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. S

    Neutron and Proton densities in a nucleus where N=Z

    1. The problem statement, all variables and given/kown data Assuming that the nuclear radius R=γ0 *A(1/3) where γ0 =1.2×10(-15) and A is the mass number, Calculate the neutron and Proton densities in a nucleus N=Z. Homework Equations A=N+Z.=2Z in this case. Mass of proton =Z*mp Mass of...
  2. W

    Neutron Star at Near Light Speed

    What would happen to a neutron star (on the cusp of becoming a black hole) if it were sped up to near the speed of light? Or more easily done, if I sped up to near the speed of light. Would the additional mass from the near light speed cause the neutron star to collapse in on itself and form a...
  3. skujesco2014

    Relationship between Ultracold neutrons and neutron stars

    Hi, PF: I'm currently about to graduate from my Ph. D. program in Physics and I want to focus my research in theoretical physics. I feel very excited by topics such as Astrophysics and GR, but also low temperature physics, such as superconductivity, bose-einstein condensation, superfluidity...
  4. R

    Calculate velocity of a 1MeV Neutron

    How would one calculate the velocity of a 1MeV neutron?? I tried the following the attached formula for V/C but E is less than the rest mass which yields the square root of a negative number. Not sure what to do for this
  5. B

    Graduate Student: Inelastic Neutron Scattering & DFT Course Prerequisites

    I am a graduate student and I am thinking of doing a project on "Inelastic neutron scattering and density functional theory". Can you please inform me what are the exact background knowledge(courses) I should have to.
  6. Warpspeed13

    Question about fast neutron leakage calculations

    Ok so the equation for the probability that a fast neutron will not leek out of a non infinite mass is Pfnl= exp(-(Bg)^2 Tth) so Bg is the geometric buckling and for a sphere that value is (pie/r)^2. My question is what is exp? And what is Tth / how do I get the value of it?
  7. anorlunda

    Free neutron vs bound neutron decay

    I was curious as to the difference in free neutron decay and the lack of decay when bound in a nucleus. I found the following statement here http://en.m.wikipedia.org/wiki/Neutron#Free_neutron_decay I don't understand that. Is the wave function of the neutron different when free or bound...
  8. Warpspeed13

    Plasma Pinch Fusion as a Neutron Source: Questions

    Ok so I recently read this article (http://www.extremetech.com/extreme/184280-focus-fusion-has-cheap-clean-earth-saving-fusion-power-been-right-under-our-noses-all-along). This gave me a few ideas and a few questions. I would like to create a smaller version of this setup to fuse deuterium into...
  9. K

    The energy released for white dwarf collapsing into neutron star

    The question is attached. I'm not sure how to approach to part (b). The energy released could be in 3 forms, the rest mass energy for those matter ejected during supernova explosion, the binding energy released as the atomic structure changed, the ejected matter carries off some kinetic...
  10. K

    How does a nebula form from a neutron star

    Here is my understanding, please correct me if I am wrong, thanks At the end of the giant stage of a star, it experiences a supernova explosion, and turns into a neutron star (could be pulsar) or black hole, the explosion releases a lot of its matter. Here is what I don't understand: 1...
  11. E

    Neutron scattering as a function of angle

    Hi thanks for reading. Is it possible to derive an explicit formula for the neutron scattering cross section as a function of energy and angle of incident and scattered neutrons respectively? This is for a (n,p) elastic collision with H-1 as the target.
  12. R

    Why doesnt neutron scattering violate charge conservation?

    p + n -> p + n + ∏^- check charge conservation: + 1 + 0 = +1 + 0 -1 it doesn't equal so it wouldn't be possible? please could someone suggest why this is, or if I'm doing something wrong? thanks in advance. edit is it because the pion is the force carrier therefore should not be...
  13. B

    Neutron Stabilization mechanism?

    If a neutron is unstable outside the nucleus, then what makes it stable within the nucleus? Does the binding of particles together somehow make them stable? Neutrons decay via the weak force, but are bound in the nucleus by the strong force. Does the strong force inhibit the weak force...
  14. Q

    Potential energy of proton vs neutron

    Consider an atom having multiple protons and neutrons in its nucleus, which of the two nucleons will have higher magnitude of potential energy?
  15. jlefevre76

    Is Neutron Star Energy a Disappointment for Nuclear Renewables?

    So, I was disappointed to find out that the surface of a neutron star is at 1 million kelvin, not 100 billion kelvin. I did some calculations a while back using the 100 billion K as a temperature (the core temperature of a neutron star), and found that it would be emitting more radiation than...
  16. M

    How can a proton form a neutron?

    This is related to a homework problem but I want to understand it as well. How can a proton break up into a positron and neutron when a neutron clearly has a greater mass than a proton?
  17. S

    Thermal neutron spectrum

    The most probable velocity of thermal neutrons can than be approximated by the Boltzmann constant and is given by the following: v = sqrt (2kT/m) where k is the Boltzmann constant T is the temperature m is the mass of the neutrons My question is why is the above equation not the...
  18. S

    Neutron energy needed to produce fission of 208Pb

    Homework Statement Estimate the neutron energy needed to produce fission of 208Pb. Is it likely that such neutrons woould be released in the resulting fission? Homework Equations Eexcitation=Qexcitation+Tn Qexcitation=[m(208Pb)+mn-m(209Pb)]c2 V=(e2/4πεo)(Z1Z2/r)...
  19. C

    Isotopes: Proton vs Neutron Counts

    I'm in year 10 and I have been studying physics and chemistry. When I learned isotopes, I notice that for isotopes, the number of neutron is always higher than that of proton. Is it possible that there are isotopes that the number of neutron is lower than that of proton? If no, is that because...
  20. R

    Form Factor and Neutron Scattering

    Hi all Can someone please describe how the form factor used in Rutherford scattering is applicable to neutron probing of nuclei? Also, is the kinetic energy required to probe a given radius simply given by the de Broglie wavelength where momentum, p >= h-bar / Radius ? (Relativity...
  21. Mr.Aaron

    Can a thimbleful of neutron star material cause damage to Earth?

    Hi everyone! First of all, I'm a brand new member and am looking forward to spending time on this forum, learning a bit more about science, and getting to know some of you. Anyway, here's what's been on my mind lately: I've heard that a thimbleful of neutron star material weighs as much as a...
  22. Spinnor

    Stimulated virtual W+, W- when supernova core-> neutron star?

    Stimulated virtual W+, W- when supernova core--> neutron star? Weak interactions allow supernova core electrons and protons to convert to neutrons and neutrinos allowing (under the right conditions) the formation of a neutron star? Large numbers virtual W+ and W-bosons are produced in a short...
  23. C

    Neutron Flux in Infinite Vaccum

    I have to figure out how to prove that the neutron flux for a point source is given by ø=\frac{S}{4πr^2}. I can get this type of solution, but I have an e^(-r/L) in the numerator. I'm assuming I'm missing some theory somewhere as apparently this is the solution for a point source in an...
  24. M

    Boron Neutron Capture Therapy

    Hello All I'm doing my theses in BNCT(Boron neutron capture therapy).I did it with 2.5 Mev imaginary accelerator. there are many reactors to compare my data with theirs.but Unfortunately I couldn't find some Real accelerators based on BNCT to compare my MCNP-X output data with theirs. could u...
  25. S

    Speed pf the neutron of thorin

    Homework Statement U → Th + α The speed of α = 6 x 105 m/s. Find the speed of neutron of Thorium! Homework Equations E = mc2 momentum The Attempt at a Solution I am pretty sure there is missing information, maybe the mass of α and Th. I just want to ask the way to solve it...
  26. V

    Protons Neutrons and Electrons in a neutron star

    Hi All, I am preparing for PhD quals and have been looking at problems from other universities. I came across this one and am stumped on how to tackle it. " Assume that the neutron density in a neutron star is 30.1/fm (that is 0.1 neutron per cubic Fermi). Assuming T=0 and ignoring any...
  27. A

    Why don't black holes look like neutron stars to outside observer?

    Yesterday, I read about Hawking's new proposal regarding the firewall paradox. A more general thought about standard black holes occurred to me. Black holes including stellar black holes are of course always presented as if the event horizon is an invisible barrier, which the unfortunate...
  28. K

    Neutron Pulse Dose: Calculating Equivalents

    This isn't really a homework question per say. I found this in some old notes and have been trying to figure out the first part of it. I cannot find the equation for parts a and b, I have parts c and d solved based off the answer to b which is in parenthesis and it matches the answer at the...
  29. S

    Some questions about neutron shielding in fast reactors

    I've been reading about fast reactor designs lately (not necessarily ones that have actually been built). A few articles I've come across < https://drive.google.com/folderview?id=0B-MNeRy61MgpTVExcUQ3T3ZWWG8&usp=sharing > discuss the possibility of building fast reactors, fueled with molten U...
  30. U

    Need help with fast neutron absorbed dose rate

    Hello everyone. I need a hint of how to do the following question. I spent long time trying to solve and I could not do it. An ionization chamber that will be used to measure fast neutron absorbed dose rate consists of ethylene (C2H4) gas at a density of (1.2×10^-4 g/cm^3) enclosed by...
  31. I

    Neutron Stars vs Atoms: A Comparison

    So how much denser than is a neutron star than an atom? Is it called a neutron star because electron's orbital effect no longer exists/acts the same, so as to no longer cause 99.99% of everything to be space?
  32. E

    Neutron Star Collision Homework: Layer Thickness & Gravitational Potential

    Homework Statement Suppose that an earth-mas object collides with a neutron star with radius 10 km and mass 1.4 $M_{sun}$. The material of the earth-like object would wrap around the neutron star and form a thin layer on top of the original neutron star surface. Assume the material gets...
  33. F

    Elastic Neutron Collision (Conservation of Momentum and Energy?)

    1. A neutron collides elastically with a helium nucleus (at rest initially) whose mass is four times that of the neutron. The helium nucleus is observed to rebound at an angle '2 = 41° from the neutron's initial direction. The neutron's initial speed is 5.6 105 m/s. Determine the angle at...
  34. I

    Neutron Flux Profile in a Spherical Moderator

    Hello People I need help with the following assignment: It states: Consider an ideal moderator with zero absorption cross section, Ʃa = 0, and a diffusion coefficient, D, which has a spherical shape with an extrapolated radius, R. If neutron sources emitting S neutrons/cm3sec are distributed...
  35. M

    How many neutrons are in a neutron star with a diameter of 42.0 km?

    How many neutrons are in a neutron star with a diameter of 42.0 km? I was under the impression it was just (42.0e3/1e-15)^3 = 7.0048e58 but that's wrong??
  36. L

    Finding the moment of inertia of a neutron star

    Homework Statement The Crab Nebula is a cloud of glowing gas about 10 light-years across, located about 6500 light years from the Earth (the figure (Figure 1) ). It is the remnant of a star that underwent a supernova explosion, seen on Earth in 1054 a.d. Energy is released by the Crab Nebula...
  37. P

    Neutron stars on collision course.

    Simply put, either by chance or a suicidal type-III Civilization, 2 neutron stars, or a neutron star an a large-ish main sequence star are thrown at each other and fall STRAIGHT into each other. What happens? Does the ~1.4 C Newtonian impact speed result in them getting blown up and releasing...
  38. S

    Analyzing Assumptions for Neutron Flux: Fast & Thermal Groups

    Assumptions 1) a=absorption 2) f=fission 3) ∅=neutron flux 4) time independent 5) group 1, fast neutrons 6) group 2, thermal neutrons 7) All fission neutron are boring in fast group 8) All neutrons created by thermal group, thus vƩf2 exists vƩf2 does not 9) Down scattering occurs but up...
  39. E

    Moderation of Fast moving thermal neutron

    If a fast moving thermal neutron can be slowed down to increase absorption chances, is there a way it can be brought a halt? If yes, what will be the behavior of such neutron?(Apart from a simple fact that reaction comes to a halt)
  40. B

    What Causes a Neutron to Eject an Electron?

    What is the force that makes a neutron eject an electron, and how strong is it?
  41. H

    Twin Paradox & Neutron Speeds: Questions Explored

    I have make many threads about this topic because I am really interested. I reading that from an pdf,but I have some "idiot" questions too. 1)A guy told me that If you run in other speed from an other you see his clock slower. I have hear about paradox of twins,that this with biggest speed...
  42. T

    Kilonovas caused by black hole neutron star mergers

    I thought readers would be interested in this interesting article today on black hole and neutron star mergers and the very small possibility of instantaneous sterilization and extinction of all life on earth:http://www.space.com/22231-gamma-ray-bursts-neutron-stars.html...
  43. L

    Neutron Beam Width after localization via a slit in a sheet (QM)

    Homework Statement A parallel beam of neutrons with speed 200m/s is incident on an absorbing sheet with a slit of width 0.01mm. Calculate the width of the beam 10m behind the slit. Hint The slit localizes the neutrons transversely (y) to their propagation direction x. The resulting ΔPy gives...
  44. K

    Calculation of neutron transport cross section

    I have a book on nuclear reactions which details the mean free paths for thermal neutron scattering as: 0.37cm for water and 2.2cm for heavy water The transport cross sections are listed as 0.45cm for water and 2.6cm for heavy water. Does anyone know how to calculate these from the thermal...
  45. M

    Calculation of Neutron star pressure/mass using 4th order Runge-Kutta

    Hi all, this is my first post here and i apologize if some rules aren't followed. I have to complete the Project 13.1 (studies of neutron stars: p 346-350) http://www.cec.uchile.cl/cinetica/pcordero/MC_libros/Hjorth-Jensen2008.pdf When browsing using pdf pages 346 to 350, assignments 1...
  46. R

    In-flight neutron capture by Cobalt-59

    Can anyone help me with an approximate answer to this or point me in the direction of avenues to get an answer to this? This has practical applications and is potentially worrying. Roughly how much (or how many atoms) of cobalt-59 exposed to the average neutron radiation at in-flight...
  47. H

    Neutron Spin Time Evolution in Interferometer

    Hey Everyone, I'm working on a question and can't quite get the answer out. QUESTION: Part (a) "\left|\alpha\right\rangle and \left|\beta\right\rangle are the eigenfunctions for neutrons polarized respectively along positive and negative z directions. If the neutron, initially in...
  48. B

    Why is thermal neutron with energy of 0.0253eV so important?

    I want to know the reason why the thermal neutrons with energy of 0.0253eV is so important. As far as I know, a neutron with an energy of 0.0253 eV is used as reference to measure nuclear cross sections such as absorption, fission, scattering, etc. And I want to know the details and more...
  49. D

    Neutron Diffusion Equation/Spherical Geometry Source Problem

    Homework Statement Solve for the flux distribution using the 1D neutron diffusion equation in a finite sphere for a uniformly distributed source emitting S0 neutrons/cc-sec. My problem right now is that I can't figure out the boundary conditions for this problem. We usually work with...
  50. xatu

    Calculate density of neutrons in a beam

    Problem: A flux of 10^12 neutrons/m^2 emerges each second from a port in a nuclear reactor. If these neutrons have a Maxwell-Boltzmann energy distribution corresponding to T=300 K, calculate the density of neutrons in the beam. Solution: The average velocity of neutrons coming from the...
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