Final answer:
The cosmic background radiation, or CMB, represents the afterglow of the hot, early universe. The other photons from the Big Bang have redshifted due to the expansion of the universe and are undetectable in the microwave range where the CMB is visible.
Step-by-step explanation:
The cosmic background radiation, also known as the cosmic microwave background (CMB), is evidence of the Big Bang and represents the afterglow of the hot, early universe. This background radiation is detected in the microwave range and has a temperature of approximately 4K.
While the question asks about the other photons from the Big Bang, it is important to note that the CMB represents the photons emitted when the universe cooled enough for atoms to form, during the recombination era.
As for the other photons from the Big Bang, they have undergone continuous redshifting due to the expansion of the universe. This means their energy has decreased over time while their wavelength has increased, making them undetectable in the microwave range where the CMB is visible. Therefore, option A is correct: the cosmic background photons are continuously redshifting and become undetectable.