Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Continuous curves

In a given motion, a particular material particle will experience a strain history The stress rate relation (5.4) and flow rule (5.11), together with suitable initial conditions, may be integrated to obtain the eorresponding stress history for the particle. Conversely, using (5.16) instead of (5.4), may be obtained from by an analogous ealeulation. As before, may be represented by a continuous curve, parametrized by time, in six-dimensional symmetric stress spaee. [Pg.127]

Fig. 2. Electrical resistance as a function of the temperature at the indicated magnetic fields for a bundle of CNTs. The dashed lines separate three temperature ranges, while the continuous curve is a fit using the two-band model for graphite (see inset) with an overlap of 3.7 meV and a Fermi levei right in the middie of the overlap [9]. Fig. 2. Electrical resistance as a function of the temperature at the indicated magnetic fields for a bundle of CNTs. The dashed lines separate three temperature ranges, while the continuous curve is a fit using the two-band model for graphite (see inset) with an overlap of 3.7 meV and a Fermi levei right in the middie of the overlap [9].
Suppose that the vector field u(f) is a continuous function of the scalar variable t. As t varies, so does u and if u denotes the position vector of a point P, then P moves along a continuous curve in space as t varies. For most of this book we will identify the variable t as time and so we will be interested in the trajectory of particles along curves in space. [Pg.7]

Pierce proposes and illustrates good agreement between the test data and the correlation for a smooth continuous curve for the Colburn factor over the entire range of Reynolds numbers for the laminar, transition, and turbulent flow regimes inside smooth tubes ... [Pg.99]

A brief digression. In the language of statistics, the results for each of the stepped distributions in Figure 10-1 constitute a sample1 of the population that is distributed according to the continuous curve for the universe. A sample thus contains a limited number of x s taken from the universe that contains all possible z s. All simple frequency distributions are characterized by a mean and a variance. (The square root of the variance is the standard deviation.) For the population, the mean is u and the variance is a2. For any sample, the mean is x and the (estimate of) variance is s2. Now, x and s2 for any sample can never be as reliable as p and a2 because no sample can contain the entire population ir and s2 are therefore only the experimental estimates of g and cr2. In all that follows, we shall be concerned only with these estimates for simplicity s sake, we shall call s2 the variance. We have already met s—for example, at the foot of Table 7-4. [Pg.268]

Figure 35 shows how the equilibrium transition curves of [(Ala-Gly-Pro)n]3Lys-Lys shift to higher temperatures with increasing chain length. The continuous curves represent the numerical fit to the experimental transition data. [Pg.193]

The working substance being initially at the temperature T2 of the refrigerator, we place the cylinder on the non-conducting stand, and compress the working substance reversibly until the temperature rises to Ti. By the conditions imposed, this is an adiabatic compression, and will be represented by a continuous curve on the indicator diagram, say AB (Fig. 8). [Pg.56]

James Thomson (1871) suggested that these prolongations of the 0i isotherm of a liquid and vapour might ultimately bend round and join, so that the discontinuous flat part of the isotherm is replaced by a continuous curve (Fig. 84). aft corresponds to... [Pg.182]

Regnault investigated the vapour-pressures of water and benzene, both in the liquid and solid states, and represented his results graphically. He con-. eluded that the curves for the liquid and solid joined at the melting-point, and gave a continuous curve. This was shown theoretically to be incorrect. by Ivirchhoff (1858), who proved, by a method to be described later, that the... [Pg.191]

The summits of the ordinates will therefore lie on a continuous curve, either wholly above (Q > 0), or wholly below (Q < 0) the composition axis, as for example, kbB or A/3B. ah = heat absorbed in the formation of unit mass of the mixture containing Ba = x parts... [Pg.311]

The values of the half-widths of the components of the rotational absorption spectrum of HC1, dissolved in various noble gases, are borrowed from [291]. In order to make this example obvious, a continuous curve is drawn through the calculated points. Comparison between experimental data and calculated results demonstrates, in line with the qualitative agreement, a good numerical coincidence of the observed. /-dependence of the half-widths of the rotational lines with the theoretical one in the case of HC1 dissolved in Kr and Xe. This allows one to estimate the model parameters for these systems dispersion of the potential... [Pg.248]

Continuous curve.- f(F) = F (The weighting fimction implying total routing collagen carbon derives only from diet protein). [Pg.228]

An important strengthening feature of mbbery solids, especially evident in particle-filled (reinforced) compounds, is knotty tearing, where cracks may split, mm abmptly at 90°, or follow a continuously curving path. Although the conditions under which knotty tearing occurs are well known, the cause is obscure. Even the detailed process is unclear. As a result, this strengthening feature cannot be predicted. [Pg.19]

Iactate]o = 0.01, [S-lactate]o = 0.01 M. [CDopen]o/[CDdosed]o 9/2 The continuous curves were obtained by kinetic modeling. [Pg.249]

The quasi-continuous curve of the density of states in the 3D case now has a staircase characteristic with discrete energy levels in z-direction. [Pg.4]

Combining these two profiles across the space or time horizon allows virtually all types of continuous curves to be produced that can be implemented in a practical design. When the two profiles are combined, two additional variables are needed. The value of tinter indicates the point in space or time where the two curves meet and xinter is the corresponding value of the control variable where the curves meet. Figure 3.14c illustrates the form of Type I followed by Type II and Figure 3.14d the form of Type II followed by Type I. [Pg.47]

Fig. 2.12. 5-factor for 12C(a, y)lsO. The dashed curve ignores the sub-threshold resonances, while the continuous curve allows for them, but the uncertainties are still significant at low energies. Koonin, Tombrello and Fox (1974). Reproduced with kind permission of Elsevier Science. Courtesy S.E. Koonin. [Pg.37]

Fig. 6.10. Results of a dynamical calculation of the r-process in the hot neutrino bubble inside a 20 Mq supernova (continuous curve) compared to the observed Solar-System abundance distribution (filled circles). After Woosley etal. (1994). Courtesy Brad Meyer. Fig. 6.10. Results of a dynamical calculation of the r-process in the hot neutrino bubble inside a 20 Mq supernova (continuous curve) compared to the observed Solar-System abundance distribution (filled circles). After Woosley etal. (1994). Courtesy Brad Meyer.
Fig. 10.3. Observed A -rat.ios (estimated error limits shown by pairs of horizontal lines) and their theoretical variation with the age of the Galaxy according to three models a pure initial spike (continuous straight lines) Fowler s (1987) model (broken-line curves) and the simple inflow model (continuous curves). Fig. 10.3. Observed A -rat.ios (estimated error limits shown by pairs of horizontal lines) and their theoretical variation with the age of the Galaxy according to three models a pure initial spike (continuous straight lines) Fowler s (1987) model (broken-line curves) and the simple inflow model (continuous curves).
Fig. 10.4. Above spectrum of the solar-type G-dwarf star HR 509 showing features of Th ii and Nd n near k 4019 A, after Butcher (1987). Th ii is blended with a strong feature due to Fe and Ni, as well as weaker features. The tracing around the zero level shows 10 x the difference between the observed spectrum (dots) and the fitted synthetic spectrum (continuous curve). Reproduced with permission from Macmillan Magazines Ltd. Below spectrum of the same region in the very metal-poor giant star CS 22892—052 ([Fe/H] —3) with a large relative excess of r-process elements ([r/Fe] = 1.7), adapted from Sneden el al. (1996). Fig. 10.4. Above spectrum of the solar-type G-dwarf star HR 509 showing features of Th ii and Nd n near k 4019 A, after Butcher (1987). Th ii is blended with a strong feature due to Fe and Ni, as well as weaker features. The tracing around the zero level shows 10 x the difference between the observed spectrum (dots) and the fitted synthetic spectrum (continuous curve). Reproduced with permission from Macmillan Magazines Ltd. Below spectrum of the same region in the very metal-poor giant star CS 22892—052 ([Fe/H] —3) with a large relative excess of r-process elements ([r/Fe] = 1.7), adapted from Sneden el al. (1996).
The parameters they obtained for neutron stars of different masses are listed in Table 1. Between white dwarfs and neutron stars there is a neutronization and a transition from normal matter with electrons and nuclei to superdense matter consisting of neutrons and other strongly interacting particles mesons and hadrons. The continuous curve M pc) in the whole region from white... [Pg.7]

The stellar conversion process, described so far, will start to populate the new branch of quark stars (the part of the QS sequence plotted as a continuous curve in Fig. 3). Long term accretion on the QS can next produce stars with masses up to the limiting mass Mqs max for the quark star configurations. [Pg.365]

Figure 8.9 Third stage of SIM. The sections of the creep modulus curve are shifted parallel to the time axis to produce a single continuous curve. Small corrections are applied to allow for fibre shrinkage and for the thermal history of the material. Figure 8.9 Third stage of SIM. The sections of the creep modulus curve are shifted parallel to the time axis to produce a single continuous curve. Small corrections are applied to allow for fibre shrinkage and for the thermal history of the material.
The chain overlap parameter has been very successful at superimposing the data from the systems without hydrophobic modification, producing the continuous curve. However, it is clear from Flynn s work that once the hydrophobes are introduced into the polymer the viscosity rapidly increases at lower values of the chain overlap parameter. Increasing the mole percentage of hydrophobes also increases the viscosity at lower values of the chain overlap parameter. The position and number of the hydrophobes on a chain are important in determining the structure that forms and the onset of the increase in viscosity. The addition of side chains to hydroxyethyl cellulose modifies the network modulus as a function of concentration. This is discussed further in Section 2.3.4. [Pg.208]

Since the size analysis is represented by the continuous curve ... [Pg.14]

Figure 12,19. Temperature tuning of an optical parametric oscillator. The continuous curve is a theoretical prediction and the circles represent measured data. (From Ref. 75.)... Figure 12,19. Temperature tuning of an optical parametric oscillator. The continuous curve is a theoretical prediction and the circles represent measured data. (From Ref. 75.)...

See other pages where Continuous curves is mentioned: [Pg.1075]    [Pg.27]    [Pg.26]    [Pg.263]    [Pg.452]    [Pg.104]    [Pg.103]    [Pg.15]    [Pg.56]    [Pg.364]    [Pg.233]    [Pg.36]    [Pg.119]    [Pg.28]    [Pg.264]    [Pg.952]    [Pg.122]    [Pg.179]    [Pg.679]    [Pg.9]    [Pg.292]    [Pg.324]    [Pg.39]    [Pg.39]   
See also in sourсe #XX -- [ Pg.17 ]




SEARCH



Continuously curved chain

Corrosion fatigue continued curves

© 2024 chempedia.info