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Coulomb definition

Coulomb — Si-derived measurement unit of electric charge. Symbol C (named in honor of the French physicist - Coulomb). Definition 1 coulomb is the amount of electric charge carried by a constant electric - current of 1 ampere flowing for 1 second. 1C represents the charge of 6.24 x 1018 electrons. 1C = 1 As. [Pg.120]

Cosecant function, A-6 to 7 Cosine function, A-6 to 7 Cosmic Radiation, 11-267 to 270 Cosmic rays, 11-267 to 270 Cotangent function, A-6 to 7 Coulomb, definition, 1-23 to 26 Critical Constants, 6-39 to 58 Critical constants... [Pg.2478]

By contrast, in SI units, the coulomb (C) is the unit of charge and is defined as an ampere second (A sec). To reconcile this with newtons and meters, the units of F and r, respectively, a proportionality constant that is numerically different from unity and which has definite units is required. For charges under vacuum we write... [Pg.715]

If classical Coulombic interactions are assumed among point charges for electrostatic interactions between solute and solvent, and the term for the Cl coefficients (C) is omitted, the solvated Eock operator is reduced to Eq. (6). The significance of this definition of the Eock operator from a variational principle is that it enables us to express the analytical first derivative of the free energy with respect to the nuclear coordinate of the solute molecule R ,... [Pg.421]

Both entropic and coulombic contributions are bounded from below and it can be verified that the second variation of is positive definite so that the above equations correspond to a minimum [27]. Using conditions in the bulk we can eliminate //, from the equations. Then we get the Boltzmann equation in which the electric potential verifies the Poisson equation by construction. Hence is equivalent within MFA to the... [Pg.810]

As mentioned in the start of Chapter 4, the correlation between electrons of parallel spin is different from that between electrons of opposite spin. The exchange energy is by definition given as a sum of contributions from the a and /3 spin densities, as exchange energy only involves electrons of the same spin. The kinetic energy, the nuclear-electron attraction and Coulomb terms are trivially separable. [Pg.182]

In Section II.C we gave a general discussion of the Coulomb correlation, and we will now define the correlation error in the independent-particle model in greater detail. It is convenient to study the first- and second-order density matrices and, according to the definitions (Eq. II.9) applied to the symmetryless case, we obtain... [Pg.231]

Here q represents the coulomb energy of an electron occupying a definite p]h orbital in unsubstituted benzene its value has been estimated to be about —2.7 v. e. = —60 kcal./mole.5 /3 is a resonance integral between adjacent orbitals its value has been estimated to be about —0.85 v. e. = — 20 kcal./mole.6 Sk is a constant, the purpose of which is to allow for the different electron affinities of the different atoms. For Sk > 0, the... [Pg.196]

In electroanalysis, coulometry is an important method in which the analyte is specifically and completely converted via a direct or indirect electrolysis, and the amount of electricity (in coulombs) consumed thereby is measured. According to this definition there are two alternatives (1) the analyte participates in the electrode reaction (primary or direct electrolysis), or (2) the analyte reacts with the reagent, generated (secondary or indirect electrolysis) either internally or externally. [Pg.232]

The expression for V(r), given as Eq. (3.1), follows from the definition of electrical potential, which will be reviewed here. Any distribution of electrical charge creates a potential V(r) in the surrounding space. For an assembly of point charges ). located at positions r, this electrical potential is simply a sum of Coulombic potentials, as given in Eq. (3.2). [Pg.50]

An equation of the type (16) makes most physical sense when there exists a large capture radius Rc however, it can be applied to any diatomic capture case if regarded simply as a definition of Rc. Its utility is twofold. For one thing, physical common sense can sometimes give a value, or a bound, for Rc. When there is a Coulomb attraction between the reacting species, as for our case of H+ and A-, Rc can be plausibly estimated from... [Pg.254]

Two of the three SI base units have in the meantime acquired redefinitions in atomic terms (e.g., the second is now defined as 9 192 631 770 hyperfine oscillations of a cesium atom). However, the definitions (C.2a)-(C.2c) conceal another unfortunate aspect of SI units that cannot be overcome merely by atomic redefinitions. In the theory of classical or quantal electrical interactions, the most fundamental equation is Coulomb s law, which expresses the potential energy V of two charged particles of charge q and 2 at separation R as... [Pg.725]

For quantitative considerations it is convenient to use atomic units (a.u.), in which h = eo = me = 1 (me is the electronic mass) by definition. They are based on the electrostatic system of units so Coulomb s law for the potential of a point charge is = q/r. Conversion factors to SI units are given in Appendix B here we note that 1 a.u. of length is 0.529 A, and 1 a.u. of energy, also called a hartree, is 27.211 eV. Practically all publications on jellium use atomic units, since they avoid cluttering equations with constants, and simplify calculations. This more than compensates for the labor of changing back and forth between two systems of units. [Pg.233]

The SI unit of current I is the ampere (A). An ampere was first defined as the current flowing when a charge of 1 C (coulomb) passed per second through a perfect (i.e. resistance-free) conductor. The SI definition is more rigorous the ampbre is that constant current which, if maintained in two parallel conductors (each of negligible resistance) and placed in vacuo 1 m apart, produces a force between of exactly 2 x 10-7 N per metre of length . We will not employ this latter definition. [Pg.16]

The solute-solvent system, from the physical point of view, is nothing but a system that can be decomposed in a determined collection of electrons and nuclei. In the many-body representation, in principle, solving the global time-dependent Schrodinger equation with appropriate boundary conditions would yield a complete description for all measurable properties [47], This equation requires a definition of the total Hamiltonian in coordinate representation H(r,X), where r is the position vector operator for all electrons in the sample, and X is the position vector operator of the nuclei. In molecular quantum mechanics, as it is used in this section, H(r,X) is the Coulomb Hamiltonian[46]. The global wave function A(r,X,t) is obtained as a solution of the equation ... [Pg.286]

The interesting point with these definitions is that the total Coulomb energy is correctly obtained as the sum of two independent terms ... [Pg.296]

This is certainly not the only possibility, and MQSM can be defined using many choices of il(ir,r2) provided it remains positive definite. Examples include the Coulomb MQSM and kinetic QSM. In case of the Coulomb operator, one does not perform the point-by-point similarity calculation as in Equation 16.4 but introduces weighting of the surrounding points using as an operator ... [Pg.232]

To simplify the solution we will write amperes as its definition of coulomb/second. [Pg.274]


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