What Are the Properties of Dark Energy?

So, it is still a mystery.In summary, there has been progress in understanding the properties of dark energy, particularly in narrowing down the uncertainty range for the "w" parameter. This parameter, which describes dark energy's negative pressure and acceleration of expansion, is the key factor in connecting observations and predictions. However, there is still a confidence gap between the current estimate of w being -1 and the lower limit of -0.6. Possible explanations for dark energy include vacuum energy, but so far, attempts to measure it have not aligned with the observed amount of dark energy. Therefore, the true nature of dark energy remains a mystery.
  • #1
Theory Andy
Properties of "Dark Energy" ?

Has their been any progress in discovering what properties this Dark Energy might have?
 
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  • #2


Originally posted by Theory Andy
Has their been any progress in discovering what properties this Dark Energy might have?

Depends on what you think constitutes progress. For starters, the main feature of dark energy
cosmologists want to get a grip on is the "w" parameter
and according to Michael Turner's review they have made some progress in narrowing down the range of uncertainty about "w"

see for example
http://arxiv.org/astro-ph/0202007

section 3.5 "The Universe: The Lab for Studying Dark Energy"

"Present cosmological observations prefer w = -1, with a 95% confidence limit w < -0.6"
...
"A high-quality sample of 2000 supernovae distributed from z = 0.2 to z = 1.7 could measure w to within a precision &sigma;w = 0.05..."

section 3.4 "Parametrizing Dark Energy: For Now, It's w"

Here's my comment on Turner's survey article: OUT OF HUNDREDS OF QUESTIONS about dark energy that cosmologists could be asking the foremost question they want answered is what is the value of w, the parameter describing dark energy that most affects their models and the predictions about the universe---w is the parameter that determines the negative pressure that accelerates expansion (otherwise the expansion of space would be slowing down).

TURNER SAYS THEY'VE MADE SOME PROGRESS and can say based on observations of supernovae so far that with 95% confidence w is less than -0.6

they think it is -1.0

but there is a confidence gap between -0.6 and -1.0

to narrow it down to a sigma (stand. statistical deviation) of 0.05, he says, they would need to observe 2000 supernovae at moderate to high redshifts. That means getting observation time on expensive instruments like the Hubble space telescope and
whatever will be launched as its successor.

OK THIS SOUNDS VERY TECHNICAL, WHAT IS THIS W?

We have talked about the dark energy parameter w some already at PF and if you want we can discuss it some more. It is not hard to understand w, what it tells about dark energy and why they think it is -1.
There are a whole bunch other questions people can speculate about, but the key one for connecting observations and predictions is this w parameter. Ask more if you want to know more.

edit: your question made me look for more recent articles by Turner and others---there is an august 2003 survey article by him and Wendy Freedman that says they now can say w < - 0.8 with 95 percent confidence-----some improvement over the w < -0.6 I quoted from last year. The parameter w is called the "equation of state" for dark energy and is the ratio of its pressure to its
density.
 
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  • #3
Is it possible that the writer who suggests observations on 2000 supernovas is pointing to the fact that the accelerated expansion data came from a handful of supernovas and it's still ok to imagine the universe of last century?
Please consider looking at my post, CONTINUOUS CREATION in Theoretical Forum. I haven't learned to use symbols so the math is unruly---and unnecessary; it only shows that accepting the postulates precludes a fully developed black-hole. Note it is testable as it explains why galaxy arms spin fast.
 
  • #4
does dark energy=vaccum energy?
if it's true then why it has two names?
 
  • #5
Originally posted by loop quantum gravity
does dark energy=vaccum energy?
if it's true then why it has two names?

Perhaps. That is, vacuum energy is one candidate to explain dark enrgy, but we do not yet know whether it is the correct explanation. The biggest problem so far, as I understand it, is that all attempts to measure vacuum energy have come up with energy densities billions or trillions of times greater than the appearent amount of dark energy.
 

1. What is dark energy?

Dark energy is a hypothetical form of energy that is believed to make up approximately 70% of the total energy in the universe. It is thought to be responsible for the accelerated expansion of the universe and is characterized by negative pressure, causing a repulsive force between objects.

2. How is dark energy different from dark matter?

Dark energy and dark matter are two separate concepts. Dark matter is a type of matter that does not interact with light and makes up about 25% of the total energy in the universe. On the other hand, dark energy is a form of energy that does not interact with matter and makes up about 70% of the total energy in the universe.

3. How do scientists study dark energy?

Scientists study dark energy through various methods such as measuring the cosmic microwave background radiation, observing the large-scale structure of the universe, and analyzing the brightness of distant supernovae. These methods help to understand the effects of dark energy on the expansion of the universe.

4. What is the significance of understanding dark energy?

Understanding dark energy is crucial in piecing together the puzzle of the universe's evolution. It can also help explain the observed accelerated expansion of the universe and provide insights into the ultimate fate of the universe.

5. Is there a consensus among scientists about dark energy?

While there is no definitive answer to the nature of dark energy, most scientists agree that it exists and plays a significant role in the universe's expansion. However, there are ongoing debates and research to better understand this mysterious energy.

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