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Consider the elements Rubidium (Rb) and Tin (Sn). Their atomic mass, density and electronic shell structure are provided in the table below. Using the free electron gas model, evaluate the Fermi energy of Rubidium and Tin and their corresponding degenerate pressure (pressure of the electron gas). Express your pressure values in kbars. The experimental Fermi energy values for Rb and Sn are 1.85 eV and 10.2 eV respectively. How many free electrons per atom did you employ in your calculations? Explain.

Consider the elements Rubidium (Rb) and Tin (Sn). Their atomic mass, density and electronic shell structure are provided in the table below. Using the free electron gas model, evaluate the Fermi energy of Rubidium and Tin and their corresponding degenerate pressure (pressure of the electron gas). Express your pressure values in kbars. The experimental Fermi energy values for Rb and Sn are 1.85 eV and 10.2 eV respectively. How many free electrons per atom did you employ in your calculations? Explain.

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TRQ8. Solve completely the following Quantum problem. Need full detailed answer, equations and if possible, theory/literature.
Consider the elements Rubidium (Rb) and Tin (Sn). Their atomic mass, density and electronic shell structure are provided in the table below. Using the free electron gas model, evaluate the Fermi energy of Rubidium and Tin and their corresponding degenerate pressure (pressure of the electron gas). Express your pressure values in kbars. The experimental Fermi energy values for Rb and Sn are 1.85 eV and 10.2 eV respectively. How many free electrons per atom did you employ in your calculations? Explain. element atomic mass(gm/mol) density (gm/cm³) shell structure (Kr)5s' Rb 85.47 1.53 Sn 118.7 7.30 (Kr)4d105s25p?
Transcribed Image Text:Consider the elements Rubidium (Rb) and Tin (Sn). Their atomic mass, density and electronic shell structure are provided in the table below. Using the free electron gas model, evaluate the Fermi energy of Rubidium and Tin and their corresponding degenerate pressure (pressure of the electron gas). Express your pressure values in kbars. The experimental Fermi energy values for Rb and Sn are 1.85 eV and 10.2 eV respectively. How many free electrons per atom did you employ in your calculations? Explain. element atomic mass(gm/mol) density (gm/cm³) shell structure (Kr)5s' Rb 85.47 1.53 Sn 118.7 7.30 (Kr)4d105s25p?
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