What is Neutron: Definition and 766 Discussions

The neutron is a subatomic particle, symbol n or n0, which has a neutral (not positive or negative) charge, and a mass slightly greater than that of a proton. Protons and neutrons constitute the nuclei of atoms. Since protons and neutrons behave similarly within the nucleus, and each has a mass of approximately one atomic mass unit, they are both referred to as nucleons. Their properties and interactions are described by nuclear physics.
The chemical properties of an atom are mostly determined by the configuration of electrons that orbit the atom's heavy nucleus. The electron configuration is determined by the charge of the nucleus, which is determined by the number of protons, or atomic number. The number of neutrons is the neutron number. Neutrons do not affect the electron configuration, but the sum of atomic and neutron numbers is the mass of the nucleus.
Atoms of a chemical element that differ only in neutron number are called isotopes. For example, carbon, with atomic number 6, has an abundant isotope carbon-12 with 6 neutrons and a rare isotope carbon-13 with 7 neutrons. Some elements occur in nature with only one stable isotope, such as fluorine. Other elements occur with many stable isotopes, such as tin with ten stable isotopes.
The properties of an atomic nucleus depend on both atomic and neutron numbers. With their positive charge, the protons within the nucleus are repelled by the long-range electromagnetic force, but the much stronger, but short-range, nuclear force binds the nucleons closely together. Neutrons are required for the stability of nuclei, with the exception of the single-proton hydrogen nucleus. Neutrons are produced copiously in nuclear fission and fusion. They are a primary contributor to the nucleosynthesis of chemical elements within stars through fission, fusion, and neutron capture processes.
The neutron is essential to the production of nuclear power. In the decade after the neutron was discovered by James Chadwick in 1932, neutrons were used to induce many different types of nuclear transmutations. With the discovery of nuclear fission in 1938, it was quickly realized that, if a fission event produced neutrons, each of these neutrons might cause further fission events, in a cascade known as a nuclear chain reaction. These events and findings led to the first self-sustaining nuclear reactor (Chicago Pile-1, 1942) and the first nuclear weapon (Trinity, 1945).
Free neutrons, while not directly ionizing atoms, cause ionizing radiation. So they can be a biological hazard, depending on dose. A small natural "neutron background" flux of free neutrons exists on Earth, caused by cosmic ray showers, and by the natural radioactivity of spontaneously fissionable elements in the Earth's crust. Dedicated neutron sources like neutron generators, research reactors and spallation sources produce free neutrons for use in irradiation and in neutron scattering experiments.

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  1. A

    Formation of Black Holes from Neutron Stars and White Dwarfs

    how is a black hole formed exactly from a neutron star or a white dwarf?? what is it? is it a star? is it defined as a matter?? and what happens when light gets sucked into it? there ought to be an increase in energy in it right? what happens to this energy?
  2. wolram

    Neutron stars seem an oddity to me

    neutron stars seem an oddity to me, they seem to have to much mass to size to be held together purly by gravity do neutrons have mutual attraction? or is space very very distorted by them?
  3. K

    Strange stars and neutron stars

    Do strange stars exist? Apparently they are denser than neutron stars and consist of up down and strange quarks. But are they theory or reality?
  4. R

    Why don't hydrogen atoms -> neutron + neutrino?

    Hey all, I'm a Theoretical Physics undergrad and so far I've only done one course in QM. Mainly playing with the TISE pushing wavefunctions around. Anyway after some trolling on here I've gotten to wondering, in a hydrogen atom why doesn't the electron just collapse into the nucleus? The...
  5. arivero

    Status of neutron magnetic moment?

    I believe to remember some recent comments about the measurement of neutron magnetic moment or some other quantity of this particle, which was not very well in agreement with standard model calculations. I can not remember which measurement it was, or when. Can anyone help my poor neurons?
  6. A

    Avg. density of neutron star

    Okay, I am told to find the average density of a neutron star with the same mass of the sun but with a radius of only 20km. I figured this would be pretty simple so I just would divide the Sun's mass (found using Google) by the volume of the neutron star which would be (4/3)*pi*r^3 with r being...
  7. A

    Detecting Neutrons: Simple Methods for Beginners

    Hello all I am new here, please pardon me if I have posted to the wrong board. My question should be fairly simple. I am building a fusor which I am hoping will generate neutrons from a D-D reaction. However, I have no way to detect them:frown: I was wondering if there are simple ways to...
  8. S

    Were in the neutron is the electron?

    Perhaps the proton is a spheare and the electron is a dot! Is the electron in the middle of the neutron?
  9. R

    Gravitation, neutron starlooks simple

    A neutron star is formed when a star has burned all its nuclear fuel and begins to collapse in upon itself. It then packs roughly the mass of our Sun into a region with the same radius as that of a small city while continuing to spin at very rapid rate. Let's say you have a neutron star with a...
  10. P

    Can We Create a Neutron Star in an Earth Lab?

    I heard, somewhere, that an thimble full of a neutron star would weigh on Earth many thousands of elephants. Hmmm... I suppose that this is true. But I wonder this: With all of our advanced technologies, is it possible to form such high density matter, even a thimble full, in an Earth lab?
  11. wolram

    Could New Pulsar Discoveries Lead to Direct Detection of Cosmic Gravity Waves?

    4 dec 2003. http://www.physlink.com/News/120403PulsarGravity.cfm A discovery made with CSIRO's Parkes radio telescope in eastern Australia may have brought forward the day when astronomers will directly detect cosmic gravity waves for the first time...
  12. Chi Meson

    Why can't a neutron be thought of as a proton plus an electron and neutrino?

    Wow. Clean slate! I like the format! And I've got a question. In elementary physics, it is said that the neutron can "sorta" be thought of as a proton plus an electron together. The mass of the neutron is slightly higher than a proton, by approximately the mass of an electron; in beta...
  13. P

    Coalescence between a neutron and a K+ meson

    I think it is simply the coalescence between a neutron and a K+ meson. What are your thoughts?
  14. radagast

    Neutron energies at which C14 is produced

    Some time back a friend (PhD Nuclear Engineer), told me that the energies a neutron needed to form C14 from nitrogen were (and this is where my memory gets real fuzzy) around 15 MEV. Furthermore that neither nuclear explosions or the Sun produced neutrons of this energy. The implications were...
  15. Nebula

    Magnetic Fields of Neutron Stars

    It is a known fact that neutron stars and pulsars, remnants of super nova explosions, have very strong magnetic fields. It is said that the collapse of the core amplifies the magnetic field of the progenitor. This is due to the fact that the magnetic fields lines are drawn closer together during...
  16. C

    Uncovering the Mystery of Neutron Decay and the Origins of the Universe

    If in a beta decay when a neutron decays into a proton,electron,and a anti nutrino,that the answer to where all the particles came from is not answer by this alone?the universe started with just neutrons,then half of them decayed into protons and electrons,and started the universes...
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