As outlined previously there is a considerable interest in methods to sample the canonical distribution with MD simulations and various techniques have been invented.
In the case of the canonical (,,) ensemble the instantaneous kinetic
energy is the conserved quantity in place of the total energy in the case
of the microcanonical (,,) ensemble.
The most simple method to realize this situation in a simulation is
by scaling the velocities. But one cannot expect to sample thereby
the canonical ensemble. The same
is true for two other techniques, the first one [2] employs
random forces, the second one [3] is a more subtle way to
scale the velocities.
The scaling factor of the Berendsen thermostat is given by
[1]
Nosé was the first to come up with a proper modification of the equations
of motion so that they reproduce the canonical ensemble [13].
He introduces another degree of freedom which acts
as a scaling factor for the velocities (or the time step, equivalently).
Due to the parameter additional terms associated with its potential and
kinetic energy appear in the Lagrangian and Hamiltonian, respectively. The
conserved quantities in this system are the Hamiltonian, the total momentum
and the total angular momentum. The equations of motion as derived from the
Hamiltonian
Nosé's equations were reformulated [11] avoiding the scaling of
the time step by introducing a new timestep containing . Furthermore
Hoover defined a friction coefficient
.
The equations of motion become
Posch showed the effectiveness of the Nosé thermostat in sampling phase space for the classical one-dimensional harmonic oscillator [16]. Plotting versus for the microcanonical ensemble a perfect circle is obtained. Andersenīs method generates a number of points scattered over a circle. The Nosé-Hoover thermostat gives a broadened circle as expected if one allows fluctuations in the total energy (noting that the phase space volume corresponds to energy).