胶状 发表于 2025-3-23 12:29:10
S. M. Mayer,D. M. Lawson,C. A. Gormal,S. M. Roe,B. E. Smithion gives in general a family of partial differential equations with invariant solution variety. Throughout this article we will call the corresponding partial differential operators also . in this case. For .(.) this family contains the Schrödinger operator.出血 发表于 2025-3-23 14:19:03
http://reply.papertrans.cn/67/6667/666676/666676_12.pngBRINK 发表于 2025-3-23 21:01:02
http://reply.papertrans.cn/67/6667/666676/666676_13.pngcogitate 发表于 2025-3-23 23:09:35
http://reply.papertrans.cn/67/6667/666676/666676_14.png易碎 发表于 2025-3-24 02:43:14
http://reply.papertrans.cn/67/6667/666676/666676_15.png低位的人或事 发表于 2025-3-24 08:44:59
G. J. Leigh,R. L. Richardsimensional linear space. The approaches mentioned above are not satisfactory for such definition. Besides, when considering representations of the quantum groups ..(.1) and ..(.,1) we are interested in reducing them onto the quantum subgroup ..(.). This reduction would give the analog of the Gel’fanBUDGE 发表于 2025-3-24 12:23:48
C. J. Pickett,Steven P. Best,Thierry LeGalll,C. A. Gormall,S. K. Ibrahim,B. E. Smith,Kylie Vincentphysical conclusions are drawn, based upon the internal relationships of the various subalgebras which are assigned physical meaning. The Dirac γ matrices are shown to carry, as “operator states”, the 4-dimensional vector representation of .(4). Differential operator realizations are obtained on the打火石 发表于 2025-3-24 14:54:54
http://reply.papertrans.cn/67/6667/666676/666676_18.pngHPA533 发表于 2025-3-24 21:07:04
T. A. Bazhenova,M. A. Bazhenova,G. N. Petrova,A. E. Shilovn the neutrino sector and others. These results are comfortably competitive to corresponding results from high-energy accelerators like TEVATRON, HERA, etc. One of the enriched .Ge detectors also yields the most-stringent limits for cold dark matter (WIMPs) to date by using raw data. Second, futureforthy 发表于 2025-3-25 01:45:18
Masanobu Hidaiations between three neutrinos yields, together with the result of supersymmetry, that the third neutrino mass lies between 2 × 10. and 10. eV. The two lightest neutrino masses are in supersymmetry on the tree level zero. The averaged electron neutrino mass which is the essential parameter in the ne