SUMMARY
The equation of state (EOS) of radiation, specifically for photon gas surrounding a black hole, is established as P = 1/3 * energy density. This relationship arises from the derivation involving the momentum components and the EM Stress tensor, demonstrating that the pressure remains isotropic. The energy-momentum tensor for radiation is represented as T^{\mu}_{\nu} = diag(\rho, -p, -p, -p), confirming its perfect fluid nature. Recommended resources for further understanding include the textbook 'Gravitation' by Hartle.
PREREQUISITES
- Understanding of the equation of state in thermodynamics
- Familiarity with electromagnetic stress tensors
- Basic knowledge of general relativity concepts
- Proficiency in tensor calculus
NEXT STEPS
- Study the derivation of the energy-momentum tensor for radiation
- Explore the concept of isotropic pressure in general relativity
- Learn about the implications of photon gas in black hole physics
- Read 'Gravitation' by Hartle for foundational concepts in general relativity
USEFUL FOR
Physicists, astrophysicists, and students of general relativity seeking to deepen their understanding of the behavior of radiation in extreme gravitational fields.