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Equilibria stable

Figure 7. Equilibrium stable configurations on the mass M, central rest-mass density pc diagram for superdense isentropic stars (hatched). The stars become stable at sufficiently large densities because of nucleon pressure, and become unstable again at larger densities due to GR effects, from Bisnovatyi-Kogan (1968). Figure 7. Equilibrium stable configurations on the mass M, central rest-mass density pc diagram for superdense isentropic stars (hatched). The stars become stable at sufficiently large densities because of nucleon pressure, and become unstable again at larger densities due to GR effects, from Bisnovatyi-Kogan (1968).
General rules governing equilibrium stable isotope fractionations... [Pg.67]

Equilibrium stable isotope fractionation is a quantum-mechanical phenomenon, driven mainly by differences in the vibrational energies of molecules and crystals containing atoms of differing masses (Urey 1947). In fact, a list of vibrational frequencies for two isotopic forms of each substance of interest—along with a few fundamental constants—is sufficient to calculate an equilibrium isotope fractionation with reasonable accuracy. A succinct derivation of Urey s formulation follows. This theory has been reviewed many times in the geochemical... [Pg.69]

Figure 1. Translation, rotation, and vibration of a diatomic molecule. Every molecule has three translational degrees of freedom corresponding to motion of the center of mass of the molecule in the three Cartesian directions (left side). Diatomic and linear molecules also have two rotational degrees of freedom, about rotational axes perpendicular to the bond (center). Non-linear molecules have three rotational degrees of freedom. Vibrations involve no net momentum or angular momentum, instead corresponding to distortions of the internal structure of the molecule (right side). Diatomic molecules have one vibration, polyatomic linear molecules have 3V-5 vibrations, and nonlinear molecules have 3V-6 vibrations. Equilibrium stable isotope fractionations are driven mainly by the effects of isotopic substitution on vibrational frequencies. Figure 1. Translation, rotation, and vibration of a diatomic molecule. Every molecule has three translational degrees of freedom corresponding to motion of the center of mass of the molecule in the three Cartesian directions (left side). Diatomic and linear molecules also have two rotational degrees of freedom, about rotational axes perpendicular to the bond (center). Non-linear molecules have three rotational degrees of freedom. Vibrations involve no net momentum or angular momentum, instead corresponding to distortions of the internal structure of the molecule (right side). Diatomic molecules have one vibration, polyatomic linear molecules have 3V-5 vibrations, and nonlinear molecules have 3V-6 vibrations. Equilibrium stable isotope fractionations are driven mainly by the effects of isotopic substitution on vibrational frequencies.
This relation correctly predicts that most equilibrium stable isotope fractionations are inversely proportional to the square of absolute temperature, and is the basis of equilibrium fractionation rule (1). A detailed derivation of the Bigeleisen and Mayer model has been presented in an earlier review (Criss 1991). [Pg.77]

It should be clear from the preceding discussions that practical application of equilibrium stable isotope fractionation theory often requires a certain amormt of simplification of complex and poorly studied systems. Given this reality, one should not be surprised to find that theoretically determined equilibrium fractionations rarely achieve accuracies approaching the nominal precisions of measurements made with modem analytical techniques. It should... [Pg.91]

Atmospheric Equilibrium (Stable condensed phases constituents mole fraction at staqdard conditions... [Pg.124]

Note that when the mole fraction of dissolved oxygen is higher than the solubility limit of oxygen in M, precipitation of an MpOq oxide occurs. However, for the sake of homogeneity, only the dissolution reaction will be considered when establishing the reactivity scale. In other words, the value of X0 used in the reactivity scale is that for equilibrium, stable or metastable, between a M-A-0 ternary alloy and the AnOm oxide (Figure 6.1). [Pg.200]

Corrosion Rate by CBD Somewhat similarly to the Tafel extrapolation method, the corrosion rate is found by intersecting the extrapolation of the linear portion of the second cathodic curve with the equilibrium stable corrosion potential. The intersection corrosion current is converted to a corrosion rate (mils penetration per year [mpy], 0.001 in/y) by use of a conversion factor (based upon Faraday s law, the electrochemical equivalent of the metal, its valence and gram atomic weight). For 13 alloys, this conversion factor ranges from 0.42 for nickel to 0.67 for Hastelloy B or C. For a quick determination, 0.5 is used for most Fe, Cr, Ni, Mo, and Co alloy studies. Generally, the accuracy of the corrosion rate calculation is dependent upon the degree of linearity of the second cathodic curve when it is less than... [Pg.2187]

The pyranose 35 and the furanose 164 are stable in neutral solution at room temperature, and are separable by column chromatography without equilibration. On heating, or by acid catalysis (0.1 M hydrochloric acid, room temperature, 35 hours), an equilibrium between forms 35 and 164 is established. From the optical rotation, the ratio of the six-membered to the five-membered ring is calculated to be about 2 1. Alkaline catalysis causes very rapid attainment of equilibrium, but, simultaneously, decomposition occurs. The 5-acetamidopyranose 35 is, after attainment of its equilibrium, stable toward acids, and shows no dehydration reaction to form 3-pyridinol. However, under conditions in which the N-acetyl group is hydrolytically removed (heating with 2 M hydrochloric acid), 35 is transformed into 3-pyridinol through the intermediate formation of free 5-amino-5-deoxy-D-xylopyranose. ... [Pg.168]

Calculation of fluid/rock ratios. The amount of fluid that has infiltrated and exchanged with a rock is often estimated from stable isotope data by mass-balance calculations assuming equilibrium stable isotope exchange. Taylor (1977, p. 523-524) derived the following relation for a 0-dimensional or box model ... [Pg.450]

In position (b), it is possible to imagine the ball balanced and unmoving, so that the first part of the definition would be fulfilled, and this is sometimes referred to as a third type of equilibrium, admittedly a trivial case, called unstable equilibrium. However, it does not survive the second part of the definition, so we are left with only two types of equilibrium, stable and metastable. [Pg.39]

This is a remarkable restriction, since as we look around us we see rather few systems at stable equilibrium. Stable equilibrium is, in fact, often very difficult or impossible to achieve in many systems, and is never achieved in an absolute sense. Nevertheless, our thermodynamic equations are restricted to using properties in equilibrium states. [Pg.55]

Look up the definitions of equilibrium, stable, metastable, reversible and quasistatic in any textbooks on thermodynamics or physical chemistry you have at hand, and reflect on the differences between them and the definitions in this text. [Pg.59]

Thus, the entropy inequality (1.21) was proved for any process p from state to af with entropies 5, and 5/ respectively, defined relative to the same (equilibrium stable) reference state ao (states a,, a/ and processes p between them may be arbitrary). [Pg.26]

In the remaining part of this AppendixA.1, we obtain the important result (A.9) using an ideal cyclic process from subset C of Sect. 1.2, namely the Carnot cycle [1, 2, 4, 5]. Carnot cycle is a cyclic process with (fixed number of mols, n, of) uniform ideal gas composed from isothermal and adiabatic (no heat exchange) expansions followed by isothermal (at lower temperature) and adiabatic compressions back to the starting state. All these processes pass the equilibrium (stable) states and they are reversible (cf. definition in Sect. 1.2), see also Rem. 48 in Chap. 3. [Pg.281]

Black J.R., Kavner A., and Schauble E.A. (2011) Calculation of equilibrium stable isotope partition function ratios for aqueous zinc complexes and metallic zinc. Geochim. Cosmochim. Acta., 75, 769-783. [Pg.348]

Schauble, E.A. (2007) Role of nuclear volume in driving equilibrium stable isotope fractionation of mercury. [Pg.349]

A) CrystaUizable Materials Their equilibrium stable state is crystalline at low temperatures with certain symmetries. Examples are rock or quartz crystals, various forms of ice, metals, and salt. The MSs in these systems are defined with respect to the ordered crystalline phase, an EQS. [Pg.435]


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Complex systems locally stable equilibrium

Equilibrium departure from stable

Equilibrium state stable

Equilibrium, chemical stable

Exponentially stable equilibrium state

Heat capacity stable equilibrium

Isotopes, stable equilibrium

Metastable and stable equilibrium contact angles

Semi-stable equilibrium state

Stable and Metastable Equilibrium

Stable complex equilibrium state

Stable equilibrium point

Stable equilibrium postulate

Stable equilibrium thick film

Stable equilibrium, conditions

Stable equilibrium, conditions relation between

Stable equilibrium: definition

Stable focus equilibrium state

Stable isotopes equilibrium isotope effects

Stable node equilibrium state

Stable phase chemical equilibrium

Structurally stable equilibrium state

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