Derivation of Probability Current Density and Equation of Continuity

Derivation of Probability Current Density In Quantum Mechanics, the motion of a material particle is associated with a wave function. If the probability of finding a particle in a bounded region decreases with time, the probability of finding it outside must increase by the same amount. This is described by the Probability Current Density . 1. The Schrödinger Basis We start with the Time-Dependent Schrödinger Equation (TDSE): iℏ (∂Ψ/∂t) = -(ℏ²/2m)∇²Ψ + VΨ --- (i) Taking the Complex Conjugate of equation (i): -iℏ (∂Ψ*/∂t) = -(ℏ²/2m)∇²Ψ* + VΨ* --- (ii) 2. Mathematical Manipulation To find the rate of change, we perform the following: Multiply eq (i) by Ψ* from the left. Multiply eq (ii) by Ψ from the left. Subtract the resulting equations. Using the UV derivation method for ∇·(Ψ*∇Ψ - Ψ∇Ψ*), we simplify the expression to relate it to the Equation of Continuity . 3. The Equation of Continuity In hydrodynamics, t...

Derivation of Time Dependent and Time Independent Schrodinger Wave Equation (Step-by-Step)

Mastering the Schrödinger Equation: Time-Dependent & Independent Forms

In quantum mechanics, the Schrödinger Equation is the cornerstone that describes the behavior of subatomic particles. Unlike classical physics, it uses wave functions to determine the probability of a particle's state. In this guide, Admin Focus breaks down the complete derivations for both forms as studied in BSc Physics.

1. Derivation of the Time-Dependent Schrödinger Equation (TDSE)

We begin with the principle of conservation of energy, where Total Energy (E) is the sum of Kinetic Energy (K.E.) and Potential Energy (P.E.):

E = (p² / 2m) + V

To transition to a wave representation, we apply this to the wave function Ψ:

EΨ = (p² / 2m)Ψ + VΨ --- (Eq. 1)

Operator Substitution

In quantum mechanics, we replace physical quantities with operators. Based on the fundamental postulates:

  • Energy Operator (E): -(ℏ/i) (∂/∂t)
  • Momentum Operator (p): -(ℏ/i) (∂/∂x)

Squaring the momentum operator gives us p² = -ℏ² (∂² / ∂x²). Substituting these into Eq. 1, we arrive at the final Time-Dependent form:

-(ℏ/i) (∂Ψ / ∂t) = - (ℏ² / 2m) (∂²Ψ / ∂x²) + VΨ


2. Derivation of the Time-Independent Schrödinger Equation (TISE)

The Time-Independent form is used when the potential V is constant over time. We start by using the Method of Separation of Variables for the wave function:

Ψ = A e i/ℏ (Et - px)

Mathematical Steps

We let the spatial part be ψ₀ = A e ipx/ℏ . This allows us to express the total wave function as:

Ψ = ψ₀ e -iEt/ℏ

By differentiating this equation with respect to t and x (twice), we find the respective derivatives for the TDSE. After substituting these values back into the Time-Dependent equation, the time-dependent exponential terms cancel out, leaving us with the spatial equation:

E ψ₀ = - (ℏ² / 2m) (∂²ψ₀ / ∂x²) + V ψ₀

(∂²ψ₀ / ∂x²) + (2m / ℏ²) (E - V) ψ₀ = 0

Conclusion & Significance

These equations allow us to solve for allowed energy levels in various systems, such as the Quantum Harmonic Oscillator or the Hydrogen Atom. Understanding the transition between the time-dependent and independent forms is essential for any BSc Physics student.

— Admin Focus

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Derivation of Probability Current Density and Equation of Continuity