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Nuclear reactions energy from

With its half-life of approximately 6 h, how much technetium-99m would remain 18 h after injection into a patient  [Pg.303]

If two radioisotopes available for diagnosis worked equally well and each decayed by giving off gamma rays, but one had a half-life of 13 h and the other had a half-life of 6 h, which one would you recommend  [Pg.303]

There is a huge difference between the amount of energy liberated in an ordinary chemical reaction, like the burning of methane in air, and the energy liberated in a nuclear fission reaction. If you compared the energy from the burning of only 16 g of methane with that from the fission of an equivalent amount of uranium-235, the fission reaction would produce almost 25 million times more energy. [Pg.303]

Nuclear fission can occur when a neutron (Jn) enters a heavy nucleus. Certain heavy nuclei with an odd number of neutrons g Pu) will undergo [Pg.303]

One kilogram of uranium fuel undergoing fission in a nuclear reactor can produce the same amount of energy as the combustion of 3000 tons of coal or 14,000 barrels of oil. [Pg.303]


The tremendous release of energy from nuclear reactions makes possible a unique family of applications for long-lived radioisotopes that are important to health, science, and industry. Whereas fission and fusion occur almost instantaneously, other radioactive decay processes occur in times ranging from a few minutes to thousands of years. The general areas of application may be grouped into irradiation, thermal energy generation, and tracer applications.57... [Pg.990]

Chapter 13 is Chapter 4 from the previous edition and focuses on fundamental nuclear chemistry. Usefiil apphcations of radioactivity are considered. In this context, a discussion of the nse of radiocarbon dating has been added. A msgor focus of the chapter is the use of energy from nuclear reactions and this discussion has driven the chapter placement after the chapter on hydrocarbon fiiels. Comparisons between low-level radioactive waste and high-level radioactive waste have been added. [Pg.607]

Certain stars obtain their energy from nuclear reactions such as... [Pg.894]

Uses. Potassium peroxide is used as an oxidizing agent and in oxygen generating units for gas masks (Ref 5). Another use has been found by Hatterer who developed a device which extracts the thermal energy from nuclear reactors in a reaction which generates H2 and 02 gases by... [Pg.668]

Energy from nuclear fusion might also be used for propelling jets and rockets. Formidable difficulties would be encountered, however. For reactions occurring at ca 10 °K, such as those between the hydrogen isotopes, chamber pressures of around 100 atm could give rates of energy production comparable to those from the familiar chemical fuels. [Pg.504]

Figure 7. A spectrum of particles resulting from nuclear reactions and scattering from a thick Si3Ni standard. Conditions 2H ions normally incident at an energy of 1.41 MeV, and resulting reaction particles detected at a 165° angle by a surface-barrier diode detector. The particle group marked a, is from the 14N(d,a)i2C reaction and is used to profile N in samples. Figure 7. A spectrum of particles resulting from nuclear reactions and scattering from a thick Si3Ni standard. Conditions 2H ions normally incident at an energy of 1.41 MeV, and resulting reaction particles detected at a 165° angle by a surface-barrier diode detector. The particle group marked a, is from the 14N(d,a)i2C reaction and is used to profile N in samples.
The enormous amounts of energy produced from nuclear reactions makes them a logical choice for energy production. Essentially, the generation of electricity by nuclear means occurs as follows. [Pg.235]

A nuclear reactor is a device for generating energy from nuclear fission reactions. Nuclear fission is the process in which large atoms are split, releasing large amounts of energy and smaller atoms. In a nuclear reactor, it is essential that just the right number of neutrons are present. Too many neutrons can cause a fission reaction to get out of control. Too few neutrons and a fission reaction stops. [Pg.67]

Thermonuclear energy Energy from nuclear fusion reactions. [Pg.1034]

It is clear, for example from radio-carbon dating of rocks in the earth s surface, that the solar system must be very much older than the Kelvin age of 3 x 107 years. It is now taken for granted that the main source of stellar energy comes from nuclear reactions. The fusion of four protons (hydrogen nuclei) to an alpha-particle (helium nucleus) is associated with the release of energy Q, where Q k, 26 MeV. The total available energy is thus... [Pg.17]


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See also in sourсe #XX -- [ Pg.303 , Pg.304 , Pg.305 ]




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