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Beryllium

Chemical element with atomic number 4 (Be)

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Beryllium , >99 % pure, crystalline big fragment >140 g
Alchemist-hp = Alchemist-hp ( pse-mendelejew.de ) · CC BY-SA 3.0

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In structural applications, the combination of high flexural rigidity, thermal stability, thermal conductivity and low density (1.85 times that of water) make beryllium a desirable aerospace material for aircraft components, missiles, spacecraft, and satellites. Because of its low density and atomic mass, beryllium is relatively transparent to X-rays and other forms of ionizing radiation; therefore, it is the most common window material for X-ray equipment and components of particle detectors. When added as an alloying element to aluminium, copper (notably the alloy beryllium copper), iron, or nickel, beryllium improves many physical properties. For example, tools and components made of beryllium copper alloys are strong and hard and do not create sparks when they strike a steel surface. In air, the surface of beryllium oxidizes readily at room temperature to form a passivation layer 1–10 nm thick that protects it from further oxidation and corrosion. The metal oxidizes in bulk (beyond the passivation layer) when heated above 500 °C (932 °F), and burns brilliantly when heated to about 2,500 °C (4,530 °F).

The commercial use of beryllium requires the use of appropriate dust control equipment and industrial controls at all times, because inhaled beryllium-containing dusts is toxic, and can cause berylliosis, a chronic life-threatening allergic disease, in some people. Berylliosis is typically manifested by chronic pulmonary fibrosis and, in severe cases, right-sided heart failure and death.

Characteristics

Physical properties

Beryllium is a steel gray and hard metal that is brittle at room temperature and has a close-packed hexagonal crystal structure. It has exceptional stiffness (Young's modulus 287 GPa) and a melting point of 1287 °C. The modulus of elasticity of beryllium is approximately 35% greater than that of steel. The combination of this modulus and a relatively low density results in an unusually high sound conduction speed in beryllium – about 12.9 km/s at ambient conditions. Among all metals, beryllium dissipates the most heat per unit weight, with both high specific heat (1925 J·kg−1·K−1) and thermal conductivity (216 W·m−1·K−1). Beryllium's conductivity and relatively low coefficient of linear thermal expansion (11.4×10−6 K−1) make it uniquely stable under extreme temperature differences.

Nuclear properties

Naturally occurring beryllium, save for slight contamination by the radioisotopes created by cosmic rays, is isotopically pure beryllium-9, which has a nuclear spin of ⁠3/2⁠−. The inelastic scattering cross section of beryllium increases with relation to neutron energy, allowing for significant slowing of higher-energy neutrons. Therefore, it works as a neutron reflector and neutron moderator; the exact strength of neutron slowing depends on the purity and size of the crystallites in the material.

The isotope 9Be can undergo a (n, 2n) neutron reaction with fast neutrons, to produce 8Be, which almost immediately breaks into two alpha particles. Thus, for high-energy neutrons, beryllium is a neutron multiplier, releasing more neutrons than it absorbs. This nuclear reaction is:

9
4Be + n → 2 4
2He + 2 n

The isotope can liberate the neutron when struck by an alpha particle. The nuclear reaction

9
4Be + 4
2He → 12
6C + n

is strongly exothermic, liberating a fast neutron.

The isotope can also release the neutron when absorbing a gamma ray of sufficient energy (photodisintegration) at a useful cross-section:

9
4Be + gamma → 2 4
2He + n

Thus, natural beryllium bombarded by alpha or gamma radiation from a suitable radioisotope is the most common radioisotope-powered neutron source for laboratory use.

Finally, small amounts of tritium are also liberated by the high-energy neutrons in the three-step nuclear reaction

9
4Be + n → 4
2He + 6
2He, 6
2He → 6
3Li + β−, 6
3Li + n → 4
2He + 3
1H

6
2He has a half-life of only 0.8 seconds, β− is an electron, and 6
3Li has a high neutron absorption cross section. This is equivalent to the neutron-multiplication reaction with three output neutrons replaced by a triton, and a beta decay allowing that conversion. Tritium is a radioisotope of concern in nuclear reactor waste streams.

Optical properties

As a metal, beryllium is transparent or translucent to most wavelengths of X-rays and gamma rays, making it useful for the output windows of X-ray tubes and other such apparatus.

Isotopes and nucleosynthesis

Natural beryllium is made up of solely the stable isotope beryllium-9. Beryllium is the only monoisotopic element with an even atomic number.

Beryllium-7 and beryllium-8 are key intermediates in stellar nucleosynthesis, but do not last long. It is believed that the beryllium in the universe was created in the interstellar medium when cosmic rays induced fission in heavier elements found in interstellar gas and dust, a process called cosmic ray spallation.

About one billionth (10−9) of the primordial atoms created in the Big Bang nucleosynthesis were 7Be. This is a consequence of the low density of matter when the temperature of the universe cooled enough for small nuclei to be stable. Creating such nuclei requires nuclear collisions that are rare at low density. Although 7Be is unstable and decays by electron capture into 7Li, with a half-life of 53.22 days under standard conditions, in the early universe the atoms were fully ionized and electron capture not significant. The conversion of 7Be to Li was only complete near the time of recombination.

The isotope 7Be is also a cosmogenic nuclide and shows an atmospheric abundance inversely proportional to solar activity. It decays exclusively by electron capture, and the 2s electrons of beryllium are the valence electrons responsible for chemical bonding. Therefore, when 7Be decays by L-electron capture, it does so by taking electrons from its atomic orbitals that may be participating in bonding. This makes its decay rate dependent to a measurable degree upon its chemical surroundings – a rare occurrence in nuclear decay.

7Be is also produced in cooling water of high-energy accelerators; it can be extracted from the water at high purity and sold for scientific experiments.

The isotope 10Be is similarly cosmogenic, and is produced in the same way – by cosmic ray spallation of nitrogen and oxygen. Its behavior differs only because of its much longer half-life of 1.387 million years. It entirely accumulates at the soil surface and has a long residence time before decaying to boron-10. Thus, 10Be and its daughter product are used to examine natural soil erosion, soil formation and the development of lateritic soils, and as a proxy for measurement of the variations in solar activity and the age of ice cores. As with 7Be, production of 10Be is inversely related to solar activity, because increased solar wind during periods of high solar activity decreases the flux of galactic cosmic rays that reach the Earth. Nuclear explosions also form 10Be by the reaction of fast neutrons with 13C in the carbon dioxide in air. This is one of the indicators of past activity at nuclear weapon test sites.

8Be is unstable but has a ground state resonance with an important role in the triple-alpha process in stellar helium burning. As first proposed by British astronomer Sir Fred Hoyle based solely on astrophysical analysis, the energy levels of 8Be and 12C allow carbon nucleosynthesis by increasing the effective cross-section between the three alpha particles in the carbon production process. The main carbon-producing reaction in the universe is 4He+8Be→12C+γ where 4He is an alpha particle.

The exotic isotopes 11Be and 14Be are known to exhibit a nuclear halo. That is, their nuclei have, respectively, 1 and 4 neutrons orbiting substantially outside the expected nuclear radius and in each case the core the neutrons float around is one of 10Be.

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