SUMMARY
The discussion centers on calculating the temperature of a black body emitting photons at a frequency of 4 GHz, with a photon energy of 2.65E-24 J. Participants clarify the use of Wien's Displacement Law and the relationship between wavelength and temperature, emphasizing that the temperature can be derived by dividing the constant (b) by the wavelength (lambda). The correct wavelength was determined to be 0.075 m, leading to a calculated temperature of approximately 25.88 K, which is incorrect according to the participants, prompting further discussion on the methodology.
PREREQUISITES
- Understanding of black body radiation concepts
- Familiarity with Wien's Displacement Law
- Knowledge of photon energy calculations using Planck's Constant
- Basic physics of electromagnetic radiation
NEXT STEPS
- Study Wien's Displacement Law in detail
- Learn how to calculate photon energy using Planck's Constant
- Explore the relationship between frequency, wavelength, and temperature in black body radiation
- Investigate the limits of black body radiation equations in different energy spectra
USEFUL FOR
Students in physics, particularly those studying thermodynamics and electromagnetic theory, as well as educators looking for practical examples of black body radiation calculations.