The discussion centers on the relationship between cosmic microwave background (CMB) mass and dark matter, with skepticism about the idea that they correspond. The CMB consists of evenly distributed photons at a temperature of about 2.7 K, while dark matter is unevenly distributed, forming large clouds around galaxies due to gravitational attraction. The two phenomena do not align, as dark matter represents a significantly larger mass and behaves differently than the CMB photons. The conversation also touches on the CMB power spectrum, which supports the existence of dark matter. Overall, the notion of a direct correspondence between CMB mass and dark matter is deemed unlikely without a clear mechanism.