What are the properties and characteristics of charginos?

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Discussion Overview

The discussion revolves around the properties and characteristics of charginos, particularly in relation to their potential as dark matter candidates, their stability, and their interactions with standard model particles. Participants explore theoretical aspects, definitions, and implications of charginos within the framework of supersymmetry.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants suggest that charginos are charged, fermion-like particles with a spin of 1/2, and question whether they are elementary particles.
  • There is uncertainty about the stability of charginos, with one participant stating they are not stable and decay promptly due to their mass.
  • Concerns are raised about the classification of charginos as dark matter candidates, with one participant arguing that their charge disqualifies them from being viable dark matter candidates.
  • Another participant mentions that charginos decay to supersymmetric particles and standard model particles, and that they cannot annihilate with standard model particles due to R-parity considerations.
  • Participants express frustration over the lack of accessible information regarding the fundamental nature of charginos and their interactions.

Areas of Agreement / Disagreement

Participants express differing views on the viability of charginos as dark matter candidates, with some asserting that their charge excludes them from this role, while others acknowledge the complexity of the topic without reaching a consensus.

Contextual Notes

There are unresolved questions regarding the definitions and characteristics of charginos, including their stability and potential interactions with normal matter. The discussion reflects a reliance on various sources, including Wikipedia, which some participants question for its validity.

jerich1000
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I understand that some lighter variants of the theoretical chargino are charged, with 1/2 spin, are possibly stable, are fermion-like, and are possible candidates for dark matter. Is a chargino an elementary particle?

(I thought that dark matter had to have no charge, else it could be detected by how it affects the electromagentic spectrum.)

What's hard about trying to learn about these particles is that there are 1000's of articles that talk "about" chaginos and neutralinos as if the reader already knows what they are. But I cannot find one that tells me what one "is." If I had enough of them would they form a solid? Do they annihilate when they come in contact with normal matter? These kinds of questions are ignored by articles I've found on the I-net. Is this because no one knows their answers?

Thanks
 
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The Dark Matter Supersymmetric candidates are neutralino dark matter (http://en.wikipedia.org/wiki/Lightest_Supersymmetric_Particle) , this consists of binos (http://en.wikipedia.org/wiki/Bino), neutral wino (http://en.wikipedia.org/wiki/Gaugino) and a neutral Higgsino (http://en.wikipedia.org/wiki/Higgsino) neutralinos are electrically neutral. These are good sources for information about Supersymmetric particles: http://en.wikipedia.org/wiki/Minimal_Supersymmetric_Standard_Model, http://en.wikipedia.org/wiki/Neutralino#Relationship_to_dark_matter
 
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Therefore Chargino's cannot be a dark matter candidate, given that they have charge?
 
Assumingly, yes, but my opinion is as considerable as everyone else's, especially since I'm relying on the validity of Wikipedia.
 
Thanks! Wikipedia still knows more than I (notice the correct English), so for a time I'll continue to admire is awesomeness.
 
Charginos are mixtures of charged higgsinos and winos. There are two charginos, called light and heavy. Their mass is higher than 103 GeV (LEP limit) but in many scenarios their masses are usually much higher than that. Now, about your questions. Charginos are not stable, they are heavy so they decay promptly. Due to R-parity they decay to susy particles + SM particles (never to SM particles only). Only lightest susy particle is stable and scenarios in which charginos are lightest susy particles are not acceptable phenomenologically. Also, they cannot annihilate with SM particles, because that would violate R-parity (but there are many other reasons).
 

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