# ⓘ Energy operator. In quantum mechanics, energy is defined in terms of the energy operator, acting on the wave function of the system as a consequence of time tra ..

## ⓘ Energy operator

In quantum mechanics, energy is defined in terms of the energy operator, acting on the wave function of the system as a consequence of time translation symmetry.

## 1. Definition

It is given by:

E ^ = i ℏ ∂ ∂ t {\displaystyle {\hat {E}}=i\hbar {\frac {\partial }{\partial t}}\,\!}

It acts on the wave function the probability amplitude for different configurations of the system

Ψ r, t {\displaystyle \Psi \left\mathbf {r},t\right\,\!}

## 2. Application

The energy operator corresponds to the full energy of a system. The Schrodinger equation describes the space- and time-dependence of the slow changing non-relativistic wave function of a quantum system. The solution of this equation for a bound system is discrete a set of permitted states, each characterized by an energy level which results in the concept of quanta.

### 2.1. Application Schrodinger equation

Using the energy operator to the Schrodinger equation:

i ℏ ∂ ∂ t Ψ r, t = H ^ Ψ r, t {\displaystyle i\hbar {\frac {\partial }{\partial t}}\Psi \mathbf {r},\,t={\hat {H}}\Psi \mathbf {r},t\,\!}

can be obtained:

E ^ Ψ r, t = H ^ Ψ r, t {\displaystyle {\begin{aligned}&{\hat {E}}\Psi \mathbf {r},\,t={\hat {H}}\Psi \mathbf {r},\,t\\\end{aligned}}\,\!}

where i is the imaginary unit, ħ is the reduced Planck constant, and H ^ {\displaystyle {\hat {H}}} is the Hamiltonian operator.

In a stationary state additionally occurs the time-independent Schrodinger equation:

E Ψ r, t = H ^ Ψ r, t {\displaystyle {\begin{aligned}&E\Psi \mathbf {r},\,t={\hat {H}}\Psi \mathbf {r},\,t\\\end{aligned}}\,\!}

where E is an eigenvalue of energy.

### 2.2. Application Klein–Gordon equation

The relativistic mass-energy relation:

E 2 = p c 2 + m c 2 {\displaystyle E^{2}=pc^{2}+mc^{2}^{2}\,\!}

where again E = total energy, p = total 3-momentum of the particle, m = invariant mass, and c = speed of light, can similarly yield the Klein–Gordon equation:

E ^ 2 = c 2 p ^ 2 + m c 2 E ^ 2 Ψ = c 2 p ^ 2 Ψ + m c 2 Ψ {\displaystyle {\begin{aligned}&{\hat {E}}^{2}=c^{2}{\hat {p}}^{2}+mc^{2}^{2}\\&{\hat {E}}^{2}\Psi =c^{2}{\hat {p}}^{2}\Psi +mc^{2}^{2}\Psi \\\end{aligned}}\,\!}

that is:

∂ 2 Ψ ∂ t 2 = c 2 ∇ 2 Ψ − m c 2 ℏ 2 Ψ {\displaystyle {\frac {\partial ^{2}\Psi }{\partial t^{2}}}=c^{2}\nabla ^{2}\Psi -\left{\frac {mc^{2}}{\hbar }}\right^{2}\Psi \,\!}

## 3. Derivation

The energy operator is easily derived from using the free particle wave function plane wave solution to Schrodingers equation. Starting in one dimension the wave function is

Ψ = e i k x − ω t {\displaystyle \Psi =e^{ikx-\omega t}\,\!}

The time derivative of Ψ is

∂ Ψ ∂ t = − i ω e i k x − ω t = − i ω Ψ {\displaystyle {\frac {\partial \Psi }{\partial t}}=-i\omega e^{ikx-\omega t}=-i\omega \Psi \,\!}.

By the De Broglie relation:

E = ℏ ω {\displaystyle E=\hbar \omega \,\!},

we have

∂ Ψ ∂ t = − i E ℏ Ψ {\displaystyle {\frac {\partial \Psi }{\partial t}}=-i{\frac {E}{\hbar }}\Psi \,\!}.

E Ψ = i ℏ ∂ Ψ ∂ t {\displaystyle E\Psi =i\hbar {\frac {\partial \Psi }{\partial t}}\,\!},

where the energy factor E is a scalar value, the energy the particle has and the value that is measured. The partial derivative is a linear operator so this expression is the operator for energy:

E ^ = i ℏ ∂ ∂ t {\displaystyle {\hat {E}}=i\hbar {\frac {\partial }{\partial t}}\,\!}.

It can be concluded that the scalar E is the eigenvalue of the operator, while E ^ {\displaystyle {\hat {E}}\,\!} is the operator. Summarizing these results:

E ^ Ψ = i ℏ ∂ ∂ t Ψ = E Ψ {\displaystyle {\hat {E}}\Psi =i\hbar {\frac {\partial }{\partial t}}\Psi =E\Psi \,\!}

For a 3-d plane wave

Ψ = e i k ⋅ r − ω t {\displaystyle \Psi =e^{i\mathbf {k} \cdot \mathbf {r} -\omega t}\,\!}

the derivation is exactly identical, as no change is made to the term including time and therefore the time derivative. Since the operator is linear, they are valid for any linear combination of plane waves, and so they can act on any wave function without affecting the properties of the wave function or operators. Hence this must be true for any wave function. It turns out to work even in relativistic quantum mechanics, such as the Klein–Gordon equation above.

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