The First Supernova Explosions in the Universe
Author(s) -
Volker Bromm,
Naoki Yoshida,
Lars Hernquist
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/379359
Subject(s) - physics , supernova , astrophysics , metallicity , redshift , stars , universe , population , halo , astronomy , instability , galaxy , demography , sociology , mechanics
We investigate the supernova explosions that end the lives of massivePopulation III stars in low-mass minihalos (M~10^6 M_sun) at redshifts z~20.Employing the smoothed particle hydrodynamics method, we carry out numericalsimulations in a cosmological set-up of pair-instability supernovae withexplosion energies of E_SN=10^51 and 10^53 ergs. We find that the moreenergetic explosion leads to the complete disruption of the gas in theminihalo, whereas the lower explosion energy leaves much of the halo intact.The higher energy supernova expels > 90% of the stellar metals into a region ~1kpc across over a timescale of 3-5 Myr. Due to this burst-like initial starformation episode, a large fraction of the universe could have been endowedwith a metallicity floor, Z_min>10^-4 Z_sun, already at z>15.Comment: Published in ApJ Letter
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