Zobrazeno 1 - 10
of 142
pro vyhledávání: '"J R Rygg"'
Autor:
C K Li, A B Zylstra, J A Frenje, F H Séguin, N Sinenian, R D Petrasso, P A Amendt, R Bionta, S Friedrich, G W Collins, E Dewald, T Döppner, S H Glenzer, D G Hicks, O L Landen, J D Kilkenny, A J Mackinnon, N Meezan, J Ralph, J R Rygg, J Kline, G Kyrala
Publikováno v:
New Journal of Physics, Vol 15, Iss 2, p 025040 (2013)
Energy spectra and spectrally resolved one-dimensional fluence images of self-emitted charged-fusion products (14.7 MeV D ^3 He protons) are routinely measured from indirectly driven inertial-confinement fusion (ICF) experiments utilizing ignition-sc
Externí odkaz:
https://doaj.org/article/9cb34e5e1ee94a2b87f9e34cdf700079
Autor:
D. Kim, R. F. Smith, I. K. Ocampo, F. Coppari, M. C. Marshall, M. K. Ginnane, J. K. Wicks, S. J. Tracy, M. Millot, A. Lazicki, J. R. Rygg, J. H. Eggert, T. S. Duffy
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-9 (2022)
Using ramp compression, silicon carbide was compressed to pressures of 1.5 terapascals, more than seven times higher than previous work. The results show that large carbon-rich exoplanets would be ~10% less dense than corresponding rocky planets.
Externí odkaz:
https://doaj.org/article/1fabdd63f8b34131b959de6f8ec88967
Publikováno v:
Physical Review Letters. 130
Autor:
P. Davis, T. Döppner, J. R. Rygg, C. Fortmann, L. Divol, A. Pak, L. Fletcher, A. Becker, B. Holst, P. Sperling, R. Redmer, M. P. Desjarlais, P. Celliers, G. W. Collins, O. L. Landen, R. W. Falcone, S. H. Glenzer
Publikováno v:
Nature Communications, Vol 7, Iss 1, Pp 1-8 (2016)
High-pressure experiments play a critical role in understanding planetary interiors, but are notoriously difficult to carry out. Here, the authors demonstrate a laboratory platform for the controlled exploration of deuterium, with results that challe
Externí odkaz:
https://doaj.org/article/00816916d4454912bc4c4bf63a4c3421
Autor:
X. Gong, D. N. Polsin, R. Paul, B. J. Henderson, J. H. Eggert, F. Coppari, R. F. Smith, J. R. Rygg, G. W. Collins
Publikováno v:
Physical Review Letters. 130
Autor:
G. Bruhaug, M. S. Freeman, H. G. Rinderknecht, L. P. Neukirch, C. H. Wilde, F. E. Merrill, J. R. Rygg, M. S. Wei, G. W. Collins, J. L. Shaw
Publikováno v:
Scientific Reports. 13
Contact and projection electron radiography of static targets was demonstrated using a laser–plasma accelerator driven by a kilojoule, picosecond-class laser as a source of relativistic electrons with an average energy of 20 MeV. Objects with areal
Autor:
F. Coppari, D. E. Fratanduono, M. Millot, R. G. Kraus, A. Lazicki, J. R. Rygg, R. F. Smith, J. H. Eggert
Publikováno v:
Physical Review B. 106
Autor:
M. G. Gorman, S. Elatresh, A. Lazicki, M. M. E. Cormier, S. A. Bonev, D. McGonegle, R. Briggs, A. L. Coleman, S. D. Rothman, L. Peacock, J. V. Bernier, F. Coppari, D. G. Braun, J. R. Rygg, D. E. Fratanduono, R. Hoffmann, G. W. Collins, J. S. Wark, R. F. Smith, J. H. Eggert, M. I. McMahon
Publikováno v:
Gorman, M G, Elatresh, S, Lazicki, A, Cormier, M M E, Bonev, S A, McGonegle, D, Briggs, R, Coleman, A L, Rothman, S D, Peacock, L, Bernier, J V, Coppari, F, Braun, D G, Rygg, J R, Fratanduono, D E, Hoffmann, R, Collins, G W, Wark, J S, Smith, R F, Eggert, J H & McMahon, M I 2022, ' Experimental observation of open structures in elemental magnesium at terapascal pressures ', Nature Physics, vol. 18, no. 11, pp. 1307-1311 . https://doi.org/10.1038/s41567-022-01732-7
Investigating how solid matter behaves at enormous pressures, such as those found in the deep interiors of giant planets, is a great experimental challenge. Over the past decade, computational predictions have revealed that compression to terapascal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d49dec3df572fd9c4341dd1b39725d28
https://www.pure.ed.ac.uk/ws/files/301689202/s41567_022_01732_7.pdf
https://www.pure.ed.ac.uk/ws/files/301689202/s41567_022_01732_7.pdf
Autor:
J. R. Rygg, Marius Millot, Peter M. Celliers, Paul Loubeyre, Raymond Jeanloz, Gilbert Collins, Stephanie Brygoo, Jon Eggert
Publikováno v:
Nature. 593:517-521
The phase behaviour of warm dense hydrogen-helium (H-He) mixtures affects our understanding of the evolution of Jupiter and Saturn and their interior structures1,2. For example, precipitation of He from a H-He atmosphere at about 1-10 megabar and a f
Autor:
Federica Coppari, Raymond F. Smith, J. R. Rygg, D. Kim, Jue Wang, Marius Millot, Sebastien Hamel, Jon Eggert, Thomas S. Duffy
Publikováno v:
Nature Geoscience. 14:121-126
The discovery of an extraordinary number of extrasolar planets, characterized by an unexpected variety of sizes, masses and orbits, challenges our understanding of the formation and evolution of the planets in the Solar System and the perception of t