Robertus Maximus wrote: ↑Sat Mar 15, 2025 11:06 am
No mention of Birkeland currents!
As we are aware, the plasma cosmological model states that galaxies form from rotating Birkeland currents. Observable galaxies at all distances and directions will show a preferred direction rotation depending upon the nature of the Birkeland currents in that direction.
... snip ... The survey considered only 263 galaxies, an infinitesimally small number in an infinite universe!
That's an excellent point. In a sample that small, you could just happen to pick a set that would make you think the galaxies mostly spin in one direction, especially when a large number of galaxies in the field of survey were not included in the study because the methodology they used couldn’t detect the direction of rotation.
But even more likely, if you read the study report (
https://academic.oup.com/mnras/article/ ... ogin=false), you find it states … “The RA of the objects used in this study ranged from 53.01885 [degrees] to 53/2184 [degrees], and the declination ranged between -27.9145 [degrees] to -27.7292 [degrees].” In other words, the galazies weren’t taken from random locations in the sky but from one small area of the sky. It is more likely that Birkeland currents tend to run mostly in one direction or the other in a sample from only one small area of the sky.
Now they also measured the redshift of the galaxies used in the study. Their zs ranged from 0-0.5 to greater than 2. One graph divided them into 5 z brackets. I observe that about 70% of the sampled galaxies were in just two of the five z brackets (between z 0.5-1.5). I would imagine that galaxies at the same z in the same area of the sky might also tend to rotate in the same direction, thus being suggestive of Birkeland currents playing a role in the direction they rotate.
The RA and DEC of the 263 galaxies and their direction of otation is included in the study report (
https://academic.oup.com/view-large/506645363 and
https://academic.oup.com/view-large/506645364). They don’t provide the z for the data but the study does claim that the discrepancy in rotation is larger at higher z. Indeed, this chart of a large amount of data from SDSS (an earlier study) shows that at lower z, rotation direction seems to be close to random:
https://academic.oup.com/view-large/506645396 . Indeed a whole section of the paper is devoted to discussing previous studies that showed random direction of rotation. This study seems to be the first to suggest a major discrepancy.
The study report does mentions that previous work done with the DESI Legacy Survey found that from dataset of 1.3x10^^6 galaxies, that galaxies in certain areas of the sky tend to rotate one direction or another, although the difference one way or the other was much smaller than the JWST survey, which looked at the deeper Universe. Here’s the image showing preferred rotation direction from the DESI survey:
https://academic.oup.com/view-large/fig ... 2fig10.jpg.
The 263 galaxies (GOODS-S) came from a region of the sky where the tendency in the DESI study was to rotate clockwise (orange to red), but notice that there were equally large areas in DESI survey where the tendency was counterclockwise (blue to purple) and even larger areas (light green) where there was no tendency. Perhaps if they’d picked the 263 galaxies from the light green area they'd have concluded there is no discrepancy? Thus, it seems to me that without this latest paper, maybe there would be no-one thinking our universe is inside a black hole. So perhaps astrophysicists and the mainstream media should be cautious before making sweeping claims that sound ... well ... like nonsense. Just saying …