Zobrazeno 1 - 10
of 21
pro vyhledávání: '"T. J. B. Collins"'
Publikováno v:
Frontiers in Physics, Vol 9 (2021)
The dynamic-shell target is a new class of design for inertial confinement fusion (ICF). These targets address some of the target fabrication challenges prevalent in current ICF targets and take advantage of advances in manufacturing technologies. Th
Externí odkaz:
https://doaj.org/article/fd274cd4afaf4b06bc4e7576587c0500
Autor:
Brian M. Haines, D. E. Keller, K. P. Long, M. D. McKay, Z. J. Medin, H. Park, R. M. Rauenzahn, H. A. Scott, K. S. Anderson, T. J. B. Collins, L. M. Green, J. A. Marozas, P. W. McKenty, J. H. Peterson, E. L. Vold, C. Di Stefano, R. S. Lester, J. P. Sauppe, D. J. Stark, J. Velechovsky
Publikováno v:
Physics of Plasmas. 29:083901
Hohlraums are hollow cylindrical cavities with high-Z material walls used to convert laser energy into uniform x-ray radiation drives for inertial confinement fusion capsule implosions and high energy density physics experiments. Credible computation
Autor:
K. M. Woo, R. Betti, C. A. Thomas, C. Stoeckl, K. Churnetski, C. J. Forrest, Z. L. Mohamed, B. Zirps, S. P. Regan, T. J. B. Collins, W. Theobald, R. C. Shah, O. M. Mannion, D. Patel, D. Cao, J. P. Knauer, V. Yu. Glebov, V. N. Goncharov, P. B. Radha, H. G. Rinderknecht, R. Epstein, V. Gopalaswamy, F. J. Marshall, S. T. Ivancic, E. M. Campbell
Publikováno v:
Physics of Plasmas. 29:082705
Three-dimensional effects play a crucial role during the hot-spot formation in inertial confinement fusion (ICF) implosions. A data analysis technique for 3D hot-spot reconstruction from experimental observables has been developed to characterize the
Autor:
T. J. B. Collins, C. Stoeckl, R. Epstein, W. A. Bittle, C. J. Forrest, V. Yu. Glebov, V. N. Goncharov, D. R. Harding, S. X. Hu, D. W. Jacobs-Perkins, T. Z. Kosc, J. A. Marozas, C. Mileham, F. J. Marshall, S. F. B. Morse, P. B. Radha, S. P. Regan, B. Rice, T. C. Sangster, M. J. Shoup, W. T. Shmayda, C. Sorce, W. Theobald, M. D. Wittman
Publikováno v:
Physics of Plasmas. 29:012702
Autor:
S. P. Regan, T. C. Sangster, D. D. Meyerhofer, K. Anderson, R. Betti, T. R. Boehly, T. J. B. Collins, R. S. Craxton, J. A. Delettrez, R. Epstein, O. V. Gotchev, V. Yu. Glebov, V. N. Goncharov, D. R. Harding, P. A. Jaanimagi, J. P. Knauer, S. J. Loucks, L. D. Lund, J. A. Marozas, F. J. Marshall, R. L. Mccrory, P. W. Mckenty, S. F. B. Morse, P. B. Radha, W. Seka, S. Skupsky, H. Sawada, V. A. Smalyuk, J. M. Soures, C. Stoeckl, B. Yaakobi, J. A. Frenje, C. K. Li, R. D. Petrasso, F. H. SÉguin
Publikováno v:
Astrophysics and Space Science. 298:227-233
Autor:
J. P. Knauer, Terrance J. Kessler, T. R. Boehly, T. J. B. Collins, D. D. Meyerhofer, O. V. Gotchev, T. C. Sangster
Publikováno v:
Journal of Applied Physics. 92:1212-1215
The growth of surface perturbations due to nonuniformities in the drive laser is an important subject in laser–matter interactions. We present results of experiments using drive lasers with known, single-mode modulations to produce nonuniform shock
Autor:
T. J. B. Collins, S. Skupsky
Publikováno v:
Physics of Plasmas. 9:275-281
A novel technique for reducing laser imprint in OMEGA [T. R. Boehly et al., Opt. Commun. 133, 495 (1997)] cryogenic targets has been developed. A typical direct-drive inertial confinement fusion target consists of a shell of deuterium–tritium ice w
Publikováno v:
The Astrophysical Journal. 534:944-966
We present the results of a linearized perturbation analysis for the models of cataclysmic variable (CV) disks and their boundary layers (BLs), discussed in a previous companion paper. For the case of large-scale, azimuthal oscillations in the BL, we
Publikováno v:
The Astrophysical Journal. 534:934-943
We consider numerical models of accretion disks and boundary layers (BLs) around white dwarfs in cataclysmic variables (CVs). Our models include the effects of the radial viscous force and are created using the realistic OPAL opacities. We present th
Publikováno v:
The Astrophysical Journal. 512:322-331
In this paper we provide a possible link between the structure of the bipolar nebula surrounding SN 1987A and the properties of its progenitor star. A wind-blown bubble (WBB) scenario is employed in which a fast, tenuous wind from a blue supergiant e