With Heisenberg's uncertainty principle calculator, you will learn about one of the most fundamental quantum mechanics concepts. We say "fundamental" not to write "controversial" and "mind-blowing". Follow us in this short article to learn:

  • What is Heisenberg's uncertainty principle: formula and definition;
  • How do we calculate Heisenberg's uncertainty principle;
  • Why does the observer don't matter in the definition of Heisenberg's uncertainty principle; and
  • How to use Heisenberg's uncertainty principle: examples of real-world situations.

Quantum mechanics primer

The quantum nature of objects is (most of the time) hidden from our eyes. We have to zoom in to discover it and its effect. Past the structure of our material, past the molecular scale, and finally, at an atomic scale. Here, the laws of classical physics are merely a suggestion: you can cross walls, pop into existence from a vacuum, and so on.

One of the fundamental reasons for the quantum world to be so distant from our usual understanding is that everything has a double nature on a quantum scale: subatomic particles behave both as particles and as waves. This peculiarity is progressively less relevant for objects of increasing size, nevertheless still existing. We can define a wavelength for every object: our De Broglie wavelength calculator explains how!

What is Heisenberg's uncertainty principle: definition and explanation?

Heisenberg's uncertainty principle is a fundamental consequence of the probabilistic nature of quantum objects. We hook on the De Broglie equation to explain it. The equation that assigns a wavelength to every object with particle-wave dualism is:

p=hλp = \frac{h}{\lambda}

where:

  • pp — The momentum measured in kgm/s\mathrm{kg\cdot m/s};
  • hh — The Planck's constant, a physical constant at the base of quantum phenomena (h=6.62607015×1034 J/Hzh = 6.62607015×10−34\ \mathrm{J/Hz}); and
  • λ\lambda — The De Broglie wavelength.
position uncertainty on a rope
This wave has a high uncertainty on the momenum. On the other hand, its wavelength is easily measurable.

This relation connects the momentum and the wavelength of the object in analysis. Now think of a practical example. Tie a rope to a wall, pull on the other end, and shake it. First, do it slowly: you will create a nice wave. This wave has a very well-defined wavelength (or momentum, if you look at it through the De Broglie equation) but an ill-defined position. Where is the wave? On the rope, but where? Now give it a jerk: the small dent is not even a wave as we understand it, and defining its wavelength (momentum!) is not easy. On the other side, apart from a small spread, its position is easily measurable.

Now, imagine an object that can be both things at the same time: that's a quantum particle. The lack of precision on the momentum lives along with the lack of precision on the position along the rope.

Momentum uncertainty
You can find the position of this "wave" with little uncertainty. However, what's its wavelength? Hard to say!

🙋 Quantum, quantum, quantum: at Omni, we love the topic: that's why we spent so much time creating tools for you: try our quantum number calculator, our photon energy calculator, or explore the phenomenon that finally made quantum mechanics impossible to deny with our photoelectric effect calculator!

Calculate Heinsenberg's uncertainty principle: formula for the statistical uncertainity

The mathematics behind Heisenberg's uncertainty principle formula is not the easiest one. We will first give you the equation: the explanation comes later! You will see Heisenberg's uncertainty principle equation in two forms in your physics studies. Let's see the first one:

ΔxΔphΔx\cdot Δp \geq h

where ΔxΔx and ΔpΔp are uncertainties. The modern formulation (and what we regularly use to calculate Heisenberg's uncertainty principle) uses the reduced Planck's constant =h/2π\hbar = h/2\pi and substitutes the uncertainties of the variables with their standard deviations:

σxσp2\sigma_x\cdot \sigma_p \geq \frac{\hbar}{2}

When calculating Heisenberg's uncertainty principle, we use this inequality's lowest bound. The equality between the two sides represents the highest possible quality of information on the two variables: the nature of our particle would prevent us from arbitrarily reducing the uncertainty of the variables: once their product reaches that bound, one of the two begins rising.

Intuitively, you can think of the behavior of the particle as follows:

  • If undisturbed, your quantum particle would look like a blurry dot moving in an unspecified direction;
  • If you try to fix its velocity, you will find out that the blurred spot increased in size: the uncertainty in position got worse!
  • Try to pinpoint the particle in space. Now its position is well-defined, but the particle is trying to escape in all directions at the same time! The momentum is not defined as well as before.
  • What if you try to decrease both at the same tim... you can't!

How to use the Heisenberg's uncertainty principle calculator

To use our Heisenberg's uncertainty principle calculator, you have to know the values of the uncertainty of one of three possible quantities:

  • The momentum;
  • The position; or
  • The velocity.

If you are using the velocity, you will also have to define the mass of the object: we will use these two quantities to calculate the momentum uncertainty

Once you input the variables necessary to compute the equality, we will output the result of the lowest possible uncertainty on the other variable(s):

ΔxΔp=2Δx \cdot Δp = \frac{\hbar}{2}

A short note: \hbar, being a constant of the quantum world, has a very small value: =1.05457182×1034 m2kg/s\hbar =1.05457182 \times10^{-34}\ \mathrm{m^2 kg / s}. Be careful when inserting large values of uncertainties (large from a microscopic point of view): the other quantities will easily go to 00 as a consequence. This calculator is best suited to operate for particles and atoms than for cars and squirrels!

What about the observer?

The definition of Heisenberg's uncertainty principle equation was, for a long time, associated with the presence of an observer. Usually, we are taught that if an observer zeroes in the position, the momentum of the particle skyrockets, and vice-versa. Well, that's not precisely true. It's not the observer that causes this phenomenon: the way we define Heisenberg's uncertainty principle rules out the observer altogether. The origin of the uncertainty relation stems from the probabilistic wave-like nature of quantum objects.

What depends on the measurement is the observer effect, which causes a quantum wavefunction to collapse in a single state.

An example of Heisenberg's uncertainty principle in action

Take an electron traveling at 2020% the speed of light with an uncertainty of Δv=0.12Δv = 0.12% of cc. We know the mass of an electron me=9.109×1031 kgm_\mathrm{e}= 9.109\times10^{-31}\ \mathrm{kg}. The uncertainty on the momentum then becomes:

Δp=Δvm=0.12%cme=0.0012299, ⁣792, ⁣458 m/s9.109×1031 kg=327.7×1027 kgm/s\begin{split} Δp &= Δv\cdot m \\ &= 0.12\%c \cdot m_{\mathrm{e}} \\ &= 0.0012\cdot 299,\!792,\!458\ \mathrm{m/s}\\ &\cdot 9.109\times10^{-31}\ \mathrm{kg} \\ &= 327.7\times10^{-27}\ \mathrm{kg\cdot m/s} \end{split}

Let's apply Heisenberg's uncertainty principle formula to find the uncertainty on the position of our electron. As said in the previous sections, we will use the limit case of the equality:

ΔpΔx=2Δp\cdot Δx = \frac{\hbar}{2}

Invert this equation and substitute the values we found before:

Δx=2Δp ⁣ ⁣ ⁣ ⁣=1.055×1034 m2kg/s2327.7×1027 kgm/s ⁣ ⁣ ⁣ ⁣=0.1609 nm\begin{split} Δx &= \frac{\hbar}{2\cdot Δp}\\ & \!\!\!\!= \frac{1.055\times10^{-34}\ \mathrm{m^2\cdot kg / s}}{2\cdot327.7\times10^{-27}\ \mathrm{kg\cdot m/s}}\\ &\!\!\!\!=0.1609\ \mathrm{nm} \end{split}

This value is around one hundred thousand times bigger than the electron radius used in most calculations (notice that the electron, most likely, has no size at all: we assign one when we need to consider its interactions).

🙋 Visit our electron speed calculator for a better understanding of how these elementary particles move!

Davide Borchia
Position uncertainty (σₓ)
nm
Momentum uncertainty (σₚ)
x10⁻²⁷
kg⋅m/s
Object mass
u
Velocity uncertainty (σᵥ)
m/s
People also viewed…

De Broglie wavelength

On a human scale, matter is as solid as something can be. However, from a quantum perspective, objects show a double nature: find out why with our de Broglie wavelength calculator.

Schwarzschild radius

Discover the fundamental of black hole physics with our Schwarzschild radius calculator.

Wavelength to energy

Effortlessly find the energy of a photon from its wavelength with this wavelength to energy calculator.
main background