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A disconnectivity graph summarizes how local minima of an energy landscape become connected as the allowed maximum energy increases. Each terminal branch represents a basin around a local minimum. Two branches merge at the lowest threshold for which a permitted path joins their basins without exceeding that threshold. Vertical height therefore carries barrier information; horizontal spacing is usually chosen for readability.

For example, two low-energy states may sit at similar energies but merge only high in the graph, indicating a difficult transition between them. A cluster of branches merging low down instead suggests easy rearrangement within that group. The graph is useful for separating energetic preference from kinetic accessibility in thermal activation. It does not determine transition rates by itself: the allowed dynamics, path widths and kinetic prefactors remain necessary. Changing the permitted moves changes which paths exist and can therefore change the graph.

A single-domain precipitate has no internal domain wall available to move. Magnetization changes therefore require rotation, curling or reversal of a particle's magnetization, rather than ordinary wall displacement through that particle. Relative to a larger multidomain material this can increase coercivity, but the actual coercivity depends on anisotropy, shape and particle interactions. If thermal activation over the anisotropy barrier is rapid on the observation timescale, superparamagnetic behavior can instead suppress remanence. Ferromagnetic composition plus small size alone does not prove a permanent hard magnet.

For an elementary wall-energy comparison, imagine one planar wall through a sphere of radius $r$. Its area is $A_w=\pi r^2$. If that trial two-domain state removes essentially all of the specified stray-field energy while adding wall energy ${\gamma }_w{A}_w$, stability of the uniform state requiresWith $r\simeq 0.33\mu \mathrm{m}$ and the supplied $U_{\mathrm{stray}}=5\times 10^{-18}\mathrm{J}$,This is the requested scale under a full stray-energy-release and one-planar-wall approximation; it is a lower-bound estimate within that model.

A more exact comparison uses the actual energy reduction $\Delta U_{\mathrm{stray}}$ of the competing domain pattern, not necessarily the whole original stray energy:No domain geometry, anisotropy energy or barrier is supplied to determine $\zeta$ or establish that the observed state is the thermodynamic ground state rather than kinetically trapped. Thus the given information alone does not establish an unconditional positive numerical lower bound independent of the competing pattern; the elementary estimate must retain its stated assumptions.

Quantum escape of a current-biased Josephson junction is decay of a trapped collective quantum phase state through a barrier in the tilted Josephson washboard potential. This barrier lies in the potential energy of an electrical circuit coordinate. Transfer of Cooper pairs across the physical insulating layer already supplies the Josephson coupling energy; it does not by itself demonstrate this further collective escape. Single-electron superconducting tunneling is a third, distinct process.

At higher temperature $T$, thermal activation instead lifts the coordinate over the barrier. In the rare-escape regime its characteristic form is the Kramers escape ratewhere $k_B$ is the Boltzmann constant and the prefactor depends on damping and thermal equilibration. Cooling suppresses this route. For a quasistationary energy level at energy $E$, the leading conservative WKB approximation instead haswith the two turning points bracketing the forbidden barrier. This is an exponential estimate requiring a large action compared with $\hslash$, slow escape compared with intrawell motion, and weak environmental corrections. It is not a complete rate prediction near the barrier top or with substantial damping.

The familiar cubic-barrier exponent can be checked independently. Choose $V(x)=M_{\varphi }{\omega }_p^2{x}^2(1-x/a)/2$, with $a>0$. Its top is at $2a/3$ and $\Delta U=2M_{\varphi }{\omega }_p^2{a}^2/27$. At the well-bottom reference energy $E=0$,Substitution $u=x/a$ reduces the dimensionless integral to ${\int }_0^{1}u\sqrt{1-u}du=4/15$. This leading semiclassical action uses a cubic potential and a well-bottom reference; actual ground-state escape also needs the zero-point correction, prefactor and environment. In the chosen washboard example it gives $B\simeq 74.0$ after matching the exact barrier and curvature. This matching is an illustrative approximation, not an exact action integral for the cosine potential.

Escape need not yield a sustained voltage: the coordinate can become trapped again. The running-state readout assumes sufficient underdamping and bias to avoid such retrapping. The parallel model has quality factor $Q={\omega }_{p}RC$; large $Q$ makes energy loss per oscillation small. Low-temperature rate saturation alone cannot distinguish quantum tunnelling from unwanted heating or external noise.

A ferromagnetic particle with no internal domain wall. Magnetization reversal can proceed by rotation or nonuniform modes; thermal activation and anisotropy determine blocking and coercivity. Small size alone does not guarantee a permanent hard magnet.

Thermal activation is barrier crossing enabled by thermal fluctuations. A system can remain for a long time near a local minimum of an energy landscape, then receive a fluctuation large enough to cross an energy barrier. Its most probable state and its waiting time for escape are therefore different questions.

In a simple high-barrier regime, the escape rate is approximated by $r(T)=r_0\exp [-\Delta E/(k_{B}T)]$, an Arrhenius equation. The barrier $\Delta E$ controls the strong temperature dependence, while the prefactor $r_0$ depends on dynamics near the initial state and transition region. Plotting $\log r$ against $1/T$ tests the exponential model: a constant prefactor gives slope $-\Delta E/k_B$. Interpreting a slope still requires care if several escape paths compete or the prefactor varies with temperature. A large barrier can delay approach to thermal equilibrium even when the final equilibrium state is known.

At fixed positive bias ratio $s=I_b/I_c$ with $0<s<1$, the Josephson coupling energy and work of the ideal bias source combine intoThis is the effective potential energy for an unwrapped Gauge-invariant Josephson phase; it includes the bias source and decreases by $2\pi s{E}_J$ on advancing one period. A local minimum and the adjacent downhill barrier areTo verify the barrier, solve $U^{\prime }=E_J(\sin \varphi -s)=0$, select $U^{\prime \prime }({\varphi }_m)>0$ and $U^{\prime \prime }({\varphi }_b)<0$, and subtract their potential energies. The small-oscillation angular frequency is fixed by the curvature:Thus the barrier and oscillation frequency both vanish as $s\to 1^{-}$, but with different powers. For $ϵ=1-s\ll 1$, expanding $\arccos (1-ϵ)$ and $\sqrt{2ϵ-{ϵ}^2}$ givesThe first approximation is for a nearly critical bias. At $s=0$ the exact downhill barrier is $2E_J$; at $s\ge 1$ there is no confining local minimum in this model.

For those stipulated parameters, direct evaluation gives $E_J/h=496.684\mathrm{GHz}$, $\Delta U/h=29.7670\mathrm{GHz}$, and ${\omega }_p/(2\pi )=2.89608\mathrm{GHz}$. Hence $\Delta U/(\hslash {\omega }_p)=10.2784$. The nearly critical barrier approximation gives $29.6165\mathrm{GHz}$, about $0.51\%$ below the exact result. These are original circuit calculations, not parameters assigned to the historical samples.