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. K

    Charge Conservation in Neutron Decay

    A neutron can decay into a proton, a positron, and a neutrino. A proton is made up of two up quarks and a down quark. A neutron is made up of one up quark and two down quarks. An up quark has a charge of +2/3, and a down quark has a charge of -1/3. Given the statements above, can someone...
  2. Astronuc

    Diffusion equation and neutron diffusion theory

    Basically the steady-state diffusion equation can be written in a form \nabla^2\phi\,+\,k^2\phi\,=\,S When S = 0, this is just the Helmholtz equation - http://mathworld.wolfram.com/HelmholtzDifferentialEquation.html See also -...
  3. T

    Neutron flux in finite medium.

    In the text I use for class, the examples and derivations for functions showing the neutron flux at some point, are all about sources within infinite mediums. Now I have a probelm where I must show that neutron flux, for a point source within a finite sphere, is found by the following equation...
  4. U

    What happens to the remaining energy in the neutron?

    I am to calculate everything in a non-relativistic state: a 15MeV photon is completely absorbed in colliding with a neutron initially at rest. Determine the speed of the neutron: conservation of momentum: E=\frac{hc}{\lambda} 15MeV=\frac{1240MeV nm}{\lambda} \lambda=8.2667x10^{-5}nm...
  5. R

    Light bending around neutron and bound photon

    I assume that the neutron is a particle with finite size and is <really> a single particle (that is that it does not have any further structure or components-like nucleus) and lastly it is electric nutral. I hope that these assumptions are close to the experimental observations. I am making life...
  6. fargoth

    A neutron star collapses - where's pauli?

    neutrons are fermions, with half spin, as such the must not occupy the same quantum state (meaning the wave functions can't overlap - atleast not with a big probability density portion of each other). so, if neutron star is in the most dense state it can get, meaning its degenerate and every...
  7. J

    The constituents of a neutron?

    Hello, I'm new to this forum. I was hoping someone might be able to help me understand what the constituents of a neutron are. Last month I read a book that stated that the neutron was composed of 2 'd quarks' and 1 'u quark'... while the proton is composed of 2 'u quarks' and 1 'd quark'...
  8. P

    Understanding the Behavior of Electrons in Neutron Stars

    I was reading about neutron stars and wonder if anyone can help me with something that puzzled me , namely what happens to the electrons in such a mass of atomic neuclii? I can only see there might be 2 possibilities .Either 1) that the electrons are expelled from the atoms during the collapse...
  9. J

    Neutron-Electron and Neutron-Positron Interactions: Is There a Difference?

    I understand the difference between the two main Neutron decays but, is there an observable difference when an electron collides with a neutron compared to a positron colliding with a neutron? In particular, I need to know if there is a difference in the behaviour of the neutron.
  10. S

    Neutron Energy Spectrum vs. Neutron Flux

    what is deffrence between nutron energy spectrum and nutron flux
  11. J

    Neutron Stars: Strong Force, Density & Black Holes

    Is a neutron star held together mainly by the strong force? Are they dense enough so that this is the case, or is gravity the only thing to consider? What about black holes?
  12. Astronuc

    Neutron Embrittlement of Pressure Vessels

    Neutron fluence at the reactor pressure vessel wall a comparison of French and German procedures and strategies in PWRs U. Jendrich (GRS), N. Tricot (IRSN) Abstract: While the neutrons within the core may take part in the chain reaction, those neutrons emitted from the core are basically...
  13. V

    Conservation of momentum of a neutron

    A He4 nucleus, with a mass of 4 amu moving with speed v breaks up into a neutron 1amu and a He3 nucleus 3amu . If the neutron moves in a direction perpendicular to the direction of motion of the original He4 nucleus with speed 3v, what is the speed of the He3 nucleus? if the neutron moves...
  14. S

    Blackhole gulps down Neutron Star

    Nasa team has solved a great mystery:http://www.nasa.gov/mission_pages/swift/bursts/short_burst_oct5.html
  15. marcus

    Fastest neutron star, 1100 km/second

    press release from NRAO http://www.nrao.edu/pr/2005/fastpulsar/ The fastest-moving neutron star ever seen, clocked at 1100 kilometers per second, a speed that will take it out of the Milky Way galaxy, was given its initial "kick-off" by the supernova that formed it. journal article...
  16. B

    What Makes Neutron Stars So Unique?

    What are they? :confused:
  17. L

    Unraveling the Mystery of Neutron Decay: A Fundamental QFT Explanation

    Why does a neutron not decay in some nuclei? Why does it decay in other nuclei? Is there some mechanism suppressing the d quark -> u quark + W- boson channel? I'm looking for a fundamental QFT / Standard Model explanation. Thanks!
  18. wolram

    Neutron diffusion and nucleosynthesis

    http://arxiv.org/abs/astro-ph/0506364 Title: Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model Authors: Juan F. Lara Comments: accepted for publication in Physical Review D This article presents an original code for Big Bang Nucleosynthesis in a baryon...
  19. G

    Question about exploding neutron stars

    I have a question about the time scale for a certain type occurance causing a neturon star to explode, and a related question about the conditions of this occurrance. If you have a binary star system with one of the stars being a neutron star, I read that if the other star sucks off enough...
  20. S

    Quasars,white dwarf and neutron stars

    quasars are highly active but extremely distant galaxies, right?what kind of galaxies are they and do they represent an earlier stage of the lives of the conventional galaxies?i've a vague idea that quasars a galaxies in which the supermassive black holes at the centres are actively gobbling up...
  21. S

    Neutron Star Evolution and Possible Blackhole Formation in Proton Star Collapse

    Are Neutron Stars the major factors of Proton Stars? :http://arxiv.org/abs/astro-ph/0506092 Why do Neutron Stars evolve from Proton Star collapse, and what is the next evolving stage?..if any? :http://arxiv.org/abs/astro-ph/0506100 Can a further collapse occur that does 'not' produce...
  22. G

    What does a neutron star look like

    What does a neutron star "look" like Hi, I have some questions for a scifi story I'm working on. First, what would a neutron star look like? What color are they, and how bright do they tend to be? By look like, I mean both seen from a theortical planet surface orbiting one (or mabye it would...
  23. M

    Neutron star's angular velocity

    Under some circumstances, a star can collapse into an extremely dense object made mostly of neutrons and called a neutron star. The density of a neutron star is roughly 10^14 times as great as that of ordinary solid matter. Suppose we represent the star as a uniform, solid, rigid sphere...
  24. B

    Neutron Star Mass & Life Span

    undefined what mass does a neutron star hove and what is its life span? and any other information on the subject would not go un-apiretiated
  25. S

    Exploring the Neutron Sprayer: How it Works and its Role in Nuclear Technology

    At the centre of an atomic bomb, there is a neutron sprayer, something that can produce neutron streams. What is this component? how do they work? How do we produce free neutrons on particle accelerators? Thanks
  26. wolram

    What is the Explanation for the Cosmic Microwave Background Radiation?

    http://www.physics.ubc.ca/~heyl/ns2005/prospectus.html Neutron Stars at the Crossroads of Fundamental Physics I. Organizers Jeremy Heyl – University of British Columbia Vicky Kaspi – McGill University Feryal Özel – University of Arizona Krishna Rajagopal – Massachusetts Institute...
  27. N

    Where can I find PDF Black holes White Dwars and Neutron Stars

    Where can I find PDF "Black holes White Dwars and Neutron Stars" Gents, Could u pls advise me if you know where can i find book "Black holes White Dwars and Neutron Stars" Authors Shapiro, Tuekolsky (free PDF or DJVu or other format) Thks
  28. J

    Form and Features of Asteroids and Neutron Stars

    What are the forces that give asteroids their shapes? And what shape do neutron stars that do not rotate around its axis have?
  29. F

    Energy to remove a proton and a neutron from a nucleus

    Hey guys, I know this is basic nuclear physics but I've forgotten how to do it. Given the atomic mass of Oxygen 16 (8p 8n), Oxygen 15(7n 8p) and Nitrogen 15(8n 7p), having found the average energy binding energy per nucleon (i think i have it right) find how much energy is required to remove...
  30. marcus

    Neutron stars: good short article

    one reason it's good is that it is written for the Wiley "Encyclopedia of Physics" http://arxiv.org/abs/physics/0503245 Neutron Stars Gordon Baym, Frederick K. Lamb Comments: Encyclopedia of Physics 3rd ed., R.G. Lerner and G.L. Trigg, eds., Wiley-VCH, Berlin Abstract: "This short...
  31. L

    Calculating Weight on a Neutron Star

    Came across this forum while searching the net for help. It's great to have a forum dedicated to physics. So hi to everyone :) Now to business. I'm stuck with this question. If you weigh 660N on the earth, what would you weigh on the surface of a neutron star that has the same...
  32. L

    Neutron Activation: Isotope Identification by Half Life, Beta Particles

    Is there a website where I can find out what isotope I have if I know it's half life and energies of the beta particles emitted?
  33. L

    To verify the estimated mass of a neutron

    with the use of the conservation of momentum.. Is it possible? what does it exactttly mean anyways? :bugeye:
  34. S

    Understanding Beta Decay: How It Affects Atoms and Ionization

    When an atom experience beta decay, will the atom become ion? This is my deduction: 1.An atom will release an electron in beta decay. 2.The electron is replaced by the electon produced from the decay of neutron. 3.However, the proton number increase by one. It still need one more electron...
  35. E

    Understanding Neutron Decay in Elementary Particle Physics

    In ‘Introduction to Elementary Particles’, David Griffiths makes the following two statements: a neutron decays into a proton, an electron, and an antineutrino (1.8) And later: but the following decay is not observed an antineutrino plus a neutron decay into a proton and an electron...
  36. M

    Calculating Proton & Electron Kinetic Energies from Neutron Decay

    A neutron at rest in the laboratory spontaneously decays into a proton, an electron, and a small essentially massless particle called a neutrino. Calculate the kinetic energy of the proton and the electron in each of the following cases: a) the neutrino has no kinetic energy b) the neutrino...
  37. E

    Neutron Star Matter & Planet X: What Could Be Lurking Closer?

    There are no neutron stars within 1000s of light years that we know of but there could be chunks of one much closer. The speculation of a planet X in our solar system has been written about many times and some think the new found planetoid Sedna may be that object.However, a much smaller object...
  38. C

    Calculating the Escape Velocity from a Neutron Star

    Question: The radius of a neutron star is 750 times smaller than the Earth's radius, and its mass is 1.8 times larger than the Earth's mass. What is the escape velocity from the surface of a neutron star? (Ignore the fact that, at high speeds, one should not really use mv^2/2 for the kinetic...
  39. B

    What happens as a neutron star collapses into a black hole

    I've heard this explained numerous times, most recently in my General Relativity course today, where he talked about how smaller stars will collapse into white dwarfs, while more massive ones will overcome the electron fermi gas pressure, effectively forcing the electrons into the protons, so...
  40. Garth

    Neutron star at Centre of Sun?

    What do members think of this: http://arxiv.org/abs/astro-ph/0411163 ? Garth
  41. C

    Solve Neutron Flux Problem with 27Al(p, 3pn)24Na Reaction

    Hello. I'm a little unsure of how to proceed on this problem... Here it is: A 3-Gev proton flux is monitored by measuring 24Na activity induced in 25 microm (6.85 microg/cm2) aluminum foil via 27Al(p, 3pn)24Na reaction (for 3 Gev protons, cross section = 9.1 mb). Exactly 15 hr after the end...
  42. Orion1

    Neutron stars and colour force

    Einstein field equation gravitational potential: \nabla^2 \phi = 4 \pi G \left( \rho + \frac{3P}{c^2} \right) General Relativity gravitational pressure: P_e = \frac{c^2}{3} \left( \frac{\nabla^2 \phi}{4 \pi G} - \rho \right) Classical Yukawa Pressure: P_y = f^2 \frac{e^{-...
  43. C

    Proton vs Neutron: Mass Comparison

    isn't a neutron more massive thatn a proton?
  44. DrChinese

    Coaxing a Neutron from Deuterium

    Question: What would it take to coax a deuterium atom to give up its neutron? In terms of input energy? Would you need to hit it with an energetic electron to have a reasonable chance of disassociation? Thanks!
  45. K

    Neutron stars and colour force

    If neutrons stay intact and get closer together than 10^-15 metres in a neutron star, would the exchange of mesons between neutrons stop and be replaced by the exchange of gluons, and would the gluons cause an attractive or repulsive force between neutrons? A repulsive force could stop the...
  46. K

    Can dark energy prevent neutron stars from collapsing into black holes?

    How can gravity overcome the degeneracy pressure of neutrons in a neutron star? Isn't such a thing the same as violating the uncertainty principle?
  47. M

    Comparing Neutron Bombs vs Nukes: What's the Difference?

    Ok I've done quite some reading on neutron bombs. What exactly is the difference between them in the way they work? The way i see it now its a nuke, but not focused on heat/blast damage but radiation. How does it work? Other material used? And what isn't really clear to me is if they have...
  48. turin

    Observational Difference Between Neutron Star & Black Hole

    What is the observational difference between a neutron star and a black hole? Is the evidence conclusive, or is it based on a strong reasonability argument?
  49. R

    Why do neutron stars have magnetic fields

    An article by W Tucker and K Tucker at NASA says that neutron stars have magnetic fields. If a magnetic field is created by moving charges, and neutron stars have not net charges to move, how are the fields created?
  50. D

    Question-can a neutron star shed mass?

    Question--can a neutron star shed mass? Once the steller core of a massive star collapses into a neutron star, is there any known mechanism by which the neutron star can shed mass?
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