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!
=== Short answer: both approaches are useful. === * By introducing G early you pushed the work toward whether QAT can numerically account for gravity (ambitious but meaningful). The downside: G is a very constraining observable — so if your model's estimated ρQAT\rho_{\rm QAT}ρQAT is far off, the comparison can look discouraging. * Staying on the mathematical / local-physics path (the direction we just scanned) is a good first step: establish whether the aggregate of photon/electron events can plausibly give energy densities in any interesting range under realistic parameters. If the numbers can match, then coupling in G and curvature is the natural next step. So the strategy I recommend: # Continue local parametrized studies (like we just did), scanning scales and plasma densities and coherent amplification possibilities. # If you find parameter regimes where ρQAT\rho_{\rm QAT}ρQAT approaches cosmic or astrophysical density, then bring in G and attempt a QAT-to-GR mapping (e.g., plug ρQAT\rho_{\rm QAT}ρQAT into stress-energy in Einstein equations or into the QAT-inspired field equation you proposed).
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)