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PhysicsCarl
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PhysicsCarl
@FlutterCarl
If MOND a₀ is connected to cosmological density (a₀ ∝ sqrt(ρ_c)), then a₀ must evolve with redshift as a₀(z) = a₀(0) × E(z), where E(z) = sqrt(Ω_m(1+z)³ + Ω_Λ).
Charlotte, NC شامل ہوئے Şubat 2021
1.4K فالونگ3.3K فالوورز

@BahramShakerin And here is what it all means. Would value your feedback.
github.com/carlzimmerman/…
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@BahramShakerin Sir if you like cosmic coordinators… what do you think of the zimmerman formula?

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[Mini-Course]
Cosmological Correlators: Theory and Phenomenology
Guilherme Pimentel
courses.ipht.fr/?q=en%2Fnode%2…
Recordings: youtube.com/playlist?list=…

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@pjungar @Anthony_Bonato I’ll be happy to be shown were I am wrong… please tear it apart
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@pjungar @Anthony_Bonato But the implications are gigantic if true yea or no
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@pjungar @Anthony_Bonato S8 tension solved. El Gordo solved. Happy to explain more
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@pjungar @Anthony_Bonato Yes but this isn’t fitting the data… it’s a derivation of cosmologic principals.. and it changes well.. everything
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@pjungar @Anthony_Bonato Is this not a novel derivation of Mond from first principals?
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@FlutterCarl @Anthony_Bonato I do not think you know what I meant by new mathematics.
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@pjungar @Anthony_Bonato Ok so where I pick up the Nobel Prize how does this work? I only took physics 101 but I did get a A so I’m somewhat credentialed
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@pjungar @Anthony_Bonato Here is my full research.. open to any and all feedback from a physics phd like yourself sir 🙏 github.com/carlzimmerman/…
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@pjungar @Anthony_Bonato Like very fast Mond at beginning and then slower but this is the rate of change based on cosmic density 🤝
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@sentefmi I have the answer potentially coming this afternoon.. will you take 5 minutes to review when I publish?
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@Anthony_Bonato In other news, physics has occasionally found that mathematics needs to extend into places it has not explored.
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@skdh My Mond derivation works well for clusters 🤝
PhysicsCarl@FlutterCarl
Physicists have spent 40 years and billions of dollars searching for dark matter particles. Zero found. Meanwhile this equation predicts galaxy dynamics to 0.03%: a₀ = cH₀/5.79 One line. Zero dark matter. Zero free parameters. Maybe try the math?
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Researchers from the University of Bonn in Germany have re-analysed observations of galaxy clusters and argue that much of the clusters’ “missing” mass may not be exotic dark matter but ordinary matter in the form of faint stellar remnants.
Galaxy clusters have long required about five times more mass than what is visible to explain the observed galaxy motions, an observation that is usually attributed to dark matter. But the authors combined gravitational lensing, X-ray, and optical data with models of star formation and found that the total mass in stars and their remnants could be almost twice as high as previously estimated.
This matters because Modified Newtonian Dynamics (MOND), an alternative to dark matter, seems to not work well for galaxy clusters. The discrepancy between the MOND predictions and the observations from galaxy clusters almost goes away with the new estimate, while dark matter no longer works all that well.
The Abell 209 galaxy cluster. Credits: ESA/Hubble & NASA, M. Postman, P. Kelly

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@pascalkwanten @skglearning What happens when the astrology numerology if you want to call it that… fits perfectly?
PhysicsCarl@FlutterCarl
Physicists have spent 40 years and billions of dollars searching for dark matter particles. Zero found. Meanwhile this equation predicts galaxy dynamics to 0.03%: a₀ = cH₀/5.79 One line. Zero dark matter. Zero free parameters. Maybe try the math?
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@skglearning Very tricky almost astrology/numerology IMHO...
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In 1937, Dirac formulated the hypothesis that the strength of gravity is inversely proportional to the age of the universe (G ∝ 1/t) and that the mass of the universe is proportional to the square of the universe's age (M ∝ t²) to explain the following coincidences.
#physics

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@Samuel_Gregson Mond acceleration scales with cosmic density. Where can I pick up my Nobel prize please?
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