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Elements counting atoms

With modern detectors and electronics most Enei -Dispersive X-Ray Spectroscopy (EDS) systems can detect X rays from all the elements in the periodic table above beryllium, Z= 4, if present in sufficient quantity. The minimum detection limit (MDL) for elements with atomic numbers greater than Z = 11 is as low as 0.02% wt., if the peaks are isolated and the spectrum has a total of at least 2.5 X 10 counts. In practice, however, with EDS on an electron microscope, the MDL is about 0.1% wt. because of a high background count and broad peaks. Under conditions in which the peaks are severely overlapped, the MDL may be only 1—2% wt. For elements with Z < 10, the MDL is usually around 1—2% wt. under the best conditions, especially in electron-beam instruments. [Pg.120]

Count atoms of each element to see if the elements are in balance ... [Pg.204]

Multiple bonds to an element count as multiple single bonds to that element. That is, the carbon-oxygen double bond of carbonyl group (C=0) is oxidatively equivalent to a carbon atom with two single bonds to oxygen originating from it (-O-C-O-). [Pg.33]

How can you use this relationship to relate mass and moles The periodic table tells us the average mass of a single atom in atomic mass units (u). For example, zinc has an average atomic mass of 65.39 u. One mole of an element has a mass expressed in grams numerically equivalent to the element s average atomic mass expressed in atomic mass units. One mole of zinc atoms has a mass of 65.39 g. This relationship allows chemists to use a balance to count atoms. You can use the periodic table to determine the mass of one mole of an element. [Pg.180]

In addition, quantitative and qualitative elemental analysis of inorganic compounds with high accuracy and high sensitivity can be effected by mass spectrometry. For elemental analysis, atomization of the analysed sample that corresponds to the transformation of solid matter in atomic vapour and ionization of these atoms occur in the source. These atoms are then sorted and counted with the help of mass spectrometry. The complete decomposition of the sample in the ionization source into its constituent atoms is necessary because incomplete decomposition results in complex mass spectra in which isobaric overlap might cause unsuspected spectral interferences. Furthermore, the distribution of any element in different species leads to a decrease in sensitivity for this element. [Pg.65]

With our broad definition in mind, we find that there are now some 56 transition elements, counting the heaviest elements through the one of atomic number 104. Clearly the majority of all known elements are transition elements. All these transition elements have certain general properties in common ... [Pg.633]

The circumstances under which intermetallics form were elucidated by the British metallurgist William Hume-Rothery (1899-1968) for compounds between the noble metals and the elements to their right in the periodic table (Hume-Rothery, 1934 Reynolds and Hume-Rothery, 1937). These are now applied to all intermetaUic compounds, in general. The converse to an intermetaUic, a solid solution, is only stable for certain valence-electron count per atom ratios, and with minimal differences in the atomic radii, electronegativities, and crystal structures (bonding preferences) of the pure components. For example, it is a mle-of-thumb that elements with atomic radii differing by more than 15 percent generally have very little solid phase miscibility. [Pg.145]

The meaning of a chemical formula was discussed in Chapter 5, and we learned how to interpret formulas in terms of the numbers of atoms of each element per formula unit. In this chapter, we will learn how to calculate the number of grams of each element in any given quantity of a compound from its formula and to do other calculations involving formulas. Formula masses are presented in Section 7.1, and percent composition is considered in Section 7.2. Section 7.3 discusses the mole—the basic chemical quantity of any substance. Moles can be used to count atoms, molecules, or ions and to calculate the mass of any known number of formula units of a substance. Section 7.4 shows how to use relative mass data to determine empirical formulas, and the method is extended to molecular formulas in Section 7.5. [Pg.197]

The situation is similar in counting atoms, but much more difficult. Individual atoms cannot be seen to be counted, nor can they be weighed in the ordinary manner. Still, if the mass of 1 atom can be determined (in amu, for example) the number of atoms in a mole can be calculated. Historically, what chemists have done in effect is to weigh very large numbers of atoms of different elements where the ratio of atoms of the elements is known they have gotten the ratio of the masses of individual atoms from the ratio of the mass of the different elements and the relative numbers of atoms of the elements. [Pg.105]

The determination of sodium by atomic absorption spectroscopy has been applied successfully by several workers using a variety of equipment. The first element to be determined by Alkemade and Milatz (A2), in fact, was sodium. While sensitivity in emission is slightly higher for this metal than sensitivity in absorption, sodium still counts as one of the most sensitive elements in atomic absorption spectroscopy. The absence of any spectral interference (P3) and the relative freedom from other interferences appear to offer promising advantages of absorption over emission also for this element. [Pg.38]

Count atoms of each element frequently as you try different coefficients. Watch for elements whose atoms become unbalanced as a result of your work. [Pg.286]

Each uth row sum of the atom-type autocorrelation matrix is the number of vertices of any type located at distance k from vertices of type u if all the graph vertices are assigned an atom type, then the Wiener-type index of the matrix gives the graph distance count of order k. Note that since diagonal elements of atom-type autocorrelation matrices can be different from zero, the —> Wiener operator has to be applied as the following ... [Pg.922]

These are simple molecular descriptors based on counting the defined elements of a compound. The most common chemical count descriptors are —> atom number A, —> bond number B, cyclomatic number C, hydrogen-bond acceptor number, and —> hydrogen-bond donor number, distance-counting descriptors, —> path counts, —> walk counts, atom pairs, and other related —> substructure descriptors. [Pg.1261]

ZA and ZB are the valences of the pure elements counting s and p-states only. The mean number density n0 = 1 / 20 of the liquid state has been used as an approximation assuming the ionic volume of the individual atoms as concentration independent ... [Pg.175]

Now let s take similar steps to count atoms of the element carbon. Because of the size and number of carbon atoms in any normal sample of carbon, it is impossible to count the atoms direcdy. Therefore, we want to develop a way of converting from mass of carbon, which we can measure, to the number of carbon atoms. To do this, we will follow steps that are similar to those we followed to count nails by weighing. [Pg.332]

If you missed 16, go to Elements Moles and Counting Atoms, page 114. [Pg.8]

If you want to count atoms, Avogadro s number must be part of the solution. Keep in mind that 1 mole of any element represents 6.022 x 1023 atoms of that element. This fact provides the necessary equality to develop two conversion factors. In terms of iron, Fe ... [Pg.114]

A balanced equation has the same number of atoms of each element on both sides of the arrow. Because atoms are neither destroyed nor created in chemical reactions, every atom must be accounted for. If there are 10 carbon atoms in the reactants, there must be 10 carbon atoms in the products. Because every atom is accounted for, a balanced equation always obeys the Law of Conservation of Mass. It is important that you know how to balance chemical equations. Most equations are not difficult to balance, but you have to pay attention to the details of counting atoms. [Pg.160]

Geiger Flow-proportional Proportional Scintillation Routine control analysis where low counting rates and physical discrimination are adequate. Determination of all elements of atomic number 24 or below. Unique applications where the maximum resolution of a detector is required. Determination of all elements of atomic number 25 and above. [Pg.393]

The mole is often referred to as a chemist s unit of quantity. Counting atoms is a difficult process and beyond the scope of most calculators, but measuring the mass of a sample is easy when we can relate the number of atoms in a sample to its mass. This is the unique purpose of the mole. A mole of any substance is its molecular formula weight expressed in grams. Avogadro s number s a universal constant that states the number of molecules in a mole Nq = 6.023 x 10 molecules/mole. One mole (abbreviated mol) of any element (chemical compound) has the same number of chemical particles as one mole of another element (chemical compound). In other words, 1 mole of any compound contains 6.02 x 10 molecules. Review the following problem using the mole concept. [Pg.397]


See other pages where Elements counting atoms is mentioned: [Pg.117]    [Pg.117]    [Pg.117]    [Pg.117]    [Pg.83]    [Pg.630]    [Pg.62]    [Pg.212]    [Pg.270]    [Pg.518]    [Pg.19]    [Pg.35]    [Pg.192]    [Pg.201]    [Pg.193]    [Pg.114]    [Pg.160]    [Pg.25]    [Pg.83]    [Pg.25]    [Pg.211]    [Pg.1]    [Pg.75]    [Pg.173]    [Pg.155]    [Pg.296]    [Pg.297]    [Pg.259]    [Pg.166]   
See also in sourсe #XX -- [ Pg.114 , Pg.115 ]




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