Quasars & Antimatter: Evidence of Abundance?

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    Antimatter Quasars
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Discussion Overview

The discussion revolves around the potential abundance of antimatter in the universe, particularly in relation to quasars and their high-energy emissions. Participants explore the implications of antimatter in explaining observed phenomena in distant galaxies and the nature of energy production in these regions.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that the absence of observed high-energy radiation anomalies indicates a lack of a balanced matter-antimatter distribution in the local universe, raising questions about the role of quasars in this context.
  • One participant proposes that the high-energy emissions from quasars could be linked to antimatter, potentially explaining the energy levels observed in distant galaxies and contributing to dark matter discussions.
  • Another participant argues that gravity alone can produce significant energy levels without the need for antimatter, challenging the necessity of antimatter in these processes.
  • There is a claim that quasars might produce antimatter rather than consume it, although this is presented as an unstudied opinion.
  • Concerns are raised regarding the implications of antimatter-matter collisions, with one participant questioning the feasibility of such collisions producing the expected energy signatures and characteristics.

Areas of Agreement / Disagreement

Participants express differing views on the role of antimatter in quasars and the energy dynamics of distant galaxies. There is no consensus on the necessity or implications of antimatter in explaining the observed phenomena.

Contextual Notes

Participants acknowledge various assumptions regarding the nature of energy emissions and the characteristics of antimatter interactions, but these remain unresolved within the discussion.

thebaron
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We know it is implausible that the local observable universe contains a near-balanced distribution of matter and antimatter because we fail to observe predicted anomalies of high-energy radiation brought about by spontaneous annihilation from matter-antimatter collisions on the borders of such antimatter regions. However, what about quasars, particularly high-energy gamma emitters? We may surmise that yes, this radiation is brought about by relativistic jets emitting Hawking radiation. But shouldn't the necessarily quantum nature of their production require at least some of this radiation to be composed of antimatter, at least in larger quantities than we observe locally? Combined with the fact we observe these severaly redshifted objects so far away, could we percieve this as evidence that antimatter may be more plentiful near the far fringes of the universe?
 
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Or perhaps a better articulation of what I mean is (tl;dr): could antimatter explain the ridiculous levels of energy we see in very distant and very active galaxies, and therefore account for a portion of very distant dark matter?
 
gravity is surprisingly good at producing 'ridiculous' amounts of energy without any help from antimatter.

quasars would be more likely to produce antimatter than consume it, in my unstudied opinion.
 
Yes, that is what I am saying. And antimatter-matter collisions on the border of these areas would emit the kind of energies we see.
 
thebaron said:
And antimatter-matter collisions on the border of these areas would emit the kind of energies we see.

Do you have any evidence for this? This sounds very unlikely to me - virtually everything would be different. The spectrum would be much harder, the durations would be much shorter, the area of emission would be more diffuse, and you wouldn't get jets.
 

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