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  2. Bragg's law - Wikipedia

    en.wikipedia.org/wiki/Bragg's_law

    This equation, Bragg's law, describes the condition on θ for constructive interference. [12] A map of the intensities of the scattered waves as a function of their angle is called a diffraction pattern. Strong intensities known as Bragg peaks are obtained in the diffraction pattern when the scattering angles satisfy Bragg condition.

  3. Vacancy defect - Wikipedia

    en.wikipedia.org/wiki/Vacancy_defect

    where N v is the vacancy concentration, Q v is the energy required for vacancy formation, k B is the Boltzmann constant, T is the absolute temperature, and N is the concentration of atomic sites i.e. = where ρ is density, N A the Avogadro constant, and M the molar mass. It is the simplest point defect.

  4. Standard enthalpy of formation - Wikipedia

    en.wikipedia.org/wiki/Standard_enthalpy_of_formation

    Since the pressure of the standard formation reaction is fixed at 1 bar, the standard formation enthalpy or reaction heat is a function of temperature. For tabulation purposes, standard formation enthalpies are all given at a single temperature: 298 K, represented by the symbol Δ f H ⦵ 298 K.

  5. Standard Gibbs free energy of formation - Wikipedia

    en.wikipedia.org/wiki/Standard_Gibbs_free_energy...

    The standard Gibbs free energy of formation (G f °) of a compound is the change of Gibbs free energy that accompanies the formation of 1 mole of a substance in its standard state from its constituent elements in their standard states (the most stable form of the element at 1 bar of pressure and the specified temperature, usually 298.15 K or 25 ...

  6. Fermi energy - Wikipedia

    en.wikipedia.org/wiki/Fermi_energy

    The Fermi energy is an important concept in the solid state physics of metals and superconductors. It is also a very important quantity in the physics of quantum liquids like low temperature helium (both normal and superfluid 3 He), and it is quite important to nuclear physics and to understanding the stability of white dwarf stars against ...

  7. Surface states - Wikipedia

    en.wikipedia.org/wiki/Surface_states

    A simple model for the derivation of the basic properties of states at a metal surface is a semi-infinite periodic chain of identical atoms. [1] In this model, the termination of the chain represents the surface, where the potential attains the value V 0 of the vacuum in the form of a step function, figure 1.

  8. Equation of state - Wikipedia

    en.wikipedia.org/wiki/Equation_of_state

    At present, there is no single equation of state that accurately predicts the properties of all substances under all conditions. An example of an equation of state correlates densities of gases and liquids to temperatures and pressures, known as the ideal gas law, which is roughly accurate for weakly polar gases at low pressures and moderate temperatures.

  9. Structure factor - Wikipedia

    en.wikipedia.org/wiki/Structure_factor

    An alternative derivation gives good insight, but uses Fourier transforms and convolution. To be general, consider a scalar (real) quantity ϕ ( r ) {\displaystyle \phi (\mathbf {r} )} defined in a volume V {\displaystyle V} ; this may correspond, for instance, to a mass or charge distribution or to the refractive index of an inhomogeneous medium.