Discussion Overview
The discussion explores the hypothesis of whether dark matter could be explained as clouds of protons existing in space, particularly at 0 kelvins. Participants examine the implications of such clouds on electromagnetic radiation, charge interactions, and the visibility of these protons in the context of dark matter theories.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
- Technical explanation
Main Points Raised
- Some participants propose the existence of primordial clouds made strictly of protons at 0 kelvins, questioning their visibility and detectability due to the absence of electrons.
- Others argue that protons, being made of quarks, would not remain at 0 kelvins due to inherent kinetic energy, raising doubts about the feasibility of such clouds.
- Concerns are raised about the charge of these proton clouds, with some suggesting that they would exhibit a slight positive charge, which could lead to electromagnetic repulsion and expansion of the cloud.
- Participants discuss the interaction of protons with electromagnetic waves, noting that moving protons could emit electromagnetic radiation, while stationary protons at 0K would not.
- Questions are posed regarding the absence of electrons in the vicinity of these protons and the implications for electromagnetic wave generation and potential voltage.
- Some participants highlight that if protons were to account for dark matter, there would be observable effects on the interstellar medium and interactions with magnetic fields, which should produce detectable signals.
- Clarifications are made regarding the nature of electric and magnetic fields, emphasizing that both protons and electrons contribute to these fields, and that accelerating charges are necessary for electromagnetic wave emission.
Areas of Agreement / Disagreement
Participants express a range of views, with no consensus reached on the viability of proton clouds as a dark matter explanation. Disagreements persist regarding the physical properties and implications of such clouds, particularly concerning their charge, detectability, and interactions with electromagnetic fields.
Contextual Notes
Limitations in the discussion include unresolved assumptions about the behavior of protons at 0 kelvins, the implications of charge interactions, and the potential for electromagnetic wave generation in the absence of electrons.
Who May Find This Useful
This discussion may be of interest to those exploring theories of dark matter, the properties of protons, and the interactions of charged particles in astrophysical contexts.