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Beryllium nucleus

The component functions may be chosen in a variety of ways. For example, if the nuclear field were only a single beryllium nucleus, the one-electron spatial functions could be constructed to mimic the atomic Is and 2s orbitals. For a molecular system, the functions can be constructed as a linear combination of atomic orbitals (AOs) in which each one-electron function... [Pg.35]

Nuclear reactions can form a beryllium nucleus by fusing helium nuclei. The beryllium nucleus can then fuse with another helium nucleus to form a carbon nucleus. [Pg.162]

The temperatures in stars get high enough to fuse helium nuclei with one another. As helium nuclei fuse, elements of still higher atomic numbers form. Figure 28 illustrates such a process two helium nuclei fuse to form a beryllium nucleus, and gamma radiation is released. The beryllium nucleus can then fuse with another helium nucleus to form a carbon nucleus. Such repeated fusion reactions can form atoms as massive as iron and nickel. [Pg.162]

The BeH2 molecule is known to linear. Let s define the z-axis of the coordinate system to lie along the H—Be—H bonds, and place the beryllium nucleus at the origin. We mix the 2s and Ip orbitals of beryllium to form two new orbitals on the beryllium atom ... [Pg.257]

The formation and the shapes of the sp hybrid orbitals and their participation in chemical bonds are shown in Figure 6.41. The first column shows the non-hybridized orbitals on the Be atom, and the second column shows the hybrid orbitals. The amplitude for each hybrid at any point r from the beryllium nucleus is easily visualized as the result of constructive and destructive interference of the 2s and 2p wave functions at that point. Because the sign of the 2s orbital is always positive, whereas that of the 2p orbital is different in the -I- and -z directions, the amplitude of Xi is greatest along -l-z, and that of 2 is greatest along —z. Because the probabilities are the squares of the amplitudes, an electron in xi is much more likely to be found on the left side of the nucleus than on the right the opposite is... [Pg.257]

However, such processes occur relatively seldom, while E. Salpeter (Cornell University) showed that a two-step reaction should be more easily realisable (Kipper-hahn, 1980). A collision of two helium nuclei leads to the formation of a beryllium nucleus, which decomposes very rapidly to the starting materials unless it is hit by a further helium nucleus the newly-formed nucleus 12C is stabilized by radiation emission. The lifetime of the beryllium nucleus is only about 0.05 s (Hillebrand and Ober, 1982) thus, the density of the helium nuclei must be very high in order to give a high collision probability. [Pg.22]

At this point, the synthesis of new elements stopped. The reason is that nuclei larger than those of hydrogen and helium can form only when like-charged particles (such as protons or helium nuclei) combine to form heavier nuclei. A hypothetical example is the formation of a beryllium nucleus by the combination of two helium nuclei ... [Pg.12]

This process is exothermic, the sum of the masses of the beryllium nucleus and the a particle exceeding the sum of the product masses by an amount equivalent to an energy of 5.7 MeV. [Pg.35]

A weakness in these early designs was the initiator. This is designed to flood the fissile core with neutrons at the moment of maximum compression. The early initiators used beryllium and polonium 210, which is a powerful alpha emitter. If the alpha particles hit a beryllium nucleus, a neutron is ejected ... [Pg.83]

The rapid fission of a mass of or another heavy nucleus is the principle of the atomic bomb, the energy liberated being the destructive power. For useful energy the reaction has to be moderated this is done in a reactor where moderators such as water, heavy water, graphite, beryllium, etc., reduce the number of neutrons and slow those present to the most useful energies. The heat produced in a reactor is removed by normal heat-exchange methods. The neutrons in a reactor may be used for the formation of new isotopes, e.g. the transuranic elements, further fissile materials ( °Pu from or of the... [Pg.44]

The magnitude and shape of such a mean-field potential is shown below [21] in figure B3.1.4 for the two 1 s electrons of a beryllium atom. The Be nucleus is at the origin, and one electron is held fixed 0.13 A from the nucleus, the maximum of the Is orbital s radial probability density. The Coulomb potential experienced by the second electron is then a function of the second electron s position along the v-axis (coimecting the Be nucleus and the first electron) and its distance perpendicular to the v-axis. For simplicity, this second electron... [Pg.2159]

It is known that the oxygen abundance in the interstellar medium increases all the time this nucleus is produced by type 11 supernovas which, one after the other, also contribute their iron production to the Galaxy (Fig. 8.7). The pO mechanism is thus likely to grow in importance as the Galaxy evolves. In other words, clues to the Op mechanism should be sought in the early phases of galactic evolution, that is, in halo stars. The fact remains that the two mechanisms induce different evolution in beryllium and boron as a function of oxygen. [Pg.186]

Atomic numbers are like name tags They identify an element as carbon, nitrogen, beryllium, and so on by telling you the number of protons in the nucleus of that element. Atoms are known by the numbers of their protons. Adding a proton or removing one from the nucleus of an atom changes the elemental identity of an atom. [Pg.35]

In addition, one must consider the possibility of interaction between adjacent groups. This is of particular importance when dealing with the beryllium derivatives in which the metal nucleus is very small and may also be of significance in other systems such as the lithium aggregates. Unfortunately, little quantitative information has appeared with regard to this feature other than statements of distance observed in a few systems. [Pg.238]

An important feature of beryllium amide studies since 1980 has been the acquisition of Be NMR data. NMR signals for this nucleus, which has 100% abundance, 1= 3/2 and a receptivity almost two orders of magnitude greater than the nucleus,can be obtained without major difficulties. Some chemical shift data gathered from Refs. 17,18 and 20 are... [Pg.42]

The difference between these two transitions is that the beryllium has a stronger nuclear charge. Boosting berylliums electron away from the nucleus, therefore, requires more energy. [Pg.687]

Because a 2s electron is on average closer to the nucleus than a 2p electron, it is held more tightly and is harder to remove. Thus, the E of beryllium is larger than that of boron. An alternative way of saying the same thing is to note that the 2p electron of boron is shielded somewhat by the 2s electrons, feels a smaller Zeff, and is thus more easily removed than a 2s electron of beryllium. [Pg.206]


See other pages where Beryllium nucleus is mentioned: [Pg.1620]    [Pg.312]    [Pg.317]    [Pg.23]    [Pg.7]    [Pg.259]    [Pg.40]    [Pg.215]    [Pg.603]    [Pg.3332]    [Pg.5]    [Pg.603]    [Pg.328]    [Pg.355]    [Pg.187]    [Pg.1620]    [Pg.312]    [Pg.317]    [Pg.23]    [Pg.7]    [Pg.259]    [Pg.40]    [Pg.215]    [Pg.603]    [Pg.3332]    [Pg.5]    [Pg.603]    [Pg.328]    [Pg.355]    [Pg.187]    [Pg.1595]    [Pg.34]    [Pg.273]    [Pg.131]    [Pg.240]    [Pg.141]    [Pg.126]    [Pg.73]    [Pg.12]    [Pg.31]    [Pg.80]    [Pg.8]    [Pg.179]    [Pg.1067]    [Pg.1068]    [Pg.157]    [Pg.42]   
See also in sourсe #XX -- [ Pg.22 ]




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