Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Seth Root"'
Autor:
Sakun Duwal, Chad A. McCoy, Daniel H. Dolan III, Cody A. Melton, Marcus D. Knudson, Seth Root, Richard Hacking, Bernardo Farfan, Christopher Johnson, C. Scott Alexander, Christopher T. Seagle
Publikováno v:
Scientific Reports, Vol 12, Iss 1, Pp 1-13 (2022)
Abstract Lattice and electronic structure interactions for f-electrons are fundamental challenges for lanthanide equation of state development. Difficulties in first-principles calculations, such as density functional theory (DFT), emphasize the need
Externí odkaz:
https://doaj.org/article/d8ea65f9cf4a4d94846094a37d5c72be
Autor:
Seth Root, Chad A. McCoy, Kyle R. Cochrane, John H. Carpenter, Raymond W. Lemke, Luke Shulenburger, Thomas R. Mattsson, Philip A. Sterne
Publikováno v:
Physical Review B. 106
Autor:
Sarah Stewart, Josh Townsend, Dylan Spaulding, Seth Root, Patricia Kalita, Stein Jacobsen, Margaret Huff, Megan Harwell, Dayne Fratanduono, Erik Davies, Razvan Caracas, James Badro, Marius Millot, Bethany Chidester
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a27723c7d96e97a5d149a5469fb5720d
https://doi.org/10.26226/m.62a9d1f09deaf4fdb6b3fee3
https://doi.org/10.26226/m.62a9d1f09deaf4fdb6b3fee3
Autor:
D. K. Spaulding, Stein B. Jacobsen, Seth Root, E. J. Davies, M. S. Duncan, R. G. Kraus, Sarah T. Stewart
Publikováno v:
Journal of Geophysical Research. Planets
The physical processes during planet formation span a large range of pressures and temperatures. Giant impacts, such as the one that formed the Moon, achieve peak pressures of 100s of GPa. The peak shock states generate sufficient entropy such that s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb688269c82d695ff5c22842dbf10bf9
https://hdl.handle.net/10919/104456
https://hdl.handle.net/10919/104456
Publikováno v:
Physical Review B. 102
The equation of state (EOS) and shock compression of bulk vanadium were investigated using canonical ab initio molecular dynamic simulations, with experimental validation to 865 GPa from shock data collected at Sandia's Z Pulsed Power Facility. In si
Autor:
Sarah T. Stewart, M. S. Duncan, Seth Root, Stein B. Jacobsen, Simon J. Lock, E. J. Davies, Razvan Caracas, Richard Kraus, Joshua P. Townsend
We discuss major challenges in modeling giant impacts between planetary bodies, focusing on the equations of state (EOS). During the giant impact stage of planet formation, rocky planets are melted and partially vaporized. However, most EOS models fa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24622f13f5b8536cda9a58904956865a
https://resolver.caltech.edu/CaltechAUTHORS:20201105-094348685
https://resolver.caltech.edu/CaltechAUTHORS:20201105-094348685
Publikováno v:
Physical Review B. 102
We report the atomic- and nanosecond-scale quantification of kinetics of a shock-driven phase transition in Zr metal. We uniquely make use of a multiple shock-and-release loading pathway to shock Zr into the $\ensuremath{\beta}$ phase and to create a
Autor:
Philippe F. Weck, C. A. McCoy, Heath L. Hanshaw, Seth Root, Patricia Kalita, Sakun Duwal, Tommy Ao, Kyle Robert Cochrane
Publikováno v:
Physical Review B. 102
The high-pressure response of titanium dioxide (${\mathrm{TiO}}_{2}$) is of interest because of its numerous industrial applications and its structural similarities to silica (${\mathrm{SiO}}_{2}$). We used three platforms---Sandia's Z machine, Omega
Direct observations of shock-induced melting in a porous solid using time-resolved x-ray diffraction
Publikováno v:
Physical Review Materials. 4
In this work we provide direct evidence of shock-induced melting and associated kinetics in a porous solid (aluminum powder) using time-resolved x-ray diffraction. Unambiguous evidence of melting in 50% porous aluminum (Al) powder samples, shocked to