Normalizing Functions: Basics & Examples

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How does you normalize a function? Could someone explain it very basically and give an example.
 
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In Quantum Mechanics, when we talk about normalizing a function, we mean that we want its integral over all space to be equal to 1. So a function is normalized if \int^\infty_{-\infty}f(x)\:dx = 1

If a function is not normalized, then we can normalize it by dividing the function by whatever its total integral is. So if we define A = \int^\infty_{-\infty}f(x)\:dx, and we define a new function f'(x) = \frac{f(x)}{A}, then by definition, \int^\infty_{-\infty}f'(x)\:dx = 1, so f'(x) is normalized.
 
Thank you! :D
 
You're welcome, glad to help!

Also, I should point out that what I gave above was a very generic definition of normalization. In the specific case of quantum mechanics, what we're usually normalizing is the probability density, which is the magnitude squared of the wavefunction. So in practice, the way that you will usually see normalization conditions written is \int^\infty_{-\infty}|\Psi(x)|^2\:dx = 1.
 
Insights auto threads is broken atm, so I'm manually creating these for new Insight articles. Towards the end of the first lecture for the Qiskit Global Summer School 2025, Foundations of Quantum Mechanics, Olivia Lanes (Global Lead, Content and Education IBM) stated... Source: https://www.physicsforums.com/insights/quantum-entanglement-is-a-kinematic-fact-not-a-dynamical-effect/ by @RUTA

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