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X-WR-CALDESC:Events for INPA
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TZOFFSETFROM:-0800
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DTSTART:20170312T100000
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DTSTART;TZID=America/Los_Angeles:20170113T120000
DTEND;TZID=America/Los_Angeles:20170113T130000
DTSTAMP:20260528T015207
CREATED:20170112T222843Z
LAST-MODIFIED:20170224T202417Z
UID:100-1484308800-1484312400@inpa.lbl.gov
SUMMARY:Initial results from the Majorana Demonstrator - By Alan Poon - LBNL
DESCRIPTION:Neutrinoless double-beta decay experiments play a major role in the search for lepton number violation and the Majorana nature of the neutrino mass. The MAJORANA Collaboration has assembled two modules of high-purity Ge detectors to search for neutrinoless double-beta decay in 76-Ge at the Sanford Underground Research Facility in Lead\, South Dakota. One of the primary goals of the MAJORANA DEMONSTRATOR (MJD) is to establish the required background and scalability of a Ge-based\, next-generation\, tonne-scale experiment. Commissioning of MJD started in 2015 and its two detector modules are taking data. I will discuss the initial results on the search for neutrinoless double-beta decays and dark matter from the commissioning run and the first physics run of Module 1.
URL:https://inpa.lbl.gov/event/initial-results-from-the-majorana-demonstrator-by-alan-poon-lbnl/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
ORGANIZER;CN="Kawana Yancey":MAILTO:kyancey@lbl.gov
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BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20170120T120000
DTEND;TZID=America/Los_Angeles:20170120T130000
DTSTAMP:20260528T015207
CREATED:20170112T221628Z
LAST-MODIFIED:20170117T182607Z
UID:95-1484913600-1484917200@inpa.lbl.gov
SUMMARY:Marcelo Alvarez -Simulating Large Scale Structure Observables from Reionization to the Present
DESCRIPTION:The next generation of large scale structure surveys will map out the universe in unprecedented detail. Transformative techniques in computational astrophysics are emerging as the optimal ways to extract information from these surveys\, with realistic and routine full sky simulations finally within reach. I will describe a new pipeline for efficiently simulating high resolution maps of the sky from the radio to x-ray and from reionization to the present. I will conclude with what questions are likely to be answered in the next decade.
URL:https://inpa.lbl.gov/event/mohammadjavad-vakili-nyu-topic-tba/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
ORGANIZER;CN="Kawana Yancey":MAILTO:kyancey@lbl.gov
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