Nose-Hoover-chain thermostat

The standard Nosé-Hoover thermostat suffers from well-known issues, such as the ergodicity violation in the case of simple harmonic oscillator. As proposed by Martyna and Klein, these problems can be solved by using multiple Nose Hoover thermostats connected in a chain. Although the underlining dynamics is non-Hamiltonian, the corresponding equations of motion conserve the following energy term:

$\mathcal{H'} = \mathcal{H}(\bold{r},\bold{p}) + \sum\limits_{j=1}^{M} \frac{p_{\eta_j}^2}{2Q_j} + (3N-N_c)k_{B} T \eta_1 + k_{B} T \sum\limits_{j=2}^{M} \eta_j,$

where $\mathcal{H}(\bold{r},\bold{p})$ is the Hamiltonian of the physical system, $M$, $N$ and $N_c$ are the numbers of thermostats, atoms in the cell, and geometric constraints, respectively, and $\eta_{j}$, $p_{\eta_j}$, and $Q_{j}$ are the position, momentum, and mass-like parameter associated with the thermostat $j$. Just like the total energy in NVE ensemble,$\mathcal{H'}$ is valuable for diagnostics purposes. Indeed, a significant drift in $\mathcal{H'}$ indicates that the corresponding computational setting is suboptimal. Typical reasons for this behavior involve noisy forces (e.g., because of a poor SCF convergence) and/or a too large integration step (defined via POTIM).

The number of thermostats is controlled by the flag NHC_NCHAINS. Typically, this flag is set to a value between 1 and 5, the maximal allowed value is 20. In the special case of NHC_NCHAINS=0, the thermostat is switched off, leading to a MD in microcanonical ensemble. Another special case of NHC_NCHAINS=1 corresponds to the standard Nose-Hoover thermostat.

The only parameter of this thermostat is the characteristic time scale ($\tau$), defined via flag NHC_PERIOD. This parameter is used to setup the mass-like variables via the relations:

$Q_1 = 3 (N -N_c)k_{B} T \tau^2$

$Q_j = k_{B} T \tau^2; \; \; \; j=2,\dots,M$

In accurate calculations, the RESPA methodology can be used split the integration step used in thermostat variables propagation into NHC_NRESPA equal parts, each of which may be further divided into NHC_NS smaller parts treated by Suzuki-Yoshida scheme of fourth or sixth order.

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