BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:The status and prospects of the muon g-2 DTSTART;VALUE=DATE-TIME:20200709T140000Z DTEND;VALUE=DATE-TIME:20200709T144000Z DTSTAMP;VALUE=DATE-TIME:20260627T162825Z UID:indico-contribution-2-0-121@cern.ch DESCRIPTION:Speakers: MASJUAN\, Pere ()\nhttps://indico.nucleares.unam.mx/ event/1546/session/2/contribution/121 LOCATION:Mexico City Virtual URL:https://indico.nucleares.unam.mx/event/1546/session/2/contribution/121 END:VEVENT BEGIN:VEVENT SUMMARY:The HAWC sky survey at the highest photon energies DTSTART;VALUE=DATE-TIME:20200709T144500Z DTEND;VALUE=DATE-TIME:20200709T150200Z DTSTAMP;VALUE=DATE-TIME:20260627T162825Z UID:indico-contribution-2-0-155@cern.ch DESCRIPTION:Speakers: Dr. CARRAMINANA\, Alberto (INAOE)\nAt 4100m\, from t he privileged site of Sierra Negra\, the HAWC gamma-ray observatory has be en surveying 2/3 of the sky\, between declinations -26 and +64. With 1523 days of live data\, HAWC has now the deepest unbiased view of most of the Northern sky\, in particular along the Galactic Plane\, including the anti -center region\, as well as constant monitoring of active galactic nuclei. Sources have been detected at photon energies beyond 100 TeV\, pointing t o Galactic accelerators of cosmic rays up to 1 PeV. These observations pro vide also tests on fundamental physics\, like potential Lorentz Invariance violations.\n\nhttps://indico.nucleares.unam.mx/event/1546/session/2/cont ribution/155 LOCATION:Mexico City Virtual URL:https://indico.nucleares.unam.mx/event/1546/session/2/contribution/155 END:VEVENT BEGIN:VEVENT SUMMARY:Potential of MATHUSLA for cosmic ray research DTSTART;VALUE=DATE-TIME:20200709T150500Z DTEND;VALUE=DATE-TIME:20200709T152200Z DTSTAMP;VALUE=DATE-TIME:20260627T162825Z UID:indico-contribution-2-0-164@cern.ch DESCRIPTION:Speakers: Dr. ARTEAGA VELAZQUEZ\, Juan Carlos (Instituto de F ísica y Matemáticas\, Universidad Michoacana)\nThe main objective behind the MATHUSLA proposal is to build a large area hodoscope detector at grou nd level\, close to the interaction point of the CMS detector\, to look f or the decay signals of neutral long lived particles (LLP) at the next HL- LHC runs in an environment with low background. LLPs are expected in the c ontext of Beyond Standard Models\, which try to solve open problems in fun damental particle physics. The idea behind MATHUSLA is to monitor a large volume of air (100 m x 100 m x 25 m) with a series of layers of tracking detectors to look for displayed vertices produced by the LLPs. The updated MATHUSLA design considers extruded scintillators for the tracking detecto rs. However\, it has been also considered to add an extra layer of RPCs to enhance the extensive air shower detection capabilities of MATHUSLA to c arry out cosmic ray studies in the 100 TeV - 100 PeV regime. In this talk\ , a brief introduction to MATHUSLA will be presented\, with an emphasis on its sensitivity to cosmic ray detection. A comparison of its performance with that of other present and future cosmic ray facilities working in the same energy range as MATHUSLA will also be shown.\n\nhttps://indico.nucle ares.unam.mx/event/1546/session/2/contribution/164 LOCATION:Mexico City Virtual URL:https://indico.nucleares.unam.mx/event/1546/session/2/contribution/164 END:VEVENT BEGIN:VEVENT SUMMARY:Initial development of a control system for the FDD detector in th e ALICE experiment for operation on LHC Run-3 DTSTART;VALUE=DATE-TIME:20200709T152500Z DTEND;VALUE=DATE-TIME:20200709T154200Z DTSTAMP;VALUE=DATE-TIME:20260627T162825Z UID:indico-contribution-2-0-171@cern.ch DESCRIPTION:Speakers: Mr. MEJIA CAMACHO\, Juan Manuel (National Technologi cal of Mexico)\nThe selection of diffraction events in ALICE is limited by the range over which speed gaps could be detected. Thus\, it is possible to achieve better measurements by extending the range of directions in whi ch the production of particles (or their absence) can be detected. The stu dy of diffractive events with ALICE experiment of the Large Hadron Collide r (LHC) in proton-proton (pp)\, lead-lead (Pb-Pb)\, and proton-lead (p-Pb) collisions could improve its efficiency with the installation of the FDD (Fast Interaction Trigger Diffractive) detector for Run-3\, since such det ector will increase the time resolution compared to AD (ALICE diffractive) detector used in Run-2. The proposal of this work is the initial developm ent of a control system (DCS\, Detector Control System) for the new FDD de tector and its integration in the ALICE experiment\, according to the rule s of the new Online-Offline (O2) infrastructure for Run-3 of the LHC\, by using the SCADA system (Supervisory Control and Data Acquisition) called W inCC-OA. This proposal will allow the DCS of FDD detector to have an optim al performance in the physical data acquisition runs\, mainly. This perfor mance can be quantitatively assessed by estimating and comparing the param eters such as: number and duration of runs\, Data Taking Efficiency (DTE)\ , End Of Runs (EOR) and Pause And Reconfiguration (PAR)\; with respect to the other detectors and systems of the experiment.\n\nhttps://indico.nucle ares.unam.mx/event/1546/session/2/contribution/171 LOCATION:Mexico City Virtual URL:https://indico.nucleares.unam.mx/event/1546/session/2/contribution/171 END:VEVENT END:VCALENDAR