jonmtkisco
- 532
- 1
Hi Wallace,
I bought Hartle's textbook some months ago on your recommendation. I'm looking at Section 18.2 The Cosmological Redshift. As I read it, it seems to describe cosmological redshift only in terms of the size increase of the scale factor. I don't see any specific mention of an additional effect caused by the gravity gradient of the cosmic fluid's decreasing density over time. For example:
"In an expanding universe where a(t) grows with t, the ratio a(te) / a(t0) will be less than 1 and the received frequency w0 less than the emitted one we. That is the cosmological redshift. As the universe expands, the frequency of the photon decreases, and its wavelength increases linearly with the scale factor a(t)."
Section 9.2 describes gravitational redshift in terms of the Schwarzschild metric, but not in terms of the FLRW metric.
Can you please point me to Hartle's description of how the temporal gravity gradient of an FLRW cosmic fluid affects the cosmological redshift?
Jon
I bought Hartle's textbook some months ago on your recommendation. I'm looking at Section 18.2 The Cosmological Redshift. As I read it, it seems to describe cosmological redshift only in terms of the size increase of the scale factor. I don't see any specific mention of an additional effect caused by the gravity gradient of the cosmic fluid's decreasing density over time. For example:
"In an expanding universe where a(t) grows with t, the ratio a(te) / a(t0) will be less than 1 and the received frequency w0 less than the emitted one we. That is the cosmological redshift. As the universe expands, the frequency of the photon decreases, and its wavelength increases linearly with the scale factor a(t)."
Section 9.2 describes gravitational redshift in terms of the Schwarzschild metric, but not in terms of the FLRW metric.
Can you please point me to Hartle's description of how the temporal gravity gradient of an FLRW cosmic fluid affects the cosmological redshift?
Jon
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