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JOB DESCRIPTION AND POSITION REQUIREMENTS:

The Department of Physics is seeking to hire a Part Time Research Intern. This individual will work with Dr. Sathyaprakash Bangalore on understanding spins of binary black hole merger remnants. Enhanced sensitivity of current and new gravitational-wave observatories will enable the study of a greater variety of binary black hole systems and, therefore, to test general relativity in sharper novel ways. In particular, there is an opportunity to test our understanding of the thermodynamic nature of black holes––a fundamental theoretical approach that has not been solidly connected to experiments yet. This project aims to use thermodynamics to better understand the spin magnitudes of remnants that form in the aftermath of binary black hole mergers of arbitrary spins. Numerical relativity simulations predict that the dimensionless spin of the remnant black hole, formed from the merger of a pair of equal-mass Schwarzschild black holes in a quasi-circular orbit, is approximately 0.69. For progenitor Kerr black holes with unequal masses, simulations also make a prediction of remnant spin that depends on the binary's mass ratio and spin orientations of black holes. Although post-Newtonian theory provides a plausible explanation of the remnant's spin magnitude, there are hints that there ought to be a more fundamental explanation. The researcher will formulate the problem in the language of black hole thermodynamics to gain a deeper insight into the process.

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