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000291447 0881_ $$aDESY-PROC-2014-04
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000291447 1001_ $$aBanik, Sarmistha$$b0
000291447 1112_ $$aPanic2014$$cHamburg$$d2014-08-25 - 2014-08-29$$gPanic2014$$wGermany
000291447 245__ $$aCore-collapse supernova simulation using $\Lambda$ hyperon EoSwith density-dependent couplings
000291447 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2014
000291447 300__ $$a391-394
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000291447 520__ $$aRecently we generated an equation of state (EoS) table of dense matter relevant to neutron star and supernova with $\Lambda$ hyperons. We use this EoS to investigate the role of strange hyperons in the dynamical collapse of a non-rotatingmassive star to a black hole(BH) using 1D General relativistic simulation $GR1D$. We follow the dynamical formation and collapseof the protoneutron star (PNS) from the gravitational collapse of a massive progenitor, adopting this EoS table.
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000291447 650_7 $$2INSPIRE$$aprotoneutron star: collapse
000291447 650_7 $$2INSPIRE$$agravitation: collapse
000291447 650_7 $$2INSPIRE$$acoupling: density dependence
000291447 650_7 $$2INSPIRE$$astar: massive
000291447 650_7 $$2INSPIRE$$ahyperon
000291447 650_7 $$2INSPIRE$$asupernova
000291447 650_7 $$2INSPIRE$$aequation of state
000291447 650_7 $$2INSPIRE$$aneutron star
000291447 650_7 $$2INSPIRE$$anumerical calculations
000291447 650_7 $$2INSPIRE$$arelativistic
000291447 650_7 $$2INSPIRE$$ablack hole
000291447 650_7 $$2INSPIRE$$aformation
000291447 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000291447 7001_ $$aChar, Prasanta$$b1
000291447 773__ $$a10.3204/DESY-PROC-2014-04/115
000291447 7870_ $$0PUBDB-2015-03603$$aSchmidt, Alexander et.al.$$dHamburg : Deutsches Elektronen-Synchrotron, DESY, Hamburg, 2014$$iIsPartOf$$rDESY-PROC-2014-04$$tProceedings, 20th International Conference on Particles and Nuclei (PANIC 14)
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