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Radek Zlebcik

Publications and source records attributed to Radek Zlebcik.

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Unlocking time-dependent $CP$ violation without signal vertexing at $B$ factories

We present a method to measure time-dependent $CP$ violation in $B^0$ decays produced in $Υ(4S) \to B^0\overline{B}^0$ events at $B$ factories without reconstructing the signal decay vertex. The method exploits the sensitivity of the tag $\overline{B}^0$ decay time to $CP$ violation in the $B^0$ signal. It relies on a compact $e^+e^-$ interaction region and excellent vertex resolution, which enable precise measurement of the displacement between production and decay vertices of the tag meson. We study an application to $B^0\toπ^0π^0$ decays using a simplified simulation that approximates the conditions of the Belle II experiment at the SuperKEKB collider. Our approach achieves a sensitivity on mixing-induced $CP$ violation that would require 20 times larger samples with standard approaches. When incorporated into the $B \to ππ$ isospin analysis, the expected results would reduce the degeneracy of $ϕ_2$ solutions and significantly increase precision. This work opens a path to previously inaccessible $CP$-violation studies enhancing and accelerating the reach of Belle II and future flavor physics programs.

hep-ph

Space-time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology

Solar supergranulation remains a mystery in spite of decades of intensive studies. Most of the papers about supergranulation deal with its surface properties. Local helioseismology provides an opportunity to look below the surface and see the vertical structure of this convective structure. We present a concept of a (3+1)-D segmentation algorithm capable of recognising individual supergranules in a sequence of helioseismic 3-D flow maps. As an example, we applied this method to the state-of-the-art data and derived descriptive statistical properties of segmented supergranules -- typical size of 20--30 Mm, characteristic lifetime of 18.7 hours, and estimated depth of 15--20 Mm. We present preliminary results obtained on the topic of the three-dimensional structure and evolution of supergranulation. The method has a great potential in analysing the better data expected from the helioseismic inversions, which are being developed.

astro-ph.SR