I Why is the DM density near the sun so small?

AI Thread Summary
The discussion centers on the surprisingly low dark matter (DM) density near the sun, estimated at 0.35 × GeV/cm3, compared to the average DM density in the universe of 2.26 × 10−24 g/cm3. This indicates that the local DM density is approximately 3.6 times lower than the universal average. A participant expresses difficulty in finding references to explain this discrepancy and seeks assistance from knowledgeable forum members. An error regarding the units of density was corrected, clarifying the average density in the universe is indeed 2.26 × 10−24 g/m3. The thread highlights a need for further exploration into the factors influencing local DM density.
Buzz Bloom
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This question arose in the context of another thread.
Wikipedia gives an estimated value for the DM density near the sun of
0.35 × GeV/cm3 = 6.2 ×10−25 g/cm3.​
The value of the average DM density in the universe
ρDM = 2.26 ×10−24 g/cm3.
https://en.wikipedia.org/wiki/Milky_Way - Bottom of list of Observation data​
This means that ρDM is approximately 3.6 times the density of DM near the sun.

I unsuccessfully have tried to find references that provide an answer to the question, but my skills are not up to the challenge. I am hopeful that one or more knowledgeable participants here the PFs can help me.

Regards,
Buzz
 
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The average density in the universe is 2.26*10-30 g/cm3, 4.5 orders of magnitude thinner than the local density. I guess you mixed cm3 and m3, as the number is equal to 2.26*10-24 g/m3.

http://pdg.ge.infn.it/2015/reviews/rpp2014-rev-astrophysical-constants.pdf
 
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Hi @mfb:
Thank you very much for spoting and letting me know about my careless error.

Regards,
Buzz
 
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