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• W2590278329 endingPage "83" @default.
• W2590278329 startingPage "83" @default.
• W2590278329 abstract "Supermassive black holes observed at high redshift $zgtrsim6$ could grow from direct collapse black holes (DCBHs) with mass $sim10^5,M_{odot}$, which result from the collapse of supermassive stars (SMSs). If a relativistic jet is launched from a DCBH, it can break out of the collapsing SMS and produce a gamma-ray burst (GRB). Although most of the GRB jets are off-axis from our line of sight, we show that the energy injected from the jet into a cocoon is huge $sim10^{55-56},{rm{erg}}$, so that the cocoon fireball is observed as ultra-luminous supernovae of $sim10^{45-46}rm{,erg,s^{-1}}$ for $sim5000 [(1+z)/16] rm{,days}$. They are detectable by the future telescopes with near infrared bands, such as, $Euclid$, $WFIRST$, $WISH$, and $JWST$ up to $zsim20$ and $sim 100$ events per year, providing a direct evidence of the DCBH scenario." @default.
• W2590278329 created "2017-03-03" @default.
• W2590278329 creator A5028851543 @default.
• W2590278329 creator A5033145073 @default.
• W2590278329 creator A5059168304 @default.
• W2590278329 creator A5081957737 @default.
• W2590278329 date "2016-05-25" @default.
• W2590278329 modified "2023-09-27" @default.
• W2590278329 title "THE JET-POWERED SUPERNOVAE OF ∼10⁵<i>M</i>_⊙POPULATION III STARS ARE OBSERVABLE BY<i>EUCLID, WFIRST, WISH</i>, AND<i>JWST</i>" @default.
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