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Nuclear processes

Limitations may be imposed on activation analysis by conflicting nuclear processes. These have been mentioned above as becoming of increasing importance in neutron activation when the particle energy increases above that necessary to bring about the required interaction. [Pg.331]

In the nuclear reactor the normal reaction used in activation analysis is the (n,y) induced by thermal neutrons but there are several routes by which a nuclide A of atomic number Z and mass M may be produced  [Pg.331]

The following are indirect methods of forming the radio-nuclide 7a. [Pg.331]

Isotopes of elements of intermediate mass number may be formed by nuclear fission of heavy elements. [Pg.331]

The more important of these reactions will be considered below. Reactions 3, and 4 are brought about by the fast neutron flux in the pile, which flux Mellish et al. 59) calculated to be 0.17 of the slow flux in the center of the Harwell pile (BEPO). Fortunately, however, the cross sections for these reactions are usually considerably lower than those for normal (TO,y) reactions induced by thermal neutrons. Contributions brought about by n,p) and (to, ) reactions can often be greatly reduced, as mentioned previously, by irradiating in the thermal column of the reactor, with some loss of sensitivity. Reaction 4, in,2n), is produced by [Pg.331]


The decay of radioisotopes iavolves both the decay modes of the nucleus and the associated radiations that are emitted from the nucleus. In addition, the resulting excitation of the atomic electrons, the deexcitation of the atom, and the radiations associated with these processes all play a role. Some of the atomic processes, such as the emission of K x-rays, are inherently independent of the nuclear processes that cause them. There are others, such as internal conversion, where the nuclear and atomic processes are closely related. [Pg.448]

Several important applications of fluid beds exist outside the petroleum industry. Fluid bed roasting of pyritic ores is widely used in the metallurgical industry. Calcination of lime is a commercial process. There are also fluidization processes for various nuclear processing steps. [Pg.28]

Humans control all chemical and nuclear processes, and to some extent all accidents result from human error, if not directly in the accident then in the process design and in the process inadequate design to prevent human error. Some automatic systems such used in nuclear power reactors because the response time required is too short for human decisions. Even in these, human error can contribute to failure by inhibiting the systems. [Pg.163]

C. F. Powell (Bristol) development of the photographic method of studying nuclear processes and discoveries regarding mesons made with this method. [Pg.1302]

Deuterium occurs naturally, mixed m with plain hydrogen in the tiny proportion of 0.015 percent in other words, plain hydrogen is the more common isotope by a factor of 6,600. Tritium for fusion energy can be created from another nuclear process involving the interaction of the neutron (in the equation above) with lithium ... [Pg.874]

The shaking and continuous filters are regenerative, but there is a third group usually associated with ventilation work rather than dust and fume. These are throwaway filters, which, as the name implies, means that when they become too caked with dust to operate correctly the filters are removed and replaced with new ones. They will only handle low incoming dust burdens, but their efficiencies are the highest of any filter. Typical applications are fresh air input plants, clean-room filtration and nuclear processes. [Pg.769]

Sflf-Test 13.8B Soil at the Rocky Flats Nuclear Processing Facility in Colorado was found to be contaminated with radioactive plutonium-239, which has a half-life of 24 ka (2.4 X 104 years). The soil was loaded into drums for storage. How many years must pass before the radioactivity drops to 20.% of its initial value ... [Pg.665]

What Do We Need to Know Already Nuclear processes can be understood in terms of atomic structure (Section B and Chapter 1) and energy changes (Chapter 6). The section on rates of radioactive decay builds on chemical kinetics (particularly Sections 13.4 and 13.5). [Pg.818]

Consider any region of space that has a hnite volume and prescribed boundaries that unambiguously separate the region from the rest of the universe. Such a region is called a control volume, and the laws of conservation of mass and energy may be applied to it. We ignore nuclear processes so that there are separate conservation laws for mass and energy. For mass. [Pg.1]

Each different unstable isotope has its own characteristic rate of decomposition. Some isotopes survive for only a fraction of a second, but others decompose slowly, sometimes over thousands of years. Most of chemistry involves the stable isotopes, so we defer further consideration of nuclear decomposition until Chapter 22, which covers nuclear processes In detail. [Pg.91]

One hundred years after the discovery of radioactivity and fifty years after the dawn of the nuclear age, society continues to debate the benefits and costs of nuclear technology. Understanding nuclear transformations and the properties of radioactivity is necessary for intelligent discussions of the nuclear dilemma. In this chapter, we explore the nucleus and the nuclear processes that it undergoes. We describe the factors that make nuclei stable or unstable, the various types of nuclear reactions that can occur, and the effects and applications of radioactivity. [Pg.1554]

For a steady-state process the accumulation term will be zero. Except in nuclear processes, mass is neither generated nor consumed but if a chemical reaction takes place a particular chemical species may be formed or consumed in the process. If there is no chemical reaction the steady-state balance reduces to... [Pg.35]

As with mass, energy can be considered to be separately conserved in all but nuclear processes. [Pg.60]

Chemical elements including technetium are being produced in nuclear reactions occurring in the stars today. This has been proved by observing of the presence of technetium in some stars [1]. Technetium has no stable isotopes and none of the technetium isotopes has a half-life long enough to survive the age of the universe. So the technetium observed must have been synthesized by nuclear processes in the stars. [Pg.6]

Fig. 9. Formation of the TcCp2-radical from a chemical and b nuclear processes, and abstraction... Fig. 9. Formation of the TcCp2-radical from a chemical and b nuclear processes, and abstraction...
Synthesis during nuclear processes occurring in the interior of the sun. [Pg.33]

Fig. 2.1. Energy and temperature scales for chemical and nuclear processes. The scale on the left shows temperature, and that on the right indicates the average thermal energy for the particles present. Column (a) shows typical environments with different temperatures (b) shows the stable forms of matter present (c) indicates the types of reaction possible (1.0 eV = 23.06 kcals mol-1) (reproduced with permission from Cox, P.A. (1989)). Fig. 2.1. Energy and temperature scales for chemical and nuclear processes. The scale on the left shows temperature, and that on the right indicates the average thermal energy for the particles present. Column (a) shows typical environments with different temperatures (b) shows the stable forms of matter present (c) indicates the types of reaction possible (1.0 eV = 23.06 kcals mol-1) (reproduced with permission from Cox, P.A. (1989)).
Wexler, S., Primary Physical and Chemical Effects Associated with Emission of Radiation in Nuclear Processes, Acta Chem. Biol. Radiat. 3 148 (1965). [Pg.266]

Linked to 1) is of course the enrichment of the interstellar medium, to which they are important contributors in nuclearly processed elements as He, C, N, s-elements (Ba etc). Goal 2) can be pursued with nuclearly unprocessed elements , the best accessible of them being O, Ne, Ar and S. [Pg.29]

Recent observations of the HF (1-0) R9 line at 2.3 /tm with the Phoenix spectrograph on the Gemini-South telescope has opened a new window that sheds light on understanding the chemical evolution of fluorine and the nuclear processes that produce this element. Until recently, only a small number of observations of fluorine were available and the trend of fluorine abundances with metallicity had yet to be probed in the Galaxy. [Pg.46]

In this framework the different nuclear processes which produce or destroy Li, Be and B must be studied in details and an accurate knowledge of the involved nuclear cross sections are necessary. In particular we will focus our attention on one of the main destruction channels for these elements in stellar environments, the (p, a) reactions. [Pg.171]


See other pages where Nuclear processes is mentioned: [Pg.459]    [Pg.454]    [Pg.455]    [Pg.477]    [Pg.110]    [Pg.320]    [Pg.51]    [Pg.429]    [Pg.1120]    [Pg.232]    [Pg.116]    [Pg.10]    [Pg.818]    [Pg.19]    [Pg.165]    [Pg.209]    [Pg.310]    [Pg.326]    [Pg.309]    [Pg.1562]    [Pg.1564]    [Pg.1574]    [Pg.303]    [Pg.665]    [Pg.46]    [Pg.15]    [Pg.324]    [Pg.37]    [Pg.311]   
See also in sourсe #XX -- [ Pg.948 , Pg.949 , Pg.950 , Pg.951 , Pg.952 ]

See also in sourсe #XX -- [ Pg.1236 ]




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Cooperative electron-y-nuclear process

Corrosion Process for Nuclear Waste Glasses

Critical nuclear process

Exothermic reactions nuclear processes

Fuels nuclear, chemical process steps

Neutron activation analysis nuclear processes

New Isotopes Can Be Produced Through the Process of Nuclear Transmutation

Nitrogen nuclear processes

Non-nuclear (process) instrumentation

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Nuclear PUREX process

Nuclear chemistry decay process

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Nuclear magnetic resonance relaxation processes

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Nuclear scattering processes, schematic

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Subcritical nuclear process

Supercritical nuclear processes

The process of nuclear fission

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