Dark Matter density given specific location
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Discussion Overview
The discussion revolves around the density of dark matter in relation to specific locations, particularly at a distance of approximately 4000 Mpc from Earth. Participants explore various methods for estimating dark matter density, the nature of dark matter, and its interactions with baryonic matter.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- Some participants suggest using the Navarro-Frenk-White (NFW) profile for estimating dark matter density, while others express skepticism about its applicability at 4000 Mpc.
- There is a discussion about whether dark matter exists in regions devoid of baryonic matter, with some arguing that dark matter tends to accumulate where baryonic matter is present.
- Participants propose that dark matter could theoretically exist in clusters without baryonic matter, although detecting such clusters would be challenging.
- One viewpoint posits that dark matter shapes the structure of galaxies, while another questions how dark matter and baryonic matter can coexist without direct interaction.
- Several participants discuss the potential for dark matter to interact via gravity and possibly the weak interaction, but they note that such interactions are minimal and not well understood.
- There is speculation about dark matter decaying into antimatter and the implications of such decay, with some questioning why such phenomena have not been observed.
- Participants highlight the uncertainty surrounding dark matter, suggesting that many possibilities remain valid due to the lack of concrete knowledge.
Areas of Agreement / Disagreement
Participants express multiple competing views regarding the nature and behavior of dark matter, particularly in relation to its interactions with baryonic matter and its potential detection methods. The discussion remains unresolved with no consensus reached.
Contextual Notes
Participants note limitations in current understanding, particularly regarding the interactions of dark matter and the conditions under which it may be detected. There are also references to unresolved mathematical steps and the dependence on various theoretical models.
Who May Find This Useful
This discussion may be of interest to researchers and enthusiasts in astrophysics, cosmology, and particle physics, particularly those focused on dark matter and its properties.
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RyanH42 said:I am doing research and I need to find the dark matter density of Galaxies or dust clusters (It can be any type of thing) which the distance from Earth will be ≅4000 Mpc.Here the picture
Think the radius of sphere.
I'm not sure how you would go about it from the Earth as a reference point, however the NFW profile will probably do from galactic center.https://en.m.wikipedia.org/wiki/Navarro–Frenk–White_profile
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https://en.m.wikipedia.org/wiki/Lambda-CDM_model which the Planck 2013 can be found here
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I want to give an example consider a massive star and a planet.And If planet is close enough to sun then the planet will be fall into the sun.So sun here DM and planet is BM.Dark matter curves space-time and makes a dense place.As this place DM attracts BM.So they must be interact somehow but there's not interaction ? Why I think there must be an interaction.Cause there's a force of gravity right.If Earth pulls meteorite,meteorite should fall into earth.So If BM fall this dense area then İt mmust be contact somehow with dark matter.
I hope I clarify myself
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Both attract each other.RyanH42 said:(This question can be also ask when BM attracts Dark matter-which I learned that's not possible- )
We have 5 times more dark matter than baryonic matter. It's like attaching an RC car to an actual car via a string. Sure, the RC car has its own motor, but the system will go in whatever direction the car moves.
Where is the problem? They interact via gravity and maybe via the weak interaction, but not via anything else. The weak interaction is negligible, and the interaction via gravity is relevant at the scale of galaxies only.RyanH42 said:My question will be how can dark matter and baryonic matter can be same place without any interaction.
The planet that falls into the sun is stopped there via the electromagnetic interaction. A dark matter particle will just move through the star and continue to fly through space, just with a slightly different direction due to gravity.
A tiny fraction of dark matter particles could interact via the weak interaction - that's what experiments on Earth try to see.
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In general we won't expect any interaction but somehow we expect a little bit interaction which we want to see in experimentsmfb said:A tiny fraction of dark matter particles could interact via the weak interaction - that's what experiments on Earth try to see.
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I'm not sure if scientists expect it or not, it's just something that we could theoretically observe, so they are checking on it. The weak interaction would cause the dark matter to decay, creating antimatter, which will produce a gamma ray photon of a very specific energy.RyanH42 said:In general we won't expect any interaction but somehow we expect a little bit interaction which we want to see in experiments
No one said dark matter is not expected to interact with anything, they only said it doesn't seem to interact with matter and the electromagnetic forces, which are a small fraction of the universe.
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How can this decay can be possible ? If DM decays anti mattter then we have to seen it already.But we didnt observe such a thing.I am wrong ?newjerseyrunner said:The weak interaction would cause the dark matter to decay, creating antimatter, which will produce a gamma ray photon of a very specific energy.
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Not sure, probably some assumed symmetries and conservation of certain quantum numbers. I'd not be the best to explain why this might be expected.RyanH42 said:How can this decay can be possible ? If DM decays anti mattter then we have to seen it already.But we didnt observe such a thing.I am wrong ?
Because dark matter is known because of it produces gravity, only things with mass produce gravity. Remember that matter is energy.RyanH42 said:Why it should be matter it can't be an energy ? A energy which never interects with matter ? Thats the reason why we can't see it ?
There is still way too much that isn't known to give you any good answers, when you are almost completely ignorant of something, all possibilities are valid. The whole thing could be an illusion caused by our formulas being wrong. Could be a fleet of Death Stars. All we can say is what it's not: It's not neutrinos, it's not black holes...
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Well, at least gravitationally it has to.newjerseyrunner said:It's possible for dark matter to not even interact with itself.
There are four main ways dark matter can be detectable:
- it could decay with a very long lifetime (much longer than the age of the universe - after all, it is still there) to known particles like photons, electrons, muons, quarks and so on. The decay has to be mediated by the weak force or some yet unknown mechanism, as the dark matter particles do not couple to the strong and electromagnetic interaction directly. The detection would happen via telescopes and particle detectors in space.
- it could annihilate with other dark matter particles. Not a decay in the strict sense, but it gives a signature very similar to decays. The "effective lifetime" depends on the dark matter density then, but it has to be much longer than the age of the universe again.
- it could interact with matter in underground detectors. The most likely interaction is elastic - we would just see a "kick" for some particle in the detector without a visible cause.
- it could be produced in particle accelerators. The detectors wouldn't detect the dark matter directly, but it would be notable as an imbalance in the observed transverse momentum of the visible particles (simplified: we see the recoil with known particles on one side, but not the produced dark matter going to the other side)
What do you mean with "if DM decays anti matter"?RyanH42 said:If DM decays anti mattter then we have to seen it already.
Why does it have to be a banana why can't it be yellow? Matter has energy, this is not "one or another".RyanH42 said:Why it should be matter it can't be an energy ?
This is not true. Energy is the source of gravity, not matter. Mass has energy, but light and motion has energy without mass.newjerseyrunner said:only things with mass produce gravity.
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The reason which I said that sentence.newjerseyrunner said:The weak interaction would cause the dark matter to decay, creating antimatter, which will produce a gamma ray photon of a very specific energy.
Matter has energy yes.But we are always thinking DM like a particle but maybe its not a particle.Think dark energy we seem it like an energy.The space-time vacuum energy.So maybe DM can be sort of something like that.
But I again you are righy I guess.My idea looks like stupid.
If there's anti DM, and DM decays antimatter, then If anti DM decays we will get matter.Which it explains why there's dark matter no anti DM and no anti mattet ?
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"Dark matter" is not grouped into matter and antimatter. Whatever is there is called dark matter. It could even be a particle that is its own antiparticle.
There are good indications that dark matter behaves like particles moving around.
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Thanks
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Maybe. We don't know.RyanH42 said:Yes DM decays to anti matter.
Maybe.RyanH42 said:I see If its even correct we cannit prove anyway.
Oh well, we know it exists and we can see its gravitational influence.RyanH42 said:We disnt even know "dark matter".
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It's also conceivable that dark matter simply won't fit in with the way we currently understand the universe. Considering that dark matter requires both gravity and some sort of particle physics, we may not be able to figure out what it is until we unify the theories. That's why I'm so excited by the prospects of LHC looking for it, if we could observe some of it's other effects it might give someone the insight required to create the next paradigm in physics. Dark matter may have gone through a completely different evolution after the gravity and the other forces split, it could have it's own weird forces too.
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It is unlikely that dark matter particles pop up in a theory that unifies gravity with the other forces. The energy scales just don't fit.
Any dark matter - dark matter interactions have to be weak (as in "not strong"), as DM doesn't clump in the same way matter does.
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mfb said:There are four main ways dark matter can be detectable:
- it could decay with a very long lifetime (much longer than the age of the universe - after all, it is still there) to known particles like photons, electrons, muons, quarks and so on. The decay has to be mediated by the weak force or some yet unknown mechanism, as the dark matter particles do not couple to the strong and electromagnetic interaction directly. The detection would happen via telescopes and particle detectors in space.
- it could annihilate with other dark matter particles. Not a decay in the strict sense, but it gives a signature very similar to decays. The "effective lifetime" depends on the dark matter density then, but it has to be much longer than the age of the universe again.
- it could interact with matter in underground detectors. The most likely interaction is elastic - we would just see a "kick" for some particle in the detector without a visible cause.
- it could be produced in particle accelerators. The detectors wouldn't detect the dark matter directly, but it would be notable as an imbalance in the observed transverse momentum of the visible particles (simplified: we see the recoil with known particles on one side, but not the produced dark matter going to the other side)
I guess it depends on how you define "detectable", but the primary ways to detect dark matter are (1) to infer them from the gravitational dynamics of ordinary matter particles that are observable, and (2) to observe when doesn't happen when gravitational dynamics are observed would lead to discernible interactions if caused by ordinary matter that isn't luminous (e.g. hydrogen gas in interstellar space or dust). You can tell a lot about the inferred velocity of dark matter particles and dark matter's inferred density per volume in particular places from these methods, particularly as you get to a fine toothed level such as looking at the dynamics of stars outside the main disk in a spiral galaxy.
While strictly speaking not different from (1), another technique is to assume that dark matter of a particular type exists, run a simulation of the universe's lifetime, see what the universe looks like, and compare it statistically to the universe we observe (basically on the theory that the closer your hypothesis is to reality the better the simulation will match the model).
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