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SUMMARY:The multi-messenger magnetar legacy
DTSTART:20231213T100000Z
DTEND:20231213T120000Z
DTSTAMP:20260314T130900Z
UID:indico-event-38896@agenda.infn.it
DESCRIPTION:Speakers: Simone Dall'Osso (Istituto Nazionale di Fisica Nucle
 are)\n\nMagnetars are extraordinary neutron stars (NS). Their bright and h
 ighly variable X/γ-ray emission is powered by the dissipation of their ul
 tra-strong magnetic fields (> 10^15 G)\, providing a unique probe of the p
 hysics of NS interiors. A peculiarly fast rotation (< a few milliseconds) 
 at birth\, inherited from the properties of the progenitor\, is thought to
  be key to the formation of magnetars via a powerful dynamo\, a scenario s
 upported by recent MHD simulations. With their huge reservoirs of rotation
 al and magnetic energy\, newly born magnetars can be powerful machines cap
 able of producing bright electromagnetic (EM) transients\, e.g. gamma-ray 
 bursts (GRBs)\, Super-Luminous Supernovae\, Fast Radio Bursts (FRBs)\, and
  intense gravitational wave (GW) transients which represent their ultimate
  signatures.I will present our current understanding of magnetars\, new re
 sults linking them to GRBs and FRBs\, and ongoing efforts in the search fo
 r their GW transient signals both in the current (O4) and future (O5 and p
 ost-O5) LIGO/virgo science runs.  Zoom Linkhttps://cern.zoom.us/j/625712
 70626?pwd=SWZpVDlCdFZWZUNmR2V3Ujl6RXRnZz09ID meeting: 625 7127 0626passwor
 d: 877788\n\nhttps://agenda.infn.it/event/38896/
URL:https://agenda.infn.it/event/38896/
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