Are they running out of gnomes?

Plasma and electricity in space. Failure of gravity-only cosmology. Exposing the myths of dark matter, dark energy, black holes, neutron stars, and other mathematical constructs. The electric model of stars. Predictions and confirmations of the electric comet.
BeAChooser
Posts: 1052
Joined: Thu Oct 15, 2015 2:24 am

Are they running out of gnomes?

Unread post by BeAChooser » Thu Jul 29, 2021 2:11 am

I've noticed longer and longer periods of time when there are no new announcements about dark matter.

Could they finally be running out of gnomes?

Michael Mozina
Posts: 2295
Joined: Thu Feb 23, 2012 5:35 pm

Re: Are they running out of gnomes?

Unread post by Michael Mozina » Thu Jul 29, 2021 2:13 pm

They are certainly running out of unique ways to justify their existing gnomes. Considering the fact that 95 percent of their so called "model" is based on dark magic, it's virtually impossible to *not* be able to fudge the numbers in their favor, regardless of what the observation might be. The problem is that they really have no laboratory justification for any of it, nor do they have much "hope" of ever finding such justification. Even their "magnetic reconnection" nonsense is simply *physically incapable* of producing a *sustained* particle acceleration process that might explain something like a sustained aurora, or a sustained full sphere corona in a real laboratory experiment. The whole mathematical basis of their cosmological model is devoid of empirical laboratory support and will always remain so. It's just a pathetic time to be a professional "astrologer", er, "astronomer".

Harry
Posts: 51
Joined: Sat Jun 12, 2021 2:29 pm

Re: Are they running out of gnomes?

Unread post by Harry » Sat Jul 31, 2021 9:26 am

The core of our sun is 99 % of the mass of the solar system.
98% of the universe is found in the cores of stars and Condensates (mimic black holes).
You may think this is new info.
Not really it has been discussed for decades.

arXiv:2107.13019 [pdf, other] astro-ph.HE
A broadband radio view of transient jet ejecta in the black hole candidate X-ray binary MAXI J1535-571
Authors: J. Chauhan, J. C. A. Miller-Jones, G. E. Anderson, A. Paduano, M. Sokolowski, C. Flynn, P. J. Hancock, N. Hurley-Walker, D. L. Kaplan, T. D. Russell, A. Bahramian, S. W. Duchesne, D. Altamirano, S. Croft, H. A. Krimm, G. R. Sivakoff, R. Soria, C. M. Trott, R. B. Wayth, V. Gupta, M. Johnston-Hollitt, S. J. Tingay
Abstract: We present a broadband radio study of the transient jets ejected from the black hole candidate X-ray binary MAXI J1535-571, which underwent a prolonged outburst beginning on 2 September 2017. We monitored MAXI J1535-571 with the Murchison Widefield Array (MWA) at frequencies from 119 to 186 MHz over six epochs from 20 September to 14 October 2017. The source… ▽ More
Submitted 27 July, 2021; originally announced July 2021.
Comments: This article has been accepted for publication in PASA. This article has 16 pages, 7 figures and 1 table

Research into Transient Condensates is cutting edge.
To understand the jets formed from these Transient Condensates is most important in explaining formations.

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