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Nitrogen Noble gas

Kistemaker P. G., de Vries A. E. Rotational relaxation times in nitrogen-noble-gas mixtures, Chem. Phys. 7, 371-82 (1975). [Pg.290]

For this purpose, one should measure variation of electric conductivity of one and the same movable sensor in the saturated vapour-gas phase and in a liquid, caused by the presence of any given concentration of oxygen in a carrier gas (hydrogen, nitrogen, noble gas, etc.). From the results of these measurements the Bunsen coefficient P can be found in accordance with the relation (see Chapter 3, Section 4)... [Pg.262]

There is not much information on neutral nitrogen-noble gas compounds except some indications that a few weakly bound van der Waals complexes and exciplexes do exist. [Pg.1]

Nitrogen-noble gas monocations have been detected mass-spectrometrically for the noble gases He, Ne, Ar, Kr, and Xe some of them have also been studied spectroscopically. The major portion of this chapter deals with cations formed by argon. They comprise simple molecular cations such as ArN, ArNj as well as cluster ions of the type Ar N n with m up to 15 and n up to 23. [Pg.1]

HeN , the only nitrogen-noble gas anion described, is predicted to be unbound. [Pg.1]

There is some information on various nitrogen-noble gas species, to a large extent because of the interest in their bonding behavior. Experimental data have been obtained chiefly for some singly charged cations, particularly those formed by argon like ArN and ArNj. The existence of others has only been established by mass spectrometry. [Pg.288]

Octet rule (Section 1 3) When forming compounds atoms gain lose or share electrons so that the number of their va lence electrons is the same as that of the nearest noble gas For the elements carbon nitrogen oxygen and the halo gens this number is 8... [Pg.1290]

The atom probe field-ion microscope (APFIM) and its subsequent developments, the position-sensitive atom probe (POSAP) and the pulsed laser atom probe (PLAP), have the ultimate sensitivity in compositional analysis (i.e. single atoms). FIM is purely an imaging technique in which the specimen in the form of a needle with a very fine point (radius 10-100 nm) is at low temperature (liquid nitrogen or helium) and surrounded by a noble gas (He, Ne, or Ar) at 10 -10 Pa. A fluorescent screen or a... [Pg.179]

The number of covalent bonds an atom forms depends on how many additional valence electrons it needs to reach a noble-gas configuration. Hydrogen has one valence electron (Is) and needs one more to reach the helium configuration (Is2), so it forms one bond. Carbon has four valence electrons (2s2 2p2) and needs four more to reach the neon configuration (2s2 2p6), so it forms four bonds. Nitrogen has five valence electrons (2s2 2p3), needs three more, and forms three bonds oxygen has six valence electrons (2s2 2p4), needs two more, and forms two bonds and the halogens have seven valence electrons, need one more, and form one bond. [Pg.9]

At least since the mid-19th century, it has never been claimed that molecular nitrogen is completely unreactive with organic reagents. It was, however, known that many reactions that cannot be carried out in air because of reactions with oxygen, can be performed in a so-called inert atmosphere consisting of either a noble gas or — more cheaply — N2. This is common knowledge to the experimental chemist. [Pg.216]

NOx An oxide, or mixture of oxides, of nitrogen, typically in atmospheric chemistry, noble gas A member of Group 18/VIlI of the periodic table (the helium family). [Pg.959]

In 1894, the Scottish chemist William Ramsay removed nitrogen and oxygen from air through chemical reactions. From the residue, Ramsay Isolated argon, the first noble gas to be discovered. A year after discovering argon, Ramsay obtained an unreactive gas from uranium-containing mineral samples. The gas exhibited the same spectral lines that had been observed in the solar eclipse of 1868. After helium was shown to exist on Earth, this new element was studied and characterized. [Pg.461]

Stable noble gas compounds are restricted to those of xenon. Most of these compounds involve bonds between xenon and the most electronegative elements, fluorine and oxygen. More exotic compounds containing Xe—S, Xe—H, and Xe—C bonds can be formed under carefully controlled conditions, for example in solid matrices at liquid nitrogen temperature. The three Lewis structures below are examples of these compounds in which the xenon atom has a steric munber of 5 and trigonal bipyramidal electron group geometry. [Pg.627]

Scuba tanks usually contain compressed air, which is essentially a mixture of nitrogen (78%) and oxygen (21%). In order to avoid a painful condition called the bends, deep-sea divers replace the nitrogen with the noble gas —... [Pg.13]

The nitrogen complex had already been synthesized in a solid matrix, but its decomposition kinetics and its further photolysis could be studied only in solution. The liquid noble gas technique is superior to the solid matrix technique, especially for the synthesis of multiple substituted chromium carbonyl nitrogen complexes. Their IR spectra were extremely complex in matrices, due to "site splittings" which arise when different molecules are trapped in different matrix environments /18/. [Pg.149]

Next, we need to distribute the remaining electrons to achieve a noble gas electron configuration for each atom. Since four electrons were used to form the two covalent single bonds, fourteen electrons remain to be distributed. By convention, the valence shells for the terminal atoms are filled first. If we follow this convention, we can close the valence shells for both the nitrogen and the chlorine atoms with twelve electrons. [Pg.206]

Professor of physics at Cavendish Laboratory, Cambridge. He made elaborate investigations of the electrochemical equivalent of silver and of the combining volumes and compressibilities of gases. His observation that nitrogen prepared from the atmosphere is heavier than nitrogen prepared from ammonia led to the discovery of argon, the first noble gas. He also contributed to optics and acoustics. [Pg.780]

Most carbenes are relatively easily generated by photolysis of nitrogeneous precursors such as diazo compoundsor diazirines. The reaction is clean, as nitrogen is the only byproduct and it is also very efficient as nitrogen evolution is a highly exothermic reaction. Therefore carbenes can be easily generated even under very inert conditions, such as in a noble gas matrix at very low temperatures. [Pg.383]

Fluorine is the most energetic oxidizing element and as such is of prime importance in advanced oxidizers. The fluorine-based oxidizers discussed here include elemental fluorine, compounds containing oxygen and fluorine, nitrogen-fluorine compounds, halogen fluorides, and noble gas fluorides. [Pg.337]


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Compounds of Nitrogen with Hydrogen and Noble Gases

HYDROGEN, NITROGEN, AND NOBLE GASES

Neutral Nitrogen-Noble Gas Compounds

Nitrogen gas

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