BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Estudio de EECR desde el espacio. DTSTART;VALUE=DATE-TIME:20171107T220000Z DTEND;VALUE=DATE-TIME:20171107T223000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-23@cern.ch DESCRIPTION:Speakers: Oscar Martínez Bravo (BUAP)\nhttps://indico.buap.mx /event/4/contributions/23/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/23/ END:VEVENT BEGIN:VEVENT SUMMARY:El Observatorio HAWC\, resultados recientes DTSTART;VALUE=DATE-TIME:20171107T233000Z DTEND;VALUE=DATE-TIME:20171108T000000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-22@cern.ch DESCRIPTION:Speakers: Alberto Caramiñana (INAOE)\nhttps://indico.buap.mx/ event/4/contributions/22/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/22/ END:VEVENT BEGIN:VEVENT SUMMARY:Jarlskog invariant in SMS_3 DTSTART;VALUE=DATE-TIME:20171108T223000Z DTEND;VALUE=DATE-TIME:20171108T230000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-20@cern.ch DESCRIPTION:Speakers: Javier Montaño Peraza (UNISON)\nhttps://indico.buap .mx/event/4/contributions/20/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/20/ END:VEVENT BEGIN:VEVENT SUMMARY:Mass Composition Studies\, for Atmospheric Showers DTSTART;VALUE=DATE-TIME:20171108T220000Z DTEND;VALUE=DATE-TIME:20171108T223000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-19@cern.ch DESCRIPTION:Speakers: Alejandra Parra (BUAP)\nhttps://indico.buap.mx/event /4/contributions/19/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/19/ END:VEVENT BEGIN:VEVENT SUMMARY:COURSE DARK MATTER DTSTART;VALUE=DATE-TIME:20171108T230000Z DTEND;VALUE=DATE-TIME:20171109T000000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-18@cern.ch DESCRIPTION:Speakers: Roberto Lineros ()\nhttps://indico.buap.mx/event/4/c ontributions/18/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/18/ END:VEVENT BEGIN:VEVENT SUMMARY:Additional Symmetries in 2HDM-III as a tool for the search of New Physics effects DTSTART;VALUE=DATE-TIME:20171108T183000Z DTEND;VALUE=DATE-TIME:20171108T190000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-17@cern.ch DESCRIPTION:Speakers: Lao-Tse López Lozano (UAEH)\nhttps://indico.buap.mx /event/4/contributions/17/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/17/ END:VEVENT BEGIN:VEVENT SUMMARY:Dark matter and unusual suspects DTSTART;VALUE=DATE-TIME:20171108T180000Z DTEND;VALUE=DATE-TIME:20171108T183000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-16@cern.ch DESCRIPTION:Speakers: Selim Gómez (UAEH)\nhttps://indico.buap.mx/event/4/ contributions/16/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/16/ END:VEVENT BEGIN:VEVENT SUMMARY:Gamma-rays from MeV Dark Matter in light of CMB data DTSTART;VALUE=DATE-TIME:20171107T230000Z DTEND;VALUE=DATE-TIME:20171107T233000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-14@cern.ch DESCRIPTION:Speakers: Javier Israel Reynoso (UdeG)\nhttps://indico.buap.mx /event/4/contributions/14/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/14/ END:VEVENT BEGIN:VEVENT SUMMARY:Neutrino Theory 1967-2017 DTSTART;VALUE=DATE-TIME:20171107T223000Z DTEND;VALUE=DATE-TIME:20171107T230000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-13@cern.ch DESCRIPTION:Speakers: Ernest Ma (UC-Riverside)\nhttps://indico.buap.mx/eve nt/4/contributions/13/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/13/ END:VEVENT BEGIN:VEVENT SUMMARY:Materia oscura en los centros galáticos DTSTART;VALUE=DATE-TIME:20171107T173000Z DTEND;VALUE=DATE-TIME:20171107T180000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-11@cern.ch DESCRIPTION:Speakers: Tonatiuh Matos (CINVESTAV)\nhttps://indico.buap.mx/e vent/4/contributions/11/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/11/ END:VEVENT BEGIN:VEVENT SUMMARY:Decrypting Dark Energy with spectroscopic surveys: BOSS\,eBOSS y D ESI DTSTART;VALUE=DATE-TIME:20171106T230000Z DTEND;VALUE=DATE-TIME:20171106T233000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-10@cern.ch DESCRIPTION:Speakers: Mariana Vargas Magaña (UNAM)\nhttps://indico.buap.m x/event/4/contributions/10/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/10/ END:VEVENT BEGIN:VEVENT SUMMARY:Modern Aspects of Perturbative Quantum Field Theory and Gravity DTSTART;VALUE=DATE-TIME:20171106T220000Z DTEND;VALUE=DATE-TIME:20171106T223000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-9@cern.ch DESCRIPTION:Speakers: Bryan Larios (BUAP)\nhttps://indico.buap.mx/event/4/ contributions/9/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/9/ END:VEVENT BEGIN:VEVENT SUMMARY:Dark matter stability and flavor symmetries DTSTART;VALUE=DATE-TIME:20171106T223000Z DTEND;VALUE=DATE-TIME:20171106T230000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-8@cern.ch DESCRIPTION:Speakers: Eduardo Peinado (UNAM)\nhttps://indico.buap.mx/event /4/contributions/8/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/8/ END:VEVENT BEGIN:VEVENT SUMMARY:Search for dark matter with bubble chambers DTSTART;VALUE=DATE-TIME:20171106T183000Z DTEND;VALUE=DATE-TIME:20171106T190000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-7@cern.ch DESCRIPTION:Speakers: Eric Vázquez Jáuregui (UNAM)\nhttps://indico.buap. mx/event/4/contributions/7/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/7/ END:VEVENT BEGIN:VEVENT SUMMARY:Constrained flavor violation (CFV) DTSTART;VALUE=DATE-TIME:20171106T180000Z DTEND;VALUE=DATE-TIME:20171106T183000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-6@cern.ch DESCRIPTION:Speakers: Alfonso Díaz Furlong (BUAP)\nhttps://indico.buap.mx /event/4/contributions/6/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/6/ END:VEVENT BEGIN:VEVENT SUMMARY:BOSONES ULTRA LIGEROS COMO CANDIDATOS DE MATERIA OSCURA DTSTART;VALUE=DATE-TIME:20171106T173000Z DTEND;VALUE=DATE-TIME:20171106T180000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-5@cern.ch DESCRIPTION:Speakers: Ana A. Avilez López (CINVESTAV)\nhttps://indico.bu ap.mx/event/4/contributions/5/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/5/ END:VEVENT BEGIN:VEVENT SUMMARY:Gravitational Wave Astronomy: a New Window to the Cosmos DTSTART;VALUE=DATE-TIME:20171107T160000Z DTEND;VALUE=DATE-TIME:20171107T170000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-4@cern.ch DESCRIPTION:Speakers: Omar Lopez Cruz ()\nGravitational wave astronomy is reaching maturatirity. In this talk I comment on the\nlast results from t he LIGO and VIRGO collaborations. I will comment on the masses of merging black holes and\nthe follow up observations of neutron star merger (a.k.a kilonova). I will comment on the impact of kilonoavae on galaxy evolutio n.\n\nhttps://indico.buap.mx/event/4/contributions/4/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/4/ END:VEVENT BEGIN:VEVENT SUMMARY:Plenary: Connecting Neutrinos with light dark matter candidates DTSTART;VALUE=DATE-TIME:20171108T160000Z DTEND;VALUE=DATE-TIME:20171108T170000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-3@cern.ch DESCRIPTION:Speakers: Roberto Lineros ()\nDark Matter is an unseen sculpto r of the Universe. Its presence affects astrophysical objects at different scales. However\, its nature is still unknown. Particle dark matter candi dates have been proposed explaining the relic abundance\, properties\, and indicating search strategies. Unfortunately\, the null observational resu lts motivate the community to study other candidates and to propose new s earch strategies. A possible way to observe dark matter is by affecting th e neutrino flavor propagation at galactic scales. This effect might be man ifested at PeV neutrino energies\, which is the energy window accessible t o neutrino telescopes like ICECUBE and KM3NET. In addition\, this effect i s more sensitive to light dark matter like fuzzy dark matter or any dark m atter candidate with masses of keV\, like the Majoron or sterile neutrinos .\n\nhttps://indico.buap.mx/event/4/contributions/3/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/3/ END:VEVENT BEGIN:VEVENT SUMMARY:Plenary: Dark Revelations of $SU(3)^3$ and $SU(3)^4$ DTSTART;VALUE=DATE-TIME:20171106T160000Z DTEND;VALUE=DATE-TIME:20171106T170000Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-2@cern.ch DESCRIPTION:Speakers: Ernest Ma (UC-Riverside)\nDark Revelations of $SU(3 )^3$ and $SU(3)^4$\n\nhttps://indico.buap.mx/event/4/contributions/2/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/2/ END:VEVENT BEGIN:VEVENT SUMMARY:Inauguration DTSTART;VALUE=DATE-TIME:20171106T153000Z DTEND;VALUE=DATE-TIME:20171106T155500Z DTSTAMP;VALUE=DATE-TIME:20260618T014807Z UID:indico-contribution-4-1@cern.ch DESCRIPTION:Speakers: Lorenzo Díaz Cruz (BUAP)\nhttps://indico.buap.mx/ev ent/4/contributions/1/ LOCATION:Puebla\, Pue.\, México URL:https://indico.buap.mx/event/4/contributions/1/ END:VEVENT END:VCALENDAR