Is the Cosmological Constant the Same as Dark Energy?

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SUMMARY

The discussion centers on the relationship between the cosmological constant and dark energy, particularly in the context of the Lambda-CDM model of cosmology. Observations from 1998 regarding Type Ia supernovae indicated an accelerating universe, leading to a measured value of the cosmological constant, approximately 10−35 s−2. The cosmological constant, initially discarded by Einstein after the discovery of an expanding universe, has been reintroduced as a critical component of modern cosmological theories, representing an experimentally measured value rather than an arbitrary construct.

PREREQUISITES
  • Understanding of general relativity and its field equations
  • Familiarity with the Lambda-CDM model of cosmology
  • Knowledge of Type Ia supernovae and their role in cosmological measurements
  • Basic concepts of dark energy and its implications for the universe's expansion
NEXT STEPS
  • Research the implications of the cosmological constant in the Lambda-CDM model
  • Study the observational techniques used in measuring Type Ia supernovae
  • Explore the theoretical frameworks surrounding dark energy and quintessence
  • Investigate the historical context of Einstein's cosmological constant and its evolution in modern cosmology
USEFUL FOR

Astronomers, physicists, and cosmologists interested in the dynamics of the universe, as well as students and researchers exploring the concepts of dark energy and the cosmological constant.

FluffyFriend
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where unit conventions of general relativity are used (otherwise factors of G and c would also appear). It is common to quote values of energy density directly, though still using the name "cosmological constant".

What does this paragraph mean?

I read it somewhere that a relatively newer observation renewed the concept of "cosmological constant", and it was connected with "dark energy", again, can anyone provide detailed information on that?

Wasn't "cosmological constant" proved erroneous long ago?

Or is it something are now being called "cosmological constant", something other than "cosmological constant" itself? What is it, then?


Observations announced in 1998 of distance–redshift relation for Type Ia supernovae indicated that the expansion of the universe is accelerating. When combined with measurements of the cosmic microwave background radiation these implied a value of \Omega_{\Lambda} \simeq 0.7,[5] a result which has been supported and refined by more recent measurements. There are other possible causes of an accelerating universe, such as quintessence, but the cosmological constant is in most respects the most economical solution. Thus, the current standard model of cosmology, the Lambda-CDM model, includes the cosmological constant, which is measured to be on the order of 10−35 s−2, or 10−47 GeV4, or 10−29 g/cm3,[6] or about 10−120 in reduced Planck units.

How should I understand the word "economical" here?

I know it may be quite difficult to answer my question since I got the experience when trying to explain something to an outsider about the concept withing my speciality, so I start by telling the inquisitor whatever pertinent. I'm not trying to "teach" you how to explain this issue in any fashion (if I did made you feel so, I apologize), rather, this is just a personal suggestion, because I do not even know this question I'm asking is hard to begin with or not.

I hope my question is not so valueless. Any help will be appreciated, a paragraph, a link etc. Also, sorry for my english.
 
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FluffyFriend said:
What does this paragraph mean?

I read it somewhere that a relatively newer observation renewed the concept of "cosmological constant", and it was connected with "dark energy", again, can anyone provide detailed information on that?

Wasn't "cosmological constant" proved erroneous long ago?

Or is it something are now being called "cosmological constant", something other than "cosmological constant" itself? What is it, then?

This seems a little out of context to me but I'll try to provide what insight I can. Einstein added the cosmological constant term into his field equations for one purpose: to produce a static universe. After the realization that the universe was expanding, he saw no need for the cosmological constant term, and it was discarded as an ad-hoc construction.

When Dark Energy was discovered in the late 1990s, it is very convenient to formulate this extra repulsive force in exactly the same manner Einstein formulated his cosmological constant (an extra term in the field equations). However, the value is no longer cherry-picked to create a static universe, but is an experimentally measured value (I know of no successful theoretical predictions of its value).

Does that make sense?
 
Nabeshin said:
This seems a little out of context to me but I'll try to provide what insight I can. Einstein added the cosmological constant term into his field equations for one purpose: to produce a static universe. After the realization that the universe was expanding, he saw no need for the cosmological constant term, and it was discarded as an ad-hoc construction.

When Dark Energy was discovered in the late 1990s, it is very convenient to formulate this extra repulsive force in exactly the same manner Einstein formulated his cosmological constant (an extra term in the field equations). However, the value is no longer cherry-picked to create a static universe, but is an experimentally measured value (I know of no successful theoretical predictions of its value).

Does that make sense?


Yes it does! Thanks Nabeshin!

At least I know what "economical" means here. "If it's useful, get it back from the trashcan".

Further discussion is encouraged!
 

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