Stamp density

The matrix density , or operator density is a mathematical entity introduced by the mathematician and physicist John von Neumann. It makes it possible to summarize in only one matrix all the possible unit of the quantum states of a physical system given to a given moment, thus marrying quantum Mécanique and Physique statistics.

Definition

Pure case

The description of the system is done here thanks to a vector of state | \ psi (T) \ rangle which one can develop on the bases \ { | u_n \rangle \} :

\ left| \ psi (T) \ right \ rangle = \ sum_n {c_n (T) \ cdot \ left| u_n \right\rangle}
with \ sum_n | c_n (T) |^2 = 1 \,

The operator density is defined for a pure state by:

\ hat \ rho = |\ psi (T) \ rangle \ langle \ psi (T) | = \ sum_ {N, p} c_n^* (T) c_p (T) | p \ rangle \ langle N |

Mix statistical pure states

By admitting that a certain physical system can be, at a certain moment T, in a statistical mixture (finished or infinite) of quantum states | \ psi_i \ rangle with probabilities p_i (where \ sum_i p_i = 1 \, ), then the matrix density representing the unit of these states is:

\ hat \ rho = \ sum_i p_i |\psi_i \rangle \langle \psi_i |

The statistical aspect introduces here is of two nature, one traditional and the other quantum one:

1. traditional : had with the estimate of the ket by a statistical distribution of different the kets possible,
2. quantum : quantum uncertainty fundamental even if the system is perfectly given.

The elements of the matrix density are worth:

\ hat \ rho_ {pn} = \ sum_i p_i \ langle u_p^ {(I)} | \hat \rho_i | u_n^ {(I)} \ rangle = \ sum_i p_i c_n^ {(I) *} c_p^ {(I)}

Property

The matrix obtained has the following properties:

  • It is square, \ hat \ rho = \ hat \ rho^ {\ dagger} , it can thus be diagonalized, and its eigenvalues are positive.
  • Its trace is equal to 1, Tr (\ hat A) =1, conservation of the total probability.
  • It must be definite positive or null.
  • In the case of a pure state, the operator density is then a Projecteur: \ hat \ rho^2 = \ hat \ rho .
  • Tr (\ rho^2) \ the 1, with equality if and only if the physical system is in a pure state (i.e. all the p_i are null except one).

Median value

One can calculate the median value of a Observable has starting from the formula:

\ langle \ hat has \ rangle = \ langle \ Psi |\ hat has | \ Psi \ rangle = Tr (\ hat has \ hat \ rho) = Tr (\ hat \ rho \ hat A)
with \ hat \ rho = \ sum_i^N p_i \ hat \ rho_i is the matrix density of a statistical mixture of states.

Evolution with time

See also: Operator of evolution

The temporal evolution of the operator of state is given by the equation of Schrödinger dependant on time:

\ hat H \ left| \ Psi (T) \ right \ rangle = I \ hbar {D \ over dt} \ left| \ Psi (T) \ right \ rangle

Bond with the entropy

Lastly, one can define the Entropie Von Neumann:

S=-k_B Tr (\ hat \ rho \ ln (\ hat \ rho))
where k_B is the Boltzmann constant.

The entropy of a pure state is null, because there is no uncertainty on the state of the system. One can also find a base where the matrix is diagonal, with 0, and one 1 on the diagonal, which gives an entropy well equal to 0.

See too

References

Category: Quantum physics

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