Zobrazeno 1 - 10
of 13 245
pro vyhledávání: '"Fu, G."'
Autor:
James, R. S., Rule, K., Barberio, E., Bashu, V. U., Bignell, L. J., Bolognino, I., Brooks, G., Chhun, S. S., Dastgiri, F., Duffy, A. R., Froehlich, M., Fruth, T. M. A., Fu, G., Hill, G. C., Janssens, K., Kapoor, S., Lane, G. J., Leaver, K. T., McGee, P., McKie, L. J., McNamara, P. C., McKenzie, J., Melbourne, W. J. D., Mews, M., Milligan, L. J., Mould, J., Nuti, F., Scutti, F., Slavkovska, Z., Spinks, N. J., Stanley, O., Stuchbery, A. E., Suerfu, B., Taylor, G. N., Urquijo, P., Williams, A. G., Xing, Y., Zhong, Y. Y., Zurowski, M. J.
The persistence of the DAMA/LIBRA (DAMA) modulation over the past two decades has been a source of great contention within the dark matter community. The DAMA collaboration reports a persistent, modulating event rate within their setup of NaI(Tl) sci
Externí odkaz:
http://arxiv.org/abs/2408.08697
We have developed a hybrid code GMEC: Gyro-kinetic Magnetohydrodynamics (MHD) Energetic-particle Code that can numerically simulate energetic particle-driven Alfv\'en eigenmodes and energetic particle transport in tokamak plasmas. In order to resolve
Externí odkaz:
http://arxiv.org/abs/2402.14357
A machine learning based surrogate model for fishbone linear instability in tokamaks is constructed. Hybrid simulations with the kinetic-magnetohydrodynamic (MHD) code M3D-K is used to generate the database of fishbone linear instability, through sca
Externí odkaz:
http://arxiv.org/abs/2402.15051
A new magnetohydrodynamics (MHD) code based on initial value approach, GMEC_I, has been developed for simulating various MHD physics in tokamak plasmas, as the MHD foundation of the gyrokinetic-MHD energetic particle simulation code (GMEC) family. GM
Externí odkaz:
http://arxiv.org/abs/2402.09324
An efficient numerical code FP3D has been developed to calculate particle orbits and evaluate particle confinement in 3D magnetic fields including stellarators and tokamaks with 3D fields. The magnetic field is either calculated from coils directly o
Externí odkaz:
http://arxiv.org/abs/2310.08188
Autor:
Lustig-Yaeger, J., Fu, G., May, E. M., Ceballos, K. N. Ortiz, Moran, S. E., Peacock, S., Stevenson, K. B., López-Morales, M., MacDonald, R. J., Mayorga, L. C., Sing, D. K., Sotzen, K. S., Valenti, J. A., Adams, J., Alam, M. K., Batalha, N. E., Bennett, K. A., Gonzalez-Quiles, J., Kirk, J., Kruse, E., Lothringer, J. D., Rustamkulov, Z., Wakeford, H. R.
The critical first step in the search for life on exoplanets over the next decade is to determine whether rocky planets transiting small M-dwarf stars possess atmospheres and, if so, what processes sculpt them over time. Because of its broad waveleng
Externí odkaz:
http://arxiv.org/abs/2301.04191
Publikováno v:
High Temperature Materials and Processes, Vol 29, Iss 1-2, Pp 69-76 (2010)
Externí odkaz:
https://doaj.org/article/f92db1324dd343a7829593c8267979f4
Publikováno v:
International Journal of COPD, Vol Volume 19, Pp 981-993 (2024)
Xiaohua Li,1,* Guoxia Fu,1,* Chunrong Zhang,1,* Yu Wu,2 Hua Guo,1 Weiming Li,1 Xuefeng Zeng1 1Department of Respiratory and Critical Care Medicine, Sixth People’s Hospital of Chengdu, Chengdu, Sichuan, 61005, People’s Republic of Chin
Externí odkaz:
https://doaj.org/article/f92a405f32fc4f62b4f753490126f594
Background: Computationally tractable models of atomic nuclei is a long-time goal of nuclear structure physics. A flexible framework which easily includes excited states and many-body correlations is the configuration-interaction shell model (SM), bu
Externí odkaz:
http://arxiv.org/abs/2208.02079
Autor:
Barberio, E., Baroncelli, T., Bignell, L. J., Bolognino, I., Brooks, G., Dastgiri, F., D'Imperio, G., Di Giacinto, A., Duffy, A. R., Froehlich, M., Fu, G., Gerathy, M. S. M., Hill, G. C., Krishnan, S., Lane, G. J., Lawrence, G., Leaver, K. T., Mahmood, I., Mariani, A., McGee, P., McKie, L. J., McNamara, P. C., Mews, M., Melbourne, W. J. D., Milana, G., Milligan, L. J., Mould, J., Nuti, F., Pettinacci, V., Scutti, F., Slavkovská, Z., Spinks, N. J., Stanley, O., Stuchbery, A. E., Taylor, G. N., Tomei, C., Urquijo, P., Vignoli, C., Williams, A. G., Zhong, Y. Y., Zurowski, M. J.
SABRE (Sodium iodide with Active Background REjection) is a direct detection dark matter experiment based on arrays of radio-pure NaI(Tl) crystals. The experiment aims at achieving an ultra-low background rate and its primary goal is to confirm or re
Externí odkaz:
http://arxiv.org/abs/2205.13849