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. O

    A Conservation of Information: Neutron Formation and Decay

    Has anyone analyzed the process of Neutron formation and decay from the perspective of "information conservation"? Does anyone have any thoughts on what the results of such an analysis would be? What is the status of the observed evidence of reality in respect of whether one should conclude...
  2. J

    Initial Mass Function Question (white dwarfs, neutron stars and black holes)

    Homework Statement Calculate the number of white dwarf, neutron star and black holes the galaxy will have after 5Gyr of evolution. M<8(solar mass) for white dwarf 8(solar mass) < M < 40(solar mass) for neutron star M > 40(solar mass) for black hole Initial mass function is ξ(M) = AM-s...
  3. P

    Liquid Scintillation Counter w/ fast neutron detectin isotop

    I'm trying to make a LSC with U-238 (non-aqueous form) dipped in the scintillating cocktail to detect fast neutrons (no thermals or epithermals, only fast) from a Cf-252 source. How do I calculate the wavelength emerging from the cocktail (assuming U-238 does not react with the cocktail)? Also...
  4. edguy99

    I Does the anti-neutron decay with same timing as a neutron?

    There is some discussion regarding the decay time of the neutron here for example. Has the decay time of the anti-neutron been predicted or seen to any degree of accuracy that could be compared to the decay times seen for the neutron? Is it expected to be the same?
  5. kiwaho

    I Why to use negative hydrogen in spallation neutron source?

    Just wondering why to use negative hydrogen H- ion in spallation neutron source. I read the literature through http://neutrons2.ornl.gov/facilities/SNS/works.shtml , still not yet get the answer. If directly use proton, then still easy to accelerate, and no need to strip off the unwanted...
  6. StanEvans

    I Neutron Star Formation: Quarks, Protons, Electrons Explained

    So a programme that I watched on tv was talking about neutron stars and they said that the neutron stars neutrons were formed by protons and electrons combining to make neutrons. I was just wondering, how does this work, in the field of the quarks in the proton and how they are effected by an...
  7. Garlic

    I Intensity of the background neutron radiation

    Hello everyone, What is the average intensity of the background neutron radiation?
  8. Garlic

    I Detecting low intensity neutron radiation

    Hello everyone, Is it practically possible to detect a neutron source with an intensity of 0.1 Bq and each neutron having nearly 10MeV energies (and differentiate it from background neutron radiation)? If that's possible, what kind of equipment can be used? Do you need extremely sensitive and...
  9. D

    B The lifespan of a neutron star

    How durable are the neutron stars, ie how long can they last? Will they "evaporate" like black holes or something else will happen with them after a very long period of time (eons)? Or are they immortal? I'm asking because I have found nothing clear about the lifespan of a neutron star.
  10. Stella.Physics

    I Binary system of a neutron star with a black hole

    I am reading about mergers of a neutron star with a black hole and the association with GRB. While talking about the accretion disk, the paper I am reading says about the last stable circular orbit. Firstly I thought it was where the Roche limit lies, where mass transfer or matter ejection from...
  11. S

    A Solar drive / neutron atmosphere

    I am wondering, if the sun is a fusion reactor, it should have an "atmosphere" of neutrons ? So presumably a craft with suitable fuel eg boron or uranium, in a close pass, would be able to use that to react with the fuel in a suitable drive ? Probably not good for humans - (!) but for an...
  12. Elbert Anstein

    B Pulsars and Neutron Stars debunked?

    Now kindly pardon my ignorance but I hope one of you can explain to me how this can be possible. A rotating neutron star or pulsar have been observed to spin at between 10 to 700 times per second. Now before I proceed further I like to draw your memories back to the merry go round we played as...
  13. D

    Kinetic Energy of neutron and electron

    Question in my textbook:- The wavelength of light from the spectral emmision line of sodium is 589 nm. Find the kinetic energies of electron and neutron at which they both have same de broglie wavelength. Logically, since light of same energy is falling on both then their kinetic energies must...
  14. B

    Neutron star/Magnetar question

    My wife and I attended the Perimeter Institute for theoretical physics. We watched the public lecture called: THE COSMIC GIFT OF NEUTRON STARS by VICTORIA KASPI. I thought it was a decent lecture (perimeter has had some outstanding ones in the past). On the way to work this morning I was...
  15. B

    Shield Alternating Layers of A and B: More Neutron Attenuation?

    Suppose a shield that is infinite in the y and z directions and of thickness 1 meter in the x direction is constructed of alternating layers of materials A and B. Will this shield attenuate a beam of neutrons with more or less or the same attenuation that it would if it were constructed of the...
  16. B

    Does this neutron star have an accretion disk?

    Does this neutron star have an accretion disk?: https://en.wikipedia.org/wiki/IGR_J11014-6103#/media/File:Lighthouse_nebula.jpg
  17. B

    I Could 0.9c neutron star jets originate from the core?

    Could neutron star jets with velocity greater than 0.9c be caused by a mix of ultra-relativistic core material escaping the star? See this link: http://www.dailygalaxy.com/my_weblog/2015/08/neutron-star-jets-near-speed-of-light-rival-those-of-black-holes.html
  18. ORF

    What causes a plateau in the cross section of neutrons?

    Hello It seems to me that the nuclei have a flat elastic scattering cross section of neutrons, for neutron energies from eV to MeV. http://www.nuclear-power.net/wp-content/uploads/2015/11/Elastic-Scattering-Cross-section-light-elements-min.png I thought that maybe it was caused because the...
  19. N

    Fission neutron classification

    "Looking at time behaviour of neutrons in a reactor on time scales of both ~sec and ~days/months Start with fission process e.g. 235U + n -> 236U ->fission Usually divide into 2 Fission Fragments 10%-20% of fission emit a scission neutron (i.e. at time of scission)" I've heard...
  20. Stephanus

    Anti Proton vs Neutron annihilation

    Dear PF Forum, Just out of curiosity. What happens when an anti proton hits a 'normal' neutron? According to this: https://en.wikipedia.org/wiki/Proton https://en.wikipedia.org/wiki/Neutron A proton has 2 up quarks, 1 down quark A neutron has 1 up quark, 2 down quarks. 1. Does anti proton has 2...
  21. B

    B "Gravitational Compression in Neutron Stars"

    What happens to the neutrons in a neutron star as it collapses Into a black hole?
  22. B

    B Chemical composition of relativistic neutron star jets?

    Is there any good information about the chemical composition of relativistic jets from neutron stars? If the chemical composition of the jets was different from the accretion material it could shed light on the process that forms the jets.
  23. Jonathan Scott

    X-ray bursts might not happen for larger neutron stars?

    A method of definitely distinguishing a neutron star from a possible stellar black hole is that it produces X-ray bursts, which have a sharp rise time and may last for an extended period. I had previously thought these occurred when hydrogen fell to the surface and was immediately fused to...
  24. B

    Could accretion on a neutron star’s poles cause the jets?

    Could accreting material on a neutron star’s poles impact with enough energy to initiate fusion reactions, some of which escapes the star as ultra-relativistic jets?
  25. S

    Black hole smaller than a neutron star?

    OK so some stars evolve into neutron stars which I assume are so small (10's of kms) because ALL empty space is removed between the atoms.. absolute highest density possible? Now.. is a black hole larger (massive and in diameter) than a neutron star and called a black hole only because the...
  26. B

    Does accretion reduce the magnetic field of a neutron star?

    When a large amount of plasma radiates greatly while accreting on a magnetized neutron star, where does the radiation ultimately get its energy from, the magnetic field and/or gravitational field? Without doing the numbers, if the magnetic field does the work against the gravitational field, and...
  27. B

    Shape of quark matter bubble in a magnetized neutron star

    If a bubble of quark type matter formed near the core of a magnetized neutron star, what would happen to its shape? Would it elongate along the magnetic field lines? Could it burst out of the magnetic poles of the star?
  28. A

    Neutron Stars from White Dwarf Mergers: Under 1.4 SM?

    I think this could be a good chance that we see how neutron stars form from White Dwarf mergers. The combined mass of the two are less that than required for a type Ia Supernovae. Won't they merge and collapse into a neutron star? What does everyone else think might happen. I want to be sure if...
  29. G

    How Does Neutron Scattering Reveal Anomalies in Phonon Dispersion Curves?

    Consider a monoatomic 1-D chain of atoms (only acoustic branch). What happens with the inference of the dispersion curve through neutron scattering? In one dimension, conservation of momentum dictates $$ k'=k+K_s $$, if k_s is the phonon momentum vector and we only consider processes where a...
  30. J

    Gravitational force of a neutron star

    Hello all, I could be looking at this the wrong way but here it goes: From what I understand, if a star collapses into itself to form a neutron star, it would become more compact, denser and heavier with a larger gravitational attraction. Now, if I understand correctly, the size of...
  31. as123

    Homework -- wavelength associated with a neutron moving with energy of 2ev

    Homework Statement Calculate the de - Broglie wavelength associated with a neutron moving with energy of 2ev .( mass of proton mp= 1.67*10^-27 kg ) Homework Equations Wavelength= nh/ 2π KE = eVs = 1/ 2mv^2 eVs=hf Wavelength= v*f The Attempt at a Solution To calculate the wavelength at first...
  32. V

    Neutron star warm matter - temperature?

    In calculations of quantities in Neutron stars with degenerate matter is usual to set temperature zero. If I'm right it means that pressure of this matter is negligible against pressure due to Pauli principle. But what about situation when the matter is in neutron star locally compressed. How...
  33. M

    Exploring the Curious Case of He-3 Neutron Absorption and Fission into H-3 and H

    I'm curious, why does Helium-3 fission into H-3 and H upon neutron absorption? Surely the He-4 nucleus configuration is more stable? I get that the energy release may be what splits the nucleus, because it releases quite a lot of energy if it were to simply absorb the neutron.
  34. Low-Q

    Can Neutrons Emit Light Without Electrons to Swoosh Them Away?

    In a neutron star gravity has overcome electron degeneracy pressure allowing the protons and electrons to combine into neutrons. But if that is the case, how do neutrons emit light if there are no electrons to swoosh the photons away? I have been thinking, and wonder if the surface (or "crust")...
  35. Ryan Reed

    How do quarks determine which quarks to pair with?

    Quarks join up with other quarks to form composite particles like protons and neutrons, but in the center of something like a nucleus, how do they know which quarks are in THEIR proton or neutron? When all the quarks are together and it becomes a "soup" of quarks, why doesn't it form things like...
  36. S

    Neutron production in (strong) magnetic field?

    I'm starting a new thread; it's not just about cyclotrons this time. The question is as follows: has anybody ever heard of or read about neutron production (=fusion reactions) when a beam of fuel nuclei, such as D+ or Li3+, is bent by a (strong) magnetic field, such as a bending magnet in an...
  37. S

    Neutron production inside cyclotrons?

    There tend to occur in accelerators and ion sources, when they are "run" on deuterons, fusion reactions with neutron production, due to collisions with residual gas in the chamber. Now, I wonder if the same phenomenon has been observed with cyclotrons when they are "run" with deuterons? Or...
  38. D

    Why don't all neutron stars collapse into black holes?

    If they are so insanely dense and their gravity is so mind-numbingly great, what prevents a neutron star from immediately collapsing into a black hole?
  39. reemie

    How to calculate the mass of a hydrogen atom

    The answer according to my booklet is 1.6734×10-24 (g), but I don't understand how we got this answer. proton: 1.6725×10-24 neutron: 1.6748×10-24 electron: 0.0009×10-24 To get the mass, I added protons with neutrons, but I got 3.3473×10-24. What am I doing wrong?
  40. B

    Finding Speed of Neutron after Decay

    Homework Statement A Helium 5 at rest decays into Helium 4 and a neutron. Mass of Helium 4 = 6.648 x 10^-27 Mass of Neutron = 1.67493 x 10^-27 Helium 4 has a momentum of 1.903 x10^-20 and Ek 2.723x10^-14Homework Equations E=mc^2 v= square root of (E2/m) The Attempt at a Solution I have found...
  41. Stephanus

    Neutron Star Questions: Answers to Max/Min Mass & More

    Dear PF Forum, I have question concerning neutron star and star just simply out of curiousity. 1. Can a star reach silicon burning stage then stop. It doesn't continue to iron burning stage. 2. Once a star reach iron burning stage, there's no stopping it to blast into supernova? Is supernova...
  42. J

    How are the quarks in a proton or neutron held together?

    I've been trying to find a source for this somewhere, but I always end up with different sources explaining what holds protons and neutrons together in the nucleus of an atom. I know that the gluons hold them together, but I'm not sure exactly how they do this, and what type of transfers occur...
  43. N

    Resting masses of isolated neutrons versus neutrons in atoms

    I'm a high school student reading through a book on the discovery of the Higgs boson, and, among several other things, there's one part that I don't understand completely. I understand that the Higgs field is what gives mass to lots of particles that would otherwise be the same without the...
  44. J

    Why are fundamental particles round?

    why is each fundamental particle round
  45. Alex299792458

    Do neutron stars, pulsars, magnetars etc. have weather?

    Do neutron star, pulsars, magnetars etc. have solar flares like the sun or do they have sun spots like the sun or do they have solar winds and if they do have any of those types of weather, what are they called?
  46. K

    Impact of molecular bonding on therm. neutron cross-sections

    Hi everyone. Most of what I've read on thermal neutron cross sections talks only about what isotope makes up the neutron target. Likewise, all of the cross sections listed on Sigma: http://www.nndc.bnl.gov/sigma/index.jsp?as=9&lib=endfb7.1&nsub=10 ... are broken down just by isotope. However...
  47. Stephanus

    Proton + electron = neutron?

    This the answer that I have from Chalnoth in my other thread about nuclear fusion inside the sun (or star in main sequence). And after iron burning in the core of massive star, the star explodes and leaves a neutron star (or a black hole) behind. Is producing neutron in P+P reaction chains and...
  48. K

    Why beryllium for neutron multiplication

    I've been going over the cross sections on Sigma, and I'm a little confused as to why beryllium is the most talked about neutron multiplier I've come across. I mean, it does have a few things going for it: multiplication down to lower energy levels than most multipliers, and a very low (n...
  49. J

    Electrostatic Force Between Proton and Neutron?

    After calculating the force upon an electron and a force upon a proton in the atom of hydrogen, my result was a force of ≈8.2x10-8 Newtons acting upon the electron and proton each. If found this by using the formula Fe = (ke q1q2)/r2 Taking this number, I then applied it in the formula F = ma...
  50. K

    Mean number of neutron interactions over distance d

    Let's try something simple and hope this goes better than my last two threads. :( The problem can be stated thusly: ---- Given thermal neutrons emitted at a source S interacting with a mean interaction length of L and an evaluation point P distance d away from S, what is the average number of...
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