schrodinger-equation
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| schrodinger-equation [May 23, 2026 at 00:03] – created Ivan Janevski | schrodinger-equation [June 13, 2026 at 03:13] (current) – external edit 127.0.0.1 | ||
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| # Schrödinger equation | # Schrödinger equation | ||
| - | In quantum mechanics, | + | The **Schrödinger equation** is the equation of motion for a quantum |
| - | $$ i\hbar \frac{\partial}{\partial | + | $$i\hbar\frac{\mathrm{d}}{\mathrm{d}t}\lvert\psi\rangle = H\lvert\psi\rangle$$ |
| - | Meaning of symbols are: | + | ## Derivation from unitary evolution |
| - | * $i$ - Imaginary unit (A solution to the equation $i^2 + 1 = 0$) | + | |
| - | * $\hbar$ - Reduced planck constant ($\hbar = h/2\pi$, with value $\hbar \approx 1.054 571 817\times 10^{-34}J\cdot s$) | + | |
| - | * $\partial / \partial t$ - Derivative with respect to time | + | |
| - | * $\nabla^2$ - Sum of second derivatives with respect to space ($\nabla^2 = \partial^2 / \partial x^2 + \partial^2 / \partial y^2 + \partial^2 / \partial z^2$) | + | |
| - | * $\Psi$ - Particle wave function | + | |
| - | * $m$ - Mass of the particle | + | |
| - | * $V$ - Potential energy of the particle | + | |
| - | Because | + | The central requirement on quantum |
| - | Note that Schrödinger equation is single-order with respect to time, but second-order with respect to space. This is unlike the classical wave equation describing | + | $$\lvert\psi(t+dt)\rangle = U(t+dt,\, |
| - | ## Derivation | + | For infinitesimal |
| - | We start from the well-known equation of energy conservation: | + | |
| - | $$ E = E_K + V$$ | + | |
| - | Where $E$ is the total energy of a particle, $E_K$ is its kinetic energy and $V$ is its potential energy. **Kinetic energy** of a particle is defined as $E_K = mv^2 / 2$ while **momentum** of a particle is defined as $p = mv$. Solving the latter for $v$ and substituting it in $E_K$, then substituting $E_K$ into the equation for total energy $E$, we get the following equation: | + | |
| - | $$E = \frac{p^2}{2m} | + | |
| - | We promote energy $E$ into an operator $\hat{E} = i\hbar \partial / \partial | + | |
| - | $$\hat{E}\Psi | + | |
| - | $$\boxed{i\hbar \frac{\partial\Psi}{\partial t} = \left(-\frac{\hbar^2}{2m}\nabla^2 + V\right)\Psi}$$ | + | |
| - | Thus, we directly derived | + | |
| - | ## Limitations (relativity) | + | $$\left(I + \tfrac{i}{\hbar}H^\dagger\,dt\right)\!\left(I - \tfrac{i}{\hbar}H\,dt\right) = I + \tfrac{i}{\hbar}(H^\dagger - H)\,dt + O(dt^2) |
| - | We derived the Schrödinger from nonrelativistic energy-momentum relation | + | |
| - | $$E^2 = p^2c^2 | + | |
| - | Promoting $E$ and $p$ to operators $\hat{E} = i\hbar \partial / \partial t$ and $\hat{p} = -i\hbar\nabla^2$ yields the Klein-Gordon equation | + | |
| - | $$\left(\frac{\partial^2\Psi}{\partial t^2} - c^2\nabla^2 | + | |
| - | The issue with this equation is that, unlike Schrödinger, | + | |
| - | It was Paul Dirac who correctly found a relativistic analogue of Schrödinger equation by postulating the existence of $\alpha, \beta, \gamma, \delta$ such that: | + | which requires |
| - | $$E = \sqrt{p^2c^2 + m^2c^4} = \alpha p_x c + \beta p_y c + \gamma p_z c + \delta mc^2$$ | + | |
| - | As it turns out, $\alpha, \beta, \gamma, \delta$ cannot be ordinary complex numbers - they must be 4x4 complex matrices. Thus, wavefunction $\Psi$ in Dirac' | + | |
| - | Still, Dirac' | + | ## Time evolution operator |
| + | |||
| + | For a time-independent Hamiltonian, the Schrödinger | ||
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| + | $$\lvert\psi(t)\rangle = U(t)\, | ||
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| + | The matrix exponential is defined by its power series $e^A = \sum_{k=0}^\infty A^k / k!$. Because $H$ is Hermitian, $-iHt/ | ||
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| + | ## Lie group and Lie algebra | ||
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| + | The family of operators $\{U(t) : t \in \RR\}$ forms a one-parameter subgroup of the Lie group $\mathrm{U}(N)$ of $N\times N$ unitary matrices. The Hamiltonian $-iH$ (or $-iH/\hbar$ in SI units) belongs to the corresponding Lie algebra $\mathfrak{u}(N)$ of skew-Hermitian matrices. The exponential map $\exp : \mathfrak{u}(N) \to \mathrm{U}(N)$ is exactly the matrix exponential above — it converts | ||
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| + | This correspondence means that specifying a Hermitian | ||
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| + | ## Quantum gates | ||
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| + | When the Hamiltonian satisfies $H^2 = I$ — which holds for all Pauli matrices $X$, $Y$, $Z$ — the power series collapses to a two-term identity via Euler' | ||
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| + | $$e^{-i\theta H} = \cos\theta\, | ||
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| + | The single-qubit rotation gates are defined exactly this way: | ||
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| + | $$R_x(\theta) = e^{-i\theta X/2}, \quad R_y(\theta) = e^{-i\theta Y/2}, \quad R_z(\theta) = e^{-i\theta Z/2}$$ | ||
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| + | The factor of $1/2$ means a full rotation of the Bloch sphere requires $\theta = 2\pi$ rather than $\pi$, which is why a $180°$ physical rotation maps to a $\pi$ gate argument. The [[h-gate|Hadamard gate]] can be written as $H = e^{i\pi(X+Z)/ | ||
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| + | ## List of code implementations | ||
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| + | - [[schrodinger-equation-qutip|Schrödinger equation (QuTiP)]] | ||
| - | This is called the second quantization, | ||
schrodinger-equation.1779494585.txt.gz · Last modified: by Ivan Janevski
