State of knowledge of dark matter distribution vs Fermi Paradox:Zoo

In summary, according to the information given, dark matter is not something that we know a whole lot about, but we do know that it is not just gas, and that it is not something that is easily clumped together.
  • #1
DanK66
5
0
A question for those of you who know about the distribution of dark matter in the galaxy:

Do we know how "clumpy" dark matter is? Can we tell yet whether dark matter is distributed about as densly as a gas or whether it's possible that there are the equivalent mass distributions that might contain "dark matter star systems"?

The reason I ask is that I'm curious if that it's possible that dark matter may end up to be purposely hidden star systems in order to effect the Fermi Paradox "they choose not to interact with us" hypothesis. Granted, we'd be talking about a > type 1 civilization on the Kardashev scale, probably a type II.

See http://en.wikipedia.org/wiki/Fermi_paradox#They_choose_not_to_interact_with_us

Dan K
 
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  • #2
DanK66 said:
A question for those of you who know about the distribution of dark matter in the galaxy:

Do we know how "clumpy" dark matter is? Can we tell yet whether dark matter is distributed about as densly as a gas or whether it's possible that there are the equivalent mass distributions that might contain "dark matter star systems"?

The reason I ask is that I'm curious if that it's possible that dark matter may end up to be purposely hidden star systems in order to effect the Fermi Paradox "they choose not to interact with us" hypothesis. Granted, we'd be talking about a > type 1 civilization on the Kardashev scale, probably a type II.

See http://en.wikipedia.org/wiki/Fermi_paradox#They_choose_not_to_interact_with_us

Dan K

Given that we are not sure what dark matter is (or if it is all the same substance). As far as density, astrophysicists have successfully predicted density gradients (for instance, most of it is in the halo), but I am not really certain how to apply that to your question.
 
  • #3
Dark matter is unlike ordinary matter. The particles virtually ignore one another [they are collisionless], as well as all other matter [i.e., no clumping]. Only gravity binds DM, and only in diffuse collections. Most of the dark matter in our galaxy is believed to reside in the galactic halo, as vociferous noted.
 
  • #4
vociferous said:
As far as density, astrophysicists have successfully predicted density gradients (for instance, most of it is in the halo), but I am not really certain how to apply that to your question.

Hmm, I guess that helps me organise my thoughts about the whole subject. Perhaps it supports the idea that DM could be cloaked star systems... If the DM was all in the core, that might be an unsuitable location for life due to radiation, I've read that out in the halo, heavier elements are not so common, so perhaps that might be a knock against my hypothesis. Although recently the idea of a "Galactic Habitable Zone" has been challenged, as stars can migrate great distances. So yeah I guess I'm no closer to knowing anything... Thanks for the information though :)

Dan K
 
  • #5
Chronos said:
The particles virtually ignore one another [they are collisionless], as well as all other matter [i.e., no clumping]. QUOTE]

We know this for a fact? or is this "if DM turns out to be WIMPS" ?

Dan K
 
  • #6
It is reasonably certain DM particles are collisionless.
 
  • #7
DanK66 said:
Hmm, I guess that helps me organise my thoughts about the whole subject. Perhaps it supports the idea that DM could be cloaked star systems... If the DM was all in the core, that might be an unsuitable location for life due to radiation, I've read that out in the halo, heavier elements are not so common, so perhaps that might be a knock against my hypothesis. Although recently the idea of a "Galactic Habitable Zone" has been challenged, as stars can migrate great distances. So yeah I guess I'm no closer to knowing anything... Thanks for the information though :)

Dan K

Explaining dark matter as burned-out stars (or in your case, "cloaked" systems) has been hypothesized, but that hypothesis started loosing ground a long time ago and is pretty much considered disproved, from what I have read. Only a fraction of the Milky Way's dark matter could possibly be explained by that hypothesis. While we do not know what dark matter is, we have some idea what it is not.
 
  • #8
Virial theory requires a huge amount of missing matter to explain galactic rotation curves and clustering of galaxies in the universe. Observational studies have virtually ruled out cold baryonic matter as a significant contributor to this missing mass. We have an enormous amount of observational data supporting this assertion. Links available upon request.
 
  • #9
Chronos said:
Observational studies have virtually ruled out cold baryonic matter as a significant contributor to this missing mass. We have an enormous amount of observational data supporting this assertion. Links available upon request.

Here is one...

http://en.wikipedia.org/wiki/Gravitational_microlensing

Also the notion that dark matter could mostly be clumps of something has been pretty much ruled out. Suppose the dark matter were clumps of something. If you stare at a distant object, then from time to time the dark matter clumps will pass in front of a quasar, and you'll see this dip in brightness as you see the clump bend the light of the quasar as a result of a gravitational field.

We came, we looked, we didn't see anything. So whatever dark matter is, it doesn't form large clumps.

Now the cool thing is that we can use this technique to find star systems.
 
  • #10
DanK66 said:
The reason I ask is that I'm curious if that it's possible that dark matter may end up to be purposely hidden star systems in order to effect the Fermi Paradox "they choose not to interact with us" hypothesis. Granted, we'd be talking about a > type 1 civilization on the Kardashev scale, probably a type II.

One problem with this idea is that dark matter affects the very, very early universe, which presumably evolved long, long before there was any sort of intelligent life (although it would make a really neat exercise in writing science fiction to imagine a situation where this constraint didn't hold, and you have an intelligent civilization form right after the big bang and evolve fast enough so that they could do cosmological stuff.)

Another possibility is that dark energy does create intelligent life forms, it's just that it's a type of intelligence that doesn't obviously look intelligent to us.
 
  • #11
twofish-quant said:
One problem with this idea is that dark matter affects the very, very early universe

In what way? Just gravitationally right? If so then it would have been uncloaked at the start, and then cloaked later with the same effect right?

Although this point kinda seems moot given that most of the above mentioned points tend to point away from the dark-matter-as-cloaked-star-systems hypothesis.

Thanks for all the input by the way everyone :)

Dan K
 
  • #12
DanK66 said:
A question for those of you who know about the distribution of dark matter in the galaxy:

Do we know how "clumpy" dark matter is? Can we tell yet whether dark matter is distributed about as densly as a gas or whether it's possible that there are the equivalent mass distributions that might contain "dark matter star systems"?

The reason I ask is that I'm curious if that it's possible that dark matter may end up to be purposely hidden star systems in order to effect the Fermi Paradox "they choose not to interact with us" hypothesis. Granted, we'd be talking about a > type 1 civilization on the Kardashev scale, probably a type II.

See http://en.wikipedia.org/wiki/Fermi_paradox#They_choose_not_to_interact_with_us

Dan K

Reality is a dream. However, the dream is incomplete and certain details are missing.
Aliens don't show up because they have not been included in this dream. It's as simple
as that. This is the reason for the Fermi Paradox.
 

1. What is dark matter and how does it relate to the Fermi Paradox?

Dark matter is a hypothetical form of matter that is invisible to telescopes and other instruments. It is believed to make up about 85% of the total matter in the universe and is thought to play a key role in the formation and evolution of galaxies. The Fermi Paradox is the apparent contradiction between the high probability of the existence of extraterrestrial civilizations and the lack of evidence for their existence. The presence of dark matter can affect the distribution of matter in the universe and potentially impact the development of intelligent life.

2. How is the state of our knowledge about dark matter distribution related to the Fermi Paradox?

The state of our knowledge about dark matter distribution is closely related to the Fermi Paradox because the distribution of dark matter can greatly impact the likelihood of the development of intelligent life in the universe. If dark matter is distributed in a way that is not conducive to the formation and evolution of galaxies, it could potentially hinder the development of advanced civilizations.

3. How do scientists study the distribution of dark matter?

Scientists study the distribution of dark matter through a variety of methods, including observations of the rotation of galaxies, gravitational lensing, and simulations of the evolution of the universe. These methods allow scientists to infer the presence and distribution of dark matter based on its gravitational effects on visible matter.

4. What is the current state of our knowledge about dark matter distribution?

The current state of our knowledge about dark matter distribution is still limited. While we have strong evidence for the existence of dark matter, its exact distribution and properties are still not fully understood. Scientists continue to study and gather data on dark matter in order to improve our understanding of its distribution and its role in the universe.

5. How does the distribution of dark matter impact the search for extraterrestrial life?

The distribution of dark matter can impact the search for extraterrestrial life in a few ways. Firstly, if dark matter is distributed in a way that is not conducive to the formation of galaxies, it could potentially limit the number of habitable planets in the universe. Additionally, the presence of dark matter could affect the development of advanced civilizations by influencing the formation of stars and the availability of elements necessary for life. Further research on the distribution of dark matter could provide valuable insights into the likelihood of finding extraterrestrial life.

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