Ray McCarthy
Sentient Marmite: The Truth may make you fret.
The universe doesn't expand as expected.
The galaxies rotate more like solid disks than Keplerian orbital systems.
There are a few other anomalies.
The solutions to make the observations fit the equations was to propose dark energy and dark matter.
Dark Energy
Dark Matter
Both Dark Energy and Dark Matter are essentially fudge factors to make the equations work. If there evidence they don't exist, then there is something wrong with observations, or the models/equations or something else we didn't think of applies. If you have more "Dark Matter" then you need more Dark Energy. Recent observations have been finding more stars obscured by dust in the Milky Way, two things to reduce the "Dark Matter". The space between the spiral arms has a lot of stars, just not as many as the visible spiral arms.
Recent Hubble Telescope observations suggest the current assumptions are wrong.
Hubble Constant
El Ref says "the boffins" have narrowed it down to three possibilities.
"We know so little about the dark parts of the universe, it's important to measure how they push and pull on space over cosmic history," said Lucas Macri of Texas A&M University in College Station, a key collaborator on the study, published in The Astrophysical Journal.
The galaxies rotate more like solid disks than Keplerian orbital systems.
There are a few other anomalies.
The solutions to make the observations fit the equations was to propose dark energy and dark matter.
Dark Energy
In physical cosmology and astronomy, dark energy is an unknown form of energy which is hypothesized to permeate all of space, tending to accelerate the expansion of the universe. Dark energy is the most accepted hypothesis to explain the observations since the 1990s indicating that the universe is expanding at an accelerating rate.
Assuming that the standard model of cosmology is correct, the best current measurements indicate that dark energy contributes 68.3% of the total energy in the present-day observable universe.
Dark Matter
Dark matter is a hypothetical type of matter composing the approximately 27% of the mass and energy in the observable universe that is not accounted for by dark energy, baryonic matter, and neutrinos. The name refers to the fact that it does not emit or interact with electromagnetic radiation, such as light, and is thus invisible to the entire electromagnetic spectrum. Although dark matter cannot be directly observed with conventional electromagnetic telescopes, its existence and properties are inferred from its various gravitational effects such as the motions of visible matter, via gravitational lensing, its influence on the universe's large-scale structure, and its effects in the cosmic microwave background. Dark matter is transparent to electromagnetic radiation and/or is so dense and small that it fails to absorb or emit enough radiation to be detectable with current imaging technology.
Both Dark Energy and Dark Matter are essentially fudge factors to make the equations work. If there evidence they don't exist, then there is something wrong with observations, or the models/equations or something else we didn't think of applies. If you have more "Dark Matter" then you need more Dark Energy. Recent observations have been finding more stars obscured by dust in the Milky Way, two things to reduce the "Dark Matter". The space between the spiral arms has a lot of stars, just not as many as the visible spiral arms.
Note that all this "Dark Matter" and "Dark Energy" is hypothetical although Wikipedia gives impression it's fact, they do point out that these things are hypothetical.Estimates of masses for galaxies and larger structures via dynamical and general relativistic means are much greater than those based on the mass of the visible "luminous" matter.
The standard model of cosmology indicates that the total mass–energy of the universe contains 4.9% ordinary matter, 26.8% dark matter and 68.3% dark energy. Thus, dark matter constitutes 84.5% of total mass, while dark energy plus dark matter constitute 95.1% of total mass–energy content. The great majority of ordinary matter in the universe is also unseen, since visible stars and gas inside galaxies and clusters account for less than 10% of the ordinary matter contribution to the mass-energy density of the universe.
Recent Hubble Telescope observations suggest the current assumptions are wrong.
Also here Universe's shock rapidly expanding waistline may squash Einstein flatRiess said:If we know the initial amounts of stuff in the universe, such as dark energy and dark matter, and we have the physics correct, then you can go from a measurement at the time shortly after the Big Bang and use that understanding to predict how fast the universe should be expanding today.
However, if this discrepancy holds up, it appears we may not have the right understanding, and it changes how big the Hubble constant should be today.
Hubble Constant
The Hubble constant, named after its discoverer American astronomer Edwin Hubble, is the rate at which objects in the universe expand over time. The new value is 66.53 (plus or minus 0.62) kilometers per second per megaparsec (3.26 million light-years). That means in 9.8 billion years the distance between cosmic objects will double.
El Ref says "the boffins" have narrowed it down to three possibilities.
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Firstly, our calculation on the effects of dark energy could be wrong. Dark energy, which can't be detected on current instruments, is already causing the expansion of the universe and may have additional properties that theorists haven't accounted for.
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The second option is that in the early period after the Big Bang, a new kind of subatomic particle burst out travelling at just under the speed of light. This would have sped up the expansion of the early universe and would explain the discrepancies in current theory.
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The third option is that Einstein's theories of gravitation are wrong, or at least in serious need of revision. That opens up a whole new can of worms.
"We know so little about the dark parts of the universe, it's important to measure how they push and pull on space over cosmic history," said Lucas Macri of Texas A&M University in College Station, a key collaborator on the study, published in The Astrophysical Journal.