Undergrad Postulating a minimum gravitational field strength

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SUMMARY

This discussion centers on a paper proposing a minimum gravitational field strength and minimum acceleration, leading to the development of modified Newtonian dynamics and modified Newtonian gravity (MONG). The authors, Louise Rebecca, Arun Kenath, and C. Sivaram, extend their model to galaxy clusters, specifically the Virgo cluster, and find that their predictions align with observed radial velocities. Critics highlight the need for further validation through cosmic microwave background (CMB) data and express skepticism regarding the model's ability to accurately represent gravitational phenomena.

PREREQUISITES
  • Understanding of modified Newtonian dynamics (MOND)
  • Familiarity with cosmic microwave background (CMB) analysis
  • Knowledge of gravitational field strength and acceleration concepts
  • Experience with galaxy cluster dynamics and observational data
NEXT STEPS
  • Investigate the implications of modified Newtonian gravity (MONG) on galaxy cluster dynamics
  • Study the cosmic microwave background (CMB) temperature power spectrum in relation to dark matter models
  • Explore the impact of gravitational self-energy and dark energy on modified gravity theories
  • Review the historical context and predictions of MOND, particularly in relation to CMB observations
USEFUL FOR

Astronomers, physicists, and researchers in cosmology interested in alternative gravity theories and the implications of dark matter and dark energy in galaxy dynamics.

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TL;DR
postulating a minimum gravitational field strength postulating a minimum gravitational field strength (minimum curvature) and a minimum acceleration
this paper postulating a minimum gravitational field strength postulating a minimum gravitational field strength (minimum curvature) and a minimum acceleration but otherwise leaving Gr could reproduce MOND

[Submitted on 25 May 2022]

MONG: An extension to galaxy clusters​


Louise Rebecca (1,2), Arun Kenath (2), C Sivaram (3) ((1) Department of Physics, Christ Junior College, (2) Department of Physics and Electronics, CHRIST (Deemed to be University), (3) Indian Institute of Astrophysics)

The presence of dark matter, though well established by indirect evidence, is yet to be observed directly. Various dark matter detection experiments running for several years have yielded no positive results. In view of these negative results, we had earlier proposed alternate models by postulating a minimum gravitational field strength (minimum curvature) and a minimum acceleration. These postulates led to the modified Newtonian dynamics and modified Newtonian gravity (MONG). The observed flat rotation curves of galaxies were also accounted for through these postulates. Here we extend these postulates to galaxy clusters and model the dynamical velocity-distance curve for a typical cluster such as the Virgo cluster. The radial velocities of galaxies in the Virgo cluster are also obtained through this model. Observations show an inconsistency in the Hubble flow at a mean cluster distance of 17 Mpc, which is expected in regions of high matter density. This decrease in velocity is predicted by our model of modified gravity (MONG). The radial velocity versus distance relation for galaxies in the Virgo cluster obtained using MONG is in agreement with observations.


Comments:9 pages, 2 figures, 21 equations
Subjects: General Relativity and Quantum Cosmology (gr-qc)
Cite as:arXiv:2205.12793 [gr-qc]
 
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Yawnmaking. Here's their "evidence".
1654482387889.png
 
what is yawning their "evidence".
 
Yes @Vanadium 50 I think you should "elaborate" more on what you find yawnmaking. If you going to use the argument that you were already bored and that paper made you bored even more so you are bored to explain, then ok ...
 
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We will discuss it once it will be published.

Thread closed.
 
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Wake me up when they've run a simulation of the CMB temperature power spectrum using their model.
 
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World Scientific is real, albeit not high on the prestige list: impact factor of the journal in question is a whopping 1.5.

But does anyone seriously think the best fit to the data points is the curve I posted? With the dipsy-do in the midle?
 
page 3
they add both gravitational self-energy and dark energy to the poison equation to give rise to a MOND like physics

the gravitational self-energy add cosmological constant with reference 5-7 could reproduce many MOND like physics.

is this plausible
 
  • #10
Vanadium 50 said:
World Scientific is real, albeit not high on the prestige list: impact factor of the journal in question is a whopping 1.5.

But does anyone seriously think the best fit to the data points is the curve I posted? With the dipsy-do in the midle?
Maybe not, but it's not necessarily out of bounds for the model, and it enhances the model's falsifiability. Still, like I said, I don't have much interest in modified gravity models until they look at the CMB data, precisely because it's hard to explain the CMB with anything but dark matter and dark energy.
 
  • #11
Well, this shouldn't degenerate into a MOND thread, where the usual suspects will say the usual things. I will make three comments and then shut up.

1. A minimum gravitational field strength is exactly the same as a minimum gravitational acceleration. At best, this paper is playing with the functional form.
2. MOND did correctly prediect the 1st to 2nd peak ratio in the CMB. (McGaugh, 1999). So far as I know, this is the only correct prediction made by MOND in other-than-galactic scales.
3. The dipsy-do in the middle of the curve is absurd.
 
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  • #12
Vanadium 50 said:
Well, this shouldn't degenerate into a MOND thread, where the usual suspects will say the usual thing. I will make three comments and then shut up.

1. A minimum gravitational field strength is exactly the same as a minimum gravitational acceleration. At best, this paper is playing with the functional form.
2. MOND did correctly prediect the 1st to 2nd peak ratio in the CMB. (McGaugh, 1999). So far as I know, this is the only correct prediction made by MOND in other-than-galactic scales.
3. The dipsy-do in the middle of the curve is absurd.
The ratio of the first and second peaks in the CMB is uninteresting, as it can be explained by simply having a different baryonic matter density. It's the relationship between the first/second peak ratio and the second/third peak ratio that is the critical signal of dark matter in the CMB. Judging based upon the first and second peaks is rather like judging a 500-lap race from the winner of the first lap. Even though it's only one additional peak, the difference in explanatory power really is that stark.

Now, with the Planck data, even more peaks are measured to a very high degree of accuracy (I count seven peaks clearly visible in their power spectrum). Any competing model must accurately recreate the entire spectrum to be worth investigating further. That's a tall ask. But we have this very detailed data set that is extremely sensitive to dark matter density. Failing to take advantage of it when pursuing an alternative to dark matter is deeply suspicious.

This can be frustrating, because actually calculating the power spectrum from an alternative gravity model can be a difficult thing to do. But it really needs to be done. And the first two peaks alone don't cut it.
 
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