A Cartesian-diffusion Langevin method for hybrid kinetic-fluid Coulomb scattering in particle-in-cell plasma simulations

Autor: Higginson, Drew P. ^⁎, Link, Anthony J.

Publikováno v: In Journal of Computational Physics 15 May 2022 457

A full-angle Monte-Carlo scattering technique including cumulative and single-event Rutherford scattering in plasmas

Autor: Higginson, Drew P.

Publikováno v: In Journal of Computational Physics 15 November 2017 349:589-603

Thermonuclear neutron emission from a sheared-flow stabilized Z-pinch

Autor: Mitrani, James M, Brown, Joshua A, Goldblum, Bethany L, Laplace, Thibault A, Claveau, Elliot L, Draper, Zack T, Forbes, Eleanor G, Golingo, Ray P, McLean, Harry S, Nelson, Brian A, Shumlak, Uri, Stepanov, Anton, Weber, Tobin R, Zhang, Yue, Higginson, Drew P

Publikováno v: Physics of Plasmas, vol 28, iss 11

The fusion Z-pinch experiment (FuZE) is a sheared-flow stabilized Z-pinch designed to study the effects of flow stabilization on deuterium plasmas with densities and temperatures high enough to drive nuclear fusion reactions. Results from FuZE show h

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https://escholarship.org/uc/item/7nn2m3fz

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Laboratory unraveling of matter accretion in young stars

Autor: Revet, Guilhem, Chen, Sophia N., Bonito, Rosaria, Khiar, Benjamin, Filippov, Evgeny, Argiroffi, Costanza, Higginson, Drew P., Orlando, Salvatore, Béard, Jérôme, Blecher, Marius, Borghesi, Marco, Burdonov, Konstantin, Khaghani, Dimitri, Naughton, Kealan, Pépin, Henri, Portugall, Oliver, Riquier, Raphael, Rodriguez, Rafael, Ryazantsev, Sergei N., Yu. Skobelev, Igor, Soloviev, Alexander, Willi, Oswald, Pikuz, Sergey, Ciardi, Andrea, Fuchs, Julien

Publikováno v: Science Advances
Science Advances, American Association for the Advancement of Science (AAAS), 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩
Science Advances, 2017, 3 (11), pp.e1700982. ⟨10.1126/sciadv.1700982⟩

When matter accretes onto a young star, a shell of dense material can form around the impact, reducing its x-ray emission.
Accretion dynamics in the formation of young stars is still a matter of debate because of limitations in observations and

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=pmid_dedup__::5624936ad8109f593f8558956e6b5589
https://hal-cea.archives-ouvertes.fr/cea-01887635