BEGIN:VCALENDAR
VERSION:2.0
PRODID:-// - ECPv6.18.2//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-ORIGINAL-URL:https://capa.unizar.es
X-WR-CALDESC:Eventos para 
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Madrid
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20180325T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20181028T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20190331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20191027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20200329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20201025T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20210328T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20211031T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20220327T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20221030T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20230326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20231029T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20240331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20241027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20250330T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20251026T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20260329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20261025T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20270328T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20271031T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261021T103000
DTEND;TZID=Europe/Madrid:20261021T120000
DTSTAMP:20261014T095947Z
CREATED:20261002T082622Z
LAST-MODIFIED:20261014T095947Z
UID:2998-1792578600-1792584000@capa.unizar.es
SUMMARY:Seminario Temas Actuales: Any Light Particle Search
DESCRIPTION:Lecturer: Dr. Axel Lindner\, Spokesperson of the ALPS II collaboration at DESY in Hamburg\, Germany \nAbstract: ALPS II at DESY in Hamburg searches for axions — hypothetical particles that could help explain\ndark matter and other mysteries of modern physics. The experiment uses the “light-shining-through-awall” technique: laser light is sent toward a light-tight barrier\, while strong magnetic fields may allow a\ntiny fraction of photons to convert into axions\, pass through the wall\, and reappear as light on the other\nside.\nIn its first science run\, ALPS II excluded photon–axion conversion probabilities down to the 1e-13 level\,\nimproving the sensitivity to the axion–photon coupling strength by about a factor of 20 over previous\nexperiments of this kind. The ongoing upgrade is expected to make ALPS II the first purely laboratorybased experiment to probe beyond existing astrophysical limits on axions.\nAfter the search for new particles\, the ALPS II infrastructure will also be used to study the quantum\nvacuum through magnetic birefringence and\, ultimately\, to search for high-frequency gravitational waves
URL:https://capa.unizar.es/event/seminario/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261020T103000
DTEND;TZID=Europe/Madrid:20261020T123000
DTSTAMP:20261019T070953Z
CREATED:20261019T070850Z
LAST-MODIFIED:20261019T070953Z
UID:3033-1792492200-1792499400@capa.unizar.es
SUMMARY:Defensa de Tesis Doctoral; Cristina Margalejo
DESCRIPTION:Cristina Margalejo defiende su Tesis Doctoral: Searching for solar axions with\nultra-low background Micromegas detectors\nin the IAXO pathfinder system at CAST.
URL:https://capa.unizar.es/event/defensa-de-tesis-doctoral-cristina-margalejo/
LOCATION:Sala de Grados – Edificio A – Facultad de Ciencias\, Zaragoza\, Spain
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261008T120000
DTEND;TZID=Europe/Madrid:20261008T133000
DTSTAMP:20260922T074359Z
CREATED:20260909T084143Z
LAST-MODIFIED:20260922T074359Z
UID:2933-1791460800-1791466200@capa.unizar.es
SUMMARY:Seminario:  The saga of muon tomography at CEA Saclay: from high-energy particle detector developments to societal applications
DESCRIPTION:Abstract: Muon tomography is an imaging technique that exploits the limited flux of natural cosmic-ray muons to probe the interior of large and dense structures. At CEA Saclay\, the development of this technology emerged from detector and electronics technologies originally developed for high-energy particle physics\, and has since evolved towards applications far beyond fundamental physics. \nThis seminar will retrace this technological and scientific journey\, from the development of genetic multiplexed resistive Micromegas detectors to the realization of dedicated muon telescopes. The first MultiGen telescope\, developed within the WatTo project\, demonstrated the potential of muography to probe large-scale structures and subsequently contributed to the ScanPyramids mission\, helping reveal previously unknown structures within the Great Pyramid of Khufu. \nThe talk will then focus on applications in the nuclear field\, including the monitoring of reactors during decommissioning or in the event of an incident\, as well as the inspection of nuclear installations and waste packages where conventional techniques are difficult or impossible to use. \nBeyond these applications\, the seminar will discuss the challenges of technology transfer: detector robustness\, long-term operation\, environmental constraints\, gas management\, data acquisition and analysis. Ultimately\, the story illustrates how technologies born in fundamental physics can become scientific tools for nuclear applications and the exploration of otherwise inaccessible environments. \n  \nSpeaker: David Attié (Institute of Research into the Fundamental Laws of the Universe\, IRFU\, CEA-Saclay\, Francia) \n 
URL:https://capa.unizar.es/event/seminar/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
CATEGORIES:Seminarios
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20261001T120000
DTEND;TZID=Europe/Madrid:20261001T140000
DTSTAMP:20260917T122140Z
CREATED:20260911T094745Z
LAST-MODIFIED:20260917T122140Z
UID:2938-1790856000-1790863200@capa.unizar.es
SUMMARY:Seminario de Temas Actuales-Dark Matter: The LUX-ZEPLIN experiment and an intriguing new dark matter search result
DESCRIPTION:Abstract: The nature of dark matter remains one of the biggest mysteries in modern science. With plenty of different possible candidates and a wide mass range\, Weakly Interactive Massive Particles (WIMPs) usually rises as one of the most promising candidates. The direct detection experiment LUX-ZEPLIN (LZ) primarily searches for WIMPs using 7 tonnes of active liquid xenon at the Sanford Underground Research Facility (South Dakota). With this technology\, LZ has demonstrated world-leading sensitivity to a wide range of dark matter models. A new analysis from LZ searching for effective field theory and inelastic models of dark matter identifies a single nuclear recoil candidate at 248 keV\, in tension with the background-only hypothesis at a global significance of 2.6σ. Whilst this is far from constituting a detection\, the event is nevertheless intriguing. In this seminar\, I will give an overview of the analysis\, discuss the relevant high-energy backgrounds\, and explore the wider implications of the event for dark matter searches. I will also introduce how the LZ detector works and highlight some of the other experiment’s most recent results\, including the observation of solar neutrinos through Coherent Elastic neutrino-Nucleus Scattering and our latest search for more conventional WIMPs. \nAlberto Usón\, Institute for Particle and Nuclear Physics at the School of Physics and Astronomy\, University of Edinburgh
URL:https://capa.unizar.es/event/seminario-de-temas-actuales-dark-matter/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
CATEGORIES:Seminarios
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20260924T121000
DTEND;TZID=Europe/Madrid:20260924T140000
DTSTAMP:20260923T081012Z
CREATED:20260921T125135Z
LAST-MODIFIED:20260923T081012Z
UID:2978-1790251800-1790258400@capa.unizar.es
SUMMARY:Seminario: "New constraints on modified gravity with dimension-six operators from gravitational waves"
DESCRIPTION:Title: “New constraints on modified gravity with dimension-six operators from gravitational waves” \nSpeaker: Carlos Marat Reyes Martínez
URL:https://capa.unizar.es/event/seminario-new-constraints-on-modified-gravity-with-dimension-six-operators-from-gravitational-waves/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20260922T121000
DTEND;TZID=Europe/Madrid:20260922T140000
DTSTAMP:20260917T105529Z
CREATED:20260915T125600Z
LAST-MODIFIED:20260917T105529Z
UID:2945-1790079000-1790085600@capa.unizar.es
SUMMARY:Seminario: Beyond LCDM with future surveys: Rubin LSST\, SKAO and Simons Observatory
DESCRIPTION:Speaker: Chandra Shekhar Sara  (Korea Astronomy and Space Science Institute (KASI)\, Daejeon\, South Korea) \nTitle: Beyond LCDM with future surveys: Rubin LSST\, SKAO and Simons Observatory
URL:https://capa.unizar.es/event/seminario-beyond-lcdm-with-future-surveys-rubin-lsst-skao-and-simons-observatory/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
CATEGORIES:Seminarios
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Madrid:20191015T101000
DTEND;TZID=Europe/Madrid:20191015T111000
DTSTAMP:20260917T105529Z
CREATED:20191009T144633Z
LAST-MODIFIED:20260917T105529Z
UID:126-1571134200-1571137800@capa.unizar.es
SUMMARY:Probing strong dynamics with cosmic neutrinos
DESCRIPTION:Triggered by the IceCube detection of astrophysical neutrino candidates in the range of PeV energies\, we propose to investigate the sensitivity of future South Pole neutrino-detection experiments to the neutrino-nucleon cross section. By using the combination of up- and down-going data of neutrinos\, sensible to neutral current processes one can disentangle particle physics from astrophysics and constrain the neutrino interactions.In particular\, we show that IceCube-Gen2 will be able to determine the neutrino-nucleon cross section with a precisión comparable to the perturbative QCD informed by collider data and eventually to detect new physics. \nPonente: Carlos García Canal (Universidad de la Plata\, Argentina)
URL:https://capa.unizar.es/event/probing-strong-dynamics-with-cosmic-neutrinos/
LOCATION:Seminario de Física Nuclear\, Facultad de Ciencias\, Zaragoza\, Spain
CATEGORIES:Seminarios
ATTACH;FMTTYPE=image/jpeg:https://capa.unizar.es/wp-content/uploads/2019/10/icecube_1.jpg
END:VEVENT
END:VCALENDAR