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A review of the dense Z-pinch

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Plasma Phys. Control. Fusion 53 (2011) 093001<br />

Topical Review<br />

magnetic field to ∼5 T, unless fur<strong>the</strong>r compressed. Indeed <strong>the</strong> azimuthal magnetic field for<br />

20 MA in 1 mm radius is as high as ∼4000 T, <strong>the</strong> local β is <strong>of</strong> order 1 and <strong>the</strong> plasma density<br />

at fusion temperatures (∼10 keV) is some 10 7 times that <strong>of</strong> a tokamak. The nuclear reaction<br />

rate depends on <strong>the</strong> square <strong>of</strong> <strong>the</strong> ion density, and so <strong>the</strong> confinement time becomes a critical<br />

factor, toge<strong>the</strong>r with <strong>the</strong> instantaneous fusion power. If <strong>the</strong> confinement time is less than an ion<br />

transit time along its length, <strong>the</strong>re will be no problems with impurities unlike in o<strong>the</strong>r magnetic<br />

confinement devices unless <strong>the</strong> plasma forms at first on an insulating wall. Wire-array and<br />

gas-puff Z-<strong>pinch</strong>es do not interact with a wall, as, unlike o<strong>the</strong>r magnetic confinement devices,<br />

<strong>the</strong> currents for equilibria are not driven by outward diffusion <strong>of</strong> <strong>the</strong> plasma. For example <strong>the</strong><br />

tokamak has radially outward Pfirsch–Schluter diffusion to generate <strong>the</strong> equilibrium currents.<br />

Thus in considering reactor configurations <strong>the</strong> ‘first wall’ can be far away, and indeed could be<br />

a liquid not limited in energy flux to 10 MW m −2 , and could also carry <strong>the</strong> return current [10].<br />

The disadvantages <strong>of</strong> <strong>the</strong> Z-<strong>pinch</strong> for fusion are well documented in papers extolling <strong>the</strong><br />

virtues <strong>of</strong> tokamaks, stellarators and o<strong>the</strong>r low density quasi-steady-state devices. The first is<br />

its instability to m = 0 (sausage) and m = 1 (kink) instabilities. The second is <strong>the</strong> heat loss to<br />

<strong>the</strong> two electrodes. In section 2.3 it was shown that <strong>the</strong> power loss is mainly to <strong>the</strong> anode and<br />

is <strong>of</strong> order 5 2 IT.ForI = 2 × 107 A and T = 10 4 eV this amounts to 0.5 TW. Clearly for this<br />

to be negligible a fusion power in <strong>the</strong> tens <strong>of</strong> TW at least must be considered and <strong>the</strong>refore for<br />

a reasonable size power station <strong>the</strong> Z-<strong>pinch</strong> must be pulsed.<br />

This indeed fits in with current knowledge <strong>of</strong> dynamic Z-<strong>pinch</strong>es in which, for example<br />

<strong>the</strong> intense s<strong>of</strong>t x-ray power occurs over 1 or 2 radial Alfvén transit times. For high Z<br />

radiating loads this is sufficient time to radiate a significant fraction <strong>of</strong> <strong>the</strong> stored energy,<br />

especially if <strong>the</strong> viscous heating mechanism (section 5.8) applies. Indeed this mechanism takes<br />

advantage <strong>of</strong> MHD instabilities and in this context instabilities are excellent for Z-<strong>pinch</strong>es.<br />

The dynamic ‘bounce’ <strong>of</strong> <strong>the</strong> <strong>pinch</strong> is very non-adiabatic, and is accompanied by <strong>the</strong> onset <strong>of</strong><br />

longer wavelength modes, and later, probably a disruption (section 3.14). The disruption is<br />

characterized by <strong>the</strong> creation <strong>of</strong> electron and ion beams, <strong>the</strong> latter which for deuterium will<br />

produce neutrons from a beam–target mechanism.<br />

To provide a longer confinement time various ideas have been employed. (a) The<br />

preparation <strong>of</strong> Kadomtsev current density pr<strong>of</strong>ile (section 3.2) as in a gas-embedded <strong>pinch</strong><br />

(section 7.4) can eliminate <strong>the</strong> m = 0 instability, or at least, for a plasma–vacuum boundary<br />

condition, reduce <strong>the</strong> growth rate. Instead <strong>the</strong> m = 1 instability dominates and indeed<br />

endeavours to form a helical minimum energy configuration, i.e. an axial magnetic field is<br />

spontaneously generated (presumably <strong>of</strong> arbitrary sign). (b) Sheared axial flow can also extend<br />

<strong>the</strong> stability time (sections 3.9 and 7.7) and fur<strong>the</strong>r work at high currents is needed to explore<br />

this concept. (c) Large ion Larmor radius effects have been shown both experimentally [14]<br />

and <strong>the</strong>oretically to reduce <strong>the</strong> growth rate <strong>of</strong> <strong>the</strong> m = 0 instability (section 3.8). (d) An axial<br />

magnetic field could be applied and compressed by means <strong>of</strong> a liner to provide a more stable<br />

configuration (see section 7.10). Early ideas and concepts for a Z-<strong>pinch</strong> fusion reactor were<br />

summarized by Sethian [613], before some <strong>of</strong> <strong>the</strong> recent advances were known, and when it was<br />

considered that radiative collapse would limit <strong>the</strong> current dynamically to a few megampéres.<br />

Hartmann [614] envisaged a gas-puff or a gas-embedded Z-<strong>pinch</strong> (which with presentday<br />

knowledge is, in its hollow form, a strong candidate). Later he extended this to <strong>the</strong><br />

continuous flow <strong>pinch</strong> [615] which had earlier been proposed by Morozov [616]. This relied<br />

on sheared axial flow to stabilize <strong>the</strong> <strong>pinch</strong>. Indeed Newton et al [617] did find in an experiment<br />

conducted in 1967 that a continuous flow <strong>pinch</strong> could form at <strong>the</strong> end <strong>of</strong> a Marshall gun’s central<br />

electrode at 0.5 MA. The <strong>pinch</strong> lasted 100 µs at several ×10 17 cm −3 electron density at 100–<br />

200 eV. However reference to section 2.3 and [97] would indicate a heat loss <strong>of</strong> 2.5TI, equal<br />

to 0.25 GW to <strong>the</strong> electrodes even at this low power. At <strong>the</strong> temperature and current required<br />

132

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