Two particles are said to be identical if all their characteristic properties (like quantum numbers) are the same. Identical particles are distinguishable in classical mechanics, and indistinguishable in quantum mechanics.
Fermions and bosons#
In classical mechanics, two particles may be identical, but can always be distinguished. For instance, consider two pool balls tagged as 1 and 2. They strike each other and scatter, bouncing off. Let's call the balls after the scattering 3 and 4. Of course, these are still the same balls, with and . If 1 and 2 are differently colored, it's trivial to tell which is which after the scattering. If they are colored the same, it's harder to tell but still possible, as we can follow their trajectories instant-by-instant to see where each one goes.
Not so in quantum physics. Say the pool balls are now quantum objects. After the scattering they end up in some joint state . Classically, the states and would be different, as switching positions leads to different configurations and so different end states. But due to the indeterminacy principle, we can't follow trajectories in quantum physics (hell, quantum trajectories just don't exist), so our previous method of tracking movement to distinguish what happens fails. Thus, we have no proof that and are any different. What we can do is say that the two states are proportional to each other (they still arise from the same source, after all). In symbols, this means , where . The end state is some linear combination of the two
We have and , so . This implies or . So, there are only two possible states
This shows that there is a parity phenomenon going on. Sometimes, inverting the position causes the state to flip sign, other times nothing happens. This suggests the presence of two types of particles, one which undergoes parity flipping, and another which does not. These two types of particles are respectively called fermions and bosons. Fermions flip signs and make for odd wavefunctions (or better, antisymmetric), bosons do not and make for even wavefunctions (or better, symmetric). All quantum particles abide to one constraint or the other.
This has the remarkable outcome that fermions just can't simultaneously occupy the same state as another fermion in the system, whereas bosons can. In fact, if , the fermion mixed state would be
Meaning, there is no such state. The two fermions must end up in different states and . It doesn't matter where each fermion goes, they just need to go different ways. This odd property is called the Pauli exclusion principle. Meanwhile for bosons, we get
so not only does the state exists, it is simply a rescaling of the original. As such, it is perfectly fine for two bosons to end up in the same state.
> Of course, switching particles gets us back to the original wavefunction, so $P$ is [[Operatore unitario|unitary]] ($PP=P^{2}=1$). As with all unitary operators, applying them to a state won't change the [[Equazione agli autovalori|eigenvalues]]: > $$H\psi=E\psi \quad\to \quad H(P\psi)=E(P\psi)> Again, we see that switching two particles can only have two effects. Either it flips the sign of the state, or it doesn't. ### Correct Boltzmann counting The indistinguishability of particles affects the number of unique states that are possible in a quantum system. Since particles positions can't be determined precisely, states where the only difference is how the particles are ordered all combine into a single mixed state made up of a superposition of all of these pure states. For instance, if you have two particles at positions $a$ and $b$ and you measure them, their mixed state would beIf the eigenvalue is not degenerate, and must describe the same state and thus be proportional to each other: , where . But this is just the eigenvalue equation for , and since is unitary, must be . As such, we get
\ket{\psi} =\ket{ab} \pm \ket{ba}
(with some omitted [[Normalization|normalization]] constant). This is because it is not possible to distinguish between $\ket{ab}$ and $\ket{ba}$. The sign of $\pm$ is determined by whether we are working with fermions ($-$) or bosons ($+$). Thus, when passing from classical to quantum physics, the number of states is reduced from two to one. This can be extend to a system of $N$ particles, in which the number of identical configurations (i.e. coordinate [[permutazione|permutations]]) becomes $N!$ and so the number of distinguishable states is reduced to $1/N!$ of the classical version. This is the origin of the so called **correct Boltzmann counting**, which was needed in classical [[Ensemble|ensembles]] to solve the [[Gibbs paradox]]. The reason it is necessary even in classical statistical mechanics is because even classical ensembles deal with quantum objects such as [[Atom|atoms]] and [[molecule|molecules]] as basic elements.