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Contrast For neutrons

This means that the Flory interaction parameter y can be determined from the low wavevector limit of the scattering function of a single-phase blend of A chains (with monomers) and B chains (with monomers), where o is the volume fraction of A chains. In practice, the concentration fluctuations in the blend provide sufficient scattering contrast for neutron scattering, as long as one of the components is at least partially labelled with deuterium. [Pg.161]

The only difference between SAXS and SANS is that the contrast for neutron scattering is a variation in scattering density rather than electron density. Scattering density is a function of the nucleus (not the atomic number ) and varies in a complex way. Because the difference in scattering density between hydrogen and deuterium is large, isotopic substitution is used to create the contrast required for SANS. Perhaps the most famous use of SANS in polymer science was the experimental verification that polymer chains in the bulk assume... [Pg.617]

The contrast for neutrons is determined by the directions of spins in atomic nuclei, which has one unique and very useful practical consequence. Hydrogen and deuterium exhibit a very, very large difference in contrast even though they are chemically identical. This has the wonderful result that we can tune the contrast in our systems by doping them with different levels of deuterium. For instance, we could suspend our sample in different mixtures of ordinary and heavy water to achieve the desired... [Pg.86]

We will now turn to the description of the structure of the PMMA chains adsorbed on alumina. This system offers a much better contrast for neutrons, which makes it experimentally very convenient. Moreover, it enables one to test the universality of the observed laws and to compare with the results obtained by EWIF. [Pg.76]

Since scattering factors for neutron diffiaction are independent of the scattering angle (in contrast to the case of XRD and ED), neutron diffraction data are more frequently used for refinement than the others. [Pg.193]

Portion of the Chart of the Nuclides showing s-process and r-process pathways. The s-process pathway, shown by the dark line in the center of the valley of p-stability, shows how a nuclide that successively captures individual neutrons would evolve. Each added neutron moves the nuclide to the right on the diagram, until it reaches an unstable nuclide, in which case it will p-decay to the stable nuclide with a higher Z. In contrast, in situations where nuclides capture neutrons very rapidly ( -process), they will be driven far to the right of the valley of p-stability until the timescale for neutron capture matches that for p-decay. They will then move to higher Z and capture more neutrons until they either reach a size that causes them to fission (break) into smaller nuclei (which can then capture more neutrons) or until the neutrons disappear, in which case they will p-decay back to the first stable isotope along paths of constant A (arrows). [Pg.78]

Another trend is that radioactive nuclei with higher neutron/proton ratios (top side of the band) tend to emit j8 particles, while nuclei with lower neutron/proton ratios (bottom side of the band) tend to undergo nuclear decay by positron emission, electron capture, or a emission. This makes sense if you think about it The nuclei on the top side of the band are neutron-rich and therefore undergo a process that decreases the neutron/proton ratio. The nuclei on the bottom side of the band, by contrast, are neutron-poor and therefore undergo processes that increase the neutron /proton ratio. (Take a minute to convince yourself that a emission does, in fact, increase the neutron/proton ratio for heavy nuclei in which n > p.)... [Pg.960]

In contrast to X rays, the scattering factors for neutrons are not proportional to atomic number. Whereas X rays... [Pg.6120]

The formation of most of the heavy elements occurs in one of two processes of neutron capture the s-process or the r-process. These two broad divisions are distinguished on the basis of the relative lifetimes for neutron captures (Xn) and electron decays (t ). The condition that t > where Tp is a characteristic lifetime for /3-unstable nuclei near the valley of /3-stability, ensures that as captures proceed the neutron-capture path will itself remain close to the valley of /3-stability. This defines the s-process. In contrast, when it follows that successive neutron captures will proceed into the neutron-rich regions off the /3-stable valley. Following the exhaustion of the neutron flux, the capture products approach the position of the valley of /3-stability by /3-decay, forming the r-process nuclei. The s-process and r-process patterns in solar system matter are those shown in Figure 2. [Pg.8]

While neutron sources are not available in most laboratories, small-angle neutron scattering (SANS) has become a routine characterization method for polymer research using large-scale national and multinational facilities. To obtain the contrast needed for neutron scattering, some of the chains in a polymer melt have their hydrogen atoms replaced by deuterium. In a polymer solution, the solvent is often deuterated. This deuterium... [Pg.79]

Reflectivity measurements on monolayers have also been carried out with neutrons. In general, x-ray sources are much more intense than neutron sources even laboratory (rotating anode) x-ray sources are two orders of magnitude more intense than neutron sources. On the other hand, the scattering-length density for neutrons of an atom is that of its nucleus and, as a result, the contrast between different parts of the interface can be altered by isotopic substitution. For hydrocarbon chains, a significant change in... [Pg.411]

The heat produced during the fission process is removed by circulation of a cooler. Even if the heat outflow (which equals 6 x 107 at the ILL at Grenoble) is maximized, the neutron flux must be maintained below 1016 cm 2 s in order to ensure that the temperature of the reactor elements remains under a critical technological threshold. The flux is low as compared to the photon flux obtained with a light source (I019 cm 2s-1 for a laser with a cross-section of 1(T2 cm 2 and a power of 10-i watt).+ However, neutrons can be used to perform experiments that could not be carried out with photons (lack of contrast, for instance). [Pg.185]

For light scattering, contrast results from a difference in polarizability of the molecules. For neutron scattering, it results from a difference in nuclear interaction (different collision lengths). In a general way, the contrast can be defined from the refraction indices corresponding to the radiation and to the materials constituting the mixture. [Pg.246]

Contrast lengths for neutron radiation A value of the contrast of species st with respect to SS is given by... [Pg.257]


See other pages where Contrast For neutrons is mentioned: [Pg.375]    [Pg.18]    [Pg.194]    [Pg.257]    [Pg.19]    [Pg.47]    [Pg.357]    [Pg.375]    [Pg.18]    [Pg.194]    [Pg.257]    [Pg.19]    [Pg.47]    [Pg.357]    [Pg.1371]    [Pg.646]    [Pg.61]    [Pg.132]    [Pg.31]    [Pg.185]    [Pg.75]    [Pg.108]    [Pg.8]    [Pg.226]    [Pg.4513]    [Pg.6127]    [Pg.82]    [Pg.1050]    [Pg.1050]    [Pg.375]    [Pg.14]    [Pg.123]    [Pg.64]    [Pg.215]    [Pg.23]    [Pg.472]    [Pg.246]    [Pg.323]    [Pg.1371]    [Pg.95]    [Pg.4512]    [Pg.6126]   
See also in sourсe #XX -- [ Pg.411 , Pg.413 , Pg.414 , Pg.416 ]

See also in sourсe #XX -- [ Pg.449 , Pg.481 , Pg.483 ]




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Contrast factor for neutrons

Contrast neutrons

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