Sunday, March 8, 2020

NEUTRINOS - could they explain the Universe?

-  2657  -  NEUTRINOS  -  could they explain the Universe?  One of the universe's biggest mysteries: Why is there more matter than antimatter? That answer, in turn, could explain why everything from atoms to black holes exists.  Billions of years ago, soon after the Big Bang, cosmic inflation stretched the tiny seed of our universe and transformed energy into matter.
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 ---------------------   2657  -  NEUTRINOS  -  could they explain the Universe?
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-  Physicists think inflation initially created the same amount of matter and antimatter, which annihilate each other on contact.
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-  But, then something happened that tipped the scales in favor of matter, allowing everything we can see and touch to come into existence, and,  a new study suggests that the explanation is hidden in very slight ripples in space-time.
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-  If you just start off with an equal component of matter and antimatter, you would just end up with having “nothing“, because antimatter and matter have equal but opposite charge.  Everything would just annihilate.
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- Obviously, everything did not annihilate, otherwise I would not writing this.  Yo would ot be reading it.. The answer to or existence might involve very strange elementary particles known as “neutrinos“.  Neutrinos  do not have electrical charge and can thus act as either matter or antimatter.
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-  One idea is that about a million years after the Big Bang, the universe cooled and underwent a “phase transition“, very similar to how boiling water turns liquid into gas. This phase change prompted decaying neutrinos to create more matter than antimatter by some "small, small amount..
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-  Theoretical models and calculations have figured out a way we might be able to see this phase transition. They proposed that the change would have created extremely long and extremely thin threads of energy called "cosmic strings" that still pervade the universe.
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-  These cosmic strings would most likely create very slight ripples in space-time called “gravitational waves“.
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-  The strongest gravitational waves in our universe occur when a supernova, or star explosion, happens.  Strong gravity waves occur when two large stars orbit each other; or when two black holes merge. But the proposed gravitational waves caused by cosmic strings would be much tinier than the ones our instruments have detected before.
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-  When scientists modeled this hypothetical phase transition under various temperature conditions that could have occurred during this phase transition, they made an encouraging discovery: In all cases, cosmic strings would create gravitational waves that would be detectable.
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-   If these strings are produced at sufficiently high energy scales, they will indeed produce gravitational waves that can be detected by planned observatories.
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-  For a quarter of a century, Wolfgang Pauli’s prediction remained an educated guess. In 1930, the Austrian physicist predicted the existence of a ghostly new subatomic particle.
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-  After observing beta decay in a radioactive nucleus, Pauli noted that an undiscovered particle must exist to explain the resulting spectrum. During beta decay, a proton becomes a neutron by emitting a positron. But Pauli argued the nucleus also emitted an unknown electrically neutral particle. He thought this hypothetical particle had less than 1 percent of a proton’s mass.
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-  During the 1930s, Italian physicist Enrico Fermi investigated the problem and completed the work Pauli began. Fermi thought the weak nuclear force destabilized atomic nuclei and caused particle transformations. He called Pauli’s ghostly particle the neutrino, Italian for “little neutral one.”
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-  German physicist Hans Bethe was attacking the question of how stars shine. While investigating this question, Bethe realized that neutrinos played a key role. Fusion reactions in the Sun’s core create a torrent of neutrinos, a fraction of which passes through Earth eight minutes later. These evanescent particles carry with them a record of what happens inside a star.
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-   Normal matter comprises electrons and neutrinos, plus particles built from combinations of three quarks, like protons and neutrons. Exchanging force-carrying entities, like photons and gluons, gives rise to electromagnetism and nuclear forces.
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-  Neutrinos come in three types: electron, muon, and tau. But these elusive particles don’t interact much with other matter. Neutrinos can pass  through us, Earth, the Sun, or the super dense heart of an exploding star. While they exist in tremendous numbers, the challenge of neutrinos is detecting them. 
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-  In the 1950s, physicists Fred Reines and Clyde Cowan began a series of experiments to try. By the mid-1950s, their Project Poltergeist showed that it could be done. Their experiment picked up neutrinos by using a nuclear reactor as a source and a water tank as a detector, both sunk deep in a mine. 
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-  Although Bethe outlined the processes by which stars obtain energy through hydrogen fusion, many neutrino mysteries remain. For a long time, astronomers have known that the universe contains much more matter than the bright stuff we can see. They know this because they track galaxies moving in response to the gravitational pull of large amounts of material that neither emits nor blocks light, dark matter.
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-   Japan’s Super Kamiokande neutrino detector is a cylinder 130 feet wide and high. Light-sensors lining the water-filled tank hunt for neutrinos.  Could untold varieties of neutrinos account for much, or even all, of the dark matter astronomers believe is out there? Unfortunately, scientists now think the answer is no.
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-  Recent research suggests that while neutrinos do have mass, they do not have nearly enough to account for all the dark matter in the cosmos. Furthermore, neutrinos move at nearly the speed of light, meaning they won’t easily clump together like dark matter is observed doing in galaxies.
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-  Independent of neutrinos’ possible role as dark matter, the hard-to-catch particles may also help astronomers decipher how matter itself came to be. When the Big Bang occurred, matter and antimatter should have been created in equal amounts. And when matter and antimatter meet, they annihilate each other. If the amounts had been equal, then only radiation would have filled the universe.
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-  Why is there so much matter in the cosmos? Maybe neutrinos played a key role in the universe’s early asymmetry. If so, we owe our existence to them.
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-  Neutrinos surface in other cosmic mysteries, too. So, expect to hear a lot more about these strange particles as scientists continue to probe matter’s secret .  Stay tuned, there is a lot more to learn.
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-   March 8, 2020                                                                               2657                                                                                                                                                                                                                                 
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 ---------------------          Sunday, March 8, 2020    --------------------
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