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Systematics of the pressure dependence of the electron density at the nucleus for the elements Ag through Te: Pressure dependence of the Moessbauer isomer shift for Sn and Sb

Journal Article · · Phys. Rev., B; (United States)
Experimental Moessbauer isomer-shift studies have shown that when ..beta..-Sn is compressed, the charge density rho (0) at the nucleus decreases, viz., partial lnrho (0)/partial lnV > 0. This fact suggested a study of the systematics of partial lnrho (0)/partial lnV for the Ag row of the Periodic Table. We have calculated partial lnrho (0)/partial lnV for the elements Ag through Te in a Hartree-Dirac-Wigner-Seitz approximation. Exchange is treated through an exchange potential. These calculations indicate that both valence- and core-electron contributions play a role in determining partial lnrho (0)/partial lnV. In the Wigner-Seitz model, a positive sign for partial lnrho (0)/partial lnV for ..beta..-Sn (i.e., the sign which agrees with experimental high-pressure Moessbauer isomer-shift studies) is obtained only if the exchange multiplier lies in the range 1.3 < or = zeta < or = 1.5, where zeta = 1.5 corresponds to full Slater exchange. These Wigner-Seitz-model calculations indicate a negative sign for partial lnrho (0)/partial lnV for Ag, Cd, and In, and a positive sign for this derivative for Sb, and Te. The sign for Sn depends on zeta, as indicated.
Research Organization:
Department of Physics and Astronomy, University of North Carolina, Chapel Hill, North Carolina 27514
OSTI ID:
5201652
Journal Information:
Phys. Rev., B; (United States), Journal Name: Phys. Rev., B; (United States) Vol. 17:3; ISSN PLRBA
Country of Publication:
United States
Language:
English

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