1991
DOI: 10.1116/1.577558
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Free energy model for the analysis of bonding in a-SixNyHz alloys

Abstract: A free energy model (FEM) for the analysis of the bonding in amorphous covalent alloys is developed and applied to ternary a-SixNyHz alloys. The quasichemical approach to the thermodynamics of regular solutions is used to obtain the Gibbs free energy of mixing GM=HM−TSM for the alloys. The enthalpy of mixing HM is determined by the nearest-neighbor bond energies while the entropy of mixing SM is given by the number of possible bonding configurations in Si-centered tetrahedra. The concentrations of Si–N, Si–Si,… Show more

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Cited by 23 publications
(3 citation statements)
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“…Note that deviations due to numerical errors of the ray tracing simulations or the measurement uncertainty for the optical constants are not considered. The resulting value for λ b of 353 nm is equivalent to a photon energy of 3.5 eV, which is in good agreement with a bond energy of Si‐H between 3.34 and 3.5 eV according to References . Hence, we interpret that the UV irradiance induces the breaking of Si‐H bonds at the interface, which results in dangling bonds at the Si surface.…”
Section: Resultssupporting
confidence: 89%
“…Note that deviations due to numerical errors of the ray tracing simulations or the measurement uncertainty for the optical constants are not considered. The resulting value for λ b of 353 nm is equivalent to a photon energy of 3.5 eV, which is in good agreement with a bond energy of Si‐H between 3.34 and 3.5 eV according to References . Hence, we interpret that the UV irradiance induces the breaking of Si‐H bonds at the interface, which results in dangling bonds at the Si surface.…”
Section: Resultssupporting
confidence: 89%
“…The ion bombardment of ionized species on the film surface during the deposition leads to the densification of the film, resulting in an increase in film density. 22) We speculate that the higher N 2 gas flow ratio disturbs the ion bombardment, resulting in a decrease in film density. The SiN film with a higher density tends to stretch, resulting in a higher compressive stress.…”
Section: Resultsmentioning
confidence: 86%
“…The high‐temperature fits consist of a sum of Debye and Einstein heat capacity functions of the form:C=n1·DnormalΘDT+m1·EnormalΘET+A1·Twhere DnormalΘD/T andEnormalΘE/T are Debye and Einstein functions; m1, n1,normalΘD, and ΘE are all adjustable parameters; (n1+m1) should be approximately equal to the number of atoms in the formula unit or unit cell. The characteristic Debye temperature normalΘD obtained from the fitting shows that a‐SiNH #240 has the highest normalΘD(1261 K).…”
Section: Resultsmentioning
confidence: 99%