Wednesday, November 29, 2023

4245 - SPACE GRAVITY - how fast is?

 

-    4245   - SPACE GRAVITY  -  how fast is?     How can the universe expand faster than light travels?   It seems like it should be illegal.   The supreme iron law of the universe is that nothing can go faster than the speed of light.  Nothing further needs to be said about the issue, but here is more!

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--------------------------  4245  -   SPACE GRAVITY  -  how fast is?

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-   Some galaxies are moving away from us faster than the speed of light. What gives?

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-    We live in an expanding universe. Every day the galaxies get farther apart from each other, on average. There are slight motions on top of that general expansion, leading to instances such as the Andromeda Galaxy heading on a collision course for the Milky Way. But in general, in the biggest of pictures, the galaxies are getting farther away from each other.

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-   The objects  close to you would appear to move away with some speed, but the farther objects would appear to move faster.   The apparent stretch of space changes with distance.

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-     Edwin Hubble was the first to measure the expansion rate. The number he got was way wrong.  The more modern value is 68 kilometers per second per megaparsec.   One megaparsec is 1 million parsec, which is 3.26 million light-years.

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-    It means that if you look at a galaxy 1 megaparsec away, it will appear to be receding away from us at 68 km/s. If you look at a galaxy 2 megaparsec away, it recedes at 136 km/s. Three megaparsec away?  204 km/s. And on and on: for every megaparsec, you can add 68 km/s to the velocity of the far-away galaxy.

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-    So it's easy enough to compute: At some point, at some obscene distance, the speed tips over the scales and exceeds the speed of light, all from the natural, regular expansion of space.

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-   The movement of that galaxy can be interpreted as a "speed": you can measure the distance to it, wait awhile and measure it again. Distance moved divided by time equals speed.  The speed you measure can be faster than light.

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-    The notion of the absolute speed limit comes from “special relativity”, but who ever said that special relativity should apply to things on the other side of the universe? That's the domain of a more general theory,  “general relativity”.

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-   In special relativity, nothing can move faster than light. But special relativity is a local law of physics. In other words, it's a law of local physics. That means that you will never, ever watch a rocket ship blast faster than the speed of light. Local motion, local laws.

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-   But a galaxy on the far side of the universe? That's the domain of general relativity, and general relativity says that galaxy can have any speed it wants, as long as it stays way far away.

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-     Concepts like a well-defined "velocity" make sense only in local regions of space. You can only measure something's velocity and actually call it a "velocity" when it's nearby and when the rules of special relativity apply. Stuff  far away, like the galaxies doesn't count as a “velocity” in the way that special relativity cares about.

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- Another misintrepretation is that antimatter falls down, not up.  Physicists have shown that, like everything else experiencing gravity, antimatter falls downwards when dropped.

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-    This outcome is not surprising.  A difference in the gravitational behavior of matter and antimatter would have huge implications for physics.  Because gravity is much weaker than other ubiquitous forces such as electrostatic attraction or magnetism, separating it from other effects in the laboratory is a delicate affair. 

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-   Gravity is just so weak, you really have to be careful to get a good measurement.

Experiments aim to test whether gravity acts with the same strength on antimatter as it does on matter. Any tiny discrepancies could help to solve one of the biggest problems in physics. How the Universe came to be made almost exclusively of matter, even though equal amounts of matter and antimatter should have arisen from the Big Bang.

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-    In the world of antimatter, atomic nuclei are made of negatively charged antiprotons, orbited by positively charged antielectrons, or positrons. According to the standard model of particle physics, however, the opposite charges should be pretty much the only difference: particles and antiparticles should have nearly all the same properties.

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-    Experiments have confirmed that positrons and antiprotons have the same masses as their matter counterparts, within the limits of experimental errors.

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-    According to Einstein’s general theory of relativity, all objects of the same mass should weigh the same.  They should experience exactly the same gravitational acceleration.

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-    What would happen when the neutral atom antihydrogen was dropped.   It’s almost impossible to do an experiment with a charged particle, so antihydrogen is the perfect candidate.

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-    Antimatter particles are routinely created in laboratories.  Most particles produced by high-energy particle collisions are made in pairs, one particle of matter and its antiparticle. But it is hard to get antiparticles to combine into antiatoms because antimatter particles are typically very short-lived.

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-     When an antiparticle meets a particle, they both cease to exist and turn back into energy, in a process called annihilation. In a world made primarily of matter, this makes it hard for antimatter particles to find each other.

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-    CERN is currently the only place in the world where antihydrogen can be made. It has an accelerator that makes antiprotons from high-speed proton collisions, and a ‘decelerator’ called “ELENA” that slows them down enough to be held for further manipulation.

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-     Several different experiments feed off ELENA in CERN’s antimatter research hall. “ALPHA-g” is one of them, and it combines antiprotons with positrons it collects from a radioactive source.

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-    After making a thin gas of thousands of antihydrogen atoms, researchers pushed it up a 3-meter-tall vertical shaft surrounded by superconducting electromagnetic coils. These can create a magnetic ‘tin can’ to keep the antimatter from coming into contact with matter and annihilating.

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-    Next, the researchers let some of the hotter antiatoms escape, so that the gas in the can got colder, down to just 0.5 °C above absolute zero and the remaining antiatoms were moving slowly.

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-   The researchers then gradually weakened the magnetic fields at the top and bottom of their trap and detected the antiatoms using two sensors as they escaped and annihilated. When opening any gas container, the contents tend to expand in all directions, but in this case the antiatoms’ low velocities meant that gravity had an observable effect: most of them came out of the bottom opening, and only one-quarter out of the top.

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-    To make sure that this asymmetry was due to gravity, the researchers had to control the strength of the magnetic fields to a precision of at least one part in 10,000.

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-    The results were consistent with the antiatoms experiencing the same force of gravity as hydrogen atoms would. The error margins are still large, but the experiment can at least conclusively rule out the possibility that antihydrogen falls upwards.

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-   In 2010 scientists succeed at trapping antihydrogen for an extended time, and starting in 2016 they were able to measure how the antiatoms absorb light. But the gravity experiment required a new level of sophistication.

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-   No one would have expected antimatter to fall up because antiprotons are made of antiquarks, but these only constitute less than 1% of an antiproton’s mass: the rest is the energy that keeps them together.   Any violation, if it exists, cannot be over 1%.  Going beyond that would subvert not only the theory of gravitation, but also the standard model of particle physics.

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-    A third CERN experiment, called “AEgIS”, will attempt to measure the gravitational force on a beam of antihydrogen atoms in the absence of any magnetic fields. They will aim to reach 1% precision by first making positive antihydrogen ions (antihydrogen with an extra positron), which will help to cool the gas down to a fraction of a degree above absolute zero.

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-    Other efforts aim to measure gravity acting on positronium, a short-lived particle made of one electron and one positron orbiting each other. ALPHA-g itself plans to aim for 1% precision by letting antihydrogen atoms bump up and down and form a quantum superposition with themselves.

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-    The science goes on to understand the world we live in.  How does it work?

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November 27, 2023                  4242

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