This work uses holographic physics to compute the Hawking temperature for a Kerr-Newman black hole. Kerr-Newman black holes possess mass, angular momentum, and an electric charge. We start deriving the methodology by exploring the Unruh effect, we later extend this logic to consider black holes in the near horizon limit. Once the analytical models are derived, we simulate black hole evaporation for a variety of black holes.

• This report represents the work of one or more WPI undergraduate students submitted to the faculty as evidence of completion of a degree requirement. WPI routinely publishes these reports on its website without editorial or peer review.

Creator

• Aaron, William
• O'Mullan, Patrick

Publisher

• Worcester Polytechnic Institute

Identifier

• E-project-050522-164222
• 68406

Parola chiave

• General Relativity
• Holographic Principle
• Black Holes
• Semi-Classical Gravity
• Hawking Radiation
• Black Hole Evaporation

Advisor

• Ram-Mohan, L. Ramdas
• Olson, Sarah D
• Wills, Craig E.

Year

• 2022

Date created

• 2022-05-05

Resource type

• Major Qualifying Project

Major

• Physics

Rights statement

• In Copyright