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Science News March 1

🕑 Added 2023-03-01 16:00:09 +0000 UTC
Science News March 1

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Hi Jeffery, LambdaCDM is the current standard Big Bang cosmological model. Lambda is Einstein's cosmological constant (presumably caused by dark energy in the standard interpretation) and CDM is "cold" dark matter. "Cold" in this context just means that it moves much slower than the speed of light. Hot dark matter is ultra-relativistic (speeds near c) and warm dark matter has intermediate properties between the other two. LambdaCDM does a better job fitting observations and leading to the large scale structure in the universe than the other DM models, but it is deficient in many ways as well.

'LambdaCDM', yet another thing I hadn't heard of. I have cosmology books that I haven't gotten to and so much that I don't even know about. Life is too short, which explains specialization to a point.

Rad Antonov

Hi Tracey, thanks for all the explanations. Knowing the context really helps understand the competing explanations. It sure seems like JWST and other cosmological observatories are far more likely to deliver a discovery than any particle accelerator. To me, the biggest draw of DM was the hope to find it in a laboratory setting. Aside from an occasional anomaly, like the BOAT and a handful of other spurious observations, that hope is wearing thin.

I hadn't heard of MOND before Sabine, but had DM. I guess I see both existing together, at the same time, as just part of the process simply because reality is a bit more complicated. It's very interesting, reality shows something that we can't explain yet so there's work for scientists!

I grew up in the age of dark matter and we turned our noses up at those crazy MOND people while debating whether we would find DM as MACHOS or WIMPS. All of this MOND stuff is new to me too. One of the big criticisms of DM is that it needs to be artificially tweaked to fit observed phenomena. But, if the same level of tweaking will eventually be required of MOND, then it's no better. I don't have a horse in this race, but both horses in the race are currently lame.

Howdy, Tracey! I have never heard of TeVeS, but searching wikipedia turned this up (for others wondering about it): https://en.wikipedia.org/wiki/Tensor%E2%80%93vector%E2%80%93scalar_gravity But obviously, so far, MOND hasn't progressed past those problems. I was wondering, as a complete outsider, if there were any further developments.

TeVeS is the relativistic version of MOND (RMOND) that can explain gravitational lensing, but at this point in time there seems to be a lot of problems with it. For example it cannot simultaneously get galaxy rotation curves and lensing correct.

So, why haven't the LambdaCDM crowd packed up their bags and moved on? Well, there are several technical aspects to estimating galaxy mass that come into play. It looks like the group used a Salpeter initial mass function to estimate galaxy mass from measured stellar luminosity. The Salpeter IMF is an empirical relation derived looking at our local universe. We know that the early universe does not follow the Salpeter IMF, but we do not yet know the correct IMF to use. A "back-of-the-envelope" calculation using the Salpeter IMF is exactly the right thing to do and write a paper on, but recognize that this is not the final answer. As the paper notes, astronomers have a conundrum already with early star formation. When we measure the ages of globular clusters in the Milky Way, we find that they are as old as the universe, which implies star formation started earlier than cosmological models predict. If I recall correctly, both LambdaCDM and MOND struggle with the early star formation problem. To the extent that early galaxy formation is tied to early star formation, there is so much we just don't know. The paper also notes that they are using a Schechter function to estimate the density distribution of galaxies. Again, this function is derived using the local universe and may not be appropriate in the early universe. Until they see fit to do a JWST deep field (analogous to the Hubble deep field) the small, low surface brightness galaxy distribution in the early universe is not actually known (hypothesized, but not known). If these big galaxies are only the 1% tip of all early galaxies, then statistically, LambdaCDM is fine. If, however, these big galaxies are "common" in the early universe, then LambdaCDM has a big uphill climb. What's really great about all of this is that our sphere of ignorance about conditions in the early universe is shrinking fast and with JWST we may finally be able to break the degeneracy over whether LambdaCDM or MOND does a better job of explaining observed phenomena in the early universe. I'm salivating right now.

The assumption of mass-independent gravity (which was almost found by Albert in 1911) has similar results as MOND. But in contrast to MOND it can be deduced physically and it has so a foundation. And in contrast to MOND it does not have free parameters which have to be adapted.

1. As you discuss, the one problem with using brain organoids is that as brains were evolved to develop consciousness, the computers using these organoids could be conscious and therefore would be worthy of consideration as beings. This issue, consciousness, has been discussed in the AI community for quite some time, but as semiconductor based computers have no capacity for consciousness, I doubt that AI does either. There is a huge difference between an evolved biological system that has developed responses to sensory input and an algorithm that merely reduces the error between prediction and reality. 2. re: MOND: As a cosmologist, is there anything in MOND that can explain gravitational lensing?


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