BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Topical Seminar: Anomaly-induced neutron star cooling
DTSTART;VALUE=DATE-TIME:20231115T110000Z
DTEND;VALUE=DATE-TIME:20231115T120000Z
DTSTAMP;VALUE=DATE-TIME:20261012T150807Z
UID:indico-event-7266@indico.ific.uv.es
DESCRIPTION:Young neutron stars cool via the emission of neutrinos from th
 eir core. A precise understanding of all the different processes producing
  neutrinos in the hot and degenerate matter is essential for assessing the
  cooling rate of such stars. The main Standard Model processes contributin
 g to this effect are ν bremsstrahlung and mURCA\, which we will review in
  the talk. Then we will investigate another Standard Model process initiat
 ed by the Wess-Zumino-Witten term\, leading to the emission of neutrino pa
 irs via N γ → Nνν¯. We find that such processes\, with degenerate ne
 utrons\, can be comparable and even dominate over the prototypical and wel
 l-known cooling mechanisms\n\nhttps://indico.ific.uv.es/event/7266/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/7266/
END:VEVENT
END:VCALENDAR