Excluding the Standard Model from Dark Matter?

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SUMMARY

The discussion centers on the relationship between the Standard Model of Particle Physics and Dark Matter, particularly focusing on Weakly Interacting Massive Particles (WIMPs). It concludes that while the Standard Model does not include gravity, the absence of viable candidates for Dark Matter within it is due to the properties of known particles, not the lack of gravitational interaction. The conversation highlights that neutrinos, despite being potential candidates, are too light to account for Dark Matter. Ultimately, the existence of Dark Matter supports the pursuit of high-energy physics beyond the Standard Model.

PREREQUISITES
  • Understanding of the Standard Model of Particle Physics
  • Knowledge of Dark Matter and its properties
  • Familiarity with Weakly Interacting Massive Particles (WIMPs)
  • Basic concepts of gravitational phenomena, such as gravitational microlensing
NEXT STEPS
  • Research the properties and implications of Dark Matter in cosmology
  • Explore the role of neutrinos in the context of Dark Matter
  • Investigate theories of quantum gravity and their relevance to particle physics
  • Study high-energy physics beyond the Standard Model and its implications for Dark Matter
USEFUL FOR

Astronomers, physicists, and researchers interested in cosmology, particle physics, and the ongoing quest to understand Dark Matter and its implications for the universe.

Quds Akbar
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Usually, I like to bring up Dark Matter whenever I discuss cosmology or astronomy with someone, and whenever WIMPS (Weakly Interacting Massive Particles) are brought up, the person usually responds saying, "but there is no particle on the Standard Model that possesses all the particles of a WIMP"

And thinking about it now, all our observations on Dark Matter are mainly observed through phenomenon that depend on gravity, such as gravitational microlensing, such is the case for the rational velocities of galaxies that were much faster than calculated too, they all depend on gravitational phenomenons.

And considering that the Standard Model of Particle Physics has no full theory of gravity then it should logically be excluded from the game, the Standard Model in my opinion should not be considered (or at least not strongly considered) in "the quest for Dark Matter", so my question is: Is this idea logical?
 
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Quds Akbar said:
considering that the Standard Model of Particle Physics has no full theory of gravity then it should logically be excluded from the game

The Standard Model does not include gravity as an interaction; but it certainly does include particles that can be sources of gravity (all of them can, since anything with energy can be a source of gravity). So I don't understand what you want to "exclude" here. The fact that no known Standard Model particles are viable candidates for Dark Matter has nothing to do with the SM not including gravity as an interaction. It has to do with the fact that none of the known particles have the right combination of properties.
 
Quds Akbar said:
Usually, I like to bring up Dark Matter whenever I discuss cosmology or astronomy with someone, and whenever WIMPS (Weakly Interacting Massive Particles) are brought up, the person usually responds saying, "but there is no particle on the Standard Model that possesses all the particles of a WIMP"

And thinking about it now, all our observations on Dark Matter are mainly observed through phenomenon that depend on gravity, such as gravitational microlensing, such is the case for the rational velocities of galaxies that were much faster than calculated too, they all depend on gravitational phenomenons.

And considering that the Standard Model of Particle Physics has no full theory of gravity then it should logically be excluded from the game, the Standard Model in my opinion should not be considered (or at least not strongly considered) in "the quest for Dark Matter", so my question is: Is this idea logical?
Not really, because quantum gravity isn't likely to have any measurable impact on the nature or behavior of dark matter. Quantum gravity, if it is important at all, is only important for the densest of objects (black holes and maybe neutron stars). Dark matter doesn't experience hardly any friction, so it never collapses into dense objects.

In principle, the dark matter particle could have been a part of the standard model: neutrinos would be perfect candidates, if one or two of the three species of neutrino had enough mass. Unfortunately, they are just too light and thus both too high in temperature and comprising too little of the energy density of our universe to be a significant component of dark matter.

In a way, the existence of dark matter is a validation of decades of work on trying to look for high-energy physics beyond the standard model. One of the major issues with all attempts to bring together the standard model into a large symmetry group predict a large number of different particles that we do not observe. Dark matter might just be our first observational evidence that some of these predicted particles exist.
 

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