Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
freem
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Openai/6897769e-4ee4-800f-aba5-69cca34f701c
(section)
Add languages
Page
Discussion
English
Read
Edit
Edit source
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
Edit source
View history
General
What links here
Related changes
Special pages
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=== - A β Re-run the survey with alternate E0E_0E0β choices (proton radius, Planck length), and with higher nnn for plasma regions (e.g., 10βΆβ10Β²β° mβ»Β³). Produce new heatmaps and sample points. === * B β Keep Bohr-scale E0E_0E0β but explore a coherence-amplification factor (i.e., multiply per-event energy by a coherence factor to simulate plasma collective modes). * C β If you prefer to pursue the cosmological route: pick a realistic astrophysical region (e.g., dense plasma filament, solar corona, interstellar medium) and we compute whether QAT aggregate energy could be relevant there. * D β I can now try the next step you asked about earlier: derive a QAT-inspired stress-energy tensor from the surface-shell model (thin shell energy density) and show how it would plug into a simplified GR field equation (symbolically), keeping h/2Οh/2\pih/2Ο visible as you requested. Tell me which option you want and Iβll proceed. If you're unsure, I recommend A (different energy-radius scales + plasma densities) β it maps how robust the proposed mechanism is across physically relevant regimes.
Summary:
Please note that all contributions to freem are considered to be released under the Creative Commons Attribution-ShareAlike 4.0 (see
Freem:Copyrights
for details). If you do not want your writing to be edited mercilessly and redistributed at will, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource.
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)