no code implementations • 4 Feb 2021 • A. James, S. Metayer, S. Teber
Hence, the non-trivial IR fixed point is stable with respect to quantum corrections.
High Energy Physics - Theory Strongly Correlated Electrons
no code implementations • 4 Jan 2021 • P. G. J. Irwin, J. Dobinson, A. James, D. Toledo, N. A. Teanby, L. N. Fletcher, G. S. Orton, S. Pérez-Hoyos
We find that away from discrete cloud features, the observed reflectivity spectrum from 800-900 nm is very well approximated by a background cloud model that is latitudinally varying, but zonally symmetric, consisting of a H$_2$S cloud layer, based at 3. 6-4. 7 bar with variable opacity and scale height, and a stratospheric haze.
Earth and Planetary Astrophysics
no code implementations • 22 Jun 2016 • J. Aalbers, F. Agostini, M. Alfonsi, F. D. Amaro, C. Amsler, E. Aprile, L. Arazi, F. Arneodo, P. Barrow, L. Baudis, M. L. Benabderrahmane, T. Berger, B. Beskers, A. Breskin, P. A. Breur, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. Budnik, L. Buetikofer, J. Calven, J. M. R. Cardoso, D. Cichon, D. Coderre, A. P. Colijn, J. Conrad, J. P. Cussonneau, M. P. Decowski, S. Diglio, G. Drexlin, E. Duchovni, E. Erdal, G. Eurin, A. Ferella, A. Fieguth, W. Fulgione, A. Gallo Rosso, P. Di Gangi, A. Di Giovanni, M. Galloway, M. Garbini, C. Geis, F. Glueck, L. Grandi, Z. Greene, C. Grignon, C. Hasterok, V. Hannen, E. Hogenbirk, J. Howlett, D. Hilk, C. Hils, A. James, B. Kaminsky, S. Kazama, B. Kilminster, A. Kish, L. M. Krauss, H. Landsman, R. F. Lang, Q. Lin, F. L. Linde, S. Lindemann, M. Lindner, J. A. M. Lopes, T. Marrodan Undagoitia, J. Masbou, F. V. Massoli, D. Mayani, M. Messina, K. Micheneau, A. Molinario, K. D. Mora, E. Morteau, M. Murra, J. Naganoma, J. L. Newstead, K. Ni, U. Oberlack, P. Pakarha, B. Pelssers, P. de Perio, R. Persiani, F. Piastra, M. C. Piro, G. Plante, L. Rauch, S. Reichard, A. Rizzo, N. Rupp, J. M. F. dos Santos, G. Sartorelli, M. Scheibelhut, S. Schindler, M. Schumann, J. Schreiner, L. Scotto Lavina, M. Selvi, P. Shagin, M. C. Silva, H. Simgen, P. Sissol, M. von Sivers, D. Thers, J. Thurn, A. Tiseni, R. Trotta, C. D. Tunnell, K. Valerius, M. A. Vargas, H. Wang, Y. Wei, C. Weinheimer, T. Wester, J. Wulf, Y. Zhang, T. Zhu, K. Zuber
DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core.
Instrumentation and Methods for Astrophysics High Energy Physics - Experiment Instrumentation and Detectors