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Bruce Remington

Researcher at Lawrence Livermore National Laboratory

Publications -  433
Citations -  18011

Bruce Remington is an academic researcher from Lawrence Livermore National Laboratory. The author has contributed to research in topics: Laser & National Ignition Facility. The author has an hindex of 68, co-authored 427 publications receiving 16041 citations. Previous affiliations of Bruce Remington include Paul Scherrer Institute.

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Fuel gain exceeding unity in an inertially confined fusion implosion

TL;DR: In this article, the authors report the achievement of fusion fuel gains exceeding unity on the US National Ignition Facility using a high-foot implosion method, which is a manipulation of the laser pulse shape in a way that reduces instability in the implosion.
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Experimental astrophysics with high power lasers and Z pinches

TL;DR: High energy density (HED) laboratory astrophysics as discussed by the authors is a new class of experimental science, wherein the properties of matter and the processes that occur under extreme astrophysical conditions can be examined in the laboratory.
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Similarity Criteria for the Laboratory Simulation of Supernova Hydrodynamics

TL;DR: In this paper, the conditions for the applicability of the Euler equations are formulated, based on the analysis of localization, heat conduction, viscosity, and radiation.
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The National Ignition Facility: Ushering in a new age for high energy density science

TL;DR: The National Ignition Facility (NIF) [E. I. Moses et al. as discussed by the authors, completed in March 2009, is the highest energy laser ever constructed, which enables a number of experiments in inertial confinement fusion and stockpile stewardship, as well as access to new regimes in a variety of experiments relevant to x-ray astronomy, laserplasma interactions, hydrodynamic instabilities, nuclear astrophysics, and planetary science.
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Modeling astrophysical phenomena in the laboratory with intense lasers

TL;DR: In this paper, the authors describe the use of intense laser facilities to test and refine our understanding of phenomena such as supernovae, supernova remnants, gamma-ray bursts, and giant planets.