Gravitational Redshift: Units, Velocity & Ratio Explained

In summary, gravitational redshift is often expressed in m/s or km/s in physics papers as it is the equivalent velocity to produce the same redshift. This is often used in cosmology where redshifts are typically thought of in terms of recession velocities due to the expansion of the universe. The first accurate measurement of gravitational redshift was done in 1954 by Popper, and later in 1971 by Greenstein et al.
  • #1
Zman
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TL;DR Summary
gravitational redshift units seem to be given as a velocity and not as a ratio
I noticed in physics papers that gravitational redshift is expressed in m/s or km/s.
I assume that this must be the equivalent velocity to produce that same redshift.

So for example, if the gravitational redshift was measured as 3x10 -4 then;

z= v/c

3x10^-4= v/c

v = 9x10^4 m/s

v=90km/s

Is this what they are doing? Why do they prefer velocity over the ratio z?
 
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  • #2
Zman said:
I noticed in physics papers

Can you give an example?
 
  • #3
Hi,

This is from Wikipedia which refers to papers and gravitational redshift in km/s;
https://en.wikipedia.org/wiki/Gravitational_redshift

Initial observations of gravitational redshift of white dwarf stars
A number of experimenters initially claimed to have identified the effect using astronomical measurements, and the effect was considered to have been finally identified in the spectral lines of the star Sirius B by W.S. Adams in 1925.[1] However, measurements by Adams have been criticized as being too low[1][2] and these observations are now considered to be measurements of spectra that are unusable because of scattered light from the primary, Sirius A.[2] The first accurate measurement of the gravitational redshift of a white dwarf was done by Popper in 1954, measuring a 21 km/s gravitational redshift of 40 Eridani B.[2]

The redshift of Sirius B was finally measured by Greenstein et al. in 1971, obtaining the value for the gravitational redshift of 89±19 km/s, with more accurate measurements by the Hubble Space Telescope, showing 80.4±4.8 km/s.
 
  • #4
It looks like they are converting it to the equivalent Doppler shift.
 
  • #6
Zman said:
I assume that this must be the equivalent velocity to produce that same redshift.

Yes, as @Vanadium 50 says, they are giving the recession velocity that would produce a Doppler redshift the same as the observed gravitational redshift.

I don't think there's any deep reason for this; it was simply that cosmologists, who were the target audience of the papers mentioned in the Wikipedia article, were used to giving redshifts in velocity units because that is how they are typically thought of in cosmology--not so much because of the ordinary Doppler shift in flat spacetime, but because cosmologists are used to thinking of redshifts due to the expansion of the universe and interpreting them as recession velocities.
 
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1. What is gravitational redshift?

Gravitational redshift is a phenomenon in which light or other forms of electromagnetic radiation appear to have longer wavelengths when observed in a region with a stronger gravitational field. This is due to the effect of gravity on the frequency of the waves, causing them to stretch out and appear redder.

2. What units are used to measure gravitational redshift?

Gravitational redshift is typically measured in units of velocity, specifically meters per second (m/s). This is because the redshift is directly proportional to the velocity of the object causing the gravitational field, such as a massive star or black hole.

3. How is gravitational redshift related to velocity?

Gravitational redshift is directly proportional to the velocity of the object causing the gravitational field. This means that the greater the velocity of the object, the larger the redshift will be. This relationship is described by the equation z = Δλ/λ = v/c, where z is the redshift, Δλ is the change in wavelength, λ is the original wavelength, v is the velocity, and c is the speed of light.

4. What is the ratio in gravitational redshift?

The ratio in gravitational redshift refers to the ratio of the observed wavelength to the original wavelength. This is represented by the symbol z and is calculated using the equation z = Δλ/λ. The higher the value of z, the greater the redshift and the stronger the gravitational field.

5. How is gravitational redshift used in astronomy?

Gravitational redshift is an important tool in astronomy as it allows scientists to measure the velocity and strength of gravitational fields in distant objects. This can provide valuable information about the mass and structure of these objects, such as black holes. It is also used to study the expansion of the universe and to test theories of gravity, such as Einstein's theory of general relativity.

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