High School Difference Between Redshifts of Massive Galaxies & Accelerating Galaxies

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The discussion centers on distinguishing between gravitational redshift from supermassive black holes and cosmological redshift in galaxies. Gravitational redshift varies across a galaxy due to the influence of a black hole, while cosmological redshift is uniform for the entire galaxy. Observations rely on measured wavelengths and the hydrogen spectrum to infer redshift, but the wavelength alone does not provide definitive information. The distance of galaxies from Earth can help differentiate their gravitational effects, with closer galaxies exhibiting stronger intrinsic gravitational attraction. Understanding these differences is crucial for interpreting redshift data in astrophysics.
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How can someone tell the difference between a super massive galaxy's redshift and a galaxy that is accelerating away?
 
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I don't understand the question - "super massive galaxy" is not a term I'm familiar with, and galaxies aren't typically accelerating.

Do you mean how can we distinguish between gravitational redshift from a super massive black hole and cosmological redshift? Because the gravitational redshift from a black hole at the core of a galaxy would be different across the galaxy, and insignificant beyond a barely noticeable fraction of the core. Cosmological redshift is the same for the entire galaxy.
 
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sqljunkey said:
How can someone tell the difference between a super massive galaxy's redshift and a galaxy that is accelerating away?
If you detect light you have one parameter: the measured wavelength. Any "redshift" is inferred from other factors, such as that you are observing a shifted hydrogen spectrum. There is, therefore, nothing inherent in the measured wavelength that tells you anything other than the measured wavelength.
 
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Say you observe same amount of red-shift for the two galaxies, observe distances of these galaxies from the Earth. The Shorter distance galaxy has stronger intrinsic gravity attraction, with the expanding universe considered.
 
In an inertial frame of reference (IFR), there are two fixed points, A and B, which share an entangled state $$ \frac{1}{\sqrt{2}}(|0>_A|1>_B+|1>_A|0>_B) $$ At point A, a measurement is made. The state then collapses to $$ |a>_A|b>_B, \{a,b\}=\{0,1\} $$ We assume that A has the state ##|a>_A## and B has ##|b>_B## simultaneously, i.e., when their synchronized clocks both read time T However, in other inertial frames, due to the relativity of simultaneity, the moment when B has ##|b>_B##...

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