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Nuclear Charge Number

The functions are the associated Legendre polynomials of which a few are given in Table 1.1. They are independent of Z, the nuclear charge number, and therefore are the same for all one-electron atoms. [Pg.13]

It is instructive to look at the form of the Is, 2s and 3s orbitals (Table 9.1). By convention, we use the dimensionless variable p = Zrjaa rather than r. Here 2 is the nuclear charge number and oq the first Bohr radius (approximately 52.9 pm). The quantity Z/n is usually called the orbital exponent, written These exponents have an increasing number of radial nodes, and they are orthonormal. [Pg.157]

Kem-isomer, n. nuclear isomer, ring isomer, -isomerie, /. nucleus (or nuclear) isomerism, -kbrper, m., -korperchen, n. nucleolus, -la-dung,/. nuclear charge main charge, -la-dungszahl, /. nuclear-charge number, atomic number, -leder, n. butt or bend leather. [Pg.242]

Bohr s model of the hydrogen atom. Identification of atomic number with nuclear charge number (H. Moseley). [Pg.400]

In the case of isotopes we are dealing w/ith differing positron counts in the nucleus (mass) of the ion at identical nuclear charge numbers (gas type). Some values for relative isotope frequency are compiled in Table 4.2. [Pg.102]

Fig. 1. Relativistic and QED contributions to the electron g factor for values of the nuclear charge number Z. The data is taken from Ref. [12]... Fig. 1. Relativistic and QED contributions to the electron g factor for values of the nuclear charge number Z. The data is taken from Ref. [12]...
For a given nucleus, having nuclear charge number (atomic number) Z representing its number of nuclear protons and nucleon number (mass number) A representing its total number of nucleons (neutrons + protons), the mass excess of atom (Z, A) is defined by... [Pg.292]

Molecular Properties. Corresponding to its nuclear charge number, the nitrogen atom possesses seven shell electrons. One electron pair in in the ground state 1 s(K shell), and five electrons are distributed over the four orbitals with the principal quantum number 2 (L shell). Of these, one electron pair occupies the 2 s level and three unpaired electrons, respectively, a half of the remaining three levels, 2 px, 2 pv, 2 pz. The unpaired electrons can enter into electron-pair bonds with the 1 s electron of three hydrogen atoms. Thus, the three half occupied orbitals of the L shell become about fully accupied (formation of an octet of the neon type in accordance with the octet theory of Lewis-Langmuir). [Pg.9]

This is called the fine structure of the spectral lines. Its theory was given by Sommerfeld for the case of atoms of the hydrogen type (H, He+, Li++), and was tested by Fowler and Paschen on the spectrum of singly ionized helium (He+), which was found in complete agreement with the theory. The test is easier wdth He+ than with H for this reason, that the eiu. rgy terms of He+ are four times as far apart, on account of the nuclear charge number Z being doubled, w hereas the... [Pg.106]

Fig. 2. Expectation value of the electric field strength for the lowest-lying bound states in hydrogenlike atoms with nuclear charge numbers Z. Fig. 2. Expectation value of the electric field strength for the lowest-lying bound states in hydrogenlike atoms with nuclear charge numbers Z.
The tabulated values were interpolated with a B-spline routine to provide numerical values for any nuclear charge number Z. We display these values in Fig. 11 together with the nonrelativistic reduced mass correction which is included in AErec- For uranium, the total effect to the lsi/2-state is 0.51 eV, including the nonrelativistic correction of 0.30 eV. Compared to the radiative effects discussed so far this might be thought tiny, but an experimental precision of better than 1 eV demands also for the proper calculation of Lamb shift contributions of this size of magnitude. [Pg.138]

Tungsten (W), with an atomic mass of 182.86 and a nuclear charge number of 74, is a shiny metal with a whitish surface and density of 19.3 gcm (Stockinger 1967). [Pg.1141]

For the determination of the log /rvalues nomograms have been constructed. The input data are the experimental maximum P (or K capture) energy, the partial half-life (T1/2), and the nuclear charge number (2) (Wapstra et al. 1959). [Pg.132]

The solution of the Schrodinger equation only needs nuclear charge numbers and simulation environment parameters not involving any empirical parameters within the framework of the first-principles theory. The obtained results are eigenvalues and eigenfunctions of the systems studied, which can derive aU properties of the system from theory. Moreover, the simulated results agree better with the experiment due to the gradual improvement of the models and the calculation procedure as well as the promotion of computation precision. Therefore, the reliability of the... [Pg.173]


See other pages where Nuclear Charge Number is mentioned: [Pg.352]    [Pg.10]    [Pg.3]    [Pg.255]    [Pg.621]    [Pg.800]    [Pg.804]    [Pg.621]    [Pg.800]    [Pg.804]    [Pg.28]    [Pg.3]    [Pg.423]    [Pg.2]    [Pg.8]    [Pg.15]    [Pg.16]    [Pg.29]    [Pg.32]    [Pg.37]    [Pg.79]    [Pg.48]    [Pg.92]    [Pg.115]    [Pg.138]    [Pg.206]    [Pg.240]    [Pg.241]    [Pg.19]    [Pg.58]    [Pg.173]    [Pg.194]    [Pg.221]   
See also in sourсe #XX -- [ Pg.206 ]

See also in sourсe #XX -- [ Pg.1141 ]




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Nuclear charge

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