Einstein & Lambda: 1917 Static Model Review

In summary, the paper "Einstein's 1917 Static Model of the Universe: A Centennial Review" discusses Einstein's motivation for adding the cosmological constant to his field equations and the controversy it sparked among his peers. While it allowed him to predict the expansion of the universe, he remained ambivalent towards it and it resurrected the issue of a static universe being unstable. The conversation also touches on the lack of viable theories against the observational evidence of an expanding universe without being overly complicated.
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Chronos
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This paper; https://arxiv.org/abs/1701.07261, Einstein's 1917 Static Model of the Universe: A Centennial Review, offers an informative insight into the mind of Einstein and, to large extent, his motivation for adding the cosmological constant to his field equations. Interestingly, both the introduction of lambda, and his subsequent repudiation, inspired controversy among from his peers. Though the basic idea had been around for decades, it had never been expressed quite so eloquently. The paper goes on to address the issues he was attempting to resolve with lambda. The jury is still out on whether or not it was justified. It is clear, however, Einstein was deeply ambivalent towards lambda for the remainder of his life. While lambda may have enabled Einstein to predict the expansion of the universe, it mainly served to resurrect an issue well known and argued since the time of Newton - that a static universe was unstable against gravitational collapse.
 
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I tend to sympathize with Einstein's dislike for a non-static universe. It really complicates an otherwise orderly and sensible universe. Are there any viable theories still standing against observational evidence of an expanding universe without being bent into a pretzel?
 
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Chronos said:
Are there any viable theories still standing against observational evidence of an expanding universe without being bent into a pretzel?

Not that I'm aware of.
 

What is the significance of Einstein & Lambda's 1917 static model?

The 1917 static model proposed by Einstein & Lambda was a modification to his theory of general relativity that introduced the concept of a cosmological constant, denoted by the Greek letter lambda. This model aimed to explain the stability of the universe and its expansion without altering the fundamental principles of general relativity.

How did the 1917 static model change our understanding of the universe?

The 1917 static model challenged the existing belief that the universe was either expanding or contracting. It proposed the idea that the universe could be both static and expanding at the same time, which was a significant departure from previous theories. This model also paved the way for the later discovery of the expanding universe and the concept of dark energy.

What evidence supports Einstein & Lambda's 1917 static model?

The primary evidence for the 1917 static model comes from observations of the cosmic microwave background radiation, which is the residual energy from the Big Bang. The model predicted that this radiation should have a specific temperature, which was later confirmed by observations. Additionally, the model's predictions of the universe's size and age were in agreement with later measurements.

Why did Einstein eventually abandon the 1917 static model?

In 1929, astronomer Edwin Hubble discovered that the universe was indeed expanding. This observation contradicted the static nature of Einstein & Lambda's 1917 model, and Einstein eventually abandoned it. He later referred to the introduction of the cosmological constant as his "greatest blunder," although it remains an essential concept in modern cosmology.

How does the 1917 static model relate to modern theories of the universe?

The 1917 static model was a crucial stepping stone in the development of modern theories of the universe. While it was ultimately disproven, it paved the way for the discovery of the expanding universe and the concept of dark energy. It also highlighted the importance of considering a cosmological constant in understanding the dynamics of the universe.

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