Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries

We present a new mechanism for the ejection of a common envelope in a massive binary, where the energy source is nuclear energy rather than orbital energy. This can occur during the slow merger of a massive primary with a secondary of 1-3 Msun when the primary has already completed helium core burni...

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Main Authors: Podsiadlowski, P, Ivanova, N, Justham, S, Rappaport, S
Format: Journal article
Published: 2010
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author Podsiadlowski, P
Ivanova, N
Justham, S
Rappaport, S
author_facet Podsiadlowski, P
Ivanova, N
Justham, S
Rappaport, S
author_sort Podsiadlowski, P
collection OXFORD
description We present a new mechanism for the ejection of a common envelope in a massive binary, where the energy source is nuclear energy rather than orbital energy. This can occur during the slow merger of a massive primary with a secondary of 1-3 Msun when the primary has already completed helium core burning. We show that, in the final merging phase, hydrogen-rich material from the secondary can be injected into the helium-burning shell of the primary. This leads to a nuclear runaway and the explosive ejection of both the hydrogen and the helium layer, producing a close binary containing a CO star and a low-mass companion. We argue that this presents a viable scenario to produce short-period black-hole binaries and long-duration gamma-ray bursts (LGRBs). We estimate a LGRB rate of about 1.e-6 per year at solar metallicity, which implies that this may account for a significant fraction of all LGRBs, and that this rate should be higher at lower metallicity.
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spelling oxford-uuid:c4e53de3-7865-42ff-ad7d-378baa199a3f2022-03-27T06:26:58ZExplosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole BinariesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:c4e53de3-7865-42ff-ad7d-378baa199a3fSymplectic Elements at Oxford2010Podsiadlowski, PIvanova, NJustham, SRappaport, SWe present a new mechanism for the ejection of a common envelope in a massive binary, where the energy source is nuclear energy rather than orbital energy. This can occur during the slow merger of a massive primary with a secondary of 1-3 Msun when the primary has already completed helium core burning. We show that, in the final merging phase, hydrogen-rich material from the secondary can be injected into the helium-burning shell of the primary. This leads to a nuclear runaway and the explosive ejection of both the hydrogen and the helium layer, producing a close binary containing a CO star and a low-mass companion. We argue that this presents a viable scenario to produce short-period black-hole binaries and long-duration gamma-ray bursts (LGRBs). We estimate a LGRB rate of about 1.e-6 per year at solar metallicity, which implies that this may account for a significant fraction of all LGRBs, and that this rate should be higher at lower metallicity.
spellingShingle Podsiadlowski, P
Ivanova, N
Justham, S
Rappaport, S
Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title_full Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title_fullStr Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title_full_unstemmed Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title_short Explosive Common-Envelope Ejection: Implications for Gamma-Ray Bursts and Low-Mass Black-Hole Binaries
title_sort explosive common envelope ejection implications for gamma ray bursts and low mass black hole binaries
work_keys_str_mv AT podsiadlowskip explosivecommonenvelopeejectionimplicationsforgammarayburstsandlowmassblackholebinaries
AT ivanovan explosivecommonenvelopeejectionimplicationsforgammarayburstsandlowmassblackholebinaries
AT justhams explosivecommonenvelopeejectionimplicationsforgammarayburstsandlowmassblackholebinaries
AT rappaports explosivecommonenvelopeejectionimplicationsforgammarayburstsandlowmassblackholebinaries