GW150914 Redshift: Cosmological & Gravitational

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In summary, the conversation discusses the cosmological redshift of GW150914 and the possibility of a gravitational redshift due to its close proximity to the merging black holes. The speaker also brings up the three distance regimes and the challenges of defining a gravitational redshift in the near field. They ultimately conclude that the gravitational redshift is likely already included in the calculations and cannot be separated out.
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Leo.Ki
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The cosmological redshift of GW150914 was estimated, but what about its gravitational redshift due to it having been produced so close to the merging black holes? I am expecting varying redshifts depending on where in the vicinity of the phenomenon each stretch of wave was created, and when during the evolution of the phenomenon, resulting in a complex redshift pattern. Thoughts?
 
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A gravitational redshift can only be defined in a stationary spacetime. We have three distance regimes here: (1) the near field, (2) far field, but small distances compared to cosmological distance scales, and (3) cosmological distances. Only if you look at things from the perspective of distances in the intermediate range do you see gravitational waves on a stationary background. I would assume that since the people doing the numerical relativity simulations were competent, they got all the effects right. Most likely they sampled the results of their calculation in region 2, and then used standard cosmological Doppler shifts to extrapolate from 2 to 3.

I doubt that your idea of conceptualizing the transition from region 1 to region 2 as a varying redshift will work. We simply don't have a way to define such a gravitational redshift so that it extends into region 1, where there is no stationary background.
 
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Thank you so much, Ben. I think I see clearer now. The waves being very probably calculated as part of the whole very dynamic gravitational environment, what I described naively as the gravitational redshift would already be included in the package and would not be something that can be clipped out of the equations.
 

Related to GW150914 Redshift: Cosmological & Gravitational

1. What is GW150914 Redshift?

GW150914 Redshift is the name given to a gravitational wave event that was detected on September 14, 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO). It is the first direct detection of gravitational waves, which are ripples in the fabric of spacetime, caused by the collision of two black holes.

2. What is the significance of the redshift in GW150914?

The redshift in GW150914 refers to the stretching of the light from the gravitational wave event as it travels through the expanding universe. This redshift can provide valuable information about the distance and speed of the source of the gravitational waves, as well as the expansion rate of the universe.

3. How does the redshift in GW150914 relate to cosmology?

The redshift in GW150914 is an important tool for studying cosmology, which is the study of the origins, evolution, and structure of the universe. By measuring the redshift, scientists can determine the distance of the source of the gravitational waves and use it to calculate the expansion rate of the universe and other cosmological parameters.

4. What is the relationship between redshift and gravitational waves?

Redshift and gravitational waves are both related to the theory of general relativity, which describes how gravity works in the universe. Gravitational waves are caused by the acceleration of massive objects, which can stretch and compress spacetime, resulting in the redshift of light. By studying the redshift of gravitational waves, scientists can gain a better understanding of the nature of gravity and the structure of the universe.

5. How is the redshift in GW150914 measured?

The redshift in GW150914 is measured using spectroscopy, which involves analyzing the light from the gravitational wave event using a spectrograph. This allows scientists to determine the wavelength of the light and calculate the redshift. The redshift is then used to calculate the distance and speed of the source of the gravitational waves and make inferences about the expansion of the universe.

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