Zobrazeno 1 - 10
of 1 064
pro vyhledávání: '"Gautier D"'
Publikováno v:
Results in Physics, Vol 54, Iss , Pp 107064- (2023)
The Maxwell equations in Weyl semimetals (WSMs) with broken inversion and time-reversal symmetries are modified by the presence of the axion terms b and b0 where, for a simple two-node model, 2ℏb is the vector that connects the two nodes in momentu
Externí odkaz:
https://doaj.org/article/9003c3008d9e49e3baf5af7f602d96ce
The simplest Weyl semimetal with broken time-reversal symmetry consists of a pair of Weyl nodes located at wave vectors $\mathbf{K}_{\tau }=\tau \mathbf{b}$ in momentum space with $\tau =\pm 1$ the node index and chirality. The electronic dispersion
Externí odkaz:
http://arxiv.org/abs/2407.01807
Autor:
Vogel Sven C., Fernandez Juan C., Gautier D. Cort, Mitura Nikodem, Roth Markus, Schoenberg Kurt F.
Publikováno v:
EPJ Web of Conferences, Vol 231, p 01008 (2020)
Neutron production with laser-driven neutron sources was demonstrated. We outline the basics of laser-driven neutron sources, highlight some fundamental advantages, and quantitatively compare the neutron production at the TRIDENT laser sources with t
Externí odkaz:
https://doaj.org/article/7d759b293e524740882f524fcfc017dc
In Weyl semimetals with broken inversion and time-reversal symmetries, the Maxwell equations are modified by the presence of the axion terms $\mathbf{b} $ and $b_{0}$ where, in the simplest case of a two-node Weyl semimetal, $% 2\hslash \mathbf{b}$ i
Externí odkaz:
http://arxiv.org/abs/2304.01044
Autor:
Miglior, F., author, Pinotti, L., author, Boyle, L., author, Kenny, D., author, Lee, M., author, De Marchi, M., author, Cadavez, V.A.P., author, Millet, S., author, Evans, R., author, Veldkamp, T., author, Pastell, M., author, Pollott, G., author, Spoolder, H., author, Fischer, A., author, Deleau, D., author, Depuille, L., author, Dufour, G., author, Fauviot, S., author, Gautier, D., author, Huneau, T., author, Lerond, C., author, Mangin, P., author, Merle, L.A., author, Philibert, A., author, Thudor, A.S., author, Jomier, A., author, Lebreton, A., author
Publikováno v:
Book of Abstracts of the 73rd Annual Meeting of the European Federation of Animal Science. :396-396
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We measured the response of BAS-TR imaging plate (IP) to energetic aluminum ions in the 0 to 222 MeV energy range, and compared it with predictions from a Monte Carlo simulation code using two different IP models. Energetic aluminum ions were produce
Externí odkaz:
http://arxiv.org/abs/1912.10174
Autor:
Mousis, O., Atkinson, D. H., Spilker, T., Venkatapathy, E., Poncy, J., Frampton, R., Coustenis, A., Reh, K., Lebreton, J. -P., Fletcher, L. N., Hueso, R., Amato, M. J., Colaprete, A., Ferri, F., Stam, D., Wurz, P., Atreya, S., Aslam, S., Banfield, D. J., Calcutt, S., Fischer, G., Holland, A., Keller, C., Kessler, E., Leese, M., Levacher, P., Morse, A., Munoz, O., Renard, J. -B., Sheridan, S., Schmider, F. -X., Snik, F., Waite, J. H., Bird, M., Cavalié, T., Deleuil, M., Fortney, J., Gautier, D., Guillot, T., Lunine, J. I., Marty, B., Nixon, C., Orton, G. S., Sanchez-Lavega, A.
The Hera Saturn entry probe mission is proposed as an M--class mission led by ESA with a contribution from NASA. It consists of one atmospheric probe to be sent into the atmosphere of Saturn, and a Carrier-Relay spacecraft. In this concept, the Hera
Externí odkaz:
http://arxiv.org/abs/1510.07685
Autor:
Jung, D., Yin, L., Albright, B. J., Gautier, D. C., Dromey, B., Shah, R., Palaniyappan, S., Letzring, S., Wu, H. -C., Shimada, T., Johnson, R. P., Habs, D., Roth, M., Fernandez, J. C., Hegelich, B. M.
Laser-driven ions have compelling properties and their potential use for medical applications has attracted a huge global interest. One of the major challenges of these applications is generating beams of the required energies. To date, there has bee
Externí odkaz:
http://arxiv.org/abs/1406.0656
Autor:
Mousis, O., Fletcher, L. N., Lebreton, J. -P., Wurz, P., Cavalié, T., Coustenis, A., Courtin, R., Gautier, D., Helled, R., Irwin, P. G. J., Morse, A. D., Nettelmann, N., Marty, B., Rousselot, P., Venot, O., Atkinson, D. H., Waite, J. H., Reh, K. R., Simon-Miller, A., Atreya, S., André, N., Blanc, M., Daglis, I. A., Fischer, G., Geppert, W. D., Guillot, T., Hedman, M. M., Hueso, R., Lellouch, E., Lunine, J. I., Murray, C. D., O'Donoghue, J., Rengel, M., Sanchez-Lavega, A., Schmider, F. -X., Spiga, A., Spilker, T., Petit, J. -M., Tiscareno, M. S., Ali-Dib, M., Altwegg, K., Bouquet, A., Briois, C., Fouchet, T., Guerlet, S., Kostiuk, T., Lebleu, D., Moreno, R., Orton, G. S., Poncy, J.
Remote sensing observations meet some limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. A remarkable example of the superiority of in situ probe measurements is illustrated by the exploration of
Externí odkaz:
http://arxiv.org/abs/1404.4811