Abstract
The spin $\frac{3}{2}$ perturbations of a rotating black hole are analyzed in the framework of linearized supergravity, expressing the complete solution of the Rarita-Schwinger equation in terms of a Debye potential. The equation governing the Debye potential is separated and the radial equation is transformed into a Schr\"odinger-type equation with a short-range potential from which the reflection and transmission coefficients can be calculated.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
