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RyanH42
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Is Dark matter homogenenius in Universe ? I don't think so but I don't know any idea about it.
Thank you
Thank you
Do you think I"m making it up?RyanH42 said:I am talking about very very large scales.Not small distances.Is phinds idea true ?
The universe HAS no "radius" so that doesn't make any sense.RyanH42 said:Like universe radius distance.
You'll have to define your terms. The sand on a beach seems VERY homogenous looked at from a distance but if you hold a few grains in your had it doesn't look homogeneous at all.RyanH42 said:Isotrophic ok What about homogeneius ?.Or Isotrophy universe makes also homogeneius ?
You STILL have to define what YOU mean by "homogeneous". How much granularity is OK to still call it homogeneous?RyanH42 said:I am talking about large scales.
In the the universe dark matter distrubition homogeneius and isotrophic at the scale of observable universe radius ?
Yes, it is as isotropic as normal matter. They tend to go together at roughly the same ratio (about 5:1) in clumps we call galaxies.RyanH42 said:At least Homogeneius like the baryonic matter distrubition
Right ... that's why I've tried to stick with isotropic and have encouraged the OP to define and understand his terms and I have been specific about how I am using "homogeneous" (see post #11)Bandersnatch said:@phinds: be mindful of the terms you use. Homogeneity and isotropy are not synonymous, even though the large-scale distribution of dark as well as baryonic matter satisfies both.
Could you help me here? I am not interested in an image. I would like to have access to concrete data. Thanks!Bandersnatch said:And once again, google is your friend. That picture took maybe 5 seconds to retrieve.
Follow the link below the picture.Omega0 said:Could you help me here? I am not interested in an image. I would like to have access to concrete data. Thanks!
Dark matter is a type of matter that is believed to make up about 85% of the total matter in the universe. It does not interact with light and therefore cannot be directly observed, making it difficult to study. However, its presence is inferred through its gravitational effects on visible matter such as stars and galaxies. Understanding dark matter is important because it plays a crucial role in the formation and evolution of the universe.
Current theories suggest that dark matter is distributed in a homogeneous manner throughout the universe. This means that it is evenly spread out, with the same density in all regions of the universe. However, there are still ongoing studies and debates about the exact distribution of dark matter.
Observations of the cosmic microwave background radiation and the large-scale structures of the universe provide evidence for the homogeneity of dark matter. These observations suggest that dark matter is distributed in a uniform manner on a large scale, with variations only on smaller scales.
While the current understanding is that dark matter is homogeneous, there are some studies that suggest there may be small variations in its distribution. These variations are still under debate and further research is needed to fully understand the distribution of dark matter in the universe.
The homogeneity of dark matter is a crucial factor in the formation and evolution of galaxies. It provides the gravitational pull necessary for the formation of structures, such as galaxies and galaxy clusters. Without the presence of dark matter, the universe would look very different and the formation of galaxies would not be possible.