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Kelvin, available energy

In 1879 Lord Kelvin introduced the term nwtivity for the possession, the waste of which is called dissipation at constant temperature this is identical with Maxwell s available energy. He showed in a paper On Thermodynamics founded on Motivity and Energy Phil. Mag., 1898), that all the thermodynamic equations could be derived from the properties of motivity which follow directly from Carnot s theorem, without any explicit introduction of the entropy. [Pg.101]

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]

Fig. 2. (a) Energy, E, versus wave vector, k, for free particle-like conduction band and valence band electrons (b) the corresponding density of available electron states, DOS, where Ep is Fermi energy (c) the Fermi-Dirac distribution, ie, the probabiUty P(E) that a state is occupied, where Kis the Boltzmann constant and Tis absolute temperature ia Kelvin. The tails of this distribution are exponential. The product of P(E) and DOS yields the energy distribution... [Pg.344]

The most important modem system of units is the SI system, which is based around seven primary units time (second, abbreviated s), length (meter, m), temperature (Kelvin, K), mass (kilogram, kg), amount of substance (mole, mol), current (Amperes, A) and luminous intensity (candela, cd). The candela is mainly important for characterizing radiation sources such as light bulbs. Physical artifacts such as the platinum-iridium bar mentioned above no longer define most of the primary units. Instead, most of the definitions rely on fundamental physical properties, which are more readily reproduced. For example, the second is defined in terms of the frequency of microwave radiation that causes atoms of the isotope cesium-133 to absorb energy. This frequency is defined to be 9,192,631,770 cycles per second (Hertz) —in other words, an instrument which counts 9,192,631,770 cycles of this wave will have measured exactly one second. Commercially available cesium clocks use this principle, and are accurate to a few parts in 1014. [Pg.2]

At zero Kelvin (0 K), there is no energy available for a chemical to sample states. The absolute entropy, S, of a pure crystalline solid at 0 K is zero. Absolute entropy may be measured and calculated for different substances at different temperatures. [Pg.158]

Modem quantum-chemical methods can, in principle, provide all properties of molecular systems. The achievable accuracy for a desired property of a given molecule is limited only by the available computational resources. In practice, this leads to restrictions on the size of the system From a handful of atoms for highly correlated methods to a few hundred atoms for direct Hartree-Fock (HF), density-functional (DFT) or semiempirical methods. For these systems, one can usually afford the few evaluations of the energy and its first one or two derivatives needed for optimisation of the molecular geometry. However, neither the affordable system size nor, in particular, the affordable number of configurations is sufficient to evaluate statistical-mechanical properties of such systems with any level of confidence. This makes quantum chemistry a useful tool for every molecular property that is sufficiently determined (i) at vacuum boundary conditions and (ii) at zero Kelvin. However, all effects from finite temperature, interactions with a condensed-phase environment, time-dependence and entropy are not accounted for. [Pg.82]

Table II. Henry s Law Constants (Kh and K h) from 0 - 40°C. Values at 25°C determined from partial pressure data. Estimates calculated from available free energy data (22) are also shown. Temperature dependence (T/Kelvin) given by ln(KH, K h) = a + b/T + cT Part 1 Kh (HX(g) = H+(aq) + X (aq)) ... Table II. Henry s Law Constants (Kh and K h) from 0 - 40°C. Values at 25°C determined from partial pressure data. Estimates calculated from available free energy data (22) are also shown. Temperature dependence (T/Kelvin) given by ln(KH, K h) = a + b/T + cT Part 1 Kh (HX(g) = H+(aq) + X (aq)) ...
Entropy It is considered in the seeond law of thermodynamies. It is thermodynamic property that ean be used to determine the energy available for useM work in a thermodynamic process, such as in energy eonversion devices, engines, or maehines. In thermodynamics, the concept of entropy is defined by the second law of thermodynamics, which states that the entropy of an isolated system always inereases or remains constant. Thus, entropy is also a measure of the tendeney of a process, such as a chemical reaction. Thermodynamic entropy has the dimension of energy divided by temperature, and a unit of joules per kelvin (J/K) in the International System of Units. [Pg.49]


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See also in sourсe #XX -- [ Pg.203 ]




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Energy availability

Energy available

Kelvin

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