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DTSTART:20170326T010000
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DTSTART:20171029T010000
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DTSTART;TZID=Europe/Rome:20171220T143000
DTEND;TZID=Europe/Rome:20171220T160000
DTSTAMP:20260918T015503
CREATED:20171213T185230Z
LAST-MODIFIED:20171227T184806Z
UID:8042-1513780200-1513785600@w3.lnf.infn.it
SUMMARY:Dark Matter\, Double Supernova Neutrino Explosion\, Degenerate Vacua\, Pre-determination ? Why Standard Model Group ?
DESCRIPTION:We propose a model for dark matter\, which in principle ONLY use the Standard Model\, although it only works under use of speculated NONPERURBATIVE effects. In this model the dark matter consists of insect sized pearls or better bubbles  made from a different phase of vacuum (“condensate vacuum”) consisting of a fluid of top and anti top quarks – likely in the form of bound states of 6 top + 6 anti top\nquarks – pumped up by usual atoms under very high pressure  to compensate the very strong surface tension of the bubbles.\nWe take as fitted values of the size of the bubbles a diameter of 1 cm and a mass of $10^8$ kg\, and correspondingly the distance between the individual bubbles is between our distance to the moon and to the sun. Impacts – one about every century – would fit with causing the special type of volcanoes called kimberlite pipes\, of which there are  about 6500 known on the earth.\nIn the supernova SN1987A in the Large Margellanic Cloud there were observed a controversial neutrino signal in Mont Blanc by LSD about 5 hours before the main neutrino burst observed later; this is speculated to be due to our pearls.
URL:/event/dark-matter-double-supernova-neutrino-explosion-degenerate-vacua-pre-determination-why-standard-model-group/
LOCATION:Auditorium B. Touschek\, Via Enrico Fermi\, 54\, Frascati\, Roma\, 00044\, Italia
CATEGORIES:Seminari generali
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