The negative ions of atomic and molecular oxygen

The properties, modes of formation and of destruction of the negative ions of atomic and molecular oxygen are examined in detail, using quantal theory to interpret and amplify the somewhat meagre experimental information. A detailed examination of the (Lf)2 (2j)2 (2/>)4 (3s) excited configuration of O - is made in an attempt to decide whether it can give rise to the observed stable excited state in which the attached electron has nearly zero binding energy. This is important in attachment, detachment and electron scattering phenomena as resonance effects will occur if the configuration is on the verge of stability or instability. The Hartree-Fock equations have been solved for the deepest (4P and 2P) terms of this configuration, polarization effects being allowed for by the introduction of a term involving a polarizability p regarded as an adjustable parameter. Stable excited P terms are only found when p is two to four times as large as the polarizability of O deduced from the refractivity of 0 2. This does not completely exclude identification of the excited state as belonging to the configuration considered. To examine the possible resonance effects, radiative attachment and detachment rates are calculated for a variety of values of the polarizability parameter p. The rapid variation of these quantities with p in the region where a real or virtual level of the 3^ electron, with small energy, exists makes it unlikely that definite theoretical values can be given until more information as to the proper value of p is forthcoming. Meanwhile, the parameter p provides a convenient correlation of the probabilities of the two processes with the energy of the 3* electron. The other possible attachment and detachment processes involving O and 0 ~ are also discussed. In order to interpret experiments on attachments of electron swarms in 0 2 and to decide how to extrapolate the results to low pressures, the deep electronic states of O^" are considered in detail, employing the empirical methods commonly used in studying molecular structure. It is found that their distribution is such as to make it most unlikely that Ofl~ ions can be formed with appreciable probability by attachment of slow electrons to Oz at low pressures, by a pressure-independent process other than direct radiative attachment. However, considerable difficulties and uncertainties are found in attempting a detailed interpretation of the experimental results at the higher pressures and more experiments are required. In the final section the formation of pairs of oppositely charged ions from molecules by impact of electrons or light quanta is investigated in terms of the theory of the crossing of molecular potentialenergy curves. The same theory is also applied to obtain information as to the possible magnitude of the cross-section for mutual neutralization of oppositely charged ions by electron transfer on impact. It is shown that a cross-section of between 10~13 and 10-12 cm.2 is quite likely to occur for atomic oxygen ions, but the occurrence of one as high as 1CH1 cm.2 is most unlikely. A detailed summary of results and conclusions is given.

The electrical conductivity which is imparted to gases by their exposure to Röntgen rays has been explained by J. J. Thomson and E. Rutherford on the hypothesis of a formation of oppositely charged carriers throughout the volume of the gas. The motion of these carriers or ions when in an electric field constitutes the observed conductivity, and the recovery of the insulating property of a gas after an exposure to the rays is due partly to the recombination of the oppositely charged ions and partly to their impact with the boundaries. An estimate of the sum of the velocities with which the positive and negative ions move in air when in a unit electric field was first obtained by J. J. Thomson and E. Rutherford, and later E. Rutherford, by the same indirect method, determined the sum of the velocities of the ions in a number of gases. This method involved the determination of the rate of recombination of the ions, the saturation current obtained through the gas by the use of a strong electric field, and the current obtained with some small non-saturating electric force. E. Rutherford also describes an experiment in which the velocities of the two ions in air were obtained separately by a direct method, and found to be approximately equal. The writer has since shown that in general the two velocities are not equal, and for those gases for which the ratio of the two velocities was determined the negative ion moved the faster in nearly all cases.


2020 ◽  
Vol 2020 (8) ◽  
Author(s):  
H. Hernández-Arellano ◽  
M. Napsuciale ◽  
S. Rodríguez

Abstract In this work we study the possibility that the gamma ray excess (GRE) at the Milky Way galactic center come from the annihilation of dark matter with a (1, 0) ⊕ (0, 1) space-time structure (spin-one dark matter, SODM). We calculate the production of prompt photons from initial state radiation, internal bremsstrahlung, final state radiation including the emission from the decay products of the μ, τ or hadronization of quarks. Next we study the delayed photon emission from the inverse Compton scattering (ICS) of electrons (produced directly or in the prompt decay of μ, τ leptons or in the hadronization of quarks produced in the annihilation of SODM) with the cosmic microwave background or starlight. All these mechanisms yield significant contributions only for Higgs resonant exchange, i.e. for M ≈ MH /2, and the results depend on the Higgs scalar coupling to SODM, gs. The dominant mechanism at the GRE bump is the prompt photon production in the hadronization of b quarks produced in $$ \overline{D}D\to \overline{b}b $$ D ¯ D → b ¯ b , whereas the delayed photon emission from the ICS of electrons coming from the hadronization of b quarks produced in the same reaction dominates at low energies (ω < 0.3 GeV ) and prompt photons from c and τ , as well as from internal bremsstrahlung, yield competitive contributions at the end point of the spectrum (ω ≥ 30 GeV ). Taking into account all these contributions, our results for photons produced in the annihilation of SODM are in good agreement with the GRE data for gs ∈ [0.98, 1.01] × 10−3 and M ∈ [62.470, 62.505] GeV . We study the consistency of the corresponding results for the dark matter relic density, the spin-independent dark matter-nucleon cross-section σp and the cross section for the annihilation of dark matter into $$ \overline{b}b $$ b ¯ b , τ+τ−, μ+μ− and γγ, taking into account the Higgs resonance effects, finding consistent results in all cases.


A theory is developed which describes the scattering of radio waves by the random thermal fluctuations of electron density in a collision-free plasma. The frequency spectrum, as well as the amplitude, of the scattered radiation is calculated. Particular attention is paid to the part of the spectrum which corresponds to small Doppler shifts, this being the region of greatest significance in connexion with the phenomenon of incoherent scattering from the ionosphere. The calculations are based on a generalized version of Nyquist’s noise theorem, and they lead to the following conclusions: (1) The mean scattering cross-section for the ionosphere is equal to that which would exist if each of the electrons scattered independently with a cross-section of one-half the classical Thomson cross-section. (2) The mean Doppler broadening of the scattered signal corresponds roughly to the speed of the ions rather than to that of the electrons. (3) The spectral shape of this signal is not Gaussian. There is a mild maximum in the spectrum away from the central frequency, as can be seen in figure 1. (4) Plasma resonance effects contribute only negligibly to the scattering for frequencies currently of interest.


Author(s):  
Mars V. Muftakhov ◽  
Yury V. Vasil’ev ◽  
Rustem V. Khatymov ◽  
Victor A. Mazunov ◽  
Vyatcheslav V. Takhistov ◽  
...  
Keyword(s):  

1968 ◽  
Vol 21 (3) ◽  
pp. 239 ◽  
Author(s):  
FC Barker ◽  
HJ Hay ◽  
PB Treacy

The light even nuclei with A ;;;. 10 have 0+ excited states near 6 MeV, probably with large (X-particle reduced widths. A similar state in BBe would be very broad. Evidence for 0+ excited states in BBe has been obtained here using many-level R-matrix fits to known (X-(X scattering data, but the excitation energies depend strongly on the assumed channel radius. For a simultaneous fit to the 9Be(p, d)BBe cross section, assuming these higher states are not strongly populated, the channel radius is restricted to (7~~) fm, implying a 0+ excited state at (6=f3) MeV of width (9=f4) MeV.


Molecules ◽  
2020 ◽  
Vol 25 (5) ◽  
pp. 1038 ◽  
Author(s):  
Raphael C. Mordi ◽  
Olabisi T. Ademosun ◽  
Christiana O. Ajanaku ◽  
Ifedolapo O. Olanrewaju ◽  
John C. Walton

This article reviews the excited-state quenching, pro-vitamin A activity and anticarcinogenicity of carotenes and xanthophylls in relation to their chemical structures. Excited-state quenching improved with the length of the conjugated chain structure. Pro-vitamin A activity was dependent on the presence of at least one beta-ionyl ring structure. The effectiveness of carotenoids as antioxidants depended on their ability to trap peroxyl radicals with production of resonance-stabilized carotenyl radicals. The products identified from oxidations of carotenes and xanthophylls with molecular oxygen and other oxidizing agents are presented. The free radical-mediated mechanisms that have been proposed to account for the different classes of products are reviewed.


2019 ◽  
Vol 15 ◽  
pp. 2438-2446 ◽  
Author(s):  
Alessandro Iagatti ◽  
Baihao Shao ◽  
Alberto Credi ◽  
Barbara Ventura ◽  
Ivan Aprahamian ◽  
...  

In this work we apply a combination of steady state and time resolved luminescence and absorption spectroscopies to investigate the excited-state dynamics of a recently developed molecular photoswitch, belonging to the hydrazone family. The outstanding properties of this molecule, involving fluorescence toggling, bistability, high isomerization quantum yield and non-negligible two-photon absorption cross section, make it very promising for numerous applications. Here we show that the light induced Z/E isomerization occurs on a fast <1 ps timescale in both toluene and acetonitrile, while the excited state lifetime of the Z-form depends on solvent polarity, suggesting a partial charge transfer nature of its low lying excited state. Time-resolved luminescence measurements evidence the presence of a main emission component in the 500–520 nm spectral range, attributed to the Z-isomer, and a very short living blue-shifted emission, attributed to the E-isomer. Finally, transient absorption measurements performed upon far-red excitation are employed as an alternative method to determine the two-photon absorption cross-section of the molecule.


2018 ◽  
Vol 2018 ◽  
pp. 1-16 ◽  
Author(s):  
F. Ramírez-Sánhez ◽  
A. Gutiérrez-Rodríguez ◽  
Alejandro González-Sánchez ◽  
M. A. Hernández-Ruíz

We study the production sensitivity of Higgs bosons h and H, in relation to the possible existence of Z′ boson and a top quark pair at the energy scales that will be reached in the near future at projected e+e- linear colliders. We focus on the resonance and no-resonance effects of the annihilation processes e+e-→(γ,Z,Z′)→tt-h and e+e-→(γ,Z,Z′)→tt-H. Furthermore, we develop and present novel analytical formulas to assess the total cross section involved in the production of Higgs bosons. We find that the possibility of performing precision measurements for the Higgs bosons h and H and for the Z′ boson is very promising at future e+e- linear colliders.


Sign in / Sign up

Export Citation Format

Share Document