R. Betti
University of Rochester
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Featured researches published by R. Betti.
Physical Review Letters | 2016
S. P. Regan; V.N. Goncharov; I.V. Igumenshchev; T. C. Sangster; R. Betti; Arijit Bose; T. R. Boehly; M.J. Bonino; E.M. Campbell; D. Cao; T.J.B. Collins; R. S. Craxton; A. K. Davis; J. A. Delettrez; D. H. Edgell; R. Epstein; C.J. Forrest; J. A. Frenje; D. H. Froula; M. Gatu Johnson; V. Yu. Glebov; D. R. Harding; M. Hohenberger; S. X. Hu; D. Jacobs-Perkins; R. Janezic; Max Karasik; R. L. Keck; J. H. Kelly; Terrance J. Kessler
A record fuel hot-spot pressure P_{hs}=56±7u2009u2009Gbar was inferred from x-ray and nuclear diagnostics for direct-drive inertial confinement fusion cryogenic, layered deuterium-tritium implosions on the 60-beam, 30-kJ, 351-nm OMEGA Laser System. When hydrodynamically scaled to the energy of the National Ignition Facility, these implosions achieved a Lawson parameter ∼60% of the value required for ignition [A. Bose etxa0al., Phys. Rev. E 93, 011201(R) (2016)], similar to indirect-drive implosions [R. Betti etxa0al., Phys. Rev. Lett. 114, 255003 (2015)], and nearly half of the direct-drive ignition-threshold pressure. Relative to symmetric, one-dimensional simulations, the inferred hot-spot pressure is approximately 40% lower. Three-dimensional simulations suggest that low-mode distortion of the hot spot seeded by laser-drive nonuniformity and target-positioning error reduces target performance.
Physical Review E | 2016
A. Bose; K. M. Woo; R. Betti; E.M. Campbell; D. Mangino; A. R. Christopherson; R.L. McCrory; R. Nora; S. P. Regan; V.N. Goncharov; T. C. Sangster; C.J. Forrest; J. A. Frenje; M. Gatu Johnson; V. Yu. Glebov; J. P. Knauer; F. J. Marshall; C. Stoeckl; W. Theobald
It is shown that direct-drive implosions on the OMEGA laser have achieved core conditions that would lead to significant alpha heating at incident energies available on the National Ignition Facility (NIF) scale. The extrapolation of the experimental results from OMEGA to NIF energy assumes only that the implosion hydrodynamic efficiency is unchanged at higher energies. This approach is independent of the uncertainties in the physical mechanism that degrade implosions on OMEGA, and relies solely on a volumetric scaling of the experimentally observed core conditions. It is estimated that the current best-performing OMEGA implosion [Regan etxa0al., Phys. Rev. Lett. 117, 025001 (2016)10.1103/PhysRevLett.117.025001] extrapolated to a 1.9 MJ laser driver with the same illumination configuration and laser-target coupling would produce 125 kJ of fusion energy with similar levels of alpha heating observed in current highest performing indirect-drive NIF implosions.
Physics of Plasmas | 2017
D.H. Barnak; J.R. Davies; R. Betti; M.J. Bonino; E. M. Campbell; V. Yu. Glebov; D. R. Harding; J. P. Knauer; S. P. Regan; A. B. Sefkow; A. J. Harvey-Thompson; Kyle Peterson; Daniel Brian Sinars; Stephen A. Slutz; M. R. Weis; P.-Y. Chang
Magneto-inertial fusion (MIF) combines the compression of fusion fuel, a hallmark of inertial confinement fusion (ICF), with strongly magnetized plasmas that suppress electron heat losses, a hallmark of magnetic fusion. It can reduce the traditional velocity, pressure, and convergence ratio requirements of ICF. The magnetized liner inertial fusion (MagLIF) concept being studied at the Z Pulsed-Power Facility is a key target concept in the U.S. ICF Program. Laser-driven MagLIF is being developed on OMEGA to test the scaling of MagLIF over a range of absorbed energy of the order of 1u2009kJ on OMEGA to 500u2009kJ on Z. It is also valuable as a platform for studying the key physics of MIF. An energy-scaled point design has been developed for OMEGA that is roughly 10 × smaller in linear dimensions than Z MagLIF targets. A 0.6-mm-outer-diameter plastic cylinder filled with 2.4u2009mg/cm3 of D2 is placed in a ∼10-T axial magnetic field, generated by a Magneto-inertial fusion electrical discharge system, the cylinder is com...
Physics of Plasmas | 2015
A. Bose; K. M. Woo; R. Nora; R. Betti
The scaling of the deceleration phase of inertial fusion direct-drive implosions is investigated for OMEGA and National Ignition Facility (NIF)-size targets. It is shown that the deceleration-phase Rayleigh–Taylor instability (RTI) does not scale hydro-equivalently with implosion size. This is because ablative stabilization resulting from thermal conduction and radiation transport in a spherically converging geometry is different on the two scales. As a consequence, NIF-scale implosions show lower hot-spot density and mass ablation velocity, allowing for higher RTI growth. On the contrary, stabilization resulting from density-gradient enhancement, caused by reabsorption of radiation emitted from the hot spot, is higher on NIF implosions. Since the RTI mitigation related to thermal conduction and radiation transport scale oppositely with implosion size, the degradation of implosion performance caused by the deceleration RTI is similar for NIF and OMEGA targets. It is found that a minimum threshold for the no-α Lawson ignition parameter of χΩ ≈ 0.2 at the OMEGA scale is required to demonstrate hydro-equivalent ignition at the NIF scale for symmetric direct-drive implosions.
Physics of Plasmas | 2017
J.R. Davies; D.H. Barnak; R. Betti; E. M. Campbell; P.-Y. Chang; A. B. Sefkow; Kyle Peterson; Daniel Brian Sinars; M. R. Weis
A laser-driven, magnetized liner inertial fusion (MagLIF) experiment is designed for the OMEGA Laser System by scaling down the Z point design to provide the first experimental data on MagLIF scaling. OMEGA delivers roughly 1000× less energy than Z, so target linear dimensions are reduced by factors of ∼10. Magneto-inertial fusion electrical discharge system could provide an axial magnetic field of 10u2009T. Two-dimensional hydrocode modeling indicates that a single OMEGA beam can preheat the fuel to a mean temperature of ∼200u2009eV, limited by mix caused by heat flow into the wall. One-dimensional magnetohydrodynamic (MHD) modeling is used to determine the pulse duration and fuel density that optimize neutron yield at a fuel convergence ratio of roughly 25 or less, matching the Z point design, for a range of shell thicknesses. A relatively thinner shell, giving a higher implosion velocity, is required to give adequate fuel heating on OMEGA compared to Z because of the increase in thermal losses in smaller targe...
Physics of Plasmas | 2018
A. R. Christopherson; R. Betti; Arijit Bose; J. Howard; K. M. Woo; E. M. Campbell; J. Sanz; B. K. Spears
A comprehensive model is developed to study alpha-heating in inertially confined plasmas. It describes the time evolution of a central low-density hot spot confined by a compressible shell, heated by fusion alphas, and cooled by radiation and thermal losses. The model includes the deceleration, stagnation, and burn phases of inertial confinement fusion implosions, and is valid for sub-ignited targets with ≤10× amplification of the fusion yield from alpha-heating. The results of radiation-hydrodynamic simulations are used to derive realistic initial conditions and dimensionless parameters for the model. It is found that most of the alpha energy (∼90%) produced before bang time is deposited within the hot spot mass, while a small fraction (∼10%) drives mass ablation off the inner shell surface and its energy is recycled back into the hot spot. Of the bremsstrahlung radiation emission, ∼40% is deposited in the hot spot, ∼40% is recycled back in the hot spot by ablation off the shell, and ∼20% leaves the hot ...
Physics of Plasmas | 2017
A. Bose; R. Betti; D. Shvarts; K. M. Woo
The effect of asymmetries on the performance of inertial confinement fusion implosions is investigated. A theoretical model is derived for the compression of distorted hot spots, and quantitative estimates are obtained using hydrodynamic simulations. The asymmetries are divided into low ( l < 6 ) and intermediate ( 6 < l < 40 ) modes by comparison of the mode wavelength with the hot-spot radius and the thermal-diffusion scale length. Long-wavelength modes introduce substantial nonradial motion, whereas intermediate-wavelength modes involve more cooling by thermal losses. It is found that for distorted hot spots, the measured neutron-averaged properties can be very different from the real hydrodynamic conditions. This is because mass ablation driven by thermal conduction introduces flows in the Rayleigh–Taylor bubbles that results in pressure variations, in addition to temperature variations between the bubbles and the neutron-producing region. The differences are less pronounced for long-wavelength asymme...
Review of Scientific Instruments | 2018
D.H. Barnak; J.R. Davies; Gennady Fiksel; P.-Y. Chang; E. Zabir; R. Betti
Magnetized high energy density physics (HEDP) is a very active and relatively unexplored field that has applications in inertial confinement fusion, astrophysical plasma science, and basic plasma physics. A self-contained device, the Magneto-Inertial Fusion Electrical Discharge System, MIFEDS [G. Fiksel et al., Rev. Sci. Instrum. 86, 016105 (2015)], was developed at the Laboratory for Laser Energetics to conduct magnetized HEDP experiments on both the OMEGA [T. R. Boehly et al., Opt. Commun. 133, 495-506 (1997)] and OMEGA EP [J. H. Kelly et al., J. Phys. IV France 133, 75 (2006) and L. J. Waxer et al., Opt. Photonics News 16, 30 (2005)] laser systems. Extremely high magnetic fields are a necessity for magnetized HEDP, and the need for stronger magnetic fields continues to drive the redevelopment of the MIFEDS device. It is proposed in this paper that a magnetic coil that is inductively coupled rather than directly connecting to the MIFEDS device can increase the overall strength of the magnetic field for HEDP experiments by increasing the efficiency of energy transfer while decreasing the effective magnetized volume. A brief explanation of the energy delivery of the MIFEDS device illustrates the benefit of inductive coupling and is compared to that of direct connection for varying coil size and geometry. A prototype was then constructed to demonstrate a 7-fold increase in energy delivery using inductive coupling.
Physics of Plasmas | 2018
K. M. Woo; R. Betti; D. Shvarts; A. Bose; D. Patel; R. Yan; P.-Y. Chang; O.M. Mannion; R. Epstein; J. A. Delettrez; M. Charissis; Karen S. Anderson; P. B. Radha; A. Shvydky; Igor V. Igumenshchev; V. Gopalaswamy; A. R. Christopherson; J. Sanz; H. Aluie
The study of Rayleigh–Taylor instability in the deceleration phase of inertial confinement fusion implosions is carried out using the three-dimensional (3-D) radiation-hydrodynamic Eulerian parallel code DEC3D. We show that the yield-over-clean is a strong function of the residual kinetic energy (RKE) for low modes. Our analytical models indicate that the behavior of larger hot-spot volumes observed in low modes and the consequential pressure degradation can be explained in terms of increasing the RKE. These results are derived using a simple adiabatic implosion model of the deceleration phase as well as through an extensive set of 3-D single-mode simulations using the code DEC3D. The effect of the bulk velocity broadening on ion temperature asymmetries is analyzed for different mode numbers l=1–12. The jet observed in low mode l=1 is shown to cause the largest ion temperature variation in the mode spectrum. The vortices of high modes within the cold bubbles are shown to cause lower ion temperature variat...
Fusion Science and Technology | 2018
S. P. Regan; V.N. Goncharov; T. C. Sangster; E. M. Campbell; R. Betti; Karen S. Anderson; T. Bernat; Arijit Bose; T. R. Boehly; M. J. Bonino; D. Cao; R. Chapman; T.J.B. Collins; R. S. Craxton; A. K. Davis; J. A. Delettrez; D. H. Edgell; R. Epstein; M. Farrell; C.J. Forrest; J. A. Frenje; D. H. Froula; M. Gatu Johnson; C. R. Gibson; V. Yu. Glebov; A. L. Greenwood; D. R. Harding; M. Hohenberger; S. X. Hu; H. Huang
Abstract The goal of the National Direct-Drive Program is to demonstrate and understand the physics of laser direct drive (LDD). Efforts are underway on OMEGA for the 100-Gbar Campaign to demonstrate and understand the physics for hot-spot conditions and formation relevant for ignition at the 1-MJ scale, and on the National Ignition Facility to develop an understanding of the direct-drive physics at long scale lengths for the MJ Direct-Drive Campaign. The strategy of the National Direct-Drive Program is described; the requirements for the deuterium-tritium cryogenic fill-tube target being developed for OMEGA are presented; and preliminary LDD implosion measurements of hydrodynamic mixing seeded by laser imprint, the target-mounting stalk, and microscopic surface debris are reported.