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SUMMARY:MAGIC - how Matter's extreme phases can be revealed in Gravitation
 al wave observations and in relativistic heavy Ion Collision experiments
DTSTART;VALUE=DATE-TIME:20181205T150000Z
DTEND;VALUE=DATE-TIME:20181205T154500Z
DTSTAMP;VALUE=DATE-TIME:20260813T152838Z
UID:indico-contribution-1175@indico.tlabs.ac.za
DESCRIPTION:Speakers: Horst Stoecker (GSI\, Goethe Universität and FiAS)\
 nThis talk combines a survey of our recent advancements in two rather dist
 inct fields\, which reveal - on first sight - a surprising similarity of b
 oth\, namely relativistic collisions of nuclei and of neutron stars.\n\nRe
 cently\, the group at FiAS and at Goethe University discovered that the em
 itted gravitational waves\, as predicted from general relativistic magneto
 - hydrodynamics from binary neutron star merger - calculations\, are extre
 mely sensitive to the appearance of quark matter and the stiffnes of the e
 quation of state of QCD Matter in the inner cores of the two colliding Neu
 tron Stars\, as also in their gravitational collapse to one black hole. Th
 is is a new observable messenger from outer space\, which does provide dir
 ect signals for the phase structure of strongly interacting QCD matter at 
 high baryon density and high temperature.\n\nThose astrophysically created
  extremes of thermodynamics do  match \, to within 20% \, the values of te
 mperatures which we find in relativistic hydrodynamics and transport theor
 y of heavy ion collisions at the existing laboratories like LHC\, SpS at C
 ern\, RHIC at Brookhaven\, and HaDes - SiS18 at GSi and at the NICA and FA
 IR accelerators under construction\, if though at quite different rapidity
  windows\, impact parameters and bombarding energies of the heavy nuclear 
 systems.\n\nWe demonstrate how the gravitational wave signals from future 
 advanced LIGO-Virgo - to radiowave signals from SKA-events can be combined
  with the high multiplicity fluctuation - and flow measurements in heavy i
 on detectors in the lab to pin down the EoS and the phase structure of den
 se matter.\n\nhttps://indico.tlabs.ac.za/event/75/contributions/1175/
LOCATION:Casa do Sol
URL:https://indico.tlabs.ac.za/event/75/contributions/1175/
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