castlegates said:
... When a big Bang advocate uses phrases like "when the universe was the size of a grapefruit", others cannot accept these advocates wish to say that the universe has no boundry, when they just use one to describe it.
That is where the popularizers mislead you. they should never have said "when the universe was the size of a grapefruit"
Personally I don't like grapefruit, but it would be OK if someone says "when the OBSERVABLE universe was the size of a grapefruit". Then there is no boundary, only an horizon. That means when all the stuff which we have so far gotten light from, which is just a part of the whole, could have been contained in a volume the size of a grapefruit.
Or, if they are not talking about the observable but about the whole thing---which we can only make inferences about by measuring curvature and by modeling what we are able to see----if they are talking about the whole thing then they shouldn't say grapefruit
because spatially the whole thing is normally assumed to be either infinite (and a grapefruit is not infinite) or else something like S
3 which we don't yet have a non-techie word for in English. The technical word is "three-sphere"-----or something else but those are the two leading pictures
The CMB is the end of the line ... is it not? Although we don't know if or when the last microwave enters our picture. We simply don't know.
Observationally the CMB is not the end of the line. Primordial neutrino background is almost certainly there and waiting to be observed when people get neutrino detectors that work in the right range.
The CNB neutrinos come from the first second. The CMB comes from when the universe was 380,000 years old.
If CNB neutrinos are NOT observed when detectors are built that should see them, then there will be a huge uproar in cosmology

. Not seeing them would have to cause a revolution.
If they are seen, then people can study the CNB spectrum and map it etc just like they study the CMB now and learn more stuff.
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In your post you oftentimes say "We simply don't know."
That is par for the course. Think about it. NO SCIENTIFIC THEORY IS EVER PROVEN TO BE TRUE. All that happens is that theories get continually tested and eventually they predict something that isn't observed and get proven false.
then an improvement replacement is devised which can withstand all the other tests plus that additional one.
it is a kind of darwinian thing---or a "last man standing" except it never ends.
survival of the best fit.
When I talk at Cosmology forum, I do the best I can to report the STANDARD COSMOLOGY CONSENSUS which is based on 1915 GENERAL RELATIVITY.
And I try to leave room for some improvements to General Relativity which are under development----quantum gravity.
Do I BELIEVE 1915 general relativity? Of course not! It has singularities, places where it breaks down. Therefore it can't be right and will eventually be replaced. (I guess if I have a belief it is in this process of testing and replacement where the laws and models are gradually improved.)
I don't have time to continually be telling you my philosophy of science, which includes a deep sense of the limitations of human knowledge. I'm very interested in what are the best models so far and I want to talk about that, not philosophy.
So when people come and say "what can we know?" :zzz: "how can we be sure, we are mere finite animals on a little planet?" I just find it boring and mostly ignore it. Skepticism doesn't tell me anything I don't know already.
The amazing thing is how well the models work.
What we get a lot of at PF is INCOMPETENT skeptics who are unable to see how well the standard LCDM model works because of a FAILURE OF IMAGINATION. Either they can't imagine a big bang with infinite spatial extent, or they can't imagine a three-sphere, or some mathematical thing just boggles them.
My attitude is I don't care if someone rejects the LCDM----I don't believe in the standard model myself. What I don't accept is when someone rejects the LCDM because of a damn GRAPEFRUIT.
We have an amazingly good provisional model that matches all kinds of data better than we had any right to expect, so I don't like to see it rejected
for the wrong reasons or out of simple ignorance.
If you understand the conventional mainstream model and then go off on your own and find some other model you like better that's fine. And about saying "we don't know" all the time---OF COURSE we don't know, just don't preach us sermons about it
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For me, the hottest thing in cosmology right now is the fact that Reuter has presented a model that gets just the right amount of inflation in the early universe without having to concoct any exotic "inflaton" field or arbitrary "slow-roll" potential. he gets the amount that people decided was needed to fit the data and he gets it without adding any JUNK.
he is also able to explain some other things. It is a minimalist approach that somehow gets a lot out of meager assumptions. He goes beyond 1915 GR, but only in a way that was well-established by people like Feynman in other branches of physics a long time ago. So only in a very careful conservative way. If you want to learn about cosmology beyond the conventional consensus LCDM, then my suggestion would be to forget this boring boundary business and look at stuff like Reuter that is happening in the field.