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Neon, ionization potential

The principal mechanism for analyte response is ionization due to collision with metastable helium atoms. Hetastable helium atoms are generated by multiple collisions with beta electrons from the radioisotopic source. Since the ionization potential of helium (19.8 ev) is higher than that of all other species except neon, then all species entering the ionization chamber will be ionized. [Pg.146]

PENNING EFFECT. An increase in the effective ionization rate of a gas due to the presence of a small number of foreign metastable atoms. For instance, a neon atom has a metastable level at 16.6 volts and if there are a few neon atoms in a gas of argon which has an ionization potential of 15.7 volts, a collision between the neon metastable atom with an argon atom may lead to ionization of the argon. Thus, the energy which is stored in the metastable atom can be used to increase the ionization rate. Other gases where this effect is used are helium, with a metastable level at 19.8 volts, and mercury, with an ionization level at 10.4 volts. [Pg.1221]

A large number of studies have been devoted to measuring the ionization potential in the liquid and the solid phases (see Refs. 179-181, 189, 190). Some of these results are presented in Table VII, from which one can see that for most substances V0 is negative, and so the ionization potential in the condensed phase is smaller than the photoemission threshold Eph. However, for some substances (for instance, for n-pentane, /i-decane, and neon), VQ is positive, meaning that in this case it is more advantageous, from the energy point of view, for an electron to make a transition into vacuum than to remain in a quasi-free state. [Pg.311]

The polarization energy is always negative. Since in most cases V0 is also negative, the ionization potential of a medium lowers with transition from the gaseous state to the condensed one. The only exceptions are those rare cases where V0 is positive and, at the same time, is greater than — P+, as it is for neon. [Pg.313]

The helium ionization detector (HID) is a sensitive universal detector. In the detector, Ti3H2 or Sc3H3 is used as an ionization source of helium. Helium is ionized to the metastable state and possesses an ionization potential of 19.8 eV. As metastable helium has a higher ionization potential than most species except for neon, it will be able to transfer its excitation energy to all other atoms. As other species enter the ionization field the metastable helium will transfer its excitation energy to other species of lower ionization potential, and an increase in ionization will be measured over the standing current. [Pg.311]

Fig. 4.6. Left-hand panels Momentum correlation function (4.20) of the electron momenta parallel to the laser field for nonsequential double ionization computed with the uniform approximation using the contact interaction (4.14b). The field frequency is u> = 0.0551 a.u. and the ponderomotive energy IJP = 1.2 a.u., which corresponds to an intensity of 5.5 x 1014W/cm2. The first two ionization potentials are Soi = 0.79a.u. and I-E02I = 1.51 a.u. corresponding to neon. Panel (a) shows the yield for the case where the transverse momenta pnj (n = 1,2) are completely integrated over, whereas in the remaining panels they are restricted to certain intervals. In panels (6) and (c), p2 is integrated, while 0 < pi /[Up]1/2 < 0.1 and 0.4 < Pi /[Up]1 2 < 0.5, respectively. In panels (d), (e), and (/), both transverse momenta are confined to the intervals 0 < Pn /[Up]1/2 < 0.5, 0.5 < pjn /[Up]1/2 < 1, and 1 < pjn /[Up]1/2 < 1.5, respectively. Right-hand panels, same as left panels, but for the Coulomb interaction (4.14a). From [17]... Fig. 4.6. Left-hand panels Momentum correlation function (4.20) of the electron momenta parallel to the laser field for nonsequential double ionization computed with the uniform approximation using the contact interaction (4.14b). The field frequency is u> = 0.0551 a.u. and the ponderomotive energy IJP = 1.2 a.u., which corresponds to an intensity of 5.5 x 1014W/cm2. The first two ionization potentials are Soi = 0.79a.u. and I-E02I = 1.51 a.u. corresponding to neon. Panel (a) shows the yield for the case where the transverse momenta pnj (n = 1,2) are completely integrated over, whereas in the remaining panels they are restricted to certain intervals. In panels (6) and (c), p2 is integrated, while 0 < pi /[Up]1/2 < 0.1 and 0.4 < Pi /[Up]1 2 < 0.5, respectively. In panels (d), (e), and (/), both transverse momenta are confined to the intervals 0 < Pn /[Up]1/2 < 0.5, 0.5 < pjn /[Up]1/2 < 1, and 1 < pjn /[Up]1/2 < 1.5, respectively. Right-hand panels, same as left panels, but for the Coulomb interaction (4.14a). From [17]...
Since the ionization potential of neon is greater than that of lithium, the equilibrium constant reduces to zero at the absolute zero, showing that at low temperatures the lithium is ionized, the neon unionized. In other words, the element of low ionization potential, or the electropositive4 element, tends to lose electrons to the more electronegative element, with high ionization potential. This tendency is complete at the absolute zero. At higher temperatures, however, as the mass action law shows, there will be an equilibrium with some of each element ionized. [Pg.335]

The chemical counterpart of the roof will be a set of valence-shell electrons, and we shall look at atomic and molecular architectures that can be hosted under such a roof when bringing in stable nuclei and corresponding core electrons. In order to see what happens with such an idea in a Chemical Aufbau approach, let us start with an octet of electrons under which we place a nucleus with atomic number Z = 10 and a K-shell with two core electrons. The result is a neon atom, an exceptionally stable architecture with spherical (three-dimensional) symmetry. The same result would happen for Z = 18 (argon) with one more "floor", and so on or the following noble gas atoms. Actually, we start with the closed electronic shells allowed by the Pauli Exclusion Principle and the "n ( Rule", and we supply the nuclei corresponding to such shells. The proof for the stability of this architecture is provided by the high ionization potential and the low electron affinity. [Pg.62]

The symbol IP refers to the ionization potential of the least bound electrons on the indicated species. From the electron affinity of fluorine (3.4 eV) and the first ionization potential for neon (21.6 eV), we have k = 18.2 eV, in agreement with the Hartree-Fock values. [Pg.118]

Chandra ACIS observations of SN 1995N show a best-fit line energy at 1.02 keV which is ascribed to Ne X [170]. There is also the possibility of another line with best-fit line energy at 0.85 keV with identification as Ne IX. The ionization potentials of all ionized Neon species upto Ne VIII are less than 240 eV, whereas those of Ne IX and Ne X are above 1195 eV. Hence at temperatures found by the Chandra observations, the predominant species of Neon are expected to be Ne X and Ne XI. The mass of Neon was estimated... [Pg.269]

Argon (Ar) gas, for example, is over 30 times more abundant than carbon dioxide and, therefore, not rare. And xenon is not inert it s first compounds were created in 1962. When xenon (Xe) forms binary fluorides and oxides as well as fluoride complexes and oxoanions, the stability of these compounds is very low. It s reactivity is related to increasing atomic size as you go down the table, which leads to a decrease in the first ionization potentials. Xenon tetraflouride (XeF,) is made by mixing one part xenon gas to three parts fluorine gas in a container at 400 °C. Compounds have been confirmed for argon (HArF), krypton (KrF2), xenon (numerous fluorides, oxyfluorides, and oxides), and radon (RnF2). It s believed that compounds exist with helium and neon as well, though none have been experimentally proven to date. [Pg.204]

Associative ionization is not restricted to the formation of dimer ions by reaction (1) in pure gases. On the contrary, associative ionization is now known to be a quite general phenomenon that occurs in a variety of gas mixtures. In 1957, Pahl and Weimer observed that HeNe was formed in the positive column of a discharge in helium-neon mixtures. It was subsequently shown in mass spectrometric studies " that the appearance potential of the HeNe" ion is of the order of 23.0 eV (Table IV). Since this minimum excitation energy lies above the ionization potential of neon and is nearly the same as the appearance potential of it is most probable that the same set of excited states of helium that produce He2 also form HeNe, namely... [Pg.266]

Since the appearance potential of HeNe" lies above the ionization potential of neon, the reaction... [Pg.267]


See other pages where Neon, ionization potential is mentioned: [Pg.228]    [Pg.564]    [Pg.86]    [Pg.393]    [Pg.248]    [Pg.248]    [Pg.19]    [Pg.351]    [Pg.98]    [Pg.401]    [Pg.152]    [Pg.164]    [Pg.722]    [Pg.68]    [Pg.304]    [Pg.144]    [Pg.20]    [Pg.21]    [Pg.40]    [Pg.31]    [Pg.360]    [Pg.22]    [Pg.807]    [Pg.250]    [Pg.36]    [Pg.250]    [Pg.252]    [Pg.252]    [Pg.248]    [Pg.5]    [Pg.23]    [Pg.150]    [Pg.206]   
See also in sourсe #XX -- [ Pg.80 ]




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