Zobrazeno 1 - 10
of 1 689
pro vyhledávání: '"Collins, P. R."'
Autor:
Amouretti, A., Crépisson, C., Azadi, S., Cabaret, D., Campbell, T., Chin, D. A., Colin, B., Collins, G. R., Crandall, L., Fiquet, G., Forte, A., Gawne, T., Guyot, F., Heighway, P., Lee, H., McGonegle, D., Nagler, B., Pintor, J., Polsin, D., Rousse, G., Shi, Y., Smith, E., Wark, J. S., Vinko, S. M., Harmand, M.
We present in-situ x-ray diffraction and velocity measurements of Fe$_2$O$_3$ under laser shock compression at pressures between 38-116 GPa. None of the phases reported by static compression studies were observed. Instead, we observed an isostructura
Externí odkaz:
http://arxiv.org/abs/2402.18432
Autor:
Revalski, Mitchell, Crenshaw, D. Michael, Rafelski, Marc, Kraemer, Steven B., Polack, Garrett E., Falcão, Anna Trindade, Fischer, Travis C., Meena, Beena, Martinez, Francisco, Schmitt, Henrique R., Collins, Nicholas R., Falcone, Julia
Active galactic nuclei (AGN) can launch outflows of ionized gas that may influence galaxy evolution, and quantifying their full impact requires spatially resolved measurements of the gas masses, velocities, and radial extents. We previously reported
Externí odkaz:
http://arxiv.org/abs/2203.07387
Autor:
Zen, Andrea, Bui, Tai, Le, Tran Thi Bao, Tay, Weparn J., Chellappah, Kuhan, Collins, Ian R., Rickman, Richard D., Striolo, Alberto, Michaelides, Angelos
Publikováno v:
J. Phys. Chem. C 2022, 126, 18, 8143-8151
The aggregation of clay particles in aqueous solution is a ubiquitous everyday process of broad environmental and technological importance. However, it is poorly understood at the all-important atomistic level since it depends on a complex and dynami
Externí odkaz:
http://arxiv.org/abs/2202.02191
Autor:
Revalski, Mitchell, Meena, Beena, Martinez, Francisco, Polack, Garrett E., Crenshaw, D. Michael, Kraemer, Steven B., Collins, Nicholas R., Fischer, Travis C., Schmitt, Henrique R., Schmidt, Judy, Maksym, W. Peter, Rafelski, Marc
Outflows of ionized gas driven by active galactic nuclei (AGN) may significantly impact the evolution of their host galaxies. However, determining the energetics of these outflows is difficult with spatially unresolved observations that are subject t
Externí odkaz:
http://arxiv.org/abs/2101.06270