Possible neutrino change.
The electron neutrino is formed by one energy quantum. This particle is characterised by mass wave which is unclosed.
Muon neutrino and tauon neutrino are only one particle. This particle is formed by unsymmetrical couple of energy quanta. This particle is characterised by two mass waves (unsymmetrical and unclosed) with length proportion 1:2. Such structure consequence is periodical energy change of particle with energies proportion 3:1 in dependence on time. Both time periods are identical and relatively long. This results of considerations on the theme the Theory of Everything.
The problem was that the Sun should output a lot more electron neutrinos then were measured. This meant that the model describing the interior of the Sun would be wrong, but it was working very well in predicting other things. It was finally solved when something called neutrino oscillation was discovered. It turned out that (this might be a bit technical) the interaction state of a neutrino was not equal to its mass or propagation state. In short, this meant that electron neutrino's could become muon or tau neutrino's after a while (and change back again after that). After this people began looking for muon and tau neutrinos coming from the Sun and together with the electron neutrino number they added up to the amount the Solar model predicted. The problem was thus solved; the Sun DOES output more electron neutrino's but some of these change into muon or tau neutrinos before they reach the Earth, and since we were initially only looking for electron neutrinos we missed some.
Neutrinos are a product of beta decay. Some number of protons and some number of neutrons are in the nucleus of an atom. When a neutron decays, it turns into a proton, an electron and a neutrino. The protons stays in the nucleus, while the electron and the neutrino escape.
Cherenkov radiation is used to detect neutrinos in high-energy physics experiments by observing the faint blue light emitted when neutrinos interact with water or ice. This light is produced when neutrinos travel faster than the speed of light in the medium, creating a cone of light that can be detected by specialized instruments.
The lightest known subatomic particle is the neutrino. Neutrinos have very small or even zero mass, making them incredibly light. They are electrically neutral and interact very weakly with other particles, making them difficult to detect.
0 - neutrinos are neutral, as the name suggests (it is latin for "little neutral one")
The problem was that the Sun should output a lot more electron neutrinos then were measured. This meant that the model describing the interior of the Sun would be wrong, but it was working very well in predicting other things. It was finally solved when something called neutrino oscillation was discovered. It turned out that (this might be a bit technical) the interaction state of a neutrino was not equal to its mass or propagation state. In short, this meant that electron neutrino's could become muon or tau neutrino's after a while (and change back again after that). After this people began looking for muon and tau neutrinos coming from the Sun and together with the electron neutrino number they added up to the amount the Solar model predicted. The problem was thus solved; the Sun DOES output more electron neutrino's but some of these change into muon or tau neutrinos before they reach the Earth, and since we were initially only looking for electron neutrinos we missed some.
Neutrinos are a product of beta decay. Some number of protons and some number of neutrons are in the nucleus of an atom. When a neutron decays, it turns into a proton, an electron and a neutrino. The protons stays in the nucleus, while the electron and the neutrino escape.
Cherenkov radiation is used to detect neutrinos in high-energy physics experiments by observing the faint blue light emitted when neutrinos interact with water or ice. This light is produced when neutrinos travel faster than the speed of light in the medium, creating a cone of light that can be detected by specialized instruments.
In fact, they were. The most recent and significant experiments to detect neutrinos include the T2K and SNO (soon to be SNO+) experiments.
Neutrinos are incredibly hard to detect so the "absence" of neutrinos doesn't mean they are not there. It was long thought that neutrinos did not decay. We now know they do so. Thus, the lower than expected number of neutrinos detected coming from the Sun has been fully explained. It took four decades but the problem is now fully resolved.
The tiny subatomic particle related to the electron that has no electric charge and little mass is the neutrino. Neutrinos are extremely difficult to detect due to their neutral charge and low interaction with matter.
The lightest known subatomic particle is the neutrino. Neutrinos have very small or even zero mass, making them incredibly light. They are electrically neutral and interact very weakly with other particles, making them difficult to detect.
Yes but not at much high level
Helium. The number two element. Fusion also generates a few neutrinos that are hard to detect.
0 - neutrinos are neutral, as the name suggests (it is latin for "little neutral one")
Neutrinos are elementary particles that travel close to the speed of light, lack an electric charge, are able to pass through ordinary matter almost undisturbed and are thus extremely difficult to detect. Neutrinos have a minuscule, but non-zero, mass that was too small to be measured as of 2007.
Neutrinos are interesting because they are extremely light, neutral particles that interact very weakly with matter, making them difficult to detect. They can provide valuable insights into fundamental physics and help scientists better understand processes in the universe, such as those occurring in stars and supernovae. Studying neutrinos can also shed light on the properties of dark matter and the early universe.