http://fanyi.youdao.com/ WebSep 9, 2024 · Let $ \Gamma < {\rm{PSL}}_2( \mathbb{C}) $ be a Zariski dense finitely generated Kleinian group. We show all Radon measures on $ {\rm{PSL}}_2( \mathbb{C}) / \Gamma $ which are ergodic and invariant under the action of the horospherical subgroup are either supported on a single closed horospherical orbit or quasi-invariant with respect …
HOLOMORPHIC HOROSPHERICAL TRANSFORM ON …
WebFeb 10, 2024 · On denseness of horospheres in higher rank homogeneous spaces. Let be a connected, semisimple real algebraic group and be a Zariski dense discrete subgroup. Let denote a maximal horospherical subgroup of , and the minimal parabolic subgroup which is the normalizer of . Let denote the unique -minimal subset of and let be a -minimal subset. Web石拋光帶、壓焊鎚。. kinik.com.tw. kinik.com.tw. Incorporating two aspherical lens es, one special. [...] low-dispersion lens, and multiple high-refraction-ratio lenses, this extravagant. … booksmart palm beach state college
LOCAL MIXING AND INVARIANT MEASURES FOR …
WebThe horospherical transform decomposed under T yields the holomorphic spherical Fourier transform. The last step is the inversion of the horospherical Cauchy transform. We give the Radon type inversion formula using results from [14] for the holomorphic discrete series. Let us remark that for X = SL(2,R) WebarXiv:2303.07188v1 [math.DS] 13 Mar 2024 HOROSPHERICAL DYNAMICS IN INVARIANT SUBVARIETIES JOHN SMILLIE, PETER SMILLIE, BARAK WEISS, AND FLORENT YGOUF Abstract. We consider the hor WebCorollary 2.4. The set of horospherical limit points for is invariant under the action of the commensurator group Comm G() on @X. In particular, if = G Z (and Gis de ned over Q), then the set of horospherical limit points for G Z is invariant under the action of G Q on @X. Lemma 2.5. Let Abe a maximal R-split torus of G, x2X= KnG, such that ... booksmart olivia wilde movie