Student Work
A Holographic Approach to the Hawking Effect for a Kerr-Newman Black Hole
PublicThis 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
- Publisher
- Identifier
- E-project-050522-164222
- 68406
- Keyword
- Advisor
- Year
- 2022
- Date created
- 2022-05-05
- Resource type
- Major
- Rights statement
Relations
- In Collection:
Items
Items
| Thumbnail | Title | Visibility | Embargo Release Date | Actions |
|---|---|---|---|---|
|
|
MQP-A Holographic Approach to the Hawking Effect for a Kerr-Newman Black Hole.pdf | Public | Download |
Permanent link to this page: https://digital.wpi.edu/show/xw42nc05b