Neutrinos | Leptons

Neutrino

A neutrino (/njuːˈtriːnoʊ/ new-TREE-noh; denoted by the Greek letter ν) is a fermion (an elementary particle with spin of 1/2) that interacts only via the weak interaction and gravity. The neutrino is so named because it is electrically neutral and because its rest mass is so small (-ino) that it was long thought to be zero. The rest mass of the neutrino is much smaller than that of the other known elementary particles excluding massless particles. The weak force has a very short range, the gravitational interaction is extremely weak due to the very small mass of the neutrino, and neutrinos do not participate in the strong interaction.Thus, neutrinos typically pass through normal matter unimpeded and undetected. Weak interactions create neutrinos in one of three leptonic flavors: electron neutrinos (νe), muon neutrinos (νμ), or tau neutrinos (ντ), in association with the corresponding charged lepton. Although neutrinos were long believed to be massless, it is now known that there are three discrete neutrino masses with different tiny values, but the three masses do not uniquely correspond to the three flavors. A neutrino created with a specific flavor is a specific mixture of all three mass states (a quantum superposition). Similar to some other neutral particles, neutrinos oscillate between different flavors in flight as a consequence. For example, an electron neutrino produced in a beta decay reaction may interact in a distant detector as a muon or tau neutrino. Although only differences between squares of the three mass values are known as of 2019, cosmological observations imply that the sum of the three masses (< 2.14 × 10−37 kg) must be less than one millionth that of the electron mass (9.11 × 10−31 kg). For each neutrino, there also exists a corresponding antiparticle, called an , which also has spin of 1/2 and no electric charge. Antineutrinos are distinguished from neutrinos by having opposite-signed lepton number and weak isospin, and right-handed instead of left-handed chirality. To conserve total lepton number (in nuclear beta decay), electron neutrinos only appear together with positrons (anti-electrons) or electron-antineutrinos, whereas electron antineutrinos only appear with electrons or electron neutrinos. Neutrinos are created by various radioactive decays; the following list is not exhaustive, but includes some of those processes: * beta decay of atomic nuclei or hadrons, * natural nuclear reactions such as those that take place in the core of a star * artificial nuclear reactions in nuclear reactors, nuclear bombs, or particle accelerators * during a supernova * during the spin-down of a neutron star * when cosmic rays or accelerated particle beams strike atoms. The majority of neutrinos which are detected about the Earth are from nuclear reactions inside the Sun. At the surface of the Earth, the flux is about 65 billion (6.5×1010) solar neutrinos, per second per square centimeter. Neutrinos can be used for tomography of the interior of the earth. Research is intense in the hunt to elucidate the essential nature of neutrinos, with aspirations of finding: * the three neutrino mass values * the degree of CP violation in the leptonic sector (which may lead to leptogenesis) * evidence of physics which might break the Standard Model of particle physics, such as neutrinoless double beta decay, which would be evidence for violation of lepton number conservation. (Wikipedia).

Neutrino
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What are Neutrinos?

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From playlist Science Unplugged: Neutrinos

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Why I Love Neutrinos

Why I Love Neutrinos is a series spotlighting those mysterious, abundant, ghostly particles that are all around us. This installment features a compilation of international scientists. For more information on neutrinos, visit the Fermilab website at http://www.fnal.gov.

From playlist Why I Love Neutrinos

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What is a Neutrino?

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From playlist MinutePhysics

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NOvA: Exploring Neutrino Mysteries

Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers. There is a live feed of the f

From playlist Neutrinos

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NOvA: Building a Next Generation Neutrino Experiment

The NOvA neutrino experiment is searching for the answers to some of the most fundamental questions of the universe. This video documents how collaboration between government research institutions like Fermilab, academia and industry can create one of the largest neutrino detectors in the

From playlist Neutrinos

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Neutrinos: Nature's Identity Thieves?

The oscillation of neutrinos from one variety to another has long been suspected, but was confirmed only about 15 years ago. In order for these oscillations to occur, neutrinos must have a mass, no matter how slight. Since neutrinos have long been thought to be massless, in a very real w

From playlist Neutrinos

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Neutrinos - Sixty Symbols

Billions of these mysterious particles are blasted down from the sun and pass through our bodies undetected. More videos at http://www.sixtysymbols.com/

From playlist Neutrinos - Sixty Symbols

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Neutrinos: Nature's Ghosts?

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 exp

From playlist Neutrinos

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The case of the missing neutrinos (Lecture - 04) by G Srinivasan

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From playlist Summer Course 2017: A Journey Through The Universe

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Neutrino Physics II - André de Gouvêa

Neutrino Physics II - André de Gouvêa Prospects in Theoretical Physics Particle Physics at the LHC and Beyond Topic: Neutrino Physics II Speaker: André de Gouvêa Date: July 19th, 2017

From playlist PiTP 2017

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Neutrinos: Messengers from a Violent Universe

In this 45-minute presentation Alex Himmel, Wilson Fellow at Fermi National Accelerator Laboratory, explains how neutrinos might provide the answers to many questions that scientists have about the universe. The neutrino is a type of subatomic particle. They are produced in copious quantit

From playlist Neutrinos

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Self-Interacting Neutrinos: Unified Path to Dark Matter and Cosmological Tensions by Mansi Dhuria

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From playlist LESS TRAVELLED PATH TO THE DARK UNIVERSE

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Neutrino Physics III - André de Gouvêa

Prospects in Theoretical Physics Particle Physics at the LHC and Beyond Topic: Neutrino Physics III Speaker: André de Gouvêa Date: July 21th, 2017

From playlist PiTP 2017

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Astrophysical neutrinos and how to find them – with Jenni Adams

The aptly named IceCube collaboration, a huge telescope buried in the crystal clear ice of Antarctica, has been running for 10 years. It’s there to detect neutrinos, an almost undetectable particle. Watch the Q&A: https://youtu.be/dWRlMEso_2E Join Jenni Adams as she discusses how these ne

From playlist Ri Talks

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Pilar Hernandez & Stefania Bordoni: Neutrinos Lecture 1/4 ⎮ CERN

Neutrinos remain enigmatic and elusive particles. They are invaluable astronomical and terrestrial messengers that have provided the first hints of physics beyond the standard model. Despite being the second most abundant particles in the universe, we still know little about them and futur

From playlist CERN Academic Lectures

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Neutrino Physics I - André de Gouvêa

Prospects in Theoretical Physics Particle Physics at the LHC and Beyond Topic: Neutrino Physics I Speaker: André de Gouvêa Date: July 18, 2017

From playlist PiTP 2017

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What Happened To All The Neutrinos?

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From playlist The Entire History of the Universe

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