole solutions have a point-like curvature singularity, which is separated from the outside world by a hypothetical surface known as the event horizon.
Low energy limit of string theory gives rise to gravity coupled to other fields. As a results these theories have black hole solutions. In this way string theory gives a framework for studying classical and quantum properties of black holes. Interestingly, study of them has led to new results in string theory.

My work in this direction

  • We study thermodynamic properties of dyonic black hole and its dual field theory. We observe that the phase diagram of a dyonic black hole in constant electric potential and magnetic charge ensemble is similar to that of a Van der Waals fluid with chemical potential. Phase transitions and other critical phenomena have been studied in presence of magnetic charge and chemical potential. We also analyse magnetic properties of dual conformal field theory and observe a ferromagnetic like behavior of boundary theory when the external magnetic field vanishes. Finally, we compute susceptibility of different phases of boundary CFT and find that, depending on the strength of the external magnetic field and temperature, these phases are either paramagnetic or diamagnetic.
    References: Suvankar Dutta, Akash Jain, Rahul Soni, "Dyonic Black Hole and Holography,"