no code implementations • 2 Feb 2021 • X. Bertou, P. S. Allison, C. Bonifazi, P. Bauleo, C. M. Grunfeld, M. Aglietta, F. Arneodo, D. Barnhill, J. J. Beatty, N. G. Busca, A. Creusot, D. Dornic, A. Etchegoyen. A. Filevitch, P. L. Ghia, I. Lhenry-Yvon, M. C. Medina, E. Moreno, D. Nitz, T. Ohnuki, S. Ranchon, H. Salazar, T. Suomijärvi, D. Supanitsky, A. Tripathi, M. Urban, L. Villasenor
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies ($>10^{19}$ eV).
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics
no code implementations • 22 Dec 2020 • A. K. Rao, A. Tripathi, R. P. Malik
We exploit the theoretical strength of the supervariable and Becchi-Rouet-Stora-Tyutin (BRST) formalisms to derive the proper (i. e. off-shell nilpotent and absolutely anticommuting) (anti-)BRST symmetry transformations for the reparameterization invariant model of a non-relativistic (NR) free particle whose space $(x)$ and time $(t)$ variables are function of an evolution parameter $(\tau)$.
High Energy Physics - Theory
