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SUMMARY:Search for neutrinoless double beta decay with CUORICINO and persp
 ectives for CUORE
DTSTART;VALUE=DATE-TIME:20070705T170500Z
DTEND;VALUE=DATE-TIME:20070705T171700Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-204@cern.ch
DESCRIPTION:Speakers: Dr. GUARDINCERRI\, Elena (LBNL)\nCUORICINO is a cryo
 genic detector running in Gran Sasso National Laboratories\, Italy\nsince 
 2003.\nWith its 40.7 kg  of 130TeO2 mass\, in the form of an array of 62 c
 rystals it has\nproved the feasibility of CUORE experiment\, whose aim is 
 to be sensitive to value of\nthe effective neutrino mass as low as few ten
 s of meV.\nIt has moreover set the currently lower limit on the lifetime o
 f 130Te for\nneutrinoless double beta decay: we will report on the up-to d
 ate CUORICINO results\nand discuss the perspectives for CUORE.\n\nhttps://
 indico.nucleares.unam.mx/event/4/session/54/contribution/204
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/204
END:VEVENT
BEGIN:VEVENT
SUMMARY:Constraints on Quantum Gravity effects from a fast AGN flare
DTSTART;VALUE=DATE-TIME:20070705T171700Z
DTEND;VALUE=DATE-TIME:20070705T172900Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-592@cern.ch
DESCRIPTION:Speakers: BILAND\, A. (ETH Zurich\, Switzerland)\nIn 2005\, th
 e MAGIC telescope observed an unprecedented rapid flare from the AGN Mrk\n
 501. A fast and strong variability was found in several  adjacent energy b
 ands above\n100 GeV and was used to search for correlated flux variations 
 at different energies.\n\nThe resulting constraints on different possible 
 Quantum Gravity effects have been\ninvestigated and will be presented.\n\n
 https://indico.nucleares.unam.mx/event/4/session/54/contribution/592
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/592
END:VEVENT
BEGIN:VEVENT
SUMMARY:UPPER FLUX LIMITS FOR MASSIVE RARE PARTICLES WITH THE SLIM EXPERIM
 ENT
DTSTART;VALUE=DATE-TIME:20070705T172900Z
DTEND;VALUE=DATE-TIME:20070705T174100Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-608@cern.ch
DESCRIPTION:Speakers: Dr. CECCHINI\, stefano (INFN and INAF/IASF)\nThe sea
 rch for rare massive particles in the cosmic radiation remains one of the 
 main aim of non-accelerator particle \nastrophysics. Experiments at high a
 ltitude allow lower mass thresholds with respect to detectors at sea level
  or \nunderground. We present here the analysis of the full SLIM detector 
 (400 m^2) after 4y exposure at the \nChacaltaya site (5300m a.s.l.). A par
 t is devoted to the study carried out for defining the most efficient etch
 ing \nconditions and calibrations of the NT detectors. WE also compare our
  results for Magnetic Monopoles with masses in \nthe range 10^5 – 10^12 
 GeV with existing and future experiments. Our experiment is also sensitive
  to SQM \nnuggets and Q-balls and we discuss the implications of our obser
 vations on the characteristics of these Dark Matter \ncandidates.\n\nhttps
 ://indico.nucleares.unam.mx/event/4/session/54/contribution/608
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/608
END:VEVENT
BEGIN:VEVENT
SUMMARY:Searches for  gravitational wave bursts with  LIGO
DTSTART;VALUE=DATE-TIME:20070705T174100Z
DTEND;VALUE=DATE-TIME:20070705T175300Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-850@cern.ch
DESCRIPTION:Speakers: Dr. DESAI\, Shantanu (Pennsylvania State University)
 \nLaser Interferometer Gravitational Wave Observatory (LIGO) consists of  
                                              \nthree detectors\, located i
 n Hanford\, Washington and Livingston\, Louisiana\,                       
                     \nwhich are designed to search for gravitational waves
  from astrophysical                                              \nsources
 . In November 2005\, LIGO started collecting coincident data at           
                                      \ndesign sensitivity. One of the data
  analysis efforts is aimed at searching                                   
         \nfor short-duration transient signals with unmodeled waveforms\, 
 known as                                              \nbursts. Examples o
 f burst sources include core-collapse supernova\, binary                  
                           \nblack hole mergers\, and cosmic string cusps. 
 Two types of burst searches                                             \n
 are currently being conducted within the LIGO Scientific Collaboration.   
                                            \nIn an untriggered approach\, 
 we perform an all-sky search from all possible    \nsources. In a triggere
 d approach\, we look for signals from known transient                     
                       \nelectromagnetic sources such as gamma-ray bursts o
 r soft gamma-ray                                                   \nrepea
 ters. Recent results from these types of searches for gravitational       
                                       \nwave bursts will be presented.\n\n
 https://indico.nucleares.unam.mx/event/4/session/54/contribution/850
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/850
END:VEVENT
BEGIN:VEVENT
SUMMARY:Search for Relativistic Magnetic Monopoles with AMANDA-II
DTSTART;VALUE=DATE-TIME:20070705T175300Z
DTEND;VALUE=DATE-TIME:20070705T180500Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-870@cern.ch
DESCRIPTION:Speakers: WISSING\, Henrike (RWTH-Aachen)\nCherenkov emissions
  of magnetic charges moving through matter will exceed those of\nelectric 
 charges by several orders of magnitude. The AMANDA neutrino telescope is\n
 therefore capable of efficiently detecting relativistic magnetic monopoles
  that pass\nthrough its sensitive volume. We present a new limit on the fl
 ux of relativistic\nmagnetic monopoles based on the analysis of one\nyear 
 of data taken with AMANDA-II. In contrast to previous analyses\, which wer
 e\nrestricted to monopoles entering from below the horizon\, we also consi
 der monopoles\nentering from above. The search for down-going monopoles ha
 s a lower mass-threshold\,\nsince lighter monopoles could penetrate the li
 mited overburden above the detector.\n\nhttps://indico.nucleares.unam.mx/e
 vent/4/session/54/contribution/870
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/870
END:VEVENT
BEGIN:VEVENT
SUMMARY:Subrelativistic Particle Searches with AMANDA
DTSTART;VALUE=DATE-TIME:20070705T180500Z
DTEND;VALUE=DATE-TIME:20070705T181700Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-970@cern.ch
DESCRIPTION:Speakers: Mr. POHL\, Arvid (Uppsala University)\nSupermassive 
 particles like magnetic monopoles\, Q-balls and nuclearites may \nemit lig
 ht at subrelativistic speeds through different suggested mechanisms. \nOne
  of them is nucleon decay catalysis by magnetic monopoles\, where the \nde
 cay products would emit Cherenkov radiation along a monopole track. The \n
 emitted secondary light from subrelativistic particles could make them vis
 ible to \nthe AMANDA-II neutrino telescope\, depending on the resulting lu
 minosity. We \npresent first experimental results from searches with AMAND
 A-II for events \nof this type.\n\nhttps://indico.nucleares.unam.mx/event/
 4/session/54/contribution/970
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/970
END:VEVENT
BEGIN:VEVENT
SUMMARY:Search for Short Bursts of Gamma Rays with SGARFACE
DTSTART;VALUE=DATE-TIME:20070705T181700Z
DTEND;VALUE=DATE-TIME:20070705T182900Z
DTSTAMP;VALUE=DATE-TIME:20260615T113638Z
UID:indico-contribution-54-0-370@cern.ch
DESCRIPTION:Speakers: SCHROEDTER\, M (Iowa State University)\nThe Short GA
 mma Ray Front Air Cherenkov Experiment is designed to search for bursts\no
 f gamma rays above 200 MeV lasting from 60 nanoseconds to longer than 20\n
 microseconds. The custom-designed trigger and data-acquisition system of S
 GARFACE\npiggy-backs on the existing Whipple 10m telescope. The experiment
  has operated for\nmore than 3 years during which time about 1.2 million e
 vents were recorded. The\nmajority of events originate from cosmic-ray sho
 wers from which we see\, both\,\nCherenkov emission and fluorescence light
 . Rejection of background events is achieved\nthrough timing and imaging i
 nformation available for each event. Potential sources of\nbursts of gamma
  rays are evaporation of primordial black holes within about 240 pc and\ng
 amma-ray emission accompanying giant radio pulses. Results are presented o
 n the\nsearch for evaporation of primordial black holes and gamma-ray emis
 sion coincident\nwith giant pulses from the Crab Nebula.\n\nhttps://indico
 .nucleares.unam.mx/event/4/session/54/contribution/370
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/54/contribution/370
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