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SUMMARY:From Birth to Burst: neutron star diversity and their link to Supe
 rnovae\, Gamma-ray Bursts and Fast Radio Bursts.
DTSTART;VALUE=DATE-TIME:20260415T123000Z
DTEND;VALUE=DATE-TIME:20260415T140000Z
DTSTAMP;VALUE=DATE-TIME:20260405T205500Z
UID:indico-event-881@indico.gssi.it
DESCRIPTION:Speakers: Nanda Rea (Institute of Space Sciences - CSIC)\n\nNe
 utron stars represent one of the most diverse and dynamicpopulations in hi
 gh-energy astrophysics\, manifesting as radio pulsars\,millisecond pulsars
 \, magnetars\, X-ray binaries\, and other exoticsubclasses. In recent year
 s\, time-domain surveys have revealedunexpected connections between these 
 classes and some of the mostenergetic transients in the Universe\, includi
 ng fast radio bursts(FRBs)\, gamma-ray bursts (GRBs)\, and certain superno
 vae (SNe). Thistalk provides a comprehensive overview of the “neutron st
 ar zoo\,”emphasizing the importance and distributions of physical parame
 terssuch as magnetic field\, spin\, age\, and environment that drive their
 observational phenomenology. I will review how different neutron starclass
 es emerge from similar evolutionary pathways and how they cantransition be
 tween states. Special focus will be placed onobservational and theoretical
  links between young magnetars andcore-collapse SNe\, between compact obje
 ct formation and GRBs\, andbetween magnetar bursts and FRBs.  \n\nhttps:
 //indico.gssi.it/event/881/
URL:https://indico.gssi.it/event/881/
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