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|
{
"metadata": {
"name": "",
"signature": "sha256:6f64ae81ab14bf773565224cb22f224628ca2a0e167e3fe9ede8614fd4e3f3d5"
},
"nbformat": 3,
"nbformat_minor": 0,
"worksheets": [
{
"cells": [
{
"cell_type": "heading",
"level": 1,
"metadata": {},
"source": [
"Chapter 4: Free Electron Theory of Metals"
]
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.1,Page number 112"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Charge on an electron, C\n",
"n = 8.5*10**28; # Concentration of electron in Cu, per metre cube\n",
"rho = 1.7*10**-8; # Resistivity of Cu, ohm-m\n",
"t = m/(n*e**2*rho); # Collision time for an electron in monovalent Cu, s\n",
"print\"The collision time for an electron in monovalent Cu =\",\"{0:.3e}\".format(t),\"s\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The collision time for an electron in monovalent Cu = 2.460e-14 s\n"
]
}
],
"prompt_number": 1
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.2,Page number 112"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Charge on an electron, C\n",
"n = 10**29; # Concentration of electron in material, per metre cube\n",
"rho = 27*10**-8; # Resistivity of the material, ohm-m\n",
"tau = m/(n*e**2*rho); # Collision time for an electron in the material, s\n",
"v_F = 1*10**8; # Velocity of free electron, cm/s\n",
"lamda = v_F*tau; # Mean free path of electron in the material, cm\n",
"print\"The collision time for an electron in monovalent Cu =\",\"{0:.3e}\".format(tau),\"s\";\n",
"print\"The mean free path of electron at 0K =\",\"{0:.3e}\".format(lamda),\"cm\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The collision time for an electron in monovalent Cu = 1.317e-15 s\n",
"The mean free path of electron at 0K = 1.317e-07 cm\n"
]
}
],
"prompt_number": 6
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.3,Page number 112"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Charge on an electron, C\n",
"r = 1.28*10**-10; # Atomic radius of cupper, m\n",
"a = 4*r/sqrt(2); # Lattice parameter of fcc structure of Cu, m\n",
"V = a**3; # Volume of unit cell of Cu, metre cube\n",
"n = 4/V; # Number of atoms per unit volume of Cu, per metre cube\n",
"tau = 2.7*10**-4; # Relaxation time for an electron in monovalent Cu, s\n",
"sigma = n*e**2*tau/m; # Electrical conductivity of Cu, mho per cm\n",
"print\"The free electron density in monovalent Cu =\",\"{0:.3e}\".format(n),\"per metre cube\";\n",
"print\"The electrical conductivity of monovalent Cu =\",\"{0:.3e}\".format(sigma),\"mho per cm\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The free electron density in monovalent Cu = 8.429e+28 per metre cube\n",
"The electrical conductivity of monovalent Cu = 6.403e+17 mho per cm\n"
]
}
],
"prompt_number": 8
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.4,Page number 118"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"h = 6.625*10**-34; # Planck's constant, Js\n",
"L = 10*10**-3; # Length of side of the cube, m\n",
"# For nth level\n",
"nx = 1; ny = 1; nz = 1; # Positive integers along three axis\n",
"En = h**2/(8*m*L**2)*(nx**2+ny**2+nz**2)/e; # Energy of nth level for electrons, eV\n",
"# For (n+1)th level\n",
"nx = 2; ny = 1; nz = 1; # Positive integers along three axis\n",
"En_plus_1 = h**2/(8*m*L**2)*(nx**2+ny**2+nz**2)/e; # Energy of (n+1)th level for electrons, eV\n",
"delta_E = En_plus_1 - En; # Energy difference between two levels for the free electrons\n",
"print\"The energy difference between two levels for the free electrons =\",\"{0:.3e}\".format( delta_E),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The energy difference between two levels for the free electrons = 1.130e-14 eV\n"
]
}
],
"prompt_number": 10
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.5,Page number 119"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"T = 300.0; # Room temperature of tungsten, K\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"E_F = 4.5*e; # Fermi energy of tungsten, J\n",
"E = E_F-0.1*E_F; # 10% energy below Fermi energy, J\n",
"f_T = 1.0/(1+exp((E-E_F)/(k*T))); # Probability of the electron in tungsten at room temperature at an nergy 10% below the Fermi energy\n",
"print\"The probability of the electron at an energy 10 percent below the Fermi energy in tungsten at 300 K =\",round(f_T,3);\n",
"E = 2*k*T+E_F; # For energy equal to 2kT + E_F\n",
"f_T = 1.0/(1+exp((E-E_F)/(k*T))); # Probability of the electron in tungsten at an energy 2kT above the Fermi energy\n",
"print\"The probability of the electron at an energy 2kT above the Fermi energy =\",round(f_T,4);\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The probability of the electron at an energy 10 percent below the Fermi energy in tungsten at 300 K = 1.0\n",
"The probability of the electron at an energy 2kT above the Fermi energy = 0.1192\n"
]
}
],
"prompt_number": 4
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.6,Page number 121"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"h = 6.625*10**-34; # Planck's constant, Js\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"a = 5.34*10**-10; # Lattice constant of monovalent bcc lattice, m\n",
"V = a**3; # Volume of bcc unit cell, metre cube\n",
"n = 2.0/V; # Number of atoms per metre cube\n",
"E_F = h_cross**2.0/(2*m*e)*(3*pi**2*n)**(2.0/3); # Fermi energy of monovalent bcc solid, eV\n",
"\n",
"print\"The Fermi energy of a monovalent bcc solid =\",round(E_F,4),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Fermi energy of a monovalent bcc solid = 2.0341 eV\n"
]
}
],
"prompt_number": 6
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.7,Page number 121"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"h = 6.625*10**-34; # Planck's constant, Js\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"m = 9.11*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"V = 1*10**-5; # Volume of cubical box, metre cube\n",
"E_F = 5*e; # Fermi energy, J \n",
"D_EF = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*E_F**(1.0/2)*e; # Density of states at Fermi energy, states/eV\n",
"print\"The density of states at Fermi energy =\",\"{0:.3e}\".format( D_EF),\"states/eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The density of states at Fermi energy = 1.521e+23 states/eV\n"
]
}
],
"prompt_number": 7
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.8,Page number 121"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"h = 6.626*10**-34; # Planck's constant, Js\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"V = 1*10**-6; # Volume of cubical box, metre cube\n",
"E_F = 7.13*e; # Fermi energy for Mg, J \n",
"D_EF = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*E_F**(1.0/2); # Density of states at Fermi energy for Cs, states/eV\n",
"E_Mg = 1.0/D_EF; # The energy separation between adjacent energy levels of Mg, J\n",
"print\"The energy separation between adjacent energy levels of Mg =\",\"{0:.3e}\".format(E_Mg/e),\"eV\";\n",
"E_F = 1.58*e; # Fermi energy for Cs, J \n",
"D_EF = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*E_F**(1.0/2); # Density of states at Fermi energy for Mg, states/eV\n",
"E_Mg = 1.0/D_EF; # The energy separation between adjacent energy levels of Cs, J\n",
"print\"The energy separation between adjacent energy levels of Cs =\",\"{0:.3e}\".format(E_Mg/e),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The energy separation between adjacent energy levels of Mg = 5.517e-23 eV\n",
"The energy separation between adjacent energy levels of Cs = 1.172e-22 eV\n"
]
}
],
"prompt_number": 9
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.9,Page number 122"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"E_F = 3.2*e; # Fermi energy of sodium, J\n",
"P_F = sqrt(E_F*2*m); # Fermi momentum of sodium, kg-m/s\n",
"print\"The Fermi momentum of sodium =\",\"{0:.3e}\".format(P_F),\"kg-m/sec\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Fermi momentum of sodium = 9.653e-25 kg-m/sec\n"
]
}
],
"prompt_number": 11
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.10,Page number 122"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"T = 500.0; # Rise in temperature of Al, K\n",
"EF_0 = 11.63; # Fermi energy of Al, eV\n",
"EF_T = EF_0*(1-pi**2.0/12*(k*T/EF_0)**2); # Change in Fermi energy of Al with temperature, eV\n",
"print\"The change in Fermi energy of Al with tempertaure rise of 500 degree celsius =\",round(EF_T,3),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The change in Fermi energy of Al with tempertaure rise of 500 degree celsius = 11.63 eV\n"
]
}
],
"prompt_number": 14
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.11,Page number 122"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.18*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Charge on an electron, C\n",
"lamda = 1.0*10**-9; # Mean free path of electron in metal, m\n",
"v = 1.11*10**5; # Average velocity of the electron in metal, m/s\n",
"\n",
"# For Lead\n",
"n = 13.2*10**28; # Electronic concentration of Pb, per metre cube\n",
"sigma = n*e**2*lamda/(m*v); # Electrical conductivity of lead, mho per metre\n",
"print\"The electrical conductivity of lead =\",\"{0:.3e}\".format(sigma),\"mho per metre\";\n",
"\n",
"# For Silver\n",
"n = 5.85*10**28; # Electronic concentration of Ag, per metre cube\n",
"sigma = n*e**2*lamda/(m*v); # Electrical conductivity of Ag, mho per metre\n",
"print\"The electrical conductivity of silver =\",\"{0:.3e}\".format(sigma),\"mho per metre\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The electrical conductivity of lead = 3.316e+07 mho per metre\n",
"The electrical conductivity of silver = 1.470e+07 mho per metre\n"
]
}
],
"prompt_number": 17
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.12,Page number 125"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Charge on an electron, C\n",
"L = pi**2.0/3*(k/e)**2; # Lorentz number, watt-ohm/degree-square\n",
"print\"The Lorentz number =\",\"{0:.3e}\".format(L),\"watt-ohm/degree-square\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Lorentz number = 2.447e-08 watt-ohm/degree-square\n"
]
}
],
"prompt_number": 19
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.13,Page number 125"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"A =[[1,2,3,4],[5,6,7,8],[9,10,11,12],[13,14,15,16]]; # Declare a 4X4 cell\n",
"A[0][0] = 'Mg'; \n",
"A[0][1] = 2.54*10**-5; \n",
"A[0][2] = 1.5; \n",
"A[0][3] = 2.32*10**2; \n",
"A[1][0] = 'Cu'; \n",
"A[1][1] = 6.45*10**-5; \n",
"A[1][2] = 3.85; \n",
"A[1][3] = 2.30*10**2; \n",
"A[2][0] = 'Al'; \n",
"A[2][1] = 4.0*10**-5; \n",
"A[2][2] = 2.38;\n",
"A[2][3] = 2.57*10**2; \n",
"A[3][0] = 'Pt'; \n",
"A[3][1] = 1.02*10**-5; \n",
"A[3][2] = 0.69;\n",
"A[3][3] = 2.56*10**2; \n",
"T1 = 273; # First temperature, K\n",
"T2 = 373; # Second temperature, K\n",
"print\"_________________________________________________________________\";\n",
"print\"Metal sigma x 10**-05 K(W/cm-K) Lorentz number \";\n",
"print\" (mho per cm) (watt-ohm/deg-square)x10**-2\";\n",
"print\"_________________________________________________________________\";\n",
"for i in range (0,4) :\n",
" L1 = A[i][2]/(A[i][1]*T1); \n",
" L2 = A[i][3];\n",
" print\"\",A[i][0],\" \",A[i][1]/10**-5,\" \",A[i][2],\" \",L2/10**2,\" \",L2/10**2;\n",
"print\"_________________________________________________________________\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"_________________________________________________________________\n",
"Metal sigma x 10**-05 K(W/cm-K) Lorentz number \n",
" (mho per cm) (watt-ohm/deg-square)x10**-2\n",
"_________________________________________________________________\n",
" Mg 2.54 1.5 2.32 2.32\n",
" Cu 6.45 3.85 2.3 2.3\n",
" Al 4.0 2.38 2.57 2.57\n",
" Pt 1.02 0.69 2.56 2.56\n",
"_________________________________________________________________\n"
]
}
],
"prompt_number": 20
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.14,Page number 125"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"A = [[1,2],[3,4]]; # Declare a 2X3 cell\n",
"A[0][0] = 1.6*10**8; # Electrcal conductivity of Au at 100 K, mho per metre\n",
"A[0][1] = 2.0*10**-8; # Lorentz number of Au at 100 K, volt/K-square\n",
"A[1][0] = 5.0*10**8; # Electrcal conductivity of Au at 273 K, mho per metre\n",
"A[1][1] = 2.4*10**-8; # Lorentz number of Au at 273 K, volt/K-square\n",
"T1 = 100; # First temperature, K\n",
"T2 = 273; # Second temperature, K\n",
"\n",
"print\"___________________________________________________________________________\";\n",
"print\" T = 100 K T = 273 K \";\n",
"print\"_________________________________ ___________________________________\";\n",
"print\"Electrical conductivity) L Electrical conductivity) L \";\n",
"print\" mho per metre V/K-square mho per metre V/K-square\";\n",
"print\"___________________________________________________________________________\";\n",
"K1 = A[0][0]*T1*A[0][1]; \n",
"K2 = A[1][0]*T2*A[1][1];\n",
"print\"{0:.3e}\".format(A[0][0]),\" \",\"{0:.3e}\".format(A[0][1]),\" \",\"{0:.3e}\".format(A[1][0]),\" \",\"{0:.3e}\".format(A[1][1]) \n",
"print\"K =\",K1,\"W/cm-K K =\",K2,\"W/cm-K\";\n",
"print\"___________________________________________________________________________\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"___________________________________________________________________________\n",
" T = 100 K T = 273 K \n",
"_________________________________ ___________________________________\n",
"Electrical conductivity) L Electrical conductivity) L \n",
" mho per metre V/K-square mho per metre V/K-square\n",
"___________________________________________________________________________\n",
"1.600e+08 2.000e-08 5.000e+08 2.400e-08\n",
"K = 320.0 W/cm-K K = 3276.0 W/cm-K\n",
"___________________________________________________________________________\n"
]
}
],
"prompt_number": 29
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.15,Page number 131"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"e = 1.6*10**-19; # Electronic charge, C\n",
"a = 0.428*10**-9; # Lattice constant of Na, m\n",
"V = a**3; # Volume of unit cell, metre cube\n",
"N = 2; # No. of atoms per unit cell of Na\n",
"n = N/V; # No. of electrons per metre cube, per metre cube\n",
"R_H = -1.0/(n*e); # Hall coeffcient of Na, metre cube per coulomb\n",
"print\"The Hall coefficient of sodium =\",\"{0:.3e}\".format(R_H),\"metre cube per coulomb\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Hall coefficient of sodium = -2.450e-10 metre cube per coulomb\n"
]
}
],
"prompt_number": 2
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.16,Page number 131"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"e = 1.6*10**-19; # Electronic charge, C\n",
"n = 24.2*10**28; # No. of electrons per metre cube, per metre cube\n",
"R_H = -1.0/(n*e); # Hall coeffcient of Be, metre cube per coulomb\n",
"print\"The Hall coefficient of beryllium =\",\"{0:.3e}\".format(R_H),\"metre cube per coulomb\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Hall coefficient of beryllium = -2.583e-11 metre cube per coulomb\n"
]
}
],
"prompt_number": 4
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.17,Page number 131"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"e = 1.6*10**-19; # Electronic charge, C\n",
"R_H = -8.4*10**-11; # Hall coeffcient of Ag, metre cube per coulomb\n",
"n = -3*pi/(8*R_H*e); # Electronic concentration of Ag, per metre cube\n",
"print\"The electronic concentration of Ag =\",\"{0:.3e}\".format(n),\"per metre cube\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The electronic concentration of Ag = 8.766e+28 per metre cube\n"
]
}
],
"prompt_number": 6
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.18,Page number 134"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"# We have from Mattheissen rule, rho = rho_0 + alpha*T1\n",
"T1 = 300.0; # Initial temperature, K\n",
"T2 = 1000.0; # Final temperature, K\n",
"rho = 1*10**-6; # Resistivity of the metal, ohm-m\n",
"delta_rho = 0.07*rho; # Increase in resistivity of metal, ohm-m\n",
"alpha = delta_rho/(T2-T1); # A constant, ohm-m/K\n",
"rho_0 = rho - alpha*T1; # Resistivity at room temperature, ohm-m\n",
"print\"The resistivity at room temperature =\",\"{0:.3e}\".format(rho),\"ohm-m\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The resistivity at room temperature = 1.000e-06 ohm-m\n"
]
}
],
"prompt_number": 8
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.19,Page number 134"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"# We have from Mattheissen rule, rho = rho_0 + alpha*T1\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"rho_40 = 0.2; # Resistivity of Ge at 40 degree celsius, ohm-m\n",
"E_g = 0.7; # Bandgap for Ge, eV\n",
"T1 = 20+273; # Second temperature, K\n",
"T2 = 40 + 273; # First temperature, K\n",
"rho_20 = rho_40*exp(E_g*e/(2*k)*(1.0/T1-1.0/T2)); # Resistivity of Ge at 20 degree celsius, ohm-m\n",
"print\"The resistivity of Ge at 20 degree celsius =\",round(rho_20,1),\"ohm-m\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The resistivity of Ge at 20 degree celsius = 0.5 ohm-m\n"
]
}
],
"prompt_number": 12
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.20,Page number 135"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"rs_a0_ratio = 3.25; # Ratio of solid radius to the lattice parameter\n",
"E_F = 50.1*(rs_a0_ratio)**(-2); # Fermi level energy of Li, eV\n",
"T_F = 58.2e+04*(rs_a0_ratio)**(-2); # Fermi level temperature of Li, K\n",
"V_F = 4.20e+08*(rs_a0_ratio)**(-1); # Fermi level velocity of electron in Li, cm/sec\n",
"K_F = 3.63e+08*(rs_a0_ratio)**(-1); \n",
"print\"E_F =\",round(E_F,2),\"eV\";\n",
"print\"T_F =\",\"{0:.3e}\".format(T_F),\"K\";\n",
"print\"V_F =\",\"{0:.3e}\".format(V_F),\"cm/sec\";\n",
"print\"K_F =\",\"{0:.3e}\".format(K_F),\"per cm\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"E_F = 4.74 eV\n",
"T_F = 5.510e+04 K\n",
"V_F = 1.292e+08 cm/sec\n",
"K_F = 1.117e+08 per cm\n"
]
}
],
"prompt_number": 14
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.21,Page number 135"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"n = 6.04*10**22; # Concentration of electrons in yittrium, per metre cube\n",
"r_s = (3/(4*pi*n))**(1.0/3)/10**-8; # Radius of the solid, angstrom\n",
"a0 = 0.529; # Lattice parameter of yittrium, angstrom\n",
"rs_a0_ratio = r_s/a0; # Solid radius to lattice parameter ratio\n",
"E_F = 50.1*(rs_a0_ratio)**(-2); # Fermi level energy of Y, eV\n",
"print\"The Fermi energy of yittrium =\",round(E_F,4),\"eV\";\n",
"Ryd = 13.6; # Rydberg energy constant, eV\n",
"E_bs = 0.396*Ryd; # Band structure energy value of Y, eV\n",
"print\"The band structure value of E_F =\",round(E_bs,3),\"eV is in close agreement with the calculated value of\",round(E_F,4),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Fermi energy of yittrium = 5.6083 eV\n",
"The band structure value of E_F = 5.386 eV is in close agreement with the calculated value of 5.6083 eV\n"
]
}
],
"prompt_number": 16
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.22,Page number 137"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"rs_a0_ratio = 2.07; # Solid radius to lattice parameter ratio for Al\n",
"E_F = 50.1*(rs_a0_ratio)**(-2); # Fermi level energy of Y, eV\n",
"# According to Jellium model, h_cross*omega_P = E = 47.1 eV *(rs_a0_ratio)**(-3/2)\n",
"E = 47.1*(rs_a0_ratio)**(-3.0/2); # Plasmon energy of Al, eV\n",
"print\"The plasmon energy of Al =\",round(E,4),\"eV\";\n",
"print\"The experimental value is 15 eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The plasmon energy of Al = 15.8149 eV\n",
"The experimental value is 15 eV\n"
]
}
],
"prompt_number": 18
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.1a,Page number 137"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"E_F = 1; # For simplicity assume Fermi energy to be unity, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"dE = 0.1; # Exces energy above Fermi level, eV\n",
"T = 300; # Room temperature, K\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV above E_F\n",
"print\"At 300 K:\";\n",
"print\"=========\";\n",
"print\"The occupation probability of electron at\",round(dE,3),\"eV above Fermi energy =\",round(f_E,3);\n",
"E = E_F - dE; # Energy of the level below Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV below E_F\n",
"print\"The occupation probability of electron at\",round(dE,3),\"below Fermi energy =\",round(f_E,3);\n",
"\n",
"T = 1000; # New temperature, K\n",
"print\"At 1000 K:\";\n",
"print\"=========\";\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV above E_F\n",
"print\"The occupation probability of electron at\",round(dE,3),\"eV above Fermi energy =\",round(f_E,3);\n",
"E = E_F - dE; # Energy of the level below Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV below E_F\n",
"print\"The occupation probability of electron at\",round(dE,3),\"eV below Fermi energy =\",round(f_E,3);\n",
"\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"At 300 K:\n",
"=========\n",
"The occupation probability of electron at 0.1 eV above Fermi energy = 0.021\n",
"The occupation probability of electron at 0.1 below Fermi energy = 0.979\n",
"At 1000 K:\n",
"=========\n",
"The occupation probability of electron at 0.1 eV above Fermi energy = 0.239\n",
"The occupation probability of electron at 0.1 eV below Fermi energy = 0.761\n"
]
}
],
"prompt_number": 20
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.2a,Page number 138"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"f_E = 0.01; # Occupation probability of electron\n",
"E_F = 1; # For simplicity assume Fermi energy to be unity, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"dE = 0.5; # Exces energy above Fermi level, eV\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"# We have, f_E = 1/(exp((E-E_F)*e/(k*T))+1), solving for T\n",
"T = (E-E_F)*e/k*1.0/log(1.0/f_E-1); # Temperature at which the electron will have energy 0.1 eV above the Fermi energy, K\n",
"print\"The temperature at which the electron will have energy\",round(dE,3),\"eV above the Fermi energy =\",round(T,3),\"K\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The temperature at which the electron will have energy 0.5 eV above the Fermi energy = 1261.578 K\n"
]
}
],
"prompt_number": 22
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.3a,Page number 139"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"E_F = 10; # Fermi energy of electron in metal, eV\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"E_av = 3.0/5*E_F; # Average energy of free electron in metal at 0 K, eV\n",
"V_F = sqrt(2*E_av*e/m); # Speed of free electron in metal at 0 K, eV\n",
"print\"The average energy of free electron in metal at 0 K =\",round(E_av,3),\"eV\";\n",
"print\"The speed of free electron in metal at 0 K =\",\"{0:.3e}\".format(V_F),\"m/s\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The average energy of free electron in metal at 0 K = 6.0 eV\n",
"The speed of free electron in metal at 0 K = 1.453e+06 m/s\n"
]
}
],
"prompt_number": 26
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.4a,Page number 139"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"f_E = 0.1; # Occupation probability of electron\n",
"E_F = 5.5; # Fermi energy of Cu, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"dE = 0.05*E_F; # Exces energy above Fermi level, eV\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"# We have, f_E = 1/(exp((E-E_F)*e/(k*T))+1), solving for T\n",
"T = (E-E_F)*e/k*1.0/log(1.0/f_E-1); # Temperature at which the electron will have energy 0.1 eV above the Fermi energy, K\n",
"print\"The temperature at which the electron will have energy\",round(dE/E_F*100,3),\"percent above the Fermi energy\",round(T,3),\"K\";\n",
"\n",
"#(The answer given in the textbook is wrong) "
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The temperature at which the electron will have energy 5.0 percent above the Fermi energy 1451.106 K\n"
]
}
],
"prompt_number": 2
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.5a,Page number 139"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"T_F = 24600; # Fermi temperature of potassium, K\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"E_F = k*T_F; # Fermi energy of potassium, eV\n",
"v_F = sqrt(2*k*T_F/m); # Fermi velocity of potassium, m/s\n",
"print\"The Fermi velocity of potassium =\",\"{0:.3e}\".format(v_F),\"m/s\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Fermi velocity of potassium = 8.638e+05 m/s\n"
]
}
],
"prompt_number": 4
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.6a,Page number 139"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"E_F = 7.0; # Fermi energy of Cu, eV\n",
"f_E = 0.9; # Occupation probability of Cu\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"T = 1000; # Given temperature, K\n",
"# We have, f_E = 1/(exp((E-E_F)*e/(k*T))+1), solving for E\n",
"E = k*T*log(1.0/f_E-1) + E_F*e; # Energy level of Cu for 10% occupation probability at 1000 K, J\n",
"print\"The energy level of Cu for 10 percent occupation probability at 1000 K =\",round(E/e,3),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The energy level of Cu for 10 percent occupation probability at 1000 K = 6.81 eV\n"
]
}
],
"prompt_number": 6
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.7a,Page number 140"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of an electron, kg\n",
"e = 1.6*10**-19; # Electronic charge, C\n",
"h = 6.626*10**-34; # Planck's constant, Js\n",
"E_F = 1.55; # Fermi energy of Cu, eV\n",
"n = (pi/3)*(8*m/h**2)**(3.0/2)*(E_F*e)**(3.0/2); # Electronic concentration in cesium, electrons/cc\n",
"print\"The electronic concentration in cesium =\",\"{0:.3e}\".format(n),\"electrons/cc\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The electronic concentration in cesium = 8.733e+27 electrons/cc\n"
]
}
],
"prompt_number": 12
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.8a,Page number 141"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"E_F = 7; # Fermi energy, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"T_F = E_F*e/k; # Fermi temperature, K\n",
"print\"The Fermi temperature corresponding to Fermi energy =\",\"{0:.3e}\".format(T_F),\"K\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The Fermi temperature corresponding to Fermi energy = 8.116e+04 K\n"
]
}
],
"prompt_number": 14
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.9a,Page number 141"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of the electron, kg\n",
"h = 6.626*10**-34; # Planck's constant, Js\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"s = 0.01; # Side of the box, m\n",
"E = 2; # Energy range of the electron in the box, eV\n",
"V = s**3; # Volume of the box, metre cube\n",
"I = I = 2*E**(3.0/2)/3; # Definite integral over E : I = 2*E**(3/2)/3\n",
"D_E = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*I*e**(3.0/2); # Density of states for the electron in a cubical box, states\n",
"print\"The density of states for the electron in a cubical box =\",\"{0:.3e}\".format(D_E),\"states\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The density of states for the electron in a cubical box = 1.280e+22 states\n"
]
}
],
"prompt_number": 7
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.10a,Page number 141"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"E_F = 1; # For simplicity assume Fermi energy to be unity, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"dE = 0.5; # Exces energy above Fermi level, eV\n",
"T = 300; # Room temperature, K\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"f_E = 1./(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV above E_F\n",
"print\"At 300 K:\";\n",
"print\"=========\";\n",
"print\"The occupation probability of electron at\",dE,\"eV above Fermi energy =\",\"{0:.3e}\".format(f_E);\n",
"E = E_F - dE; # Energy of the level below Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV below E_F\n",
"print\"The occupation probability of electron at\",dE,\"eV above Fermi energy =\",\"{0:.3e}\".format(f_E);\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"At 300 K:\n",
"=========\n",
"The occupation probability of electron at 0.5 eV above Fermi energy = 4.054e-09\n",
"The occupation probability of electron at 0.5 eV above Fermi energy = 1.000e+00\n"
]
}
],
"prompt_number": 11
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.11a,Page number 141"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"E_F = 1; # For simplicity assume Fermi energy to be unity, eV\n",
"k = 1.38*10**-23; # Boltzmann constant, J/mol/K\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"dE = 0.2; # Exces energy above Fermi level, eV\n",
"T = 0+273; # Room temperature, K\n",
"E = E_F + dE; # Energy of the level above Fermi level, eV\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV above E_F\n",
"print\"At 273 K:\";\n",
"print\"=========\";\n",
"print\"The occupation probability of electron at\",dE,\"eV above Fermi energy =\",\"{0:.3e}\".format(f_E);\n",
"T = 100+273; # Given temperature of 100 degree celsius, K\n",
"f_E = 1.0/(exp((E-E_F)*e/(k*T))+1); # Occupation probability of the electron at 0.1 eV below E_F\n",
"print\"At 373 K:\";\n",
"print\"=========\";\n",
"print\"The occupation probability of electron at\",dE,\"eV above Fermi energy =\",\"{0:.3e}\".format(f_E);\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"At 273 K:\n",
"=========\n",
"The occupation probability of electron at 0.2 eV above Fermi energy = 2.047e-04\n",
"At 373 K:\n",
"=========\n",
"The occupation probability of electron at 0.2 eV above Fermi energy = 1.992e-03\n"
]
}
],
"prompt_number": 13
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.12a,Page number 142"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of the electron, kg\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"r = 1.28*10**-10; # Atomic radius of Cu, m\n",
"a = 4*r/sqrt(2); # Lattice constant of Cu, m\n",
"tau = 2.7*10**-14; # Relaxation time for the electron in Cu, s\n",
"V = a**3; # Volume of the cell, metre cube\n",
"n = 4.0/V; # Concentration of free electrons in monovalent copper, \n",
"sigma = n*e**2*tau/m; # Electrical conductivity of monovalent copper, mho per m\n",
"print\"The electrical conductivity of monovalent copper =\",\"{0:.3e}\".format( sigma/100),\"mho per cm\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The electrical conductivity of monovalent copper = 6.403e+05 mho per cm\n"
]
}
],
"prompt_number": 15
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.13a,Page number 142"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"n = 18.1*10**22; # Number of electrons per unit volume, per cm cube\n",
"N = n/2; # Pauli's principle for number of energy levels, per cm cube\n",
"E_F = 11.58; # Fermi energy of Al, eV\n",
"E = E_F/N; # Interelectronic energy separation between bands of Al, eV\n",
"print\"The interelectronic energy separation between bands of Al =\",\"{0:.3e}\".format(E),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The interelectronic energy separation between bands of Al = 1.280e-22 eV\n"
]
}
],
"prompt_number": 17
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.14a,Page number 142"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of the electron, kg\n",
"h = 6.626*10**-34; # Planck's constant, Js\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"E_F = 7; # Fermi energy of Cu, eV\n",
"V = 10**-6; # Volume of the cubic metal, metre cube\n",
"D_EF = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*(E_F)**(1.0/2)*e**(3.0/2); # Density of states in Cu contained in cubic metal, states/eV\n",
"print\"The density of states in Cu contained in cubic metal =\",\"{0:.3e}\".format(D_EF),\"states/eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The density of states in Cu contained in cubic metal = 1.796e+22 states/eV\n"
]
}
],
"prompt_number": 20
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.15a,Page number 143"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"m = 9.1*10**-31; # Mass of the electron, kg\n",
"h = 6.626*10**-34; # Planck's constant, Js\n",
"e = 1.6*10**-19; # Energy equivalent of 1 eV, J/eV\n",
"h_cross = h/(2*pi); # Reduced Planck's constant, Js\n",
"E_F = 7; # Fermi energy of Cu, eV\n",
"V = 10**-6; # Volume of the cubic metal, metre cube\n",
"D_EF = V/(2*pi**2)*(2*m/h_cross**2)**(3.0/2)*(E_F)**(1.0/2)*e**(3.0/2); # Density of states in Cu contained in cubic metal, states/eV\n",
"d = 1.0/(D_EF); # Electronic energy level spacing between successive levels of Cu, eV\n",
"print\"The electronic energy level spacing between successive levels of Cu =\",\"{0:.3e}\".format(d),\"eV\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"The electronic energy level spacing between successive levels of Cu = 5.568e-23 eV\n"
]
}
],
"prompt_number": 24
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.16a,Page number 143"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"A = [[1,2],[3,4],[5,6],[7,8]]; # Declare a 4X2 matrix \n",
"A[0][0] = 'Li'; \n",
"A[0][1] = -0.4039; # Energy of outermost atomic orbital of Li, Rydberg unit\n",
"A[1][0] = 'Na'; # \n",
"A[1][1] = -0.3777; # Energy of outermost atomic orbital of Na, Rydberg unit\n",
"A[2][0] = 'F'; # \n",
"A[2][1] = -1.2502; # Energy of outermost atomic orbital of F, Rydberg unit\n",
"A[3][0] = 'Cl'; # \n",
"A[3][1] = -0.9067; # Energy of outermost atomic orbital of Cl, Rydberg unit\n",
"cf = 13.6; # Conversion factor for Rydberg to eV\n",
"print\"________________________________________\";\n",
"print\" Atom Energy gap\";\n",
"print\"\",A[1][0],A[3][0],\" \",(A[1][1]-A[3][1])*cf,\"eV\";\n",
"print\"\",A[1][0],A[2][0],\" \",(A[1][1]-A[2][1])*cf,\"eV\";\n",
"print\"\",A[0][0],A[2][0],\" \",(A[0][1]-A[2][1])*cf,\"eV\";\n",
"\n",
"print\"________________________________________\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"________________________________________\n",
" Atom Energy gap\n",
" Na Cl 7.1944 eV\n",
" Na F 11.866 eV\n",
" Li F 11.50968 eV\n",
"________________________________________\n"
]
}
],
"prompt_number": 11
},
{
"cell_type": "heading",
"level": 2,
"metadata": {},
"source": [
"Example 4.18a,Page number 144"
]
},
{
"cell_type": "code",
"collapsed": false,
"input": [
"import math\n",
"\n",
"#Given Data\n",
"# For Cu\n",
"rs_a0_ratio = 2.67; # Ratio of solid radius to the lattice parameter\n",
"E_F = 50.1*(rs_a0_ratio)**(-2); # Fermi level energy of Cu, eV\n",
"T_F = 58.2*10**4*(rs_a0_ratio)**(-2); # Fermi level temperature of Cu, K\n",
"V_F = 4.20*10**8*(rs_a0_ratio)**(-1); # Fermi level velocity of electron in Cu, cm/sec\n",
"K_F = 3.63*10**8*(rs_a0_ratio)**(-1); \n",
"print\"For Cu :\";\n",
"print\"========\";\n",
"print\"E_F =\",round(E_F,3),\"eV\";\n",
"print\"T_F =\",\"{0:.3e}\".format(T_F),\"K\";\n",
"print\"V_F =\",\"{0:.3e}\".format(V_F),\"cm/sec\";\n",
"print\"K_F =\",\"{0:.3e}\".format(K_F),\"per cm\";\n",
"rs_a0_ratio = 3.07; # Ratio of solid radius to the lattice parameter\n",
"E_F = 50.1*(rs_a0_ratio)**(-2); # Fermi level energy of Nb, eV\n",
"T_F = 58.2*10**4*(rs_a0_ratio)**(-2); # Fermi level temperature of Nb, K\n",
"V_F = 4.20*10**8*(rs_a0_ratio)**(-1); # Fermi level velocity of electron in Nb, cm/sec\n",
"K_F = 3.63*10**8*(rs_a0_ratio)**(-1); \n",
"print\"For Nb :\";\n",
"print\"========\";\n",
"print\"E_F =\",round(E_F,3),\"eV\";\n",
"print\"T_F =\",\"{0:.3e}\".format(T_F),\"K\";\n",
"print\"V_F =\",\"{0:.3e}\".format(V_F),\"cm/sec\";\n",
"print\"K_F =\",\"{0:.3e}\".format(K_F),\"per cm\";\n"
],
"language": "python",
"metadata": {},
"outputs": [
{
"output_type": "stream",
"stream": "stdout",
"text": [
"For Cu :\n",
"========\n",
"E_F = 7.028 eV\n",
"T_F = 8.164e+04 K\n",
"V_F = 1.573e+08 cm/sec\n",
"K_F = 1.360e+08 per cm\n",
"For Nb :\n",
"========\n",
"E_F = 5.316 eV\n",
"T_F = 6.175e+04 K\n",
"V_F = 1.368e+08 cm/sec\n",
"K_F = 1.182e+08 per cm\n"
]
}
],
"prompt_number": 14
},
{
"cell_type": "code",
"collapsed": false,
"input": [],
"language": "python",
"metadata": {},
"outputs": []
}
],
"metadata": {}
}
]
}
|