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Probability, energy

We will be able to use this equation to find the most probable energy distribution after we obtain appropriate values for a and 3. [Pg.517]

Fig. 2.13. Schematic superposition of the Maxwell energy distribution and neutron capture cross-section. The most probable energy for the capture process in stars is near kT. After Rolfs and Rodney (1988). Copyright by the University of Chicago. Courtesy Claus Rolfs. Fig. 2.13. Schematic superposition of the Maxwell energy distribution and neutron capture cross-section. The most probable energy for the capture process in stars is near kT. After Rolfs and Rodney (1988). Copyright by the University of Chicago. Courtesy Claus Rolfs.
The problem to be considered now is how to tear effectively a system of such units, units interconnected by material (and probably energy) flows. We assume that the input-output relationships are known for each unit, and that outputs must be calculated from the inputs. Each physical flow corresponds to several variables, and the criterion for tearing will be to minimize the number of variables that must be assumed to solve the torn system, i.e., to have the minimum number of variables associated with the total of the torn streams. [Pg.219]

Example The thermal energy distribution curves for 1,2-diphenylethane, C14H14, 5 = 3 X 28 - 6 = 78, have been calculated at 75 and 200 °C. [34] Their maxima were obtained at about 0.3 and 0.6 eV, respectively, with almost no molecules reaching beyond twice that energy of maximum probability. At 200 °C, the most probable energy roughly corresponds to 0.008 eV per vibrational degree of freedom. [Pg.22]

The most probable energy levels Eox and Ered are connected with the standard redox potential or by the standard redox Fermi level by the following symmetrical relation ... [Pg.131]

The most probable translational energy for an atom in a gas at temperature T is equal to 3/2 KT where K = R/Ny is Boltzmann s constant. Calculate the degeneracy of the most probable energy level for an argon atom at 300 K and 1 bar pressure, assuming that the atom can be treated as a particle in a three dimensional box. The volume of the gas at these conditions is 0.022 m ... [Pg.144]

The equilibrium energy is dilferent from the most probable energy, p, defined by S E = p) = 0. p is the average energy we would find if we were... [Pg.78]

The same situation is to be expected for the excited states with the only difference that now the most probable energy states are shifted by the stored excitation energy upwards or downwards depending on whether the excited molecule acts as a donor or as an acceptor 20>. These energy distribution functions for a molecule in the ground state and in the excited state are represented in Fig. 3. They can be described by the following equations ... [Pg.40]

Fig. 7. Probable energy levels of the excited states of different types of ketones. Fig. 7. Probable energy levels of the excited states of different types of ketones.
Figure 3 indicates a probable energy supply scheme divided by consumer and assumed demand - provided sufficient power were available. However, as was the case for the 2002-2003 winter, this scheme could not be achieved. On the contrary, the consumers were receiving less than 50% of the planned power in the peak periods of January, February and March 2003. [Pg.40]

Specifically, in the first step of the energy cascade, the light is captured by the DVB dimer located in the core of the complex. The energy is then transferred to peripherally located bilins (MBV, PCB 158) through a complex network of interactions that, owing to the very similar timescales and spectral features, are hard to separate. Probably, energy migration from DBV bilins to the MBV bilins occurs on a timescale (T) 0.6 ps) faster than the transfer... [Pg.17]

L. Omstein2 discusses related questions. One should emphar size (1) his critical attitude toward the ergodic hypothesis and, as a result, his introduction of the microcanonical ensemble not as the only possible one, but only as the simplest stationary ensemble (2) some remarks on the properties of ensembles of systems which are distributed around the surface of most probable energy following a different law, e.g., with density proportional to... [Pg.74]

The different courses of the reactions of o-phenylenediamines and 1,8-diami-nonaphthalenes with quinones cannot be assigned to different terms for thermodynamic control. The spirocyclic isomers are most probably energy-preferable forms for both Type 10 and 11 compounds. The cyclization step is definitely kinetically... [Pg.319]

Additionally, the incident impurity ions in a fusion device will be multiply charged, e.g., a charge state of 4 can be assumed for Be, C, O, and even higher values for W ions. This will result in increased acceleration of the ions in the sheath potential such that the most probable energies for multiply charged ions in a divertor plasma with Te = 10 eV will be around 200 eV, i.e., well above the threshold energy. [Pg.206]

Clearly, °E1 corresponds to the most probable energy of the reduced form and °E2 to the most probable energy of the oxidised form. The midpoint... [Pg.124]

To describe the thermodynamics, the free energy can be evaluated. Assuming that the folding reaction is taking place at constant temperature and pressure, the free energy is given by eq 10, where Emp is the thermally most probable energy and S the entropy. [Pg.144]

CIP to exist remain unchanged. It should be noted, that in the case of a heterogeneous surface the solution of Eqs. (78) and (79) yields corresponding dependences on K° but not on Ki. These expressions are dependencies between intrinsic constants for the most probable energies e°. [Pg.400]

Impact measurement. The impact tests were conducted in the usual manner on single sheets with a Gardner Laboratory Impact Tester (Model IG-1120) with a 0.625" diameter punch hammer. At least ten drops were performed in the center 50% of the sheets and with points of impact at least 1" apart. The failure criterion was a brittle (not ductile or tear) break. The values reported in Table I are 50% probabilities (energy at which 50% of failures are brittle). The standard deviation of the values is about 10%. [Pg.374]

Ni(CO)4 is not affected by intense 60Co-y-irradiation and can be looked upon as one of the most radiation stable compounds 44>. A study of the radiolysis of mixtures of cyclohexane and/or benzene and Ni(CO)4 has demonstrated its protective properties. Probably, energy transfer to Ni(CO)4 and the reversible dissociation... [Pg.209]

In chemistry, the thermodynamic energy (2.21) must be used, while in nuclear reactions the most probable energy E must be used, where... [Pg.23]

Figure 9. A probable energy-level scheme for a planar rectangular N4 radical. The optically allowed transitions and polarizations ate indicated. The z axis is parallel to one edge of the rectangle. The N4 lies in two sites having z parallel to [llOJ and [ITO] andx parallel to [001]. Figure 9. A probable energy-level scheme for a planar rectangular N4 radical. The optically allowed transitions and polarizations ate indicated. The z axis is parallel to one edge of the rectangle. The N4 lies in two sites having z parallel to [llOJ and [ITO] andx parallel to [001].
Table IV, PROBABLE ENERGY REQUIREMENTS FOR A SHORT ROTATION WOOD FUEL CROP... Table IV, PROBABLE ENERGY REQUIREMENTS FOR A SHORT ROTATION WOOD FUEL CROP...

See other pages where Probability, energy is mentioned: [Pg.15]    [Pg.644]    [Pg.48]    [Pg.207]    [Pg.445]    [Pg.79]    [Pg.40]    [Pg.262]    [Pg.102]    [Pg.276]    [Pg.276]    [Pg.153]    [Pg.296]    [Pg.153]    [Pg.15]    [Pg.285]    [Pg.124]    [Pg.365]    [Pg.48]    [Pg.6]    [Pg.100]    [Pg.134]    [Pg.262]    [Pg.434]    [Pg.196]    [Pg.341]    [Pg.450]   
See also in sourсe #XX -- [ Pg.3 ]




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Electrons, crystalline solid materials probability, energy

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Energy probability density

Energy spectrum probability density

Energy spectrum probability density distribution

Energy transfer Probability

Energy transfer probability density

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Energy transition probabilities

Energy transmission probability

Excitation probability, molecular dyes in zeolite energy transfer

Fermi—Dirac distribution probability, energy

Inelastic transition probabilities transitional energy

Most probable kinetic energy

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Occupation probability, potential energy

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Potential energy surface time-dependent probabilities

Probability distribution of energy

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