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/6921ae73-3700-8000-8ab7-90012976bb8a
(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!
=== Assistant: If the universe had stayed the same crazy Big Bang–level density instead of expanding and thinning out, then: === If the universe had stayed the same crazy Big Bang–level density instead of expanding and thinning out, then: Short version: : Let’s unpack that a bit. ==== Right after the Big Bang, the universe was: ==== * Insanely hot * Insanely dense * Filled with a glowing plasma of particles and radiation Today, things like atoms, molecules, stars, and planets exist only because: * The universe expanded * Expansion made it cool down * Cooling allowed: - Quarks → protons & neutrons - Protons + electrons → atoms - Atoms → gas clouds → stars → planets If density stayed the same (super high): * No real cooling. * Particles would be constantly smashed together at insane energies. * Atoms couldn’t form and stay stable. * Without atoms → no chemistry → no matter like rocks, water, DNA, etc. So right away: no people, no stuff, no “world” you could stand on. ==== At Big Bang-like density: ==== * Gravity is insanely strong because there’s a huge amount of mass–energy in any given volume. * If the universe didn’t expand to “relieve” that density, the whole thing would act like: - A mega–black-hole-like state - Or a constant near-singularity condition Spacetime would be so curved that: * Time might flow extremely strangely. * No stable “regions” like galaxies or solar systems could exist. * Light might not escape in any usual way; it would be constantly scattered or trapped. ==== Right now, space is mostly: ==== * Cold * Thin * Transparent → light from stars and galaxies can travel to us At early-universe density: * The universe was opaque — light kept bouncing off particles (like trying to see inside the Sun). * If it stayed like that: - There would be no “night sky.” - No clear line of sight across space. - Just a constant blinding energy fog of high-energy photons and particles. ==== Life needs: ==== * Stable atoms * Long timescales * Regions that are not instantly cooked, crushed, or shredded In a universe that never stops being that dense: * No long-lived stars with calm zones. * No stable planets sitting at nice distances. * No quiet, low-energy niches where complex chemistry can slowly build life. Everything is just ongoing chaos at max settings. ===== If the universe had stayed at its early Big Bang density instead of expanding: ===== * It would never cool enough for atoms to form. * It would stay a super-hot, ultra-dense plasma of particles and radiation. * No stars, no galaxies, no planets, no life. * Spacetime itself would be in an extreme, almost “broken-looking” state. So expansion + decreasing density isn’t just a detail — it’s literally the only reason there’s a universe with structure instead of an endless cosmic pressure cooker. If you want, we can flip it and ask: * What if the universe suddenly went back to that density right now? (spoiler: instant game over for everything).
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)