MULTIMESSENGER IMPLICATIONS OF BNS DETECTIONS
GERGELY DÁLYA ELTE Dept. of Atomic Physics
ELFT Astroparticle Summer School 09/06/2018
MULTIMESSENGER IMPLICATIONS OF BNS DETECTIONS GERGELY D LYA ELTE - - PowerPoint PPT Presentation
MULTIMESSENGER IMPLICATIONS OF BNS DETECTIONS GERGELY D LYA ELTE Dept. of Atomic Physics ELFT Astroparticle Summer School 09/06/2018 MULTIMESSENGER ASTRONOMY ANATOMY OF A BNS MERGER WHAT ABOUT NEUTRINOS? May accelerate cosmic rays to high
ELFT Astroparticle Summer School 09/06/2018
May accelerate cosmic rays to high energies --> GeV-EeV neutrinos
Detection of neutrinos: restrict E dissipation mechanisms & hadronic densities No coincident neutrino was found in the end...
Rapid decline in the bluest bands
Photometric fit Spectroscopic fit
Contains Fe-group or light r-process nuclei Peak at optical wavelengths Short timescale: ~ 1 day
A>140 heavy lanthanide elements Peak at NIR wavelengths Longer timescale: ~ 1 week
GW: distance, EM: recession velocity -- does not require a ladder!
GW polarization --> binary inclination; thanks to Virgo!
Question of weighting -- B magnitude or stellar mass?
Total stochastic background from BNS ~ from BBH They should be detectable at design sensitivity
1) Prompt collapse to BH 2) Long-term stable NS 3) Supermassive NS --> collapse to BH