Neutron Definition and 746 Threads

  1. 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...
  2. 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?
  3. 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.
  4. Amith2006

    Why Can't Neutron Emission Occur in K(40,19) Decay?

    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...
  5. 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...
  6. 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...
  7. 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.
  8. 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?
  9. 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?
  10. 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...
  11. 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:
  12. 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?
  13. 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...
  14. 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...
  15. 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.
  16. 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.
  17. 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...
  18. 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...
  19. 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...
  20. 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...
  21. 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?
  22. 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.
  23. 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...
  24. 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...
  25. 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...
  26. 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...
  27. 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...
  28. 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...
  29. 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
  30. 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...
  31. V

    Neutron star: heaviest teaspoon of matter

    Is there anything in the observable universe that weighs more? 1 teaspoon = billion tons
  32. 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...
  33. 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 -...
  34. T

    Where Can I Learn About Neutron Flux in Finite Mediums?

    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...
  35. 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...
  36. 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...
  37. 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...
  38. 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'...
  39. 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...
  40. 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.
  41. S

    Neutron Energy Spectrum vs. Neutron Flux

    what is deffrence between nutron energy spectrum and nutron flux
  42. 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?
  43. 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...
  44. 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...
  45. 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
  46. 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...
  47. B

    What Makes Neutron Stars So Unique?

    What are they? :confused:
  48. 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!
  49. 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...
  50. 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...
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