SUMMARY
The discussion focuses on recreating the T-P plane from the article "Black Hole Joule-Thomson" using Mathematica. The user struggles with obtaining the correct graph and is advised to solve the pressure P directly instead of finding the horizon radius r_H. The equations provided, specifically P(r_H) and T(r_H), allow for direct plotting of T vs. P using ParametricPlot. The resulting graph shows discrepancies in peak amplitude and pressure values compared to the reference paper, necessitating a crosscheck of the user's notebook against the original article.
PREREQUISITES
- Familiarity with Mathematica for numerical computations
- Understanding of quintic polynomial equations and their solutions
- Knowledge of thermodynamic concepts related to black holes
- Experience with ParametricPlot in Mathematica for graphing functions
NEXT STEPS
- Learn how to use FindRoot in Mathematica for numerical root-finding
- Study the derivation of thermodynamic equations for black holes
- Explore advanced plotting techniques in Mathematica, particularly ParametricPlot
- Review the original article "Black Hole Joule-Thomson" for detailed methodology
USEFUL FOR
Researchers, physicists, and students interested in black hole thermodynamics, as well as Mathematica users looking to enhance their graphing and numerical solving skills.