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. C

    Who uses neutron moisture meters?

    Does anybody in PF-land use neutron moisture meters - the ones with Am-241/Be sources that probe into holes in the ground? If so, do you have a regime for regular wipe testing and leak testing? I am interested to find out if there are any cases of a wipe test result that showed contamination...
  2. humanino

    Neutron electric charge density

    I have not found a discussion open on this, and I would like to know if anybody has an opinion. My questions are triggered by the 0802.2563 arXiv paper (Meson Clouds and Nucleon Electromagnetic Form Factors by G. Miller). It has long been believed that the neutron electric charge density is...
  3. K

    What is the radial density distribution of a neutron star?

    Is there a simple-model equation for the radial density of a neutron star, from core to shell? I assume there have been models of fermionic gases, anyone have something onhand Is it a specific distribution? Linear? 1/r^2? I know its just a balancing of gravitational potential with strong...
  4. jal

    Neutron degenerate matter as dark matter

    I could not find much info on neutron degenerate matter. Only in reference to neutron stars. http://en.wikipedia.org/wiki/Degenerate_matter neutron degenerate matter Has anyone looked at the possible properties of a neuton liquid or solid to determine if it could act as dark matter? jal
  5. P

    Heat Transfer in Neutron Stars

    Not sure where to put this post, care more about what's happening on atomic scaI le so i put it here. I am currently taking Heat transfer for engineers and we were discussing the mechanicals for heat transfer, conduction, convection, raditation. In class my professor said that conduction is...
  6. CJames

    Neutron degeneracy pressure and electron degeneracy pressure

    The words neutron degeneracy pressure and electron degeneracy pressure are thrown around a lot when talk of white dwarfs, neutron stars, and black holes comes up. Despite this, I can't find a quantitative description of these critical pressures ANYWHERE. It is almost always described in terms of...
  7. B

    Neutron Star Mass: Understanding the Chandrasekhar Limit

    The Chandrasekhar limit (~1.4 Msolar) is an upper limit to the mass a white dwarf star. So this means we can not have a white dwarf star in nature that weighs more than this. But is it true that we can have a neutron star that weighs less than 1.4 Msolar? If so, this makes no sense to me...
  8. N

    Neutron Reaction: Calculating Total Cross Section

    Neutron Reaction? Now, I am doing a research about neutron reaction with many level of energy. With intermediate and high energy, I use optical model to calculate the total cross section of the reaction. But in the low energy, I can not do like that because I do not know about the parameters of...
  9. B

    Maximum Helium Fraction: Neutron Decay Time & Rest Mass Difference

    Suppose the neutron decay time n was 89 sec. AND the difference in rest mass between neutron to proton, Qn, was 0.129 MeV. What would the maximum Helium fraction, Yp, be?
  10. F

    Unravelling the Secrets of Neutron Stars

    Homework Statement "During most of its lifetime, a star maintains an equilibrium size in which the inward force of gravity on each atom is balanced by an outward pressure force due to the heat of the nuclear reactions in the core. But after all the hydrogen "fuel" is consumed by nuclear...
  11. malawi_glenn

    Understanding the Unbound Nature of the nn-Pair in Nuclear Clusters

    Why is the nn-pair unbound? I don't seem to find the answer in any of my textbooks =/
  12. M

    How Much Would You Weigh on a Neutron Star?

    Homework Statement Neutron stars, such as the one at the center of the Crab Nebula, have about the same mass as our sun but a much smaller diameter. If you weigh 675 N on the earth, what would be your weight on the surface of a neutron star that has the same mass as our sun and a diameter...
  13. H

    How to find neutron capture and fission cross section

    I'm writing a paper on Thorium utilization in nuclear reactors. In this connection I'm looking for figures which describe the neutron capture and neutron fission cross sections over a wide energy range (not only thermal). There are probably some online resources unbeknown to me, any hints?
  14. T

    Gamma energies from fast neutron activation.

    I've looked around and not found any good sources on the gamma energies from fast neutron activation. I need to find the characteristic gamma rays for an MCNP project and currently, I'm relying on energies I get from running some simple cases I set up for the element of interest. Does anyone...
  15. D

    Fusion of Neutrons and Hydrogen Nucleus: Mechanism and Possibility Explained

    It never occurred to me until now why instead of using two charged protons to fuse together, rather fuse neutrons to a hydrogen nucleus. Yes, it seems like cheating the system and therefore that's why I've not heard about this before, but what is the exact mechanism that prevents this from...
  16. T

    How Does Neutron Diffusion Theory Apply to Slab Reactors with Reflectors?

    It's part of my homework to find an analytical solution to a slab reactor with a reflector. The setup of the core is two slabs of equal thickness (-a to 0 and another 0 to +a) but different values for the diffusion coefficent, macroscopic absorption cross sections, and \nu \Sigma_f. There is a...
  17. M

    Neutron Interactions: Collisions & Absorption

    At a macroscopic level it appears that when two objects collide, they physically interact and the atoms touch. However the charges of the electrons actually repel one another and they don't physically touch. Correct? A neutron however has no charge so what happens when a neutron collides with...
  18. C

    Do Non-Rotating Neutron Stars Exist?

    Hey! I have a question, whose answer I was unable to get after reading some articles regarding neutron start. I've understood that neutron stars lose their rotational energy and emit fragments of it to earth, thus slowing down through the years. I know that this process takes billions of...
  19. R

    If Neutron and Proton have some diff. mass then why?

    I see that in some books, Proton and Neutron charge differ a bit. Why is it? :confused: I thought them to be same. But... And I am new to this forum... Let's hope we will have a great time together studying science...
  20. D

    Slow neutron beam deflection by a magnetic field

    Is it possible for a beam of slow neutrons, to be deflected by a strong magnetic field? I have found something for a beta asymmetry in Wu experiments, but haven't understood much. Is it a particle physics subject?
  21. D

    Conditions for thermal neutron induced fission

    Does anyone know what the necessary conditions are for a nucleus to undergo fission with a thermal neutron? I have found something for the chain reactions, but not very helpful. I want to find out the conditions for ONE nucleus to undergo fission with a thermal neutron.
  22. Amith2006

    Exploring Neutron Emission and Its Role in K(40,19) Decay | Solution Guide"

    Homework Statement 1)Neutron emission is not a possible mode of decay for K(40,19).Why? Homework Equations The Attempt at a Solution I think it is because the neutron to proton ratio for potassium(40,19) is almost unity(more precisely N/P=1.1). So, neutron emission is not a mode...
  23. Amith2006

    Tracing the U(235,92) + Neutron Process to Final Stable Nuclei

    Homework Statement 1) In a sequential process, U(235,92) plus a neutron forms the compound nucleus [U(236,92)]* which then fissions; the fissions then produces decays. If the initial fission fragments are Ba(143,56) and Kr(90,36), illustrate a process leading to the final stable nuclei...
  24. R

    Exploring Neutron Population in Sub-Critical Reactor with Heavy Water Reflector

    Consider a reactor being held sub-critical, Keff < 1, by control rods. The reactor has heavy water reflector and has been operatored for some time prior to the current state (we got Photo Neutrons). Keff is then bought to 1. It seems to me, for Keff = 1 the neutron population should be...
  25. J

    Neutron Decay Into Proton: Hawking's New Book

    can a neutron decay into a proton? i certainly didnt think so, but i am reading hawking's new little book "breifer history of time", and he states that in there while talking about the early universe. thanks.
  26. M

    Learning Physics: How Do Neutron Stars Form?

    Hi guys, I'm not to great at physics and all but I want to learn more. I hope you guys can help me in that aspect.First of all, how do neutron stars form? I was told their electrons shrink into their nucleuses and therefore the whole star shrinks, but what causes the atoms to behave like that?
  27. D

    Why Is a Neutron Stable in a Nucleus but Unstable When Free?

    A (free) neutron has a lifetime of some 10 minutes or so, how come it is stable in a nucleus?
  28. R

    Do Neutrons in Stable Helium-4 Undergo Continuous Transformation?

    I have a question about current experimental findings on the status of the neutron N while contained within nuclear radius of a stable atom, say Helium-4. It is well known that the N will undergo beta(-) decay when it is free from a nucleus (takes ~ 14 minutes). But... My question...
  29. D

    Calculating the Binding Energy of a Neutron | Explained

    hiii guys, what's the binding energy of a neutron and how do you arrive at the answer? durrrrrrhhhhhhhhhh :confused:
  30. S

    Difference between Thermal and Fast neutron in a reactor?

    I read a sentence in my book saying, The fast neutrons released through the first nuclear fission are passed into the moderator, thus producing (becoming) thermal neutrons. What is a Thermal neutron? What is the difference between Thermal and a Fast Neutron?
  31. S

    Neutron to start the chain reaction

    Hello, I can't find :confused: where do we get the starting neutron(s) for the chain reaction in the reactor. I'm aware that then the splitted atom emits enough(in fact even too much?) neutrons to selfsustain the reaction, which are then slowed down to be able to split uranium and so on...
  32. C

    Weighted delayed neutron fraction?

    I am plotting the in-hour equation. For the delayed neutron fraction, I was thinking of using a weighted dnf for the particular U fuel enrichment of interest, ie combination of U235 & U238 dnfs, as I cannot look one up for this particular enrichment. Any comment on the “validity” or otherwise...
  33. M

    What is the Monte Carlo Method for Simulating Neutron Transport using MPI in C?

    Can anyone hepl me with this?I need some web resource,to start learning from scratch.
  34. W

    Understanding the Impossibility of a Bound State of Two Identical Nucleons

    Hello, Can someone explain to me exactly why a bound state of two identical nucleons is not possible? I have a feeling its something to do with antisymmetric wavefunction, but haven't found a satisfactory explanation in any book. Cheers.
  35. S

    Calculating the Radius of a Neutron Star

    Homework Statement Suppose the sun collapses into a neutron star. What will its radius be? The questions also gives some backround explaining that stars fuse hydrogen into helium until they collapse into a neutron star. The protons and electrons fuse into neutrons with the density of nuclear...
  36. S

    Calculating the Radius of a Neutron Star

    The question is: Suppose the sun collapses into a neutron star. What will its radius be? The question gave a brief backround explaining that stars are powered by nuclear reactions that fuse hydrogen and helium. When the hydrogen is used up the star collapses into a neutron star. The force of...
  37. S

    Surface Gravity of a Neutron Star

    A neutron star has a mass five times that of Earth and a 10 KM radius. Find the distance from this star's surface a satellite must be at to stay in a circular orbit if the satellite is moving at 50000 km/min. First, I changed the 10 KM to meters and found the mass of this neutron star...
  38. V

    Centripetal acceleration of Neutron stars

    Neutron stars represent the final stage of life for some massive stars. Typically, they have radii of 10 km. Determine the magnitude of the centripetal acceleration for a piece of neutron star matter on the star surface at the equator (so the matter moves in a circle of radius 10km). Assume...
  39. 3

    Neutron Generator Applications

    I was wondering if some of you could describe a couple of the applications of a neutron generator and or suggest some further reading on the types of such?
  40. K

    How to Solve Tolman-Oppenheimer-Volkov Equations for Neutron Stars?

    Does anyone know of a good reference regarding solving the Tolman-Oppenheimer-Volkov equations for neutron stars? Most things I find are either too elementary and others skip multiple steps. I think the EoS to use should be that of a Fermi gas model, but I am not sure.
  41. Chronos

    Observational constraints on quarks in neutron stars

    I was intrigued by this paper, and apparent implications for Smolin's cosmic natural selection [CNS] conjecture. http://arxiv.org/abs/astro-ph/0609644 Observational constraints on quarks in neutron stars Authors: Pan Nana, Zheng Xiaoping Comments: 16 pages,6 figures We estimate the...
  42. S

    Neutron Configurations: Why Certain Atoms are More Stable

    Does anyone know if there are descriptions of the neutron and proton configurations in atoms and why certain configurations are more stable than others. For example the average atomic mass of oxygen and flourine are the whole numbers 16 and 19 while most other elements have more variation...
  43. N

    Calculating Neutron Peaks with Increased Kinetic Energy

    hi, in neutron scattering, if the lowest kinetic energy of a neutron is increased by a factor of 2, how do you work out the number of peaks produced? I have worked out the lowest kinetic energy for a beta-brass CuZn to be 2.37meV using [tex]E=\frac{\hbar^{2}k^{2}}{2m}[\tex] where...
  44. A

    Why do Neutron Stars have a Magnetic Field?

    We were having a little chat in my physics lesson about neutron stars for our A level course, and nobody really understood why neutron stars have a magnetic field if they are consist of neutrons, which are obviously neutral charge. We thought that you needed charged particles to create a...
  45. E

    How Do Airy Function Roots Determine Photon Energies in a Gravitational Field?

    The situation involves a neutron in a constant gravitational field (g=9.8). I need to find the energies of photons that transition to the excited state. I solved the Schrodinger equation by doing a variable transformation using Airy functions. To fully solve, however, I need to find the roots...
  46. ZapperZ

    Magnetic neutron scattering in hole doped cuprate superconductors

    There is a good review article on inelastic neutron scattering experiments and results on hole-doped cuprate superconductors. One of the authors (Tranquada) was the first person to report experimentally on the possible existence of the stripe phase in such a compound using the same technique...
  47. P

    What Is Produced When Nickel-60 Captures a Neutron?

    taking a set of questions and came across this one: "Capture of a neutron by nickel-60 produces a proton and what new element or isotope ? " I thought it was copper-61 since it goes through beta decay as indicated by the proton but supposedly it is not... please help
  48. R

    Neutron decay products: n → p + e + ν + DC-photon?

    This is one of those old-high school questions that never got answered (And the search mechanism here doesn't narrow on quotemarks)-- A neutron decays to a proton, electron, antineutrino ... But the highspeed escaping electron is a charge moving relative to (away from) the proton opposite...
  49. V

    Neutron star: heaviest teaspoon of matter

    Is there anything in the observable universe that weighs more? 1 teaspoon = billion tons
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