Advanced Mathematical Physics and Quantum Electron Theory of Solids

Complex Numbers

  • Fundamental Definition: A complex number zz is represented in rectangular form as z=x+iyz = x + iy, where xx is the real part and yy is the imaginary part.

  • Argand Diagram: A geometric representation of complex numbers where the horizontal axis represents the real part and the vertical axis represents the imaginary part. A point PP can be identified by coordinates (x,iy)(x, iy) or polar coordinates (r,θ)(r, \theta).

  • Polar Form: z=r(cos(θ)+isin(θ))z = r(\text{cos}(\theta) + i\text{sin}(\theta)). Here, rr is the modulus and θ\theta is the argument.

  • Modulus of zz: Denoted as z|z| or rr, it is defined as |z| = \text{modulus of } z = \text{\sqrt{x^2 + y^2}}.

  • Argument of zz: Denoted as θ\theta or arg(z)\text{arg}(z), defined as θ=tan1(yx)\theta = \text{tan}^{-1}(\frac{y}{x}). The standard range is typically -\pi < \theta \le \pi.

  • Example Representation: To represent 53i5 - 3i and 5+3i5 + 3i on an Argand diagram, 5+3i5 + 3i is in the first quadrant, while its conjugate 53i5 - 3i is in the fourth quadrant.

  • Complex Conjugate (zz^*): If z=x+iyz = x + iy, then the complex conjugate is z=xiyz^* = x - iy.

Properties and Fundamental Laws of Complex Algebra

  • Equality: If two complex numbers are equal, then their real parts must be equal and their imaginary parts must be equal (x1=x2x_1 = x_2 and y1=y2y_1 = y_2).

  • Addition: (x1+iy1)+(x2+iy2)=(x1+x2)+i(y1+y2)(x_1 + iy_1) + (x_2 + iy_2) = (x_1 + x_2) + i(y_1 + y_2).

  • Commutative Law: z1+z2=z2+z1z_1 + z_2 = z_2 + z_1 and z1z2=z2z1z_1 z_2 = z_2 z_1.

  • Associative Law: z1+(z2+z3)=(z1+z2)+z3z_1 + (z_2 + z_3) = (z_1 + z_2) + z_3 and z1(z2z3)=(z1z2)z3z_1 (z_2 z_3) = (z_1 z_2) z_3.

  • Additive Identity: The complex number 0=0+i00 = 0 + i0 such that z+0=zz + 0 = z.

  • Additive Inverse: For z=x+iyz = x + iy, the inverse is z=xiy-z = -x - iy such that z+(z)=0z + (-z) = 0.

  • Multiplicative Inverse: For z=x+iyz' = x' + iy', if zz=1zz' = 1, then z=1x+iy=xiyx2+y2z' = \frac{1}{x + iy} = \frac{x - iy}{x^2 + y^2}. Thus, x=xx2+y2x' = \frac{x}{x^2 + y^2} and y=yx2+y2y' = \frac{-y}{x^2 + y^2}.

  • Distributive Law: (z1+z2)z3=z1z3+z2z3(z_1 + z_2)z_3 = z_1z_3 + z_2z_3.

  • Identity of Multiplication: z×1=zz \times 1 = z.

  • Sum of Conjugates: The complex conjugate of a sum is the sum of the conjugates: \text{\overline{z_1 + z_2}} = z_1^* + z_2^*.

  • Product of Conjugates: zz=(x+iy)(xiy)=x2+y2=z2z \cdot z^* = (x + iy)(x - iy) = x^2 + y^2 = |z|^2.

  • Real and Imaginary Parts via Conjugates:

    • z+z=2x=2Re(z)z + z^* = 2x = 2\text{Re}(z).

    • zz=2iy=2iIm(z)z - z^* = 2iy = 2i\text{Im}(z).

Vector Spaces

  • Definition: A vector space VV is a collection of vectors in nn-dimensional space over a scalar field FF that satisfies:

    • Closure Property: Under addition (u+vVu + v \in V) and scalar multiplication (auVau \in V).

    • Commutative Law: Under addition (u+v=v+uu + v = v + u).

    • Associative Law: Under addition (u+(v+w)=(u+v)+wu + (v + w) = (u + v) + w).

    • Existence of Identity: Additive identity 00 exists.

    • Additive Inverse: For every uu, there exists u-u such that u+(u)=0u + (-u) = 0.

    • Distributive Properties: a(u+v)=au+ava(u + v) = au + av and (a+b)u=au+bu(a + b)u = au + bu.

    • Associative Law (Scalars): a(bu)=(ab)ua(b \cdot u) = (ab)u.

    • Identity of Scalar Multiplication: v1=vv \cdot 1 = v.

  • Linear Independence: A subset BB is linearly independent if for distinct vectors u1,u2,,umu_1, u_2, \dots, u_m and scalars c1,c2,,cmc_1, c_2, \dots, c_m, the equation ciui=0\sum c_i u_i = 0 implies all ci=0c_i = 0.

  • Properties of Sets:

    • Any set containing a linearly dependent subset is itself linearly dependent.

    • Any subset of a linearly independent set is linearly independent.

    • Any set containing the zero vector (00) is always linearly dependent.

  • Basis and Dimension: A basis is a linearly independent set of vectors that spans the vector space VV. The dimension is the number of elements in the basis.

  • Examples of Vector Spaces:

    • Matrices: e.g., a 2×32 \times 3 matrix set where addition and scalar multiplication are defined.

    • Polynomials: Sets of polynomials such as expressions of the form a0+a1x+a2x2++anxna_0 + a_1x + a_2x^2 + \dots + a_nx^n.

Hermite Polynomials (Orthogonal Polynomials)

  • Context: Used in signal processing, Brownian motion probability, numerical analysis, quantum mechanics (harmonic oscillator), and system theory.

  • Definitions (Rodrigues' Formula):

    • Probabilists' version: Hn(x)=(1)nex22dndxn(ex22)H_n(x) = (-1)^n e^{\frac{x^2}{2}} \frac{d^n}{dx^n}(e^{-\frac{x^2}{2}}).

    • Physicists' version (More commonly used): Hn(x)=(1)nex2dndxn(ex2)H_n(x) = (-1)^n e^{x^2} \frac{d^n}{dx^n}(e^{-x^2}).

  • Generated Polynomials:

    • H0(x)=1H_0(x) = 1

    • H1(x)=2xH_1(x) = 2x

    • H2(x)=4x22H_2(x) = 4x^2 - 2

    • H3(x)=8x312xH_3(x) = 8x^3 - 12x

    • H4(x)=16x448x2+12H_4(x) = 16x^4 - 48x^2 + 12

    • H5(x)=32x5160x3+120xH_5(x) = 32x^5 - 160x^3 + 120x

    • H6(x)=64x6480x4+720x2120H_6(x) = 64x^6 - 480x^4 + 720x^2 - 120

  • Properties:

    • Parity: For even nn, the function is symmetric (even parity). For odd nn, the function is anti-symmetric (odd parity).

    • Orthogonality: Hm(x)Hn(x)ex2dx=π2nn!δmn\int_{-\infty}^{\infty} H_m(x) H_n(x) e^{-x^2} dx = \sqrt{\pi} 2^n n! \delta_{mn}. If mnm \neq n, the integral is 00.

    • Recursive Relation: Hn(x)=(2xddx)Hn1(x)H_n(x) = (2x - \frac{d}{dx}) H_{n-1}(x).

Legendre Polynomials

  • Definition: A system of complete and orthogonal polynomials used in gravitational and Coulomb potential problems.

  • Standardization: Defined over the interval [1,1][-1, 1] with weight function w(x)=1w(x) = 1. Normalized such that Pn(1)=1P_n(1) = 1.

  • Values:

    • P0(x)=1P_0(x) = 1

    • P1(x)=xP_1(x) = x

    • P2(x)=12(3x21)P_2(x) = \frac{1}{2}(3x^2 - 1)

  • Orthogonality Condition: 11Pm(x)Pn(x)dx=22n+1δmn\int_{-1}^{1} P_m(x) P_n(x) dx = \frac{2}{2n+1} \delta_{mn}. For mnm \neq n, the integral vanishes.

  • Generating Function: (12xz+z2)12=n=0Pn(x)zn(1 - 2xz + z^2)^{-\frac{1}{2}} = \sum_{n=0}^{\infty} P_n(x) z^n, where |z| < 1.

  • Differential Equation: (1x2)Pn(x)2xPn(x)+n(n+1)Pn(x)=0(1 - x^2) P_n''(x) - 2x P_n'(x) + n(n + 1) P_n(x) = 0.

Quantum Mechanical Observables and Operators

  • Classical vs. Quantum Measurement: In classical mechanics, measurement does not disturb the system. In quantum mechanics, measurement often disturbs the system, and accuracy is limited for conjugate variables.

  • Heisenberg Uncertainty Principle: Simultaneous measurement of conjugate variables (e.g., position/momentum, time/energy) is impossible. Error is defined by ΔxΔp2\Delta x \Delta p \ge \frac{\hbar}{2}.

  • Operators: A mathematical rule performed on a function ff that produces a function gg. Order of operations matters ([A^,B^]0[\hat{A}, \hat{B}] \neq 0).

    • Position Operator: x^=x\hat{x} = x

    • Momentum Operator: p^=iddx\hat{p} = -i\hbar \frac{d}{dx}, where =h2π\hbar = \frac{h}{2\pi}.

    • Energy/Hamiltonian Operator: H^=22m2+V\hat{H} = -\frac{\hbar^2}{2m} \nabla^2 + V.

    • Laplacian Operator: 2=2x2+2y2+2z2\nabla^2 = \frac{\partial^2}{\partial x^2} + \frac{\partial^2}{\partial y^2} + \frac{\partial^2}{\partial z^2}.

Spherical Harmonics

  • Context: Specific functions defined on the surface of a sphere, used for solving partial differential equations like the Schrodinger equation for a hydrogen atom.

  • Spherical Coordinates: (r,θ,ϕ)(r, \theta, \phi) where 0 \le r < \infty, 0θπ0 \le \theta \le \pi, and 0ϕ2π0 \le \phi \le 2\pi.

  • Wavefunction Decomposition: ψ(r,θ,ϕ)=R(r)Θ(θ)Φ(ϕ)=R(r)Ylm(θ,ϕ)\psi(r, \theta, \phi) = R(r) \Theta(\theta) \Phi(\phi) = R(r) Y_l^m(\theta, \phi).

  • Associated Legendre Polynomials: Plm(cos(θ))P_l^m(\text{cos}(\theta)) is used to define the angular part.

  • Angular Momentum: L=l(l+1)L = \sqrt{l(l + 1)} \hbar. The zz-component is Lz=mL_z = m\hbar.

  • Physical Significance: Spherical harmonics are the eigenfunction of the orbital angular momentum operator.

The Drude Model and Free Electron Gas

  • Characteristics of Metals: High electrical and thermal conductivity, obedience to Ohm's Law (J=σEJ = \sigma E), and positive coefficient of resistance.

  • Wiedemann-Franz Law: The ratio of thermal conductivity (KK) to electrical conductivity (σ\sigma) is proportional to temperature (TT). K/(σT)=LK/(\sigma T) = L (Lorentz number).

  • Drude Assumptions (1900):

    • Metals consist of positive ion cores and valence electrons moving freely.

    • Repulsion between electrons is neglected.

    • Potential energy is assumed constant (zero), so total energy = kinetic energy.

    • Electron behavior follows Maxwell-Boltzmann statistics (distinguishable particles).

    • Electrons collide with ion cores, losing velocity after short periods.

  • Electrical Conductivity Equation: σ=ne2τm\sigma = \frac{ne^2 \tau}{m}, where nn is charge density and τ\tau is relaxation time (mean time between collisions).

  • Thermal Conductivity: K=13CvvλK = \frac{1}{3} C_v v \lambda. Using classical gas theory, K=3nkB2Tτ2mK = \frac{3 n k_B^2 T \tau}{2m}.

  • Limitations of Classical Free Electron Theory:

    • Cannot explain why only some crystals are metallic.

    • Cannot explain specific structures (e.g., cubic shape of iron).

    • Observed heat capacity is only 1%1\% of the calculated value.

    • Fails to explain paramagnetic behavior and temperature dependence of conductivity correctly.

Quantum Free Electron Gas (Sommerfeld Model)

  • Approach: Problem treated quantum mechanically using Fermi-Dirac distribution and Pauli Exclusion Principle.

  • 1-D Fermi Gas: Particles of mass mm confined in a box of length LL with infinite potential barriers.

    • Energy Levels: En=22m(nπL)2E_n = \frac{\hbar^2}{2m} (\frac{n\pi}{L})^2.

    • Fermi Level: The highest energy level occupied at absolute zero temperature (0K0\,K).

  • 3-D Fermi Gas: Represented in KK-space (reciprocal space).

    • Fermi Wavevector (kFk_F): kF=(3π2n)13k_F = (3\pi^2 n)^{\frac{1}{3}}, where n=N/Vn = N/V.

    • Fermi Velocity (vFv_F): vF=kFmv_F = \frac{\hbar k_F}{m}.

    • Fermi Energy (EFE_F): EF=2kF22mE_F = \frac{\hbar^2 k_F^2}{2m}.

  • Density of States (DOS): The number of available energy states per unit energy range.

    • 3D Case: D(E)=V2π2(2m2)32E12D(E) = \frac{V}{2\pi^2} (\frac{2m}{\hbar^2})^{\frac{3}{2}} E^{\frac{1}{2}}.

    • Quantum Confinement impacts DOS:

    • 3D3D (Bulk): Continuous curve proportional to E\sqrt{E}.

    • 2D2D (Thin film/Quantum Well): Step-like function.

    • 1D1D (Nanowire/CNT): Discrete spikes.

    • 0D0D (Quantum Dot): Delta functions (discrete states).

  • Fermi-Dirac Distribution at Temperature: f(E)=1e(EEF)/kBT+1f(E) = \frac{1}{e^{(E - E_F)/k_B T} + 1}.

    • At T=0KT = 0\,K: f(E)=1f(E) = 1 for E < E_F and f(E)=0f(E) = 0 for E > E_F.

    • At finite TT: At E=EFE = E_F, f(E)=0.5f(E) = 0.5.