The Quantum Dance of the Hydrogen 1s Electron
Imagine you are trying to locate a hyperactive firefly in a completely dark room. You can't predict its exact path, but if you take a million photographs and overlay them, a glowing cloud emerges. This is exactly how we visualize the electron in the quantum mechanical model of the hydrogen atom. The electron doesn't orbit the nucleus in neat, planetary circles; instead, it exists as a probability cloud defined by its wave function, ψ.
In this problem, we are tasked with identifying the incorrect statement regarding an electron in the 1s-orbital. To do this, we must dissect the subtle differences between probability density, radial probability, and the energy of quantum states.
Probability Density vs
Radial Probability
Let's address the concept of probability density, denoted by ∣ψ∣2 or R2(r). This value tells us the probability of finding the electron in a tiny, specific unit of volume at a distance r from the nucleus. For any s-orbital, the wave function is spherically symmetric and has no angular nodes. Mathematically, the function R(r) is an exponential decay curve that is at its absolute maximum right at the nucleus (r=0). Therefore, the probability density is indeed maximum at the nucleus.
However, space is three-dimensional. If we want to know the probability of finding the electron at a distance r, regardless of direction, we must consider the volume of a thin spherical shell at that distance. The volume of this shell is 4πr2dr.
When we multiply the probability density by the volume of the shell, we get the radial probability distribution function:
At the nucleus (r=0), the volume of the shell is zero, so P(0)=0. As we move away from the nucleus, the r2 term grows while the R2(r) term shrinks. The competition between these two terms creates a peak. For the 1s-orbital, this peak occurs exactly at r=a0, the Bohr radius. This means a0 is the most probable distance to find the electron.
Furthermore, the tail of this distribution curve extends to infinity. It never truly hits zero. This means there is a non-zero probability of finding the electron at 2a0, 3a0, or even a mile away (though infinitesimally small).
The Virial Theorem in Action
What about the energy of the electron? The Virial Theorem is a profound principle in mechanics that relates the average kinetic energy to the average potential energy for stable, bound systems. For a system bound by an inverse-square force (like the Coulombic electrostatic force between a proton and an electron), the theorem states:
Because kinetic energy is always positive, the potential energy is negative (indicating a bound state). If we take the magnitude, we see that ∣⟨PE⟩∣=2⟨KE⟩. The magnitude of the potential energy is exactly double the kinetic energy on average.
The Constancy of Total Energy
Finally, we arrive at the crux of the problem: the total energy of the electron. In quantum mechanics, an electron in a specific orbital (like the 1s-orbital) is in a stationary state. This means its total energy is a constant, quantized value. For the hydrogen atom, the energy of the n-th state is given by:
For the 1s state (n=1,Z=1), the total energy is strictly −13.6 eV. It does not fluctuate or reach a "maximum" as the electron moves closer to or further from the nucleus. The distance a0 is simply the location of maximum radial probability, not maximum energy.
Therefore, the statement claiming that the total energy is maximum at a0 is fundamentally flawed, making it the correct answer to our question.