FRW Derivation History: Acker's Questions Answered

In summary, the Friedmann-Lemaître-Robertson-Walker metric, also known as the FRW metric, was derived to address the expansion of the universe. This cosmological equation was derived for this purpose and was later applied after Hubble's observations. It was derived using Newton's theory of gravity before Einstein's general relativity, but was also applied between general relativity and Hubble's observations. It is a fundamental equation in cosmology and has been extensively studied and debated. For more information, refer to the Wikipedia page on the FRW metric.
  • #1
Acker
4
0
Hello All,

I wondered if anyone could fill in some details about the timeframe of FRW derivation.
Was it derived to purposefully address the expansion of a universe? and if so, how did
anyone know about this prior to Hubble's observations?
Or was it derived for some other purpose and then applied after Hubble?
I am keenly interested in this and would love to hear any information in this forum
regarding the reasons for deriving this cosmological equation.

Regards
Acker

edit. And was it derived using Newton before Einstein's gr or between gr and Hubble's observations?
 
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  • #3
Thank you Phinds, for your thoughts on the matter.

When I am asked something, I tend to refrain from handing someone an encyclopedia
and quipping 'go look it up'.

It is such a relief that we can always turn to wikipedia for definitive discourse.


Best regards
Acker
 
  • #4
Folks who come here with questions are expected to have made at least some minimal attempt to do their own homework first, and it sounded as though had not done so.

I refer you to:

https://www.physicsforums.com/blog.php?b=3588
 
Last edited by a moderator:
  • #5


Hello Acker,

The Friedmann–Lemaître–Robertson–Walker (FRW) cosmological model was first derived by Alexander Friedmann in 1922 and independently by Georges Lemaître in 1927. This model describes the expanding universe and is based on Einstein's theory of general relativity.

At the time of its derivation, the concept of an expanding universe was not widely accepted or understood. However, Friedmann and Lemaître were able to derive this model by using Einstein's equations and applying them to the entire universe, rather than just the local region as was previously done.

It is important to note that Hubble's observations of the redshift of galaxies in 1929 provided strong evidence for an expanding universe, providing support for the FRW model. However, the model was not derived specifically to address the expansion of the universe. It was more of a natural consequence of applying general relativity to the entire universe.

Furthermore, the FRW model was derived using general relativity, not Newtonian mechanics. Einstein's theory of general relativity was published in 1915, before Hubble's observations in 1929. So the FRW model was derived using general relativity before Hubble's observations.

I hope this helps to answer your questions about the history and derivation of the FRW cosmological model. If you have any further questions, please don't hesitate to ask.

Best regards,

 

1. What is the significance of FRW Derivation History?

The FRW (Friedmann-Robertson-Walker) derivation history is important because it provides a mathematical framework for understanding the evolution of the universe. It helps us to understand how the universe has expanded and changed over time, and has been crucial in the development of modern cosmology.

2. Who is Acker and why are their questions important?

Acker is a theoretical physicist who posed a series of questions about the FRW derivation. These questions were important because they helped to clarify and improve our understanding of the derivation process, and led to further advancements in the field of cosmology.

3. What are the key components of the FRW Derivation History?

The FRW Derivation History is based on a few key components, including the Friedmann equations, which describe the expansion of the universe, and the Robertson-Walker metric, which is used to describe the geometry of the universe. Other important components include the cosmological constant and the Hubble parameter.

4. How has the FRW Derivation History evolved over time?

The FRW Derivation History has evolved significantly since its initial development in the 1920s by Alexander Friedmann and George Lemaître. It has been refined and expanded upon by many scientists over the years, including Albert Einstein and Edwin Hubble. It continues to be an active area of research and has led to many important discoveries about the universe.

5. What are some potential implications of the FRW Derivation History?

The FRW Derivation History has many potential implications for our understanding of the universe. It has helped us to better understand the Big Bang theory and the early stages of the universe, as well as the expansion and acceleration of the universe. It has also been used to make predictions about the future of the universe, such as the eventual fate of the universe and the possibility of a multiverse.

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