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SUMMARY:Constraining the absolute neutrino mass via time-of-flight measure
 ments of the Supernovae electron neutrinos with DUNE.
DTSTART;VALUE=DATE-TIME:20220324T144500Z
DTEND;VALUE=DATE-TIME:20220324T145800Z
DTSTAMP;VALUE=DATE-TIME:20260517T050107Z
UID:indico-contribution-17549@indico.ific.uv.es
DESCRIPTION:Speakers: Federica Pompa (IFIC Valencia)\nSupernova (SN) explo
 sions are the most powerful cosmic factories of all-flavors\, MeV-scale\, 
 neutrinos. Their detection is of great importance not only for astrophysic
 s\, but also to shed light on neutrino properties. Since the first observa
 tion of a SN neutrino signal in the 1987\, the international network of SN
  neutrinos observatories has been greatly expanded\, in order to detect th
 e next galactic SN explosion with much higher statistics and accuracy in t
 he neutrino energy-time-flavor space. The Deep Underground Neutrino Experi
 ment (DUNE) is a proposed leading-edge neutrino experiment\, planning to b
 egin operations in 2026. DUNE will have capability to extract precious inf
 ormation about SN neutrinos. In this contribution\, I will discuss the con
 straints that we expect to achieve with DUNE on the absolute value of the 
 neutrino mass\, obtained by considering the time delay in the propagation 
 of massive electron neutrinos from production in the SN environment to the
 ir detection in DUNE. Furthermore\, the comparison of sensitivities achiev
 ed for the two possible neutrino mass orderings is discussed\, as well as 
 the effects due to propagation in the Earth matter.\n\nhttps://indico.ific
 .uv.es/event/6372/contributions/17549/
LOCATION:Salón de Actos del IFIC (PCUV)
URL:https://indico.ific.uv.es/event/6372/contributions/17549/
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