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Neutrino madness

Pondering the infinitely large and small, … there’s the neutrino. Grok this:

“The sun is emitting neutrinos like mad, so that about a hundred trillion of them pass through your body every second , …” — Carroll, Sean (2016-05-10). The Big Picture: On the Origins of Life, Meaning, and the Universe Itself (p. 177). Penguin Publishing Group. Kindle Edition.

[Wikipedia] “About 65 billion (6.5×10^10) solar neutrinos per second pass through every square centimeter perpendicular to the direction of the Sun in the region of the Earth.”

So, I got out a ruler and drew a square on a piece of paper, each side 1 centimeter long. Which looked like less surface area than the nail on my little finger. Imagine seeing 65 billion things passing through that space. Like crazy invisible “hail ” everywhere. All the time.

And an amazing property: currently the neutrino’s speed is effectively the speed of light (within measurement error) and likely has non-zero mass! — maybe one millionth that of the electron [1]. And it comes in flavors. And maybe neutrinos do not interact with each other, just like photons.

As far as size, that’s spooky: “… , it does not have a size in the same sense as everyday objects.”

The saga continues with the Big Bang model and research on the cosmic microwave background; also the Standard Model of particle physics. Chasing the ghost particle.

[1] Neutrino mass inferred from “the experimentally established phenomenon of neutrino oscillation.”

3-7-2017 Supernova 1987A: “This was the first time neutrinos known to be emitted from a supernova had been observed directly, which marked the beginning of neutrino astronomy. The observations were consistent with theoretical supernova models in which 99% of the energy of the collapse is radiated away in the form of neutrinos.”

7 thoughts on “Neutrino madness

  1. So, how is neutrino flux determined? Where does the astounding figure of “65 billion neutrinos per second” come from? Measured or estimated? If measured, how? If estimated, based on what model?

  2. Historically, the neutrino is part of a fascinating chapter in the development of modern physics and our confidence in the Standard Model. Early 20th century studies of beta decay indicated possible violation of conservation of energy (and momentum). Even Niels Bohr hypothesized a real glitch in the law. Wolfgang Pauli, on the other hand, (in 1930) hypothesized an as yet unseen particle. That particle — the neutrino — was later experimentally confirmed (in 1956).

    Pauli … had opened the door to a whole new family of elementary particles— the neutrinos. That door is being flung open wider still as we type this paragraph: the subject of neutrinos is one of the hottest research topics in both particle physics and cosmology. We should add that experimentalists still often look for missing energy and momentum in their detectors in particle collisions, but this is always interpreted nowadays as evidence for a new particle, never as evidence for the breakdown of the conservation laws of energy and momentum [and charge]. Our … confidence … in the symmetries of the structure of space and time, and Noether’s theorem would, at this point, be very hard to shake. — Lederman, Leon M.; Hill, Christopher T. (2011-11-29). Symmetry and the Beautiful Universe (p. 109). Prometheus Books. Kindle Edition.

  3. Fermilab’s “Doc Don” presents an overview of the neutrino in this YouTube 5 minute video “Neutrinos: Nature’s Ghosts?

    Published on Jun 18, 2013
    Dr. Don Lincoln introduces one of the most fascinating inhabitants of the subatomic realm: the neutrino. Neutrinos are ghosts of the microworld, almost not interacting at all. In this video, he describes some of their properties and how they were discovered. Studies of neutrinos are expected to be performed at many laboratories across the world and to form one of the cornerstones of the Fermilab research program for the next decade or more.

    Neutrinos originate from nuclear reactions and the biggest nuclear reactor around is the Sun. The Sun emits so many neutrinos that even though it is about 93 million miles away, something like 650 trillion neutrinos from the Sun hit you every second. So suppose you wanted to shield yourself from that steady barrage of neutrinos. How would you do that? Well, if you took a huge block of solid lead that extended to the nearest star…and I’m not talking about the Sun, I’m talking about Alpha Centauri, which is about 5 light years away, you’d be able to block something like half the neutrinos from the Sun. If five light years of solid lead is such a poor shield, then there is no way that you can stop them…even if you used the entire Earth as your protection. Most neutrinos blow right through the planet like it’s not even there.

  4. The YouTube video of Nobel laureate Art McDonald’s public lecture “A Deeper Understanding of the Universe from 2 km Underground” at the Perimeter Institute for Theoretical Physics on April 13, 2016, provides a good overview of neutrino research. McDonald shared the 2015 Nobel prize in physics “for the discovery of neutrino oscillations, which shows that neutrinos have mass.” He presents an overview of his personal journey studying the “ghost particle” and establishig the underground research facility for that purpose.

  5. 7-22-2017 – Here’s an article about the latest planned advance in neutrino research: Creating the largest neutrino detectors in the world.

    A new era in neutrino physics in the United States is underway, and UW–Madison’s Physical Sciences Laboratory (PSL) in Stoughton is playing a key role.

    The Long-Baseline Neutrino Facility, home to the $2 billion Deep Underground Neutrino Experiment (DUNE), will eventually send particles 800 miles through the earth from a lab outside Chicago to a mile-deep detector in an inactive gold mine in the Black Hills of South Dakota.

    Neutrinos are little-understood, but their role in understanding matter and the dynamics of the universe is growing as science continues to learn more about the enigmatic particles through a constellation of new and exotic detectors, including the new DUNE experiment.

    Groundbreaking ceremonies for the Long-Baseline Neutrino Facility (LBNF) will be held simultaneously today at the Sanford Lab in South Dakota and at Fermilab in Illinois.

  6. Space.com posted another article yesterday about neutrino research at the IceCube lab in Antarctica: “Ghostly Cosmic Neutrinos Are Stopped Cold by Planet Earth, New Study Shows.”

    Researchers from the IceCube experiment in Antarctica announced this week that they have measured the rate at which high-energy neutrinos interact with regular matter instead of passing through unencumbered.

    “Understanding how neutrinos interact is key to the operation of IceCube,” Francis Halzen, a professor of physics at the University of Wisconsin-Madison and the IceCube principal investigator, said in a statement from the university.

    So, what makes some neutrinos so much more energetic? (How is the energy bundled differently? What does the Standard Model say?)

    Most of those neutrinos come from the sun, which releases a constant stream of low-energy neutrinos out into space.

    The neutrinos that IceCube is seeking — those from cosmic sources — are almost a million times more energetic than solar neutrinos.

  7. Sterile neutrino?

    Another update on neutrino research by Don Lincoln (Senior Scientist, Fermi National Accelerator Laboratory; Adjunct Professor of Physics, University of Notre Dame) in this Space.com article (June 19, 2018) [originally published on Live Science], “The 4th Flavor? Scientists Close in on a New Kind of Neutrino.”

    A study in 2001 conducted at the Los Alamos laboratory by a collaboration called LSND (Liquid Scintillator Neutrino Detector) stood out. Their measurement didn’t fit into the accepted picture of three different flavors of neutrinos. To get their results to make sense, they needed to hypothesize a fourth type of neutrino. And this wasn’t an ordinary kind of neutrino. It is called a “sterile neutrino,” which means that, unlike ordinary neutrinos, it didn’t feel the weak force. But it did participate in neutrino oscillation … the morphing of neutrino flavors. And it was probably heavy, which means that it was an ideal candidate for dark matter.

    And now we get to the recent measurement by the MiniBooNE [Mini BOOster Neutrino Experiment] experiment at Fermilab. …

    MiniBooNE scientists found that their data actually supported the LSND measurement and, further, if they combined their data with the LSND data, the statistical strength of the measurement is strong enough to claim a discovery … possibly of sterile neutrinos.

    So, how do we resolve this? How do we find out who is right? Well, this is science and, in science, measurement and replication win the argument.

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