In inertial confinement fusion, pellets of deuterium tritium fuel are compressed and heated to the conditions where they undergo fusion and release energy. The target gain (ratio of energy released from the fusion reactions to the energy in the drive source) is a key parameter in determining the power flow and economics of an inertial fusion energy (IFE) power plant. In this study, the physics of gain is explored for laser-direct-drive targets with driver energy at the megajoule scale. This analysis is performed with the assumption of next-generation laser technologies that are expected to increase convergent drive pressures to over 200 Mbar. This is possible with the addition of bandwidth to the laser spectrum and by employing focal-spot zooming. Simple physics arguments are used to derive scaling laws that describe target gain as a function of laser energy, adiabat, ablation pressure, and implosion velocity. Scaling laws are found for the unablated mass, ablation pressure, areal density, implosion velocity, and in-flight aspect ratio. Those scaling laws are then used to explore the design space for IFE targets.

In recent years, inertial confinement fusion (ICF) experiments have seen an upward trend in fusion yield. This culminated in a significant result last year where, for the first time, a laser-driven ICF target exceeded ignition conditions and achieved target gain.1–3 In addition, laser-direct-drive implosions on OMEGA4 have reached the point at which the energy of fusion reaction products exceeded that of the hotspot internal energy.5 These achievements reflect the significant advancement in knowledge since the initial results from the Nation Ignition Campaign in 2012.6 The path of the most recent experiments on both the National Ignition Facility (NIF)7 and the omega Laser Facility, however, have pursued target regimes that will not scale to the high gains required for inertial fusion energy (IFE).

Performance of current ICF experiments is significantly degraded by poor laser coupling8–11 and, as a result, increased sensitivity to hydrodynamic instabilities seeded by capsule imperfections,12,13 engineering features14,15 (fill tubes, stalks, etc.), and non-uniformities in the drive illumination.16,17 This has led to the design of implosions that maximize shell implosion velocity and kinetic energy in an attempt to efficiently couple energy to the hotspot and reach ignition conditions. To accomplish this, the highest-performing implosions on the NIF and OMEGA use target designs with increased fuel entropy or adiabat18 in order to minimize the impact of the hydrodynamic instabilities. Fuel adiabat α is defined as the ratio of the target shell pressure to the Fermi-degenerate pressure of the fuel at solid density. The combination of high adiabat and high implosion velocity leads to a lower assembled fuel mass and lower fuel burnup fraction (because of reduced fuel areal density), limiting the target gain. To reach the performance required for IFE-relevant designs at megajoule-scale laser energies, it is necessary to develop a path toward the higher-mass, lower-adiabat regime where fuel gains are significantly higher.

A simple argument for the minimum gain required for IFE considers the power balance of a reactor. If the driver energy is given by the product of the power in P in and driver “wall-plug” efficiency η D, the fusion power output is then G η D P in, where G is the target gain. Assuming the conversion of fusion power to electric power is 40%,19 the total electric power of a power plant is P out 0.4 G η D P in. Then, if 1/4 of the output is circled back into powering the laser and other plant components, P in = 0.25 P out = 0.1 G η D P in; this leads to G η D 10. Finally, taking η D 10 %, we arrive at the requirement that target gain be G > 100.

To date, the highest-yield targets have been achieved on the NIF using the indirect-drive approach to ICF. This is where laser light is first converted into a bath of x rays contained within a high-Z casing (or Hohlraum). In indirect drive, only ∼10% to 15% of the driver energy is incident on the capsule. Conversely, laser direct drive has almost all the energy focused on target since the focal spot size is similar to that of the initial capsule size. However, the presence of the laser-plasma instabilities (LPI), such as stimulated Brillouin scattering and stimulated Raman scattering, lead to coupling losses, significantly reducing drive (ablation) pressures and limiting fuel mass and areal density. Understanding and eliminating these losses is, therefore, a priority in the development of next-generation laser-driver technology. New broadband lasers have great promise in their ability to mitigate the deleterious effects of LPI.20–23 It is expected that the use of bandwidth in combination with beam zooming will raise the absorption efficiency to upward of 90%. Laser focal spot zooming is the act of decreasing the spot size of the laser during the implosion. This helps prevent any loss of laser light that is not absorbed as the target decreases in size. A number of concepts have been proposed to achieve focal spot zooming. For excimer lasers, it has been shown that zooming can be achieved via induced spatial incoherence as demonstrated on Nike.24,25 For the solid-state laser technology considered in this paper, zooming would have to be employed by the use of multiple beam lines. If the use of bandwidth is shown to increase the convergent ablation pressure to above 200 Mbar (and possibly above 300 Mbar with zooming) without excessive fuel preheat caused by hot-electrons generated by LPI, direct drive will be a very compelling candidate for an ICF driver in an IFE facility.

In light of the demonstration of laboratory ignition at moderate laser drive energies and new laser technology on the horizon, the time is apt to revisit the ICF ignition design parameter space relevant to IFE. This manuscript establishes scaling laws that relate target gain to ICF design parameters. This is achieved by using a combination of the conclusions of simple physics arguments with the results of radiation-hydrodynamic simulations. The outcome is a set of simple scaling laws that can be used to describe the parameter space of IFE target design.

Extensive previous work has been done on deriving scaling laws for ICF-relevant metrics by Betti and Zhou.26–28 These scaling laws were derived using a flux-limited thermal conduction model with the value of the flux limiter chosen based on experiments conducted on the OMEGA laser. Significant progress in understanding laser coupling in laser-direct-drive ICF plasmas has been made over the last several years, so many of these scaling laws need to be revisited. This study re-derives these scaling laws considering the enhancement in ablation pressure due to broadband laser technology and beam zooming. This study also presents a key addition to the work, where the design space is constrained by considering the minimum implosion velocity required for ignition. In doing this, it is possible to express the target gain as a function of driver energy, incident laser intensity, drive pressure, and fuel adiabat.

To begin, a simple argument is presented to demonstrate that increasing the drive pressure in ICF implosions has the most leverage in reaching robust high gains. For such a purpose, the target gain is written as the burnup fraction f burn, multiplied by unablated fuel mass M f, multiplied by the fusion neutrons' specific energy ε DT ( ε DT = 271 TJ/kg), divided by the laser energy E laser,
(1)
It can be seen that the target gain is directly related to the unablated fuel mass. Increasing the unablated mass is a key step in increasing the gain. However, as the unablated mass is directly related to laser energy, it must be increased independently of energy to positively affect the gain. This is accomplished by reducing implosion velocity, which scales with the inverse power of drive pressure and laser energy. The fuel mass is accelerated to velocity v imp by ablation pressure p a and the maximum kinetic energy of the shell is proportional to the pdV work done on the shell. Now, because the final radius of the target is much smaller than the initial radius, it can be assumed that M f v imp 2 p a R 0 3, so
(2)
where R0 is the initial shell radius. Maximizing fuel mass at a given laser energy will require either maximizing the product p a R 0 3 or minimizing implosion velocity v imp. Implosion velocity can only be reduced, however, to a certain extent since it must remain above a threshold value for the target to ignite. This threshold is mostly dependent on laser energy and the fuel adiabat (this is discussed in detail in Sec. IV D). R0 can be estimated by noting that the target is accelerated over a distance R 0, to reach velocity v imp over acceleration time t accel E laser / P laser, where P laser is the peak laser drive power. Using R 0 v imp t accel and introducing I 0 = P laser / ( 4 π R 0 2 ) lead to
(3)
Since ablation pressure in laser-direct-drive implosions scales with incident laser intensity as p a p 0 I β with β < 1 (where β is dependent on the absorption mechanisms) and p0 is a constant that depends on the laser properties, the product p a R 0 3 depends on laser intensity as p a R 0 3 I 0 β 1. Therefore, one potential path to increasing p a R 0 3 and the fuel mass M f is to drive targets at lower intensities. This, according to Eq. (3), will require a longer acceleration distance, which leads to larger target radius and, therefore, increased surface area. While beneficial for 1D target gain, increasing the travel distance also increases the in-flight aspect ratio (IFAR), which compromises target robustness to hydrodynamic instabilities. The much more attractive option to increase p a R 0 3 is to improve laser coupling and ablation efficiency (by mitigation of LPI and implementing beam zooming), which leads to an increase in the pre-factor p0 in pressure scaling with intensity. An additional path to increasing ablation pressure is through the use of shorter wavelength lasers. Analytic scaling laws29,30 expect ablation pressure to scale like
(4)
where I L is the laser intensity and λ L is the laser wavelength. In this study, we assume the use of a broadband solid-state system centered around 351 nm as this is a well-studied regime that has been previously been considered for IFE.19,31,32 There are also concepts for lower wavelength systems using excimer laser sources.31,33 Developing next-generation laser drivers with increased bandwidth and focal-spot zooming capabilities is a vital step forward to provide robust, high-gain target designs.

This section summarizes the target design process that was used to generate a database of 1D implosion simulations. This study was carried out with the radiation-hydrodynamics code LILAC34 that has been benchmarked against direct-drive experiments. In each case, the design of each implosion began by setting the thicknesses of the different capsule layers; the laser pulse profile was then shaped to set the fuel adiabat and ignite the target.

The targets consisted of central DT gas, surrounded by a frozen DT layer encased in a DT-wetted CH foam; a 100 mg/cm3 foam was used, so the wetted foam density was 0.33 g/cm3. The central region contained DT vapor at the triple point, which corresponds to a density of 0.67 mg/cc. The inner radius of the targets varied in 100 μm steps from 750 to 1350 μm, and fuel masses were set to the values of 0.8, 1.0, 1.2, 1.4, 1.6, 1.8, 2.5, 3.5, 5, and 7 mg. The thickness of the DT-wetted CH foam ablator was optimized in each implosion, such that the wetted-foam layer is entirely ablated during the early part of the drive pulse, taking advantage of the high ablation and hydrodynamic efficiency of the DT fuel layer. Crucially, the pure DT never drops to densities below critical in the plasma corona; therefore, laser absorption takes place only in the CH DT region, which has higher inverse bremsstrahlung absorption due to the higher Z. The initial beam spot shape was a super-Gaussian order 5, with the 1/e fraction of the peak intensity at 90% of the initial outer radius of the target. Higher ablation pressures would be achieved with smaller spot shapes; however, this choice of large beam radius is purposefully cautious, with the intention to minimize low-mode asymmetries that arise from the beam-port geometry. Note that the effect of multi-dimensional perturbations is not modeled in this study. In some implosions, one- and two-stage focal-spot zooming was employed to enhance absorption and drive pressure without sacrificing implosion symmetry. For the first stage, the beam radius was reduced to 0.55 × the initial value at the time of shock breakout from the inner surface. By timing this at shock breakout, when the conduction zone and plasma are established, this aids in smoothing out nonuniformities that arise from the finite beam size. When a second zooming stage was used, the spot size was reduced to 0.275 × the initial beam radius 1 to 2 ns after the first zooming stage. It should be noted that the aggressive zooming used in this study was chosen to ensure minimal refractive losses for all implosions. It is possible for strong zooming to introduce significant low-mode perturbations as the spot size decreases. A fully considered optimization of zooming requires multi-dimensional simulations; this work is currently being pursued by the authors.

The laser wavelength used in the simulations was 351 nm (frequency tripled ND:glass). The pulse shape in this study used a 300 ps FWHM picket followed by a foot, then a rise to the peak power. The pulse was shaped systematically, iterating over a series of simulations to find the maximum gain. First the picket power was tuned to set the mass-averaged adiabat of the fuel at a desired value that varied between 1 and 7. The power of the foot was then chosen such that the shock launched from the foot breaks out soon after the breakout of the shock launched from the picket. The rise of the main pulse then had a kidder-like35 shape, with the timings chosen so the main shock is also synchronous with the picket and the peak in laser power occurs after the shock breakout. Finally, the power of the main pulse was increased until the shell velocity became sufficient to achieve ignition. In each case, the duration the peak was timed so that the pulse ended at the time the shell reaches maximum implosion velocity. The laser energy in these pulses ranged from 1 to 8 MJ. The implosion velocities varied between 223 and 473 km s−1.

It is the aim of this study to relate design parameters (energy, adiabat, ablation pressure, and incident intensity) to target performance (gain and stability characteristics). This is achieved by relating various implosion metrics to one another through simple power-law scalings. In each case, basic physics arguments are used to argue the dependence of variables upon one another, resulting in a scaling law. Where necessary, fits are then employed to find exact dependencies of the variables from a database of 1D ICF implosion simulations. In each fit, least squared regression is used to find either the equation coefficients or exponents or both. In this study, scaling laws are found for unablated target mass, ablation pressure, assembled fuel burnup fraction, areal density, and implosion velocity, all of which relate to target gain. Additionally, a scaling law for IFAR is found since it (along with fuel adiabat) has been shown to be relevant to hydrodynamic stability.36 

In Sec. II, a simple scaling law was used to relate kinetic energy to work done by the ablative drive. In that derivation, the effects of mass ablation and convergence were omitted for simplicity. These effects can be accounted for with the addition of some corrective factors.

First, consider the mass that is ablated over the course of the implosion. The term p a R 0 3 represents the total work done over the whole implosion. However, some work is done early in time on a portion of the shell that is later ablated and, therefore, does not contribute to the kinetic energy of the final mass assembly. It should then be expected that the kinetic energy is related to the product of the total work and some function of the remaining mass fraction M f / M 0, where M0 is the initial mass of the shell (pure DT plus ablator). The work done on the shell is also affected by the variation in drive pressure as the target converges. As such, there is an additional term related to target convergence. Here, target convergence is defined as the radius of the ablation front when the shell velocity reaches its maximum, R f divided by the initial inner radius of the shell, R0. Bringing together the corrective factors and assuming a power-law relation gives
(5)
where a1 and a2 are both positive power indices that can be determined by applying a fit to the simulation database; this results in a 1 = 1.41 ± 0.08 and a 2 = 0.70 ± 0.06. There are two effects that relate the target convergence to the work done. First, targets with low aspect ratios have larger shell volumes and, therefore, need to transfer more energy into the shell during the shell compression phase. These targets tend to converge less and require more work is done. Second, targets with higher convergence tend to do more work on the shell because the change in volume during the acceleration phase is higher. The data in this study find that the former effect is dominant, which results in an overall positive power for the R f / R 0 term.
Scaling laws can be found to relate the R0, mass fraction, and convergence terms to the laser energy, laser intensity, ablation pressure, implosion velocity, and adiabat. The remaining mass fraction can be expressed by the rocket equation37 
(6)
The exponent on the right-hand side of Eq. (6) was found from a fit to the database giving 0.594 ± 0.006. The simulation data suggest that the remaining mass fraction is solely a function of implosion velocity, implying that the m ̇ a / p a term is constant across all targets. This is a result of the fact that mass ablation rate and ablation pressure scale similarly with incident intensity in spherical geometry29,38–40 and, therefore, the intensity term approximately cancels out. It should be noted that the exhaust velocity will still be dependent on the choice of ablator and laser wavelength.
The convergence term R f / R 0 can be related to the remaining mass fraction and the τ parameter. The parameter τ is the ratio of acceleration time t acc to the shell transit time t sound. The full relevance of τ to implosion characteristics is discussed in more detail in Sec. IV D. A fit to the simulation data suggests
(7)
where the values with error were 0.57 ± 0.01 and 0.70 ± 0.03. For τ, the scaling relation to implosion velocity, ablation pressure, and fuel adiabat is just stated as follows (the details are discussed in Sec. IV D):
(8)
Finally, for the R0 term, it was shown earlier that R 0 3 E laser v imp / I 0. To match this relation with the simulation results, a correction must be made to the intensity term. The relation for R0 uses intensity defined as the laser power divided by the inner surface area of the shell I 0 = P laser / 4 π R 0 2, whereas in the simulations, intensity is defined at the outer surface area I out = P laser / 4 π R out 2 (this is the metric relevant to the scaling of ablation pressure with intensity). The terms R0 and R out can be related by
(9)
where ρ avg is the average density of the shell, which was found to be 0.277 g/cm3, averaged across all the targets in this study. Now the ratio of intensity at the inner surface I0 and outer surface I out can be expressed as
(10)
This can be re-expressed using Eqs. (5)–(8) to give
(11)
where the ( 0.623 ± 0.005 ) × 10 15 W/cm2 factor was found from a fit to the simulations. Then, a simplified power-law form can be found by fitting to the simulation database,
(12)
The values with error were 0.69 ± 0.02, 1.29 ± 0.05, and 0.01 ± 0.02. Now, bringing together Eqs. (5)–(8), using the relation R 0 3 E laser v imp I 0 ( I out I in ), and Eq. (12) and fitting to the database to find the pre-factor gives ( 0.678 ± 0.004 ) mg, so
(13)
with units of mg, MJ, 100 Mbar, 1015 W/cm2, and 300 km/s; the use of these units is consistent throughout this manuscript. In the simulations, M f is defined as the fuel mass between the inner surface, where the mass density is 1/e the maximum and the inflection point in the mass density ( d 2 ρ / d r 2 = 0) at the outer surface. It is taken at the point in time where the implosion velocity is at a maximum. Implosion velocity itself is the maximum in the mass-averaged velocity across the shell. Intensity is the maximum laser power divided by the initial outer surface area of the target. The definition of ablation pressure is described in detail in Sec. IV B. A comparison of the simulated unablated mass and the unablated mass predicted from Eq. (13) can be seen in Fig. 1.
FIG. 1.

A comparison of the unablated mass extracted from the simulation database to the unablated mass predicted by the scaling law in Eq. (13).

FIG. 1.

A comparison of the unablated mass extracted from the simulation database to the unablated mass predicted by the scaling law in Eq. (13).

Close modal

For each implosion, it is necessary find a value for the ablation pressure that is characteristic of the implosion. However, ablation pressure is a time-dependent variable that changes with laser power and capsule convergence. In this study, ablation pressure is defined as the pressure at the ablation front at the time where the front has converged to 1 / 3.5 × the initial outer surface of the capsule. This definition of drive pressure uses the same convention as outlined in Ref. 41 and roughly corresponds to the point in the implosion where the effect of convergence causes the pressure inside the shell to exceed the ablation pressure. The ablation front itself is defined at the minimum of the electron temperature in the shell ( d T e / d r = 0). Details of this definition can be seen in Fig. 2.

FIG. 2.

Details of the definition of ablation pressure. (a) A plot showing how the position of the ablation front and value of the ablation pressure change over time. The ablation pressure characteristic of the implosion is taken at the point in time where the ablation front has converged to 1 / 3.5 × the initial outer capsule radius, shown by the dashed lines. (b) A snapshot of the mass density, pressure, and electron temperature profiles in the target. The time-dependent ablation pressure is taken to be the pressure in the shell at the front of the electron temperature wave (red line). This position is illustrated by the vertical black dashed line.

FIG. 2.

Details of the definition of ablation pressure. (a) A plot showing how the position of the ablation front and value of the ablation pressure change over time. The ablation pressure characteristic of the implosion is taken at the point in time where the ablation front has converged to 1 / 3.5 × the initial outer capsule radius, shown by the dashed lines. (b) A snapshot of the mass density, pressure, and electron temperature profiles in the target. The time-dependent ablation pressure is taken to be the pressure in the shell at the front of the electron temperature wave (red line). This position is illustrated by the vertical black dashed line.

Close modal
With a consistent definition of ablation pressure across all simulations, the relationship between ablation pressure and incident intensity can now be analyzed. Previous work has shown that when the effects of LPI are present, ablation pressure scales as p a ( Mbar ) = 82 I out 0.57.41 For the simulations in this study (where it is assumed LPI are suppressed by laser bandwidth), the scaling laws with and without zooming were
(14)
(15)
(16)

The errors on the coefficients were ±4 Mbar, ±3 Mbar, and ±3 Mbar, respectively, and the errors on the exponents were all ±0.02. The variable p a , 1 zoom is taken from simulations, where the beam radius is decreased by a factor of 0.55 × at the time of shock breakout. Then, p a , 2 zoom is taken from simulations using a second zooming stage, reducing to 0.275 × the initial beam radius 1–2 ns after the first zoom stage. The ablation pressure with time profile in Fig. 2 shows a one-stage zoom implosion and highlights the jump in ablation pressure that is observed when the beam size is reduced. The scaling of ablation pressure with intensity from the simulation database and corresponding fits can be seen in Fig. 3. These relations are used later to explore IFE designs for different scalings of intensity and ablation pressure.

FIG. 3.

Simulation results comparing ablation pressure to incident intensity. The results are show with the fitted scaling laws for simulations without zooming (green) and with one-stage (blue) and two-stage zooming (red). The scaling law from a previous study41 that includes cross-beam energy transfer is shown in black.

FIG. 3.

Simulation results comparing ablation pressure to incident intensity. The results are show with the fitted scaling laws for simulations without zooming (green) and with one-stage (blue) and two-stage zooming (red). The scaling law from a previous study41 that includes cross-beam energy transfer is shown in black.

Close modal

Burnup fraction is well understood to be directly dependent on ρR by f burn = ρ R / ( ρ R + H B ),29 where the variable H B is dependent on the hotspot conditions and can vary between 6 and 9  g / cm 2. For the results in this study, H B = 6.67 was used across all simulations. It should be noted that more accurate models for burnup fraction have been proposed,42 but the variance of the data in this study is large enough that such a model does not improve the quality of the fit to the data.

By considering a scaling law for ρR, the burnup fraction can be related to ablation pressure, incident intensity, energy, implosion velocity, and adiabat. The following derivation makes some corrections to the model proposed in Ref. 43. The unablated mass at the beginning of shell deceleration is given by
(17)
where the right-hand terms are shell mass density, shell thickness, and shell inner radius at the onset of deceleration. The scaling of kinetic energy and work done in Eq. (5) can be re-expressed using v imp = R 0 / t accel , R 0 / R f τ 0.52 ( M f M 0 ) 0.74 to find
(18)
Relating Eqs. (17) and (18) and using t accel ( E / v imp 2 I 0 ) 1 / 3 and applying the correction for the intensity term gives
(19)
where A f is the aspect ratio R f / Δ f and can be neglected as approximately constant across all implosions A f 1.35. Substituting Eq. (19) into the following expression from Ref. 43:
(20)
and replacing ρf with ( p a / α ) 3 / 5 results in
(21)
where the ( 1.85 ± 0.01 ) g / cm 2 factor has been found from a fit to the simulation database and the fit can be seen in Fig. 4. The modeled ρR is taken from simulations with thermonuclear burn turned off, taking the maximum value at any point in time. Note that the expression for ρR is dependent on the scaling between intensity and pressure; therefore, the shell ρR is increased with zooming and the elimination of cross-beam energy transfer (CBET).
FIG. 4.

Comparison of the ρR extracted from the simulations to the ρR predicted by the scaling law in Eq. (21).

FIG. 4.

Comparison of the ρR extracted from the simulations to the ρR predicted by the scaling law in Eq. (21).

Close modal

For any given target design, the choice of implosion velocity is a result of the balancing of ignition conditions in the hotspot, target gain, and shell stability properties. As will be shown below, satisfying the ignition conditions at peak compression requires that the implosion velocity v imp exceed a threshold value v min. Since the shell mass is inversely proportional to the implosion velocity, operating at the limit of this threshold maximizes fuel mass and, therefore, target gain. The downside of such a target, however, is that there is no margin to overcome losses to 3D effects (perturbation growth, which reduces hotspot pressure and energy). On the other hand, designs that operate with implosion velocity well above the minimum threshold are also less robust to nonuniformity growth because they typically have higher IFAR's, which are susceptible to short-wavelength perturbations during shell acceleration. With this in mind, it is proposed that operating with v imp in close proximity to v min is a good compromise between stability and target gain. The target design process outlined in Sec. III is intended to find targets that ignite at the minimum implosion velocity.

It is possible to use scaling laws for the hotspot conditions at ignition to define v min in terms of ablation pressure, incident intensity, adiabat, and laser energy. The conditions for ignition are met when the energy deposition from fusion alphas exceeds the losses due to thermal conduction, radiation, and PdV work done on the shell during expansion. This is more commonly known as Lawson's criterion. Below are two simple definitions of Lawson's criterion using ICF relevant metrics.36,41 First, using the hotspot areal density and hotspot ion temperature
(22)
then alternatively, using hotspot pressure and hotspot radius
(23)
The ignition condition in Eq. (23) can be used to impose a lower limit on the implosion velocity. Starting from scaling laws for p hs and R hs found in Ref. 36,
(24)
(25)
Note that in both these equations, p a is defined as the ablation pressure at the onset of shell deceleration. It is necessary to apply a correction to the scaling for hotspot pressure in Eq. (24). The scalings in Eqs. (24) and (25) were found by only considering the pressure amplification in the central vapor due to the compression by the converging shell. In fact, there are two additional effects that contribute to the hotspot pressure. The first is the result of rarefaction of material from the inner surface of the shell.36 For the purpose of this study, the effect of rarefaction is negligible, but it should be noted that it will be much more significant in targets that have a lower initial density in the central region.44,45 The other contributor to hotspot pressure is related to the dynamics of the shell during acceleration and is much more significant in the targets considered this study. A correction to Eq. (24) can be applied to account for this effect. The original derivation for Eq. (24) relies on the use of the shell pressure at the onset of deceleration and assumes that this is the same as the ablation pressure. However, in the present study, the ablation pressure is defined at a fixed convergence and, therefore, the shell pressure at the onset of deceleration will depend on how much the target has converged at that point. To quantify this effect, it is necessary to find a parameter that is related to the convergence at the onset of deceleration. For that, we use the parameter τ defined as
(26)
where t sound is the transit time of a sound wave through the shell, Δ is the thickness of the shell, and c s is the sound speed in the shell. At the very start of the implosion, τ will have a value much less than one. Over the course of the implosion, the sound speed in the shell will increase until τ 1. At this point, the shell transit time is on the same order as the implosion time, meaning the shell thickness can no longer adapt to changes in convergence, amplifying density. If the value for τ in Eq. (24) is calculated at the same level of convergence for all targets, a low value will correspond to an implosion that will have converged more at the onset of deceleration and, therefore, will have a higher shell pressure. This then results in a higher hotspot pressure than that predicted in Eq. (24). This relationship can be seen in Fig. 5 that compares the simulation hotspot pressure p hs , sim to the nominal hotspot pressure p hs n given by Eq. (24), using a pre-factor of 600. Hotspot pressure is taken from burn-off simulations by finding the volume-averaged hotspot pressure up to the hotspot radius, defined as the point where mass density reaches 1/e times the maximum value in the shell. The value is extracted at the point in time where the product of hotspot pressure and radius reaches its maximum value.
FIG. 5.

The dependence of hotspot pressure on the parameter τ. The green line shows the fit in Eq. (29). There is an additional sensitivity of hotspot pressure on the timing of the shock trajectories in the shell. Here, a subset of the data has been selected to minimize this effect.

FIG. 5.

The dependence of hotspot pressure on the parameter τ. The green line shows the fit in Eq. (29). There is an additional sensitivity of hotspot pressure on the timing of the shock trajectories in the shell. Here, a subset of the data has been selected to minimize this effect.

Close modal
To calculate τ from the simulations, Eq. (26) can be rearranged using c s p a / ρ , ρ ( p a / α ) ( 3 / 5 ) , P laser 4 π R 0 2 I 0, and M f ρ 4 π R 2 Δ to give
(27)
where Eq. (13) has been used to replace the M f term. A fit for τ was found by using exponents on the implosion variables, resulting in
(28)
The fitted values with errors were 48.1 ± 0.04, 2.43 ± 0.03, 0.275 ± 0.008, and 0.46 ± 0.01. The fit for the variable τ can be seen in Fig. 6. The simulated value for τ is calculated from the database using the right-hand side expression in Eq. (27), where all relevant terms have been previously defined.
FIG. 6.

The fit of the τ variable scaling law to the simulation database. The τ from the simulation database is calculated using Eq. (27) and is compared against the value for τ predicted by Eq. (28).

FIG. 6.

The fit of the τ variable scaling law to the simulation database. The τ from the simulation database is calculated using Eq. (27) and is compared against the value for τ predicted by Eq. (28).

Close modal
It is now possible to find a relation between τ and hotspot pressure. As a functional form, one should expect an inverse relationship between p hs , sim / p hs n and τ (for the reasons previously discussed). The best fit was found to be
(29)
which had errors of 1.20 ± 0.05 and 0.042 ± 0.002; the fit can be seen in Fig. 5. Now, Eq. (29) can be used to find an expression for the threshold implosion velocity. Combining Eqs. (24) and (25), applying the correction to hotspot pressure in Eq. (29) and using the ignition criterion in Eq. (23), gives
(30)
where the pre-factor has been found from a fit to the simulation database and has a value of ( 266.1 ± 0.9 ) km/s. The results of the fit for implosion velocity can be seen in Fig. 7.
FIG. 7.

The fit of the implosion velocity scaling law to the simulation database. The implosion velocity from the simulation database is compared against the implosion velocity predicted by Eq. (30).

FIG. 7.

The fit of the implosion velocity scaling law to the simulation database. The implosion velocity from the simulation database is compared against the implosion velocity predicted by Eq. (30).

Close modal
Finally, the scaling of IFAR is considered as a metric related to the hydrodynamic stability of the implosion. IFAR is defined as the in-flight inner radius R divided by the in-flight shell thickness Δ inflight. The derivation for IFAR largely follows that in Ref. 46 with corrections for convergence and mass fraction. The in-flight shell thickness is given by
(31)
where Δ 0, ρ0, and R0 are the initial shell thickness, mass density, and inner radius, respectively, and R is the radius at which IFAR is defined. In this study, IFAR is defined at the point R = R 0 / 1.5, so using ρ inflight = ( p a / α ) 3 / 5, IFAR is then
(32)
Next, we multiply the numerator and denominator by R 0 2 and use the fact that M 0 ρ 0 Δ 0 R 0 2 and R 0 ( E laser v imp / I 0 ) 1 / 3 to obtain
(33)
Substituting in the mass scaling from Eq. (13) gives
(34)
Then, using the mass fraction scaling [Eq. (6)] and the τ scaling [Eq. (28)] and fitting to the simulation, we arrive at
(35)
The pre-factor term with error was 30.7 ± 0.02 and the fit from Eq. (35) can be seen in Fig. 8. IFAR has a strong dependence on implosion velocity, meaning fast implosions lead to high IFAR's. Implosions operating at high IFAR's are hydrodynamically unstable and are unlikely to ignite robustly as the shell breaks up. Operating near the limit of lowest implosion velocity is therefore more ideal for IFE.
FIG. 8.

The fit of IFAR scaling law to the simulation database. The simulated IFAR is plotted against the IFAR predicted from Eq. (35).

FIG. 8.

The fit of IFAR scaling law to the simulation database. The simulated IFAR is plotted against the IFAR predicted from Eq. (35).

Close modal
It is now possible to bring together all the scaling laws from Sec. IV to explore the design space of IFE. To start, gain is re-expressed in terms of laser energy, ablation pressure, incident intensity, adiabat, implosion velocity, and the corrective factors using Eqs. (1), (13), and (21) and f burn = ρ R / ( ρ R + 6.67 ). This gives
(36)

By finding a solution to the equations that determine the minimum implosion velocity required for ignition [Eqs. (27) and (30)], it is possible to constrain the model and express implosion velocity as a function of energy adiabat pressure and intensity. With that, the gain of a target can be calculated from the laser energy, ablation pressure incident intensity, and adiabat in the limit of the lowest implosion velocity required for ignition. Figure 9 shows the gain scaling from Eq. (36) with different levels of zooming [calculated by using the ablation pressure scaling Eqs. (14)–(16)]. It can be seen that a one-stage zoom at 1 MJ is enough to reach gain ∼100 at low adiabat α 1. Increasing the energy to 2 MJ significantly expands the parameter space and enables the adiabat to be increased without sacrificing gain. Gain can also be increased by applying a second zooming stage and/or reducing the incident laser intensity. For instance, adding a second zoom stage and decreasing the intensity to 0.5 × 10 15 W/cm2 allows a gain of 100 to be achieved at 2 MJ with an adiabat above 3. However, one must be cautious in lowering the incident intensity because this may sacrifice target stability. Previous work has shown that the IFAR and adiabat of a target are related to the growth of high-mode instabilities.36  Figure 10 compares how the IFAR predicted from Eq. (35) varies over the IFE target space for two different intensities, each using a two-stage zoom. Targets with lower incident intensity may achieve higher gains, but will make a sacrifice in the form of increasing IFAR. At present, it is not possible to estimate an upper limit on the IFAR since this will depend on the level of laser imprint present in next-generation laser technology. The addition of bandwidth is expected to reduce imprint below the levels seen in current experiments. The amount of imprint present in broadband laser sources will ultimately determine the IFAR limit for high-gain IFE targets. It should be noted that the current limit on IFAR in direct-drive implosions is dominated by imprint. Even in the event that next-generation laser technology significantly reduced imprint, targets would likely still be susceptible to other sources of high-mode perturbation such as imperfections from target manufacture. However, the low IFARs achieved when using MJ energies and higher ablation pressures will help mitigate the design sensitivity to those imperfections.

FIG. 9.

Gain curves for (a) 1 MJ and (b) 2 MJ implosions for four different intensity and pressure scalings. The region where gain is over 100 is shaded.

FIG. 9.

Gain curves for (a) 1 MJ and (b) 2 MJ implosions for four different intensity and pressure scalings. The region where gain is over 100 is shaded.

Close modal
FIG. 10.

IFAR and gain vary with energy and adiabat. A comparison is shown between (a) low-intensity and (b) high-intensity designs. Then intensities in this plot refer to the intensity at the initial outer surface I out. This plot was made using the scaling for gain in Eq. (36) and IFAR in Eq. (35), with the assumption of a two-stage zoom [Eq. (16)]. The colored regions and black lines represent the IFAR contours and the solid white lines are the gain contours.

FIG. 10.

IFAR and gain vary with energy and adiabat. A comparison is shown between (a) low-intensity and (b) high-intensity designs. Then intensities in this plot refer to the intensity at the initial outer surface I out. This plot was made using the scaling for gain in Eq. (36) and IFAR in Eq. (35), with the assumption of a two-stage zoom [Eq. (16)]. The colored regions and black lines represent the IFAR contours and the solid white lines are the gain contours.

Close modal

A reasonable estimate for the laser energy that may be available in a full-scale IFE reactor is 1–2 MJ. With that in mind, we present four IFE example targets that achieve a gain of 100 over a range of adiabats and drive pressures. The simulation characteristics are summarized in Table I. It should be noted that multi-dimensional effects in the targets summarized in Table I will reduce the total yields and as such should not be taken as suggestions for IFE targets. Instead, these results are intended to demonstrate the trade-offs that can be expected in 1D implosion performance when energy, adiabat, and ablation pressure are adjusted at the MJ scale.

TABLE I.

Summary of the implosion metrics from four simulations. All the simulations achieve gain ∼100. Targets 1 and 2 are high-intensity targets with a one-stage and 2-stage zoom, respectively. Target 3 is low-intensity that uses a two-stage zoom. Target 4 is low intensity with a two-stage zoom at a higher laser energy.

Target 1 Target 2 Target 3 Target 4
E laser  1.01 MJ  0.99 MJ  1.01 MJ  1.53 MJ 
E fus  146 MJ  119 MJ  123 MJ  189 MJ 
E neutron  118 MJ  95.1 MJ  98.7 MJ  151.3 MJ 
α  1.00  1.38  1.84  2.19 
I out  1.00 × 10 15 W / cm 2  1.00 × 10 15 W / cm 2  0.60 × 10 15 W / cm 2  0.63 × 10 15 W / cm 2 
p a  331 Mbar  358 Mbar  260 Mbar  263 Mbar 
v imp  274 km/s  295 km/s  312 km/s  306 km/s 
IFAR  13.3  9.90  14.6  12.1 
ρR  3.20 g/cm2  2.84 g/cm2  2.20 g/cm2  2.43 g/cm2 
f burn  0.334  0.294  0.230  0.255 
Τ  24.4  28.6  28.8  28.0 
Inner radius  851 μ 915 μ 1250 μ 1350 μ
M f  1.33 mg  1.22 mg  1.59 mg  2.21 mg 
Zoom stages 
Target 1 Target 2 Target 3 Target 4
E laser  1.01 MJ  0.99 MJ  1.01 MJ  1.53 MJ 
E fus  146 MJ  119 MJ  123 MJ  189 MJ 
E neutron  118 MJ  95.1 MJ  98.7 MJ  151.3 MJ 
α  1.00  1.38  1.84  2.19 
I out  1.00 × 10 15 W / cm 2  1.00 × 10 15 W / cm 2  0.60 × 10 15 W / cm 2  0.63 × 10 15 W / cm 2 
p a  331 Mbar  358 Mbar  260 Mbar  263 Mbar 
v imp  274 km/s  295 km/s  312 km/s  306 km/s 
IFAR  13.3  9.90  14.6  12.1 
ρR  3.20 g/cm2  2.84 g/cm2  2.20 g/cm2  2.43 g/cm2 
f burn  0.334  0.294  0.230  0.255 
Τ  24.4  28.6  28.8  28.0 
Inner radius  851 μ 915 μ 1250 μ 1350 μ
M f  1.33 mg  1.22 mg  1.59 mg  2.21 mg 
Zoom stages 

The work presented here has explored the design space of future IFE facilities that will make use of next-generation laser technologies. The addition of bandwidth to the laser spectrum, along with focal-spot zooming, are technologies that will significantly boost the drive pressures in laser-direct-drive. This enhancement in ablation pressure will make it possible to reach a gain of 100 with targets that are substantially more hydrodynamically stable. A gain of 100 is the minimum required for the power flow of a plant with a 10% wall-plug efficiency. However, the economics of plant will also depend on the financial cost of the driver per megajoule and target gain would need to be adjusted accordingly.

In this work, it has been shown how simple scaling laws can be used to map out the implosion parameter space. For each scaling law, a simple physics model was used to justify the dependences of implosion parameters upon one another. The terms of those simply derived scaling laws were then fit to a simulation database of ICF implosions spanning a wide range of laser energies and target scales. A hotspot model was used to constrain the parameter space to implosions that operate at the minimum possible implosion velocities. Such implosions are the most robust and have the highest performance due to the resulting large mass assemblies. Additionally, the τ parameter was proposed as a correction to previous hotspot models that accounts for the amplified shell density due to convergent effects. With the scaling relations derived in this manuscript, it is possible to predict the 1D gain and IFAR for a given energy, adiabat, and ablation pressure scaling.

This study was funded by the ARPA-E BETHE (Grant No. DE-FOA-0002212). This work was based upon the work supported by the Department of Energy National Nuclear Security Administration under Award No. DE-NA0003856, the University of Rochester, and the New York State Energy Research and Development Authority. The support of DOE does not constitute an endorsement by DOE of the views expressed in this paper.

This report was prepared as an account of work sponsored by an agency of the U.S. Government. Neither the U.S. Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the U.S. Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the U.S. Government or any agency thereof.

The authors have no conflicts to disclose.

William Thomas Trickey: Conceptualization (equal); Data curation (lead); Formal analysis (lead); Investigation (equal); Methodology (equal); Writing – original draft (lead); Writing – review & editing (lead). Valeri N. Goncharov: Conceptualization (equal); Data curation (supporting); Formal analysis (supporting); Funding acquisition (lead); Investigation (equal); Methodology (equal); Writing – original draft (supporting); Writing – review & editing (supporting). Riccardo Betti: Investigation (supporting); Writing – review & editing (supporting). E. Michael Campbell: Investigation (supporting); Writing – review & editing (supporting). Timothy J. B. Collins: Investigation (supporting); Writing – review & editing (equal). Russell K. Follett: Investigation (supporting); Writing – review & editing (equal).

The data that support the findings of this study are available from the corresponding author upon reasonable request.

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