Evidence of Dark Matter within the Solar System?

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Discussion Overview

The discussion centers around the potential for studying dark matter within the Solar System, exploring both theoretical and experimental aspects. Participants reference conflicting articles regarding the presence of dark matter near the Sun and debate the feasibility of obtaining direct samples for study.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants highlight conflicting articles about dark matter's presence near the Solar System, questioning the possibility of direct study.
  • Others assert that dark matter is currently being studied through various methods, including underground detectors and particle colliders.
  • A participant proposes the idea of directly obtaining a sample of dark matter from the Solar System, prompting questions about the feasibility of such an endeavor.
  • Concerns are raised regarding the interaction properties of dark matter, particularly its lack of interaction with forces other than gravity, which may hinder sample collection.
  • Discussion includes the role of the Higgs field in providing mass to particles and questions how dark matter, which may not interact via the strong force, can have mass.
  • Some participants emphasize that dark matter's lack of electric charge implies it would pass through normal matter, similar to neutrinos, while others clarify that lack of charge alone does not determine interaction strength.
  • There is mention of various models of dark matter, including WIMPs and sterile neutrinos, and the need for further testing to understand their interactions.

Areas of Agreement / Disagreement

Participants express a range of views on the nature of dark matter and its study, with no consensus reached on the feasibility of obtaining samples or the implications of dark matter's interaction properties.

Contextual Notes

Participants note limitations in understanding dark matter's mass and interactions, as well as the implications of current observational data, which may not fully account for alternative theories.

  • #31
The idea I liked about detecting dark matter was to look for effects inside neutron stars. The gravity of the star would attract the dark matter and there are a great many neutrons there, so if the dark matter interacts weakly it should have some effect, perhaps on the viscosity.

The trouble is that this is at best a second-order effect. We would have to understand neutron star physics so precisely that deviations of the viscosity from the model would be significant, and we are a long way from that.
 

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