BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//INPA - ECPv6.8.3//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:INPA
X-ORIGINAL-URL:https://inpa.lbl.gov
X-WR-CALDESC:Events for INPA
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:America/Los_Angeles
BEGIN:DAYLIGHT
TZOFFSETFROM:-0800
TZOFFSETTO:-0700
TZNAME:PDT
DTSTART:20200308T100000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:-0700
TZOFFSETTO:-0800
TZNAME:PST
DTSTART:20201101T090000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20200207T120000
DTEND;TZID=America/Los_Angeles:20200207T130000
DTSTAMP:20260429T230208
CREATED:20200203T232233Z
LAST-MODIFIED:20200203T232828Z
UID:724-1581076800-1581080400@inpa.lbl.gov
SUMMARY:INPA Seminar - Harikrishnan Ramani (LBNL)
DESCRIPTION:Speaker: Harikrishnan Ramani (LBNL)\n \nTitle: Nuclear Isomers as Dark Matter accelerators\nAbstract: Weak-scale dark matter particles\, in collisions with nuclei\, can mediate transitions between different nuclear energy levels. In particular\, owing to sizeable momentum exchange\, dark matter particles can enable de-excitation of nuclear isomers that are extremely long lived with respect to regular radioactive decays. In this paper\, we utilize data from a past experiment with $^{\rm 180m}$Ta to search for $\gamma$-lines that would accompany dark matter induced de-excitation of this isomer. Non-observation of such transitions above background yields the first direct constraint on the lifetime of $^{\rm 180m}$Ta against DM-initiated transitions: $T_{1/2}>1.3\times 10^{14}$~a at 90\% C.I. Using this result\, we derive novel constraints on dark matter models with strongly interacting relics\, and on models with inelastic dark matter particles. Existing constraints are strengthened by this independent new method. The obtained limits are also valid for the Standard Model $\gamma$-decay of \nuc{Ta}{\rm 180m}.
URL:https://inpa.lbl.gov/event/harikrishnan-ramani-lbnl/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
END:VEVENT
END:VCALENDAR