Discussion Overview
The discussion revolves around estimating the number of Cosmic Microwave Background (CMB) photons in a volume of 0.25 liters. Participants explore theoretical approaches and mathematical relationships related to blackbody radiation and photon density.
Discussion Character
- Exploratory
- Technical explanation
- Mathematical reasoning
- Homework-related
Main Points Raised
- One participant mentions the total energy density of blackbody radiation as E = 4σ/C * T^4 and seeks guidance on applying this to find the number of CMB photons.
- Another participant suggests using the energy of a photon (E = hv) and performing an integral to derive the result.
- A third participant references a textbook by Barbara Ryden, stating that there are approximately 411 CMB photons per cubic centimeter in the universe today, but acknowledges not having access to the book.
- Some participants express confusion about how to derive the frequency of photons and calculate their number, with one noting that the photon gas wiki page provides a direct formula for number density as a function of temperature.
- There is mention of deriving the number density by integrating over the distribution of photons using Planck's Law.
- Another participant reiterates the energy density formula and suggests using E = mc^2 and Planck's relation to find the number of photons.
Areas of Agreement / Disagreement
Participants express varying levels of understanding and approaches to the problem, with no consensus on the method to derive the number of CMB photons. Confusion remains regarding the necessary steps and formulas.
Contextual Notes
Some participants highlight the need for specific assumptions regarding temperature and frequency, as well as the potential complexity of deriving the number density from first principles.