Discussion Overview
The discussion revolves around the potential impact of intensely blue shifted cosmic microwave background (CMB) photons on Hawking radiation, particularly in the context of black holes. Participants explore theoretical implications, particle interactions, and gravitational effects related to this phenomenon.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants question the relevance of blue shifted CMB photons to Hawking radiation, suggesting that black holes are not currently evaporating due to the universe being warmer than them.
- There is a discussion on how a distant observer would perceive CMB photons as blue shifted when approaching a black hole, contrasting with red shifted photons emerging from a dense gravitational potential.
- One participant proposes that gravitational tidal forces could rip virtual particle pairs apart near a black hole, with one particle falling into the event horizon and the other remaining outside, potentially leading to observable annihilation events.
- Concerns are raised about whether incoming blue shifted CMB photons could interact with newly created electrons and positrons, potentially shortening their lifespan before they can annihilate.
- Another participant introduces the concept of "mass inflation" in the context of Reissner-Nordström black holes, suggesting that relativistic counter-streaming could destabilize the geometry near the inner horizon.
- There is mention of the differences in energy levels between gamma rays and CMB photons, with emphasis on how gravitational effects could alter their observed energies.
- Some participants express uncertainty about the implications of particle annihilation and the nature of energy release in these interactions.
Areas of Agreement / Disagreement
Participants express differing views on the impact of blue shifted CMB photons on Hawking radiation, with no consensus reached. Some argue that there is no significant effect, while others propose various interactions and consequences that remain speculative.
Contextual Notes
Participants acknowledge limitations in their understanding of particle interactions and the complexities of gravitational effects on photon behavior near black holes. The discussion includes references to theoretical frameworks and historical contributions to the topic.
Who May Find This Useful
This discussion may be of interest to those studying black hole physics, quantum mechanics, and the interplay between electromagnetic radiation and gravitational fields.